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  1. Employee Spotlight: Janice Lovato

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Careers, Jobs » Careers Stories » Employee Spotlight » Janice Lovato Janice Lovato-A gift for imagination The Associate Directorate for Nuclear and High Hazard Operations' Janice Lovato has turned her love for nature-watching and story-telling into writing a children's book called Germaine the Beetle. March 10, 2015 Janice Lovato Janice Lovato and her first children's book. "I am always telling stories, whether at bedtime, in the car going somewhere or sitting under a tree in the

  2. Janices start at Training & Technology

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    So, I am sure you will enjoy what Janice writes. As you know, the TAT School was a joint venture of the Oak Ridge Associated Universities and Y-12. It flourished at Y-12's...

  3. Employee Spotlight: Janice Lovato

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Janice Lovato March 10, 2015 A gift for imagination While the Associate Directorate for Nuclear and High Hazard Operations' Janice Lovato was still working as a cashier at Smith's Food and Drug Center in Los Alamos over a decade ago, a regular, usually friendly customer came through her line one day, but this time in an obviously disgruntled mood. As the shopper slowly placed his purchases on the cash register counter, he looked at Lovato in exasperation and told her that standing at the cash

  4. Janice Bryant Howroyd | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Janice Bryant Howroyd About Us Janice Bryant Howroyd - Founder, ACT-1 Janice Bryant Howroyd Janice Bryant Howroyd is the Founder and CEO of the ACT*1 Group, a global leader in deploying talent and resource management solutions. A North Carolina native, Janice left her hometown in 1976 armed with $900. Since then, she has dedicated her efforts to building an organization that is committed to keeping the humanity in human resources. She is a strong advocate for balance of education and

  5. Training and Technology … Janice Smiths story

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Janice Smith's story As we wind down the "TAT Treasures," as Don McMurray has dubbed these stories from TAT alumni, here is one from Janice Smith, a Y-12 employee in the Technology ...

  6. Summary of the Fall 2007 ASA Meetings

    U.S. Energy Information Administration (EIA) Indexed Site

    18 and 19, 2007 Washington, D.C. 1. Developing Key Energy Indicators, Janice Lent, (SMG) and Joseph Conklin (OOG), EIA In June of 2007, an inter-office team of EIA analysts and statisticians was chartered to identify a set of approximately 12 statistics or indicators to be designated Key Energy Indicators. The selected set of indicators will appear together, possibly in a prominent location, on the EIA website for the purposes of providing a quick, easily accessible overview-the "big

  7. QER- Comment of Janice Kurkoski

    Broader source: Energy.gov [DOE]

    Proposal for Conservation Reward Rate for Electricity First of all, thank you for the time you are taking to hear from the public along with the industry and government officials in this critical matter. I attended the public hearing in Hartford CT two days ago and was able to comment on parts of what we are proposing here. We are writing to open a conversation with you about a proposal that we have been discussing in our past meetings. We would like to see you initiate legislation that would mandate a "stepped rate" for electricity, under which consumers who used less would pay a lower rate per kilowatt hour than those who used more. Background North Quabbin Energy is a community group from the nine North Quabbin towns in north central Massachusetts that focuses on education and local action relating to ways to conserve energy and support local and regional enterprises that reduce our dependence on imported resources. The towns are Athol, Orange, Petersham, Royalston, Warwick, Wendell, New Salem, Erving and Phillipston. Our members include representatives from the appointed Energy Committees of these towns. For the past six years, we have participated in many different types of events and activities, always with an emphasis on the idea that the single best way to address the high financial, social, and environmental costs of our current energy use patterns is to consume less energy in the first place. What we have discovered in our community work is that most people seem aware of the reasons for conserving energy (lowering greenhouse gas emissions, saving money, reducing dependence on oil and other imported resources, etc.). Many are also knowledgeable about the basic weatherization and conservation strategies that utilities, municipalities, and community groups like ours try to promote (for example, adding insulation to homes, turning thermostats down, or using fluorescent or LED lighting rather than incandescent bulbs). Yet except when energy prices are extraordinarily high, it appears that there is a great deal of inertia among the general public about actually making changes in their energy consumption patterns. This proposal would address that issue of inertia by creating a direct incentive program for using less electricity. People could very quickly and easily make changes that would lower their electric use, and would see immediate results on their electric bills. Comparable programs Many utilities are beginning to offer peak and off-peak metering as a way to equalize demand on the electric grid, but although this is useful in making people more aware of their energy use patterns, it does nothing to reduce overall demand and may actually encourage more wasteful consumption at off-peak times. A few utilities are starting to offer the kind of stepped rate or rewards program that we are proposing. For example, Western Massachusetts Electric Company recently inaugurated a program that awards "points" (redeemable for consumer items) for the numbers of kilowatt hours saved. In our opinion, this kind of program sends the wrong message because it encourages people to save in one area (electricity use) in order to consume in another. Examples of programs more in line with what we are proposing already exist. One is British Columbia Hydro's "Conservation Rate," started in April 2010. Under their Residential Conservation Rate, customers pay 7.52 cents per kWh for the first 1,350 kWh they use over an average two-month billing period. Above that amount, customers pay 11.27 cents per kWh for the balance of the electricity used during the billing period. In nearby Vermont, the Washington Electric Cooperative has had stepped or tiered rates for years. They reward residential users with a relatively very low rate of 9.43 cents per kWhr for the first 200 kWhrs, and then charge a significantly higher rate of 21.06 cents thereafter. As a result, their customers use on average about 11% less than the households in our area. Points for discussion What might be a reasonable target figure for the stepped rate? The current Massachusetts average is about 610 kWh/month. Members of North Quabbin Energy have demonstrated that it is quite possible to use a half or even a third of that amount without any decline in standard or quality of living1. In fact, this level of reduction is imperative given the seriousness of climate change and resource depletion. How could this change best be promoted to the public? We would argue that this is not a rate increase, but rather a rate redistribution that rewards lower energy consumption. It seems important to emphasize the positive rewards of this kind of change, rather than framing it as a penalty for higher use2. It also seems crucial to demonstrate from the outset that reducing a household's electric use can be done with surprising ease, given a greater awareness of how much energy waste can be avoided with a change in behavior. How could the concerns of low-income customers, those with large families, or those who heat exclusively with electricity be addressed? The BCHydro and Washington Electric Cooperative programs provide useful models for addressing these questions, and there is a great deal of regional data that shows how these consumers would by no means be penalized in the kind of pricing structure we are proposing. What programs could be funded with the increased revenues? Public outrage would be justified if the money went into the general coffers of the utility companies and fossil fuel energy supply and distribution companies. Enhanced conservation programs should be the target of these revenues. Attachments: 1 NQE individual.pdf, 2 NQE proposed incentive rate Note - if attachments do not go through, see this web page for these documents: http://northquabbinenergy.org/wordpress/?page_id=205

  8. Microsoft Word - LM SMG Jan 2016 Update 18 Draft 12 no links...

    Energy Savers [EERE]

    ... LM Site Name Pre-LM Name Category Transferring Organization Regulatory Driver 1 Deepwater, NJ, Site DuPont Chambers Works 2 USACE FUSRAP 2 St. Louis, MO, Site St. Louis Downtown ...

  9. MEMORANDUM OF EX PARTE COMMUNICATION WITH THE DEPARTMENT OF ENERGY

    Broader source: Energy.gov (indexed) [DOE]

    Strangis (DOENNSA), Anatoli Welihozkiy (DOENNSA), John Wengle (DOENNSA), Gretchen Smith (DOENNSA), Madeleine Foley (DOENNSA), Janice Rivera (DOENNSA), Xavier Asconio (DOE...

  10. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... N-terminal additions to the WE14 peptide of chromogranin A create strong autoantigen agonists in type 1 diabetes Jin, Niyun ; Wang, Yang ; Crawford, Frances ; White, Janice ; ...

  11. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    N-terminal additions to the WE14 peptide of chromogranin A create strong autoantigen agonists in type 1 diabetes Jin, Niyun ; Wang, Yang ; Crawford, Frances ; White, Janice ; ...

  12. US-EU-Japan Working Group on Critical Materials

    Office of Environmental Management (EM)

    Materials Institute - Colorado School of Mines 12:20 Buffet Lunch 12:30 Canadian Rare Earth Elements - feeding the global supply chain Janice Zinck, Manager, Natural Resources ...

  13. Vehicles | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    To help you save money by saving energy, our experts are answering your home cooling questions. | Photo courtesy of iStockphotoJaniceRichard Energy Department experts answer ...

  14. Microsoft PowerPoint - Slice True-Up 101 pptx.pptx [Read-Only...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Ted Barham, Janice Johnson and many others Content Organized and Presented by Craig Larson Slice History A Review of Subscription and RD(Regional Dialogue) Slice distinctions...

  15. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... Mack, Douglas G. (1) Murphy, Guinevere A. (1) Novikov, Andrey (1) Rubtsova, Kira (1) Scott-Browne, James (1) White, Janice (1) Save Results Save this search to My Library Excel ...

  16. From: Schleicher, Heather M. To: Congestion Study Comments Cc...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    L; Abbott, Tim L; Byrd, Mark; Dawe, George C; Hanes, Spencer G Jr; Alexander, Michael D; Greene, Bill; Jett, Bill; ... Verderame, John; Kinny, Paul R; May, Sheri h; Hager, Janice ...

  17. From:

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    I urge you to consider these reasons and please do not establish any National Interest Energy Transmission Corridors. Thank you, Edwin Norman and Janice Lee Jarman 1510 County Road ...

  18. C O X Technical Services Pantex, LLC

    National Nuclear Security Administration (NNSA)

    ... changed, remains unchanged and in 5. PROJECT NO. (If applicable) X full force and ... Manager Steven L. Young Applied TechnologyR&D Manager Janice N. Tolk Maintenance Manager ...

  19. Analysis of Alternative Extensions of the Existing Production Tax Credit for Wind Generators

    Reports and Publications (EIA)

    2007-01-01

    Requestor: Ms. Janice Mays, Chief Counsel, Committee on Ways & Means, U.S. House of Representatives This is a letter response requesting analysis of alternative extensions of the existing production tax credit (PTC) that would apply to wind generators only.

  20. HANFORD ADVISORY BOARD

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    ... DOE-ORP Barb Wise, MSA Emy Laija, EPA Dale McKenney, CHPRC Susan Hayman, EnviroIssues Marc Jewett, CHPRC Hillary Johnson, EnviroIssues Janice Williams, CHPRC Dale Bignell, WCH

  1. Microsoft Word - TrainingAgenda_2013_06_25.docx

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Special Guest: Mary Hawken, Janice Johnson Content Organized and Presented by: Craig Larson Format: Net meeting with in-house room reservation for HQ AE's Note: Agenda subject to...

  2. Public Comments Received on the Draft Congestion Study | Department...

    Energy Savers [EERE]

    Norman, Edwin and Jarman, Janice Lee 09.19.2014 Smith, Laurie 09.19.2014 Wilsdorf, Jane ... Daniels, Celia 09.19.2014 Sack, Susan 09.20.2014 Smith, Dennis 09.20.2014 Smith, Laurie ...

  3. HIV/Cancer DB Match Document

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    COLLECTION AND VERIFICATION OF DATA FOR MATCHED RECORDS FROM US CANCER AND HIV/AIDS REGISTRIES Janice Watkins, Oak Ridge Associated Universities, T. Borges, Robert Stafford, Oak Ridge National Laboratory Robert Biggar, James Goedert, National Cancer Institute Janice Watkins, ORAU, MS 45, P.O. Box 117, Oak Ridge, TN 37830 Key Words: AIDS, HIV/AIDS Registry, Cancer Registry, data verification, record matching BACKGROUND Data for investigating cancer rates, cofactors, and disease progression in HIV

  4. New High-Capability Solid-State Electron Microscope Detector...

    Office of Science (SC) Website

    ... as a collaboration between SMG's group and Area Detector Systems Corp. (Poway, CA) under ... Collaborations, Non-DOE Interagency Collaboration Last modified: 7262016 9:51:05

  5. Microsoft Word - Canceled -7 Section C April 16 2010.doc

    Office of Environmental Management (EM)

    ... Law Enforcement Agency LMG Light Machine Gun LRI Live Round Inhibitor LRMB Live Round ... Incident Response Plan SMG Submachine Gun SNM Special Nuclear Material SO Office of ...

  6. Abstracts for EIA's Fall 2008 Meeting with the ASA Committee...

    Annual Energy Outlook [U.S. Energy Information Administration (EIA)]

    ... ASA Committee Recommendations: The committee recommended that the costs and effects of ... 6. Sensitivity Analysis of EIA Forecasting Systems, Preston McDowney, SMG and ...

  7. untitled

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    strategic management groups (SMGs) the work most directly supported. The SMGSMU acronyms are: NW: Nuclear Weapons SMG ... Infrastructure protection . . . . . . . . . . . 8 Materials ...

  8. Air Quality

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Heat & Cool » Home Cooling Systems » Air Conditioning Air Conditioning Air conditioners cost U.S. homeowners more than $11 billion each year, and regular maintenance can keep your air conditioner running efficiently. | Photo courtesy of ©iStockphoto/JaniceRichard Air conditioners cost U.S. homeowners more than $11 billion each year, and regular maintenance can keep your air conditioner running efficiently. | Photo courtesy of ©iStockphoto/JaniceRichard Two-thirds of all homes in the

  9. Air Conditioning | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Heat & Cool » Home Cooling Systems » Air Conditioning Air Conditioning Air conditioners cost U.S. homeowners more than $11 billion each year, and regular maintenance can keep your air conditioner running efficiently. | Photo courtesy of ©iStockphoto/JaniceRichard Air conditioners cost U.S. homeowners more than $11 billion each year, and regular maintenance can keep your air conditioner running efficiently. | Photo courtesy of ©iStockphoto/JaniceRichard Two-thirds of all homes in the

  10. DockingShop: A Tool for Interactive Molecular Docking Ting-Cheng...

    Office of Scientific and Technical Information (OSTI)

    ... Covalent bond Cova lent bond Hydrogen bond Hydro gen bond monitors the position and ... Figure 3. Small blue spheres represent water. Dashed-blue lines represent hydrogen bonds ...

  11. The Availability and Price of Petroleum and Petroleum Products...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    oil producing countries in the Middle East and North Africa, amid low global surplus crude oil production capacity, has also lent support to crude oil prices. A framework...

  12. Analysis of Selected Provisions of the Domestic Manufacturing and Energy Jobs Act of 2010

    Reports and Publications (EIA)

    2010-01-01

    This report responds to a letter dated August 16, 2010, from Janice Mays, Staff Director of the U.S. House of Representatives' Committee on Ways and Means, requesting that the U.S. Energy Information Administration (EIA) analyze several provisions included in the July 26, 2010, discussion draft of the Domestic Manufacturing and Energy Jobs Act of 2010.

  13. LM Releases Update of Site Management Guide

    Broader source: Energy.gov [DOE]

    A new edition of the U.S. Department of Energy (DOE) Office of Legacy Management (LM) Site Management Guide (SMG) was posted to the LM website, February 24, 2015.

  14. Summary of the Energy Information Administration's (EIA)

    U.S. Energy Information Administration (EIA) Indexed Site

    the Energy Information Administration's (EIA) Spring Meeting with the American Statistical Association (ASA) Committee on Energy Statistics April 3 and 4, 2003 Thursday Morning, April 3, 2003 EIA's Survey Quality Effort: Where is EIA Going? Shawna Waugh, Statistics and Methods Group (SMG) Moderator, Jim Joosten and Tom Murphy, Coal, Nuclear, Electric and Alternate Fuels (CNEAF), and Nancy Kirkendall, Tom Broene, John Vetter and Howard Bradsher-Fredrick, Facilitator, SMG. Session Overview

  15. Summary of the Fall 2005 ASA Meetings

    U.S. Energy Information Administration (EIA) Indexed Site

    0 and 21, 2005 with the Energy Information Administration 1000 Independence Ave., SW. Washington, D.C. 20585 Introductory Sessions: Opening Remarks: Guy Caruso, EIA Administrator to include: 1. Update on the External Review Team 2. New EIA Homepages 3. EIA-914 Data 4. Hurricane Katrina Updates: 5. Since the Spring Meeting, Nancy Kirkendall, Director, SMG 6. Results of the Simulation Study for the EIA-914, Preston McDowney, SMG 7. Update: EIA's Regional Short-Term Energy Outlook, Margot Anderson,

  16. Summary.qxd

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    the Energy Information Administration's (EIA) Spring Meeting with the American Statistical Association (ASA) Committee on Energy Statistics April 3 and 4, 2003 Thursday Morning, April 3, 2003 EIA's Survey Quality Effort: Where is EIA Going? Shawna Waugh, Statistics and Methods Group (SMG) Moderator, Jim Joosten and Tom Murphy, Coal, Nuclear, Electric and Alternate Fuels (CNEAF), and Nancy Kirkendall, Tom Broene, John Vetter and Howard Bradsher-Fredrick, Facilitator, SMG. Session Overview

  17. MORTALITY AMONG WORKERS AT THE SAVANNAH RIVER NUCLEAR FUELS PRODUCTION FACILITY

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    MORTALITY AMONG WORKERS AT THE SAVANNAH RIVER NUCLEAR FUELS PRODUCTION FACILITY Donna L. Cragle and Janice P. Watkins, Center for Epidemiologic Research; Kathryn Robertson-DeMers, Bechtel Hanford, Inc. Donna Cragle, Oak Ridge Associated Universities, P.O. Box 117, Oak Ridge, TN 37831-0117 Key Words: mortality study, radiation exposure, leukemia, occupational cohort, trend test INTRODUCTION Since 1952 the Savannah River Site (SRS), located in Aiken, South Carolina, has operated as a Department of

  18. Thomas Jefferson High School for Science & Technology Takes 2015 Virginia

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Science Bowl | Jefferson Lab Takes 2015 Virginia Science Bowl Thomas Jefferson High School for Science & Technology Takes 2015 Virginia Science Bowl 2014 Virginia High School Science Bowl The team from Thomas Jefferson High School for Science and Technology, Alexandria, swept through the Virginia Regional High School Science Bowl undefeated on Feb. 7. The team of (back row, left to right) Matthew Barbano, Tiger Zhang and Janice Ong, and (front, l. to r.) Franklyn Wang and Ross Dempsey

  19. EM SSAB CHAIRS Bi-Monthly Conference Call

    Office of Environmental Management (EM)

    December 15, 2014 Participants Board Chairs/Representatives Site Staff Hanford Steve Hudson, Susan Leckband Kristen Skopeck, Sharon Braswell Idaho Herb Bohrer, Harry Griffith Ann Riedesel Nevada Donna Hruska, Janice Keiserman Kelly Snyder, Barbara Ulmer Northern New Mexico Doug Sayre, Allison Majure Menice Santistevan Oak Ridge David Hemelright Pete Osborne, Dave Adler, Spencer Gross, Melyssa Noe Paducah Ben Peterson Robert Smith, Eric Roberts, Jim Ethridge Portsmouth Greg Simonton Savannah

  20. EM SSAB Chairs Conference Call

    Office of Environmental Management (EM)

    March 26, 2015 Participants Board Chairs/Representatives Site Staff Hanford Steve Hudson, Susan Leckband Kristen Skopeck, Sharon Braswell, Joni Grindstaff Idaho Lori McNamara Nevada Donna Hruska, Janice Keiserman Kelly Snyder, Barbara Ulmer Northern New Mexico Doug Sayre Lee Bishop, Menice Santistevan Oak Ridge David Hemelright Pete Osborne, Spencer Gross, Melyssa Noe Paducah Ben Peterson Robert Smith, Eric Roberts Portsmouth Greg Simonton Savannah River Harold Simon, Eleanor Hopson de'Lisa

  1. EM SSAB Chairs Conference Call

    Office of Environmental Management (EM)

    Chairs Conference Call December 17, 2015 Participants Board Chairs/Representatives Site Staff Hanford Steve Hudson, Susan Leckband Kristen Skopeck, Sharon Braswell, Joni Grindstaff Idaho Herb Bohrer Jordan Davies Nevada Donna Hruska, Janice Keiserman Kelly Snyder, Barbara Ulmer Northern New Mexico Doug Sayre, Gerard Martinez Menice Santistevan, Mike Gardipe Oak Ridge Belinda Price, Alfreda Cook David Adler, Pete Osborne, Spencer Gross, Paducah Doreen (Renie) Barger Buz Smith, Eric Roberts

  2. EM SSAB Chairs Conference Call

    Office of Environmental Management (EM)

    Chairs Conference Call March 23, 2016 Participants Board Chairs/Representatives Site Staff Hanford Steve Hudson, Susan Leckband Kristen Holmes Idaho Herb Bohrer Jordan Davies Nevada Donna Hruska, Janice Keiserman Kelly Snyder, Barbara Ulmer Northern New Mexico Doug Sayre, Gerard Martinez Menice Santistevan, Mike Gardipe Oak Ridge Alfreda Cook Pete Osborne Paducah Doreen (Renie) Barger Buz Smith, Eric Roberts, Mike Kemp Portsmouth Bob Berry Rick Greene, Julie Galloway Savannah River Harold Simon

  3. EM SSAB Chairs Conference Call

    Office of Environmental Management (EM)

    August 11, 2015 Participants Board Chairs/Representatives Site Staff Hanford Steve Hudson, Susan Leckband Kristen Skopeck, Sharon Braswell, Joni Grindstaff Idaho Herb Bohrer Melvin "Keith" Branter Nevada Donna Hruska, Janice Keiserman Kelly Snyder, Barbara Ulmer Northern New Mexico Doug Sayre Menice Santistevan Oak Ridge David Hemelright Pete Osborne, Spencer Gross, Paducah Ben Peterson Eric Roberts Portsmouth Will Henderson Savannah River Harold Simon de'Lisa Carrico DOE-HQ

  4. Open House Gives Residents New Understanding of Nevada National Security

    Energy Savers [EERE]

    Site | Department of Energy Open House Gives Residents New Understanding of Nevada National Security Site Open House Gives Residents New Understanding of Nevada National Security Site August 15, 2016 - 12:15pm Addthis Nevada Site Specific Advisory Board (NSSAB) members, left to right, Pennie Edmond, Donna Hruska (NSSAB chair), Janice Keiserman, and Don Neill in front of the NSSAB display at the Groundwater Open House. Nevada Site Specific Advisory Board (NSSAB) members, left to right, Pennie

  5. Community Partners reEnergize Industry in Nebraska | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Community Partners reEnergize Industry in Nebraska What if every time you lent your neighbor a cup of flour, he invited you and the rest of your block to share his freshly baked ...

  6. Reducing Xerostomia After Chemo-IMRT for Head-and-Neck Cancer: Beyond Sparing the Parotid Glands

    SciTech Connect (OSTI)

    Little, Michael; Schipper, Matthew; Feng, Felix Y.; Vineberg, Karen; Cornwall, Craig; Murdoch-Kinch, Carol-Anne; Eisbruch, Avraham

    2012-07-01

    Purpose: To assess whether, in addition to sparing the parotid glands (PGs), xerostomia after chemotherapy plus intensity-modulated radiotherapy (chemo-IMRT) for head-and-neck cancer is affected by reducing the dose to the other salivary glands. Patients and Methods: In a prospective study, 78 patients with Stage III-IV oropharynx/nasopharynx cancer underwent chemo-IMRT, with the aim of sparing the parts of the bilateral PGs, oral cavity (OC) containing the minor salivary glands, and contralateral submandibular gland (SMG) outside the target (when contralateral level I was not a target). Before therapy and periodically for 24 months, validated patient-reported xerostomia questionnaire (XQ) scores and observer-graded xerostomia scores were recorded. Also, the stimulated and unstimulated saliva was measured selectively from each of the PGs and SMGs. The mean OC doses served as surrogates of minor salivary gland dysfunction. Regression models assessed the XQ and observer-graded xerostomia predictors. Results: Statistically significant predictors of the XQ score on univariate analysis included the OC, PG, and SMG mean doses and the baseline XQ score, time since RT, and both stimulated and unstimulated PG saliva flow rates. Similar factors were statistically significant predictors of observer-graded xerostomia. The OC, PG, and SMG mean doses were moderately intercorrelated (r = 0.47-0.55). On multivariate analyses, after adjusting for the PG and SMG doses, the OC mean dose (p < .0001), interval from RT (p < .0001), and stimulated PG saliva (p < .0025) were significant predictors of the XQ scores and the OC mean dose and time for observer-graded xerostomia. Although scatter plots showed no thresholds, an OC mean dose of <40 Gy and contralateral SMG mean dose of <50 Gy were each associated with low patient-reported and observer-rated xerostomia at almost all post-therapy points. Conclusion: The PG, SMG, and OC mean doses were significant predictors of both patient

  7. 15th Annual DOE Small Business Forum and Expo | Department of Energy

    Energy Savers [EERE]

    Cooling #AskEnergySaver: Home Cooling July 24, 2014 - 11:13am Addthis Home cooling accounts for 6 percent of the average household's energy use. To help you save money by saving energy, our experts are answering your home cooling questions. | Photo courtesy of ©iStockphoto/JaniceRichard Home cooling accounts for 6 percent of the average household's energy use. To help you save money by saving energy, our experts are answering your home cooling questions. | Photo courtesy of

  8. Health Surveillance Outcomes in Former Rocky Flats Radiation Workers

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Surveillance of Rocky Flats Radiation Workers Janice P. Watkins 1 , Elizabeth D. Ellis 1 , F. Joseph Furman 2 , Roger B. Falk 2 , Joe M. Aldrich 2 , and Donna L. Cragle 1 ORAU Technical Report # 2006-0408 1 Oak Ridge Institute for Science and Education, Center for Epidemiologic Research; P.O. Box 117; Oak Ridge, TN 37831-0117 2 Oak Ridge Institute for Science and Education, Center for Epidemiologic Research; 9950 W. 80 th Avenue, Suite 17; Arvada, CO 80005-3914 This report was funded by

  9. Berkeley Joins the Cleantech University Prize | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Berkeley Joins the Cleantech University Prize Berkeley Joins the Cleantech University Prize March 8, 2016 - 10:13am Addthis Heating and air conditioning – an $11 billion industry in America - accounts for 5% of domestic energy use. By reducing contaminant buildup, a new technology could increase efficiency by as much as 25%. Photo courtesy: ©iStockphoto/JaniceRichard. Heating and air conditioning - an $11 billion industry in America - accounts for 5% of domestic energy use. By reducing

  10. #AskEnergySaver: Home Cooling | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Cooling #AskEnergySaver: Home Cooling July 24, 2014 - 11:13am Addthis Home cooling accounts for 6 percent of the average household's energy use. To help you save money by saving energy, our experts are answering your home cooling questions. | Photo courtesy of ©iStockphoto/JaniceRichard Home cooling accounts for 6 percent of the average household's energy use. To help you save money by saving energy, our experts are answering your home cooling questions. | Photo courtesy of

  11. 3C 220.3: A radio galaxy lensing a submillimeter galaxy

    SciTech Connect (OSTI)

    Haas, Martin; Westhues, Christian; Chini, Rolf; Leipski, Christian; Klaas, Ulrich; Meisenheimer, Klaus; Barthel, Peter; Koopmans, Lon V. E.; Wilkes, Belinda J.; Bussmann, R. Shane; Willner, S. P.; Ashby, Matthew L. N.; Kuraszkiewicz, Joanna; Vegetti, Simona; Clements, David L.; Fassnacht, Christopher D.; Horesh, Assaf; Lagattuta, David J.; Stern, Daniel; Wylezalek, Dominika

    2014-07-20

    Herschel Space Observatory photometry and extensive multiwavelength follow-up have revealed that the powerful radio galaxy (PRG) 3C 220.3 at z = 0.685 acts as a gravitational lens for a background submillimeter galaxy (SMG) at z = 2.221. At an observed wavelength of 1 mm, the SMG is lensed into three distinct images. In the observed near infrared, these images are connected by an arc of ?1''.8 radius forming an Einstein half-ring centered near the radio galaxy. In visible light, only the arc is apparent. 3C 220.3 is the only known instance of strong galaxy-scale lensing by a PRG not located in a galaxy cluster and therefore it offers the potential to probe the dark matter content of the radio galaxy host. Lens modeling rejects a single lens, but two lenses centered on the radio galaxy host A and a companion B, separated by 1''.5, provide a fit consistent with all data and reveal faint candidates for the predicted fourth and fifth images. The model does not require an extended common dark matter halo, consistent with the absence of extended bright X-ray emission on our Chandra image. The projected dark matter fractions within the Einstein radii of A (1''.02) and B (0''.61) are about 0.4 0.3 and 0.55 0.3. The mass to i-band light ratios of A and B, M/L{sub i}?84 M{sub ?} L{sub ?}{sup ?1}, appear comparable to those of radio-quiet lensing galaxies at the same redshift in the CfA-Arizona Space Telescope LEns Survey, Lenses Structure and Dynamics, and Strong Lenses in the Legacy Survey samples. The lensed SMG is extremely bright with observed f(250 ?m) = 440 mJy owing to a magnification factor ? ? 10. The SMG spectrum shows luminous, narrow C IV ?1549 emission, revealing that the SMG houses a hidden quasar in addition to a violent starburst. Multicolor image reconstruction of the SMG indicates a bipolar morphology of the emitted ultraviolet (UV) light suggestive of cones through which UV light escapes a dust-enshrouded nucleus.

  12. Summary of the Fall 2004 ASA Meeting

    U.S. Energy Information Administration (EIA) Indexed Site

    8 and 29, 2004 with the Energy Information Administration 1000 Independence Ave., SW. Washington, D.C. 20585 Thursday, October 28, 2004 1. EIA Program to Evaluate Form EIA-920, Combined Heat and Power Plant Report, Robert Rutchik, SMG, EIA In early 2004, EIA disseminated the new survey, Form EIA-920, Combined Heat and Power Plant (CHP) Report to CHP facilities to collect data on their total fuel used, fuel used to generate electricity, generation, and fossil fuel stocks. The survey's primary

  13. Summary of the Spring 2007 ASA Meetings

    U.S. Energy Information Administration (EIA) Indexed Site

    April 19 and 20, 2007 Washington, D.C. 1. Modeling Regional Electricity Generation, Phillip Tseng, SMG, EIA In recent years, natural gas use in the electric power sector has been on the rise. As a result, impacts of power generation from natural gas plants on the very tight U.S. natural gas market are becoming more pronounced. The ability to predict gas plant dispatching decisions can help analysts understand natural gas market conditions and the direction of price changes. Theoretically,

  14. DETECTION OF AN ULTRA-BRIGHT SUBMILLIMETER GALAXY BEHIND THE SMALL MAGELLANIC CLOUD

    SciTech Connect (OSTI)

    Takekoshi, Tatsuya; Minamidani, Tetsuhiro; Sorai, Kazuo; Habe, Asao; Tamura, Yoichi; Kohno, Kotaro; Oogi, Taira; Ezawa, Hajime; Komugi, Shinya; Mizuno, Norikazu; Muller, Erik; Kawamura, Akiko; Oshima, Tai; Scott, Kimberly S.; Austermann, Jason E.; Tosaki, Tomoka; Onishi, Toshikazu; Fukui, Yasuo; Matsuo, Hiroshi; Aretxaga, Itziar; and others

    2013-09-10

    We report the discovery of a new ultra-bright submillimeter galaxy (SMG) behind the Small Magellanic Cloud (SMC). This SMG is detected as a 43.3 {+-} 8.4 mJy point source (MM J01071-7302, hereafter MMJ0107) in the 1.1 mm continuum survey of the SMC by AzTEC on the ASTE telescope. MMJ0107 is also detected in the radio (843 MHz), Herschel/SPIRE, Spitzer MIPS 24 {mu}m, all IRAC bands, Wide-field Infrared Survey Explorer, and near-infrared (J, H, K{sub S} ). We find an optical (U, B, V) source, which might be the lensing object, at a distance of 1.''4 from near-infrared and IRAC sources. Photometric redshift estimates for the SMG using representative spectral energy distribution templates show the redshifts of 1.4-3.9. We estimate total far-infrared luminosity of (0.3-2.2) Multiplication-Sign 10{sup 14} {mu}{sup -1} L{sub Sun} and a star formation rate of 5600-39, 000 {mu}{sup -1} M{sub Sun} yr{sup -1}, where {mu} is the gravitational magnification factor. This apparent extreme star formation activity is likely explained by a highly magnified gravitational lens system.

  15. Properties of submillimeter galaxies in the CANDELS-S goods-south field

    SciTech Connect (OSTI)

    Wiklind, Tommy; Dahlen, Tomas; Ferguson, Henry C.; Grogin, Norman A.; Koekemoer, Anton M.; Dickinson, Mark E.; Guo, Yicheng; Barro, Guillermo; Fontana, Adriano; Castellano, Marco; Davé, Romeel; Yan, Haojing; Acquaviva, Viviana; Ashby, Matthew L. N.; Caputi, Karina I.; Dekel, Avishai; Donley, Jennifer L.; and others

    2014-04-20

    We derive physical properties of 10 submillimeter galaxies located in the CANDELS coverage of the GOODS-S field. The galaxies were first identified as submillimeter sources with the LABOCA bolometer and subsequently targeted for 870 μm continuum observation with ALMA. The high angular resolution of the ALMA imaging allows secure counterparts to be identified in the CANDELS multiband data set. The CANDELS data provide deep photometric data from UV through near-infrared wavelengths. Using synthetic spectral energy distributions, we derive photometric redshifts, stellar masses, extinction, ages, and the star formation history. The redshift range is z = 1.65-4.76, with two of the galaxies located at z > 4. Two submillimeter galaxy (SMG) counterparts have stellar masses 2-3 orders of magnitude lower than the rest. The remaining SMG counterparts have stellar masses around 1 × 10{sup 11} M {sub ☉}. The stellar population in the SMGs is typically older than the expected duration of the submillimeter phase, suggesting that the star formation history of SMGs is more complex than a single burst. Non-parametric morphology indices suggest that the SMG counterparts are among the most asymmetric systems compared with galaxies of the same stellar mass and redshift. The Hubble Space Telescope images show that three of the SMGs are associated with ongoing mergers. The remaining counterparts are isolated. Estimating the dust and molecular gas mass from the submillimeter fluxes, and comparing with our stellar masses shows that the gas mass fraction of SMGs is ∼28% and that the final stellar mass is likely to be ∼(1-2) × 10{sup 11} M {sub ☉}.

  16. Super Bowl City Leads on Energy Efficient Forefront | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Bowl City Leads on Energy Efficient Forefront Super Bowl City Leads on Energy Efficient Forefront February 2, 2013 - 11:30am Addthis New Orleans' Mercedes-Benz Superdome features more than 26,000 LED lights on the building's exterior. The system uses only 10 kilowatts of electricity, equivalent to powering a small home. | Photo courtesy of SMG. New Orleans' Mercedes-Benz Superdome features more than 26,000 LED lights on the building's exterior. The system uses only 10 kilowatts of electricity,

  17. DOE-HDBK-1122-99; Radiological Control Technician Training

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    9 Radiological Control Technician Training Fundamental Academic Training Study Guide Phase I Coordinated and Conducted for Office of Environment, Safety & Health U.S. Department of Energy DOE-HDBK-1122-99 Radiological Control Technician Study Guide ii This page intentionally left blank. DOE-HDBK-1122-99 Radiological Control Technician Study Guide iii Course Developers William Egbert Lawrence Livermore National Laboratory Dave Lent Coleman Research Michael McNaughton Los Alamos National

  18. Y-12 employees, families and friends help East Tennessee during annual

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Volunteer Day | Y-12 National Security Complex employees, families ... Y-12 employees, families and friends help East Tennessee during annual Volunteer Day Posted: May 7, 2015 - 3:34pm Chris Clark, Contractor Assurance manager, and Rick Glass, Vice President of Mission Assurance for CNS, volunteered at the Oak Ridge Children's Museum. Y-12 National Security Complex employees, their families and friends lent helping hands to some 32 projects throughout the area - painting, landscaping,

  19. Synchrotron Science at the AAAS Annual Meeting

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Synchrotron Science at the AAAS Annual Meeting Synchrotron Science at the AAAS Annual Meeting Print Light sources took center stage at several sessions at the American Association for the Advancement of Science (AAAS) 2016 Annual Meeting in Washington, DC. The meeting's theme of Global Science Engagement lent itself well to the inherently collaborative nature of synchrotron science, which was featured in the following sessions. SESAME: A Scientific Source of Light in the Middle East SESAME light

  20. Section 77

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Figure 1. Potential temperature, equivalent potential temperature, and saturation equiva- lent potential temperature for a) the decou- pled boundary-layer observed over the ARM SGP site and b) the well-mixed boundary- layer observed over central Pennsylvania. Observational Studies of Continental Stratus-Implications for Modeling B. A. Albrecht University of Miami Miami, Florida G. G. Mace University of Utah Salt Lake City, Utah H. Verlinde and T. P. Ackerman Pennsylvania State University

  1. ALMA imaging of gas and dust in a galaxy protocluster at redshift 5.3: [C II] emission in 'typical' galaxies and dusty starbursts ?1 billion years after the big bang

    SciTech Connect (OSTI)

    Riechers, Dominik A.; Carilli, Christopher L.; Capak, Peter L.; Yan, Lin; Scoville, Nicholas Z.; Smol?i?, Vernesa; Schinnerer, Eva; Yun, Min; Cox, Pierre; Bertoldi, Frank; Karim, Alexander

    2014-12-01

    We report interferometric imaging of [C II]({sup 2} P {sub 3/2}?{sup 2} P {sub 1/2}) and OH({sup 2}?{sub 1/2} J = 3/2?1/2) emission toward the center of the galaxy protocluster associated with the z = 5.3 submillimeter galaxy (SMG) AzTEC-3, using the Atacama Large (sub)Millimeter Array (ALMA). We detect strong [C II], OH, and rest-frame 157.7 ?m continuum emission toward the SMG. The [C II]({sup 2} P {sub 3/2}?{sup 2} P {sub 1/2}) emission is distributed over a scale of 3.9 kpc, implying a dynamical mass of 9.7 10{sup 10} M {sub ?}, and a star formation rate (SFR) surface density of ?{sub SFR} = 530 M {sub ?} yr{sup 1} kpc{sup 2}. This suggests that AzTEC-3 forms stars at ?{sub SFR} approaching the Eddington limit for radiation pressure supported disks. We find that the OH emission is slightly blueshifted relative to the [C II] line, which may indicate a molecular outflow associated with the peak phase of the starburst. We also detect and dynamically resolve [C II]({sup 2} P {sub 3/2}?{sup 2} P {sub 1/2}) emission over a scale of 7.5 kpc toward a triplet of Lyman-break galaxies with moderate UV-based SFRs in the protocluster at ?95 kpc projected distance from the SMG. These galaxies are not detected in the continuum, suggesting far-infrared SFRs of <18-54 M {sub ?} yr{sup 1}, consistent with a UV-based estimate of 22 M {sub ?} yr{sup 1}. The spectral energy distribution of these galaxies is inconsistent with nearby spiral and starburst galaxies, but resembles those of dwarf galaxies. This is consistent with expectations for young starbursts without significant older stellar populations. This suggests that these galaxies are significantly metal-enriched, but not heavily dust-obscured, 'normal' star-forming galaxies at z > 5, showing that ALMA can detect the interstellar medium in 'typical' galaxies in the very early universe.

  2. Climate change: Clinton affirms binding emissions reduction policy

    SciTech Connect (OSTI)

    Fairley, P.

    1996-12-04

    In Australia last month President Clinton called for an international agreement to negotiate {open_quotes}legally binding commitments to fight climate change.{close_quotes} His comments affirmed the line the Administration adopted in July and lent prominence to the effort to bring about a treaty by December 1997. Environmentalists welcomed Clinton`s comments, but industry response is divided. The Global Climate Coalition (Washington), of which CMA is a member, has tried to slow negotiations by questioning the scientific consensus on climate change and suggesting {open_quotes}serious damage to the American economy{close_quotes} could result from emissions reduction.

  3. Community Partners reEnergize Industry in Nebraska | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Partners reEnergize Industry in Nebraska Community Partners reEnergize Industry in Nebraska What if every time you lent your neighbor a cup of flour, he invited you and the rest of your block to share his freshly baked chocolate cake in return? Through your contribution, your neighbor has the ingredients to create his cake, and you share in his resulting success. That's the concept driving Nebraska's reEnergize Program. Better Buildings Neighborhood Program partner reEnergize is a collaboration

  4. SPITZER IMAGING OF HERSCHEL-ATLAS GRAVITATIONALLY LENSED SUBMILLIMETER SOURCES

    SciTech Connect (OSTI)

    Hopwood, R.; Negrello, M.; Wardlow, J.; Cooray, A.; Khostovan, A. A.; Kim, S.; Barton, E.; Da Cunha, E.; Cooke, J.; Burgarella, D.; Aretxaga, I.; Auld, R.; Baes, M.; Bertoldi, F.; Bonfield, D. G.; Blundell, R.; Buttiglione, S.; Cava, A.; Dannerbauer, H.

    2011-02-10

    We present physical properties of two submillimeter selected gravitationally lensed sources, identified in the Herschel Astrophysical Terahertz Large Area Survey. These submillimeter galaxies (SMGs) have flux densities >100 mJy at 500 {mu}m, but are not visible in existing optical imaging. We fit light profiles to each component of the lensing systems in Spitzer IRAC 3.6 and 4.5 {mu}m data and successfully disentangle the foreground lens from the background source in each case, providing important constraints on the spectral energy distributions (SEDs) of the background SMG at rest-frame optical-near-infrared wavelengths. The SED fits show that these two SMGs have high dust obscuration with A{sub V} {approx} 4-5 and star formation rates of {approx}100 M{sub sun} yr{sup -1}. They have low gas fractions and low dynamical masses compared with 850 {mu}m selected galaxies.

  5. Karl G. Jansky very large array observations of cold dust and molecular gas in starbursting quasar host galaxies at z ? 4.5

    SciTech Connect (OSTI)

    Wagg, J.; Carilli, C. L.; Lentati, L.; Maiolino, R.; Hills, R.; Aravena, M.; Cox, P.; McMahon, R. G.; Riechers, D.; Walter, F.; Andreani, P.; Wolfe, A.

    2014-03-10

    We present Karl G. Jansky Very Large Array (VLA) observations of 44 GHz continuum and CO J = 2-1 line emission in BRI 12020725 at z = 4.7 (a starburst galaxy and quasar pair) and BRI 13350417 at z = 4.4 (also hosting a quasar). With the full 8 GHz bandwidth capabilities of the upgraded VLA, we study the (rest-frame) 250 GHz thermal dust continuum emission for the first time along with the cold molecular gas traced by the low-J CO line emission. The measured CO J = 2-1 line luminosities of BRI 12020725 are L{sub CO}{sup ?}=(8.70.8)10{sup 10} K km s{sup 1} pc{sup 2} and L{sub CO}{sup ?}=(6.0 0.5)10{sup 10} K km s{sup 1} pc{sup 2} for the submillimeter galaxy (SMG) and quasar, respectively, which are equal to previous measurements of the CO J = 5-4 line luminosities implying thermalized line emission, and we estimate a combined cold molecular gas mass of ?910{sup 10} M {sub ?}. In BRI 13350417 we measure L{sub CO}{sup ?}=(7.30.6)10{sup 10} K km s{sup 1} pc{sup 2}. We detect continuum emission in the SMG BRI 12020725 North (S {sub 44} {sub GHz} = 51 6 ?Jy), while the quasar is detected with S {sub 44} {sub GHz} = 24 6 ?Jy and in BRI 13350417 we measure S {sub 44} {sub GHz} = 40 7 ?Jy. Combining our continuum observations with previous data at (rest-frame) far-infrared and centimeter wavelengths, we fit three-component models in order to estimate the star formation rates. This spectral energy distribution fitting suggests that the dominant contribution to the observed 44 GHz continuum is thermal dust emission, while either thermal free-free or synchrotron emission contributes less than 30%.

  6. A COMPREHENSIVE VIEW OF A STRONGLY LENSED PLANCK-ASSOCIATED SUBMILLIMETER GALAXY

    SciTech Connect (OSTI)

    Fu Hai; Cooray, A.; Jullo, E.; Bussmann, R. S.; Ivison, R. J.; Perez-Fournon, I.; Djorgovski, S. G.; Scoville, N.; Yan, L.; Riechers, D. A.; Bradford, M.; Aguirre, J.; Auld, R.; Baes, M.; Baker, A. J.; Cava, A.; Clements, D. L.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; and others

    2012-07-10

    We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 {mu}m flux density ({approx}300 mJy). It is the only high-redshift Planck detection in the 130 deg{sup 2} H-ATLAS Phase-I area. Keck Adaptive Optics images reveal a quadruply imaged galaxy in the K band while the Submillimeter Array and the Jansky Very Large Array show doubly imaged 880 {mu}m and CO(1{yields}0) sources, indicating differentiated distributions of the various components in the galaxy. In the source plane, the stars reside in three major kpc-scale clumps extended over {approx}1.6 kpc, the dust in a compact ({approx}1 kpc) region {approx}3 kpc north of the stars, and the cold molecular gas in an extended ({approx}7 kpc) disk {approx}5 kpc northeast of the stars. The emissions from the stars, dust, and gas are magnified by {approx}17, {approx}8, and {approx}7 times, respectively, by four lensing galaxies at z {approx} 1. Intrinsically, the lensed galaxy is a warm (T{sub dust} {approx} 40-65 K), hyper-luminous (L{sub IR} {approx} 1.7 Multiplication-Sign 10{sup 13} L{sub Sun }; star formation rate (SFR) {approx}2000 M{sub Sun} yr{sup -1}), gas-rich (M{sub gas}/M{sub baryon} {approx} 70%), young (M{sub stellar}/SFR {approx} 20 Myr), and short-lived (M{sub gas}/SFR {approx} 40 Myr) starburst. With physical properties similar to unlensed z > 2 SMGs, HATLAS J114637.9-001132 offers a detailed view of a typical SMG through a powerful cosmic microscope.

  7. A DETAILED GRAVITATIONAL LENS MODEL BASED ON SUBMILLIMETER ARRAY AND KECK ADAPTIVE OPTICS IMAGING OF A HERSCHEL-ATLAS SUBMILLIMETER GALAXY AT z = 4.243 {sup ,} {sup ,}

    SciTech Connect (OSTI)

    Bussmann, R. S.; Gurwell, M. A.; Fu Hai; Cooray, A.; Smith, D. J. B.; Bonfield, D.; Dunne, L.; Dye, S.; Eales, S.; Auld, R.; Baes, M.; Fritz, J.; Baker, A. J.; Cava, A.; Clements, D. L.; Dariush, A.; Coppin, K.; Dannerbauer, H.; De Zotti, G.; Hopwood, R.; and others

    2012-09-10

    We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 {mu}m and the Keck adaptive optics (AO) system at the K{sub S}-band of a gravitationally lensed submillimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey. The SMA data (angular resolution Almost-Equal-To 0.''6) resolve the dust emission into multiple lensed images, while the Keck AO K{sub S}-band data (angular resolution Almost-Equal-To 0.''1) resolve the lens into a pair of galaxies separated by 0.''3. We present an optical spectrum of the foreground lens obtained with the Gemini-South telescope that provides a lens redshift of z{sub lens} = 0.595 {+-} 0.005. We develop and apply a new lens modeling technique in the visibility plane that shows that the SMG is magnified by a factor of {mu} = 4.1 {+-} 0.2 and has an intrinsic infrared (IR) luminosity of L{sub IR} = (2.1 {+-} 0.2) Multiplication-Sign 10{sup 13} L{sub Sun }. We measure a half-light radius of the background source of r{sub s} = 4.4 {+-} 0.5 kpc which implies an IR luminosity surface density of {Sigma}{sub IR} (3.4 {+-} 0.9) Multiplication-Sign 10{sup 11} L{sub Sun} kpc{sup -2}, a value that is typical of z > 2 SMGs but significantly lower than IR luminous galaxies at z {approx} 0. The two lens galaxies are compact (r{sub lens} Almost-Equal-To 0.9 kpc) early-types with Einstein radii of {theta}{sub E1} 0.57 {+-} 0.01 and {theta}{sub E2} = 0.40 {+-} 0.01 that imply masses of M{sub lens1} = (7.4 {+-} 0.5) Multiplication-Sign 10{sup 10} M{sub Sun} and M{sub lens2} = (3.7 {+-} 0.3) Multiplication-Sign 10{sup 10} M{sub Sun }. The two lensing galaxies are likely about to undergo a dissipationless merger, and the mass and size of the resultant system should be similar to other early-type galaxies at z {approx} 0.6. This work highlights the importance of high spatial resolution imaging in developing models of strongly lensed galaxies discovered by Herschel.

  8. DYNAMICAL STRUCTURE OF THE MOLECULAR INTERSTELLAR MEDIUM IN AN EXTREMELY BRIGHT, MULTIPLY LENSED z {approx_equal} 3 SUBMILLIMETER GALAXY DISCOVERED WITH HERSCHEL

    SciTech Connect (OSTI)

    Riechers, Dominik A.; Cooray, A.; Carpenter, J. M.; Bock, J.; Omont, A.; Neri, R.; Cox, P.; Harris, A. I.; Baker, A. J.; Frayer, D. T.; Auld, R.; Aussel, H.; Chanial, P.; Blundell, R.; Brisbin, D.; Burgarella, D.; Chapman, S. C.; Clements, D. L.

    2011-05-20

    We report the detection of CO(J = 5 {yields} 4), CO(J = 3 {yields} 2), and CO(J = 1 {yields} 0) emission in the strongly lensed, Herschel/SPIRE-selected submillimeter galaxy (SMG) HERMES J105751.1+573027 at z = 2.9574 {+-} 0.0001, using the Plateau de Bure Interferometer, the Combined Array for Research in Millimeter-wave Astronomy, and the Green Bank Telescope. The observations spatially resolve the molecular gas into four lensed images with a maximum separation of {approx}9'' and reveal the internal gas dynamics in this system. We derive lensing-corrected CO line luminosities of L'{sub CO(1-0)} = (4.17 {+-} 0.41), L'{sub CO(3-2)} = (3.96 {+-} 0.20), and L'{sub CO(5-4)} = (3.45 {+-} 0.20) x 10{sup 10} ({mu}{sub L}/10.9){sup -1} K km s{sup -1} pc{sup 2}, corresponding to luminosity ratios of r{sub 31} = 0.95 {+-} 0.10, r{sub 53} = 0.87 {+-} 0.06, and r{sub 51} = 0.83 {+-} 0.09. This suggests a total molecular gas mass of M{sub gas} = 3.3x10{sup 10} ({alpha}{sub CO}/0.8) ({mu}{sub L}/10.9){sup -1} M{sub sun}. The gas mass, gas mass fraction, gas depletion timescale, star formation efficiency, and specific star formation rate are typical for an SMG. The velocity structure of the gas reservoir suggests that the brightest two lensed images are dynamically resolved projections of the same dust-obscured region in the galaxy that are kinematically offset from the unresolved fainter images. The resolved kinematics appear consistent with the complex velocity structure observed in major, 'wet' (i.e., gas-rich) mergers. Major mergers are commonly observed in SMGs and are likely to be responsible for fueling their intense starbursts at high gas consumption rates. This study demonstrates the level of detail to which galaxies in the early universe can be studied by utilizing the increase in effective spatial resolution and sensitivity provided by gravitational lensing.

  9. MODELING OF THE HERMES SUBMILLIMETER SOURCE LENSED BY A DARK MATTER DOMINATED FOREGROUND GROUP OF GALAXIES

    SciTech Connect (OSTI)

    Gavazzi, R.; Cooray, A.; Conley, A.; Aguirre, J. E.; Amblard, A.; Auld, R.; Beelen, A.; Blain, A.; Bock, J.; Bradford, C. M.; Bridge, C.; Djorgovski, S. G.; Blundell, R.; Brisbin, D.; Burgarella, D.; Chanial, P.; Christopher, N.; Clements, D. L.; Cox, P.

    2011-09-10

    We present the results of a gravitational lensing analysis of the bright z{sub s} = 2.957 submillimeter galaxy (SMG) HERMES found in the Herschel/SPIRE science demonstration phase data from the Herschel Multi-tiered Extragalactic Survey (HerMES) project. The high-resolution imaging available in optical and near-IR channels, along with CO emission obtained with the Plateau de Bure Interferometer, allows us to precisely estimate the intrinsic source extension and hence estimate the total lensing magnification to be {mu} = 10.9 {+-} 0.7. We measure the half-light radius R{sub eff} of the source in the rest-frame near-UV and V bands that characterize the unobscured light coming from stars and find R{sub eff,*} = [2.0 {+-} 0.1] kpc, in good agreement with recent studies on the SMG population. This lens model is also used to estimate the size of the gas distribution (R{sub eff,gas} = [1.1 {+-} 0.5] kpc) by mapping back in the source plane the CO (J = 5 {yields} 4) transition line emission. The lens modeling yields a relatively large Einstein radius R{sub Ein} = 4.''10 {+-} 0.''02, corresponding to a deflector velocity dispersion of [483 {+-} 16] km s{sup -1}. This shows that HERMES is lensed by a galaxy group-size dark matter halo at redshift z{sub l} {approx} 0.6. The projected dark matter contribution largely dominates the mass budget within the Einstein radius with f{sub dm}(< R{sub Ein}) {approx} 80%. This fraction reduces to f{sub dm}(< R{sub eff,G1} {approx_equal} 4.5 kpc) {approx} 47% within the effective radius of the main deflecting galaxy of stellar mass M{sub *,G1} = [8.5 {+-} 1.6] x 10{sup 11} M{sub sun}. At this smaller scale the dark matter fraction is consistent with results already found for massive lensing ellipticals at z {approx} 0.2 from the Sloan Lens ACS Survey.

  10. A SYNCHRONIZED FIR/VUV LIGHT SOURCE AT JEFFERSON LAB

    SciTech Connect (OSTI)

    Stephen Benson, David Douglas, George Neil, Michelle D. Shinn, Gwyn Williams

    2012-07-01

    We describe a dual free-electron laser (FEL) configuration on the UV Demo FEL at Jefferson Lab that allows simultaneous lasing at FIR/THz and UV wavelengths. The FIR/THz source would be an FEL oscillator with a short wiggler providing nearly diffraction-limited pulses with pulse energy exceeding 50 microJoules. The FIR source would use the exhaust beam from a UVFEL. The coherent harmonics in the VUV from the UVFEL are out-coupled through a hole. The FIR source uses a shorter resonator with either hole or edge coupling to provide very high power FIR pulses. Simulations indicate excel-lent spectral brightness in the FIR region with over 100 W/cm-1 output.

  11. Status of SOFCo SOFC technology development

    SciTech Connect (OSTI)

    Privette, R.; Perna, M.A.; Kneidel, K.

    1996-12-31

    SOFCo, a Babcock & Wilcox/Ceramatec Research & Development Limited Partnership, is a collaborative research and development venture to develop technologies related to planar, solid-oxide fuel cells (SOFCs). SOFCo has successfully demonstrated a kW-class, solid-oxide fuel cell module operating on pipeline natural gas. The SOFC system design integrates the air preheater and the fuel processor with the fuel cell stacks into a compact test unit; this is the platform for multi-kW modules. The cells, made of tape-cast zirconia electrolyte and conventional electrode materials, exhibit excel lent stability in single-cell tests approaching 40,000 hours of operation. Stack tests using 10-cm and 15-cm cells with ceramic interconnects also show good performance and stability in tests for many thousands of hours.

  12. Quality of Life Assessment After Concurrent Chemoradiation for Invasive Bladder Cancer: Results of a Multicenter Prospective Study (GETUG 97-015)

    SciTech Connect (OSTI)

    Lagrange, Jean-Leon; Bascoul-Mollevi, Caroline; Geoffrois, Lionnel; Beckendorf, Veronique; Ferrero, Jean-Marc; Joly, Florence; Allouache, Nedjila; Bachaud, Jean-Marc; Chevreau, Christine; Kramar, Andrew; Chauvet, Bruno

    2011-01-01

    Purpose: To evaluate bladder preservation and functional quality after concurrent chemoradiotherapy for muscle-invasive cancer in 53 patients included in a Phase II trial. Patient and Methods: Pelvic irradiation delivered 45Gy, followed by an 18-Gy boost. Concurrent chemotherapy with cisplatin and 5-fluorouracil by continuous infusion was performed at Weeks 1, 4, and 7 during radiotherapy. Patients initially suitable for surgery were evaluated with macroscopically complete transurethral resection after 45Gy, followed by radical cystectomy in case of incomplete response. The European Organization for Research and Treatment of Cancer quality of life questionnaire QLQ-C30, specific items on bladder function, and the Late Effects in Normal Tissues-Subjective, Objective, Management, and Analytic (LENT-SOMA) symptoms scale were used to evaluate quality of life before treatment and 6, 12, 24, and 36 months after treatment. Results: Median age was 68 years for 51 evaluable patients. Thirty-two percent of patients had T2a tumors, 46% T2b, 16% T3, and 6% T4. A visibly complete transurethral resection was possible in 66%. Median follow-up was 8 years. Bladder was preserved in 67% (95% confidence interval, 52-79%) of patients. Overall survival was 36% (95% confidence interval, 23-49%) at 8 years for all patients, and 45% (28-61%) for the 36 patients suitable for surgery. Satisfactory bladder function, according to LENT-SOMA, was reported for 100% of patients with preserved bladder and locally controlled disease 6-36 months after the beginning of treatment. Satisfactory bladder function was reported for 35% of patients before treatment and for 43%, 57%, and 29%, respectively, at 6, 18, and 36 months. Conclusions: Concurrent chemoradiation therapy allowed bladder preservation with tumor control for 67% patients at 8 years. Quality of life and quality of bladder function were satisfactory for 67% of patients.

  13. GREEN BANK TELESCOPE ZPECTROMETER CO(1-0) OBSERVATIONS OF THE STRONGLY LENSED SUBMILLIMETER GALAXIES FROM THE HERSCHEL ATLAS

    SciTech Connect (OSTI)

    Frayer, D. T.; Maddalena, R.; Harris, A. I.; Baker, A. J.; Ivison, R. J.; Smail, Ian; Negrello, M.; Aretxaga, I.; Baes, M.; Birkinshaw, M.; Bonfield, D. G.; Burgarella, D.; Buttiglione, S.; Cava, A.; Cooray, A.; Dannerbauer, H.

    2011-01-10

    The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) has uncovered a population of strongly lensed submillimeter galaxies (SMGs). The Zpectrometer instrument on the Green Bank Telescope (GBT) was used to measure the redshifts and constrain the masses of the cold molecular gas reservoirs for two candidate high-redshift lensed sources. We derive CO(1-0) redshifts of z = 3.042 {+-} 0.001 and z = 2.625 {+-} 0.001, and measure molecular gas masses of (1-3) x10{sup 10} M{sub sun}, corrected for lens amplification and assuming a conversion factor of {alpha} = 0.8 M{sub sun}( K km s{sup -1} pc{sup 2}){sup -1}. We find typical L(IR)/L'(CO) ratios of 120 {+-} 40 and 140 {+-} 50 L{sub sun}( K km s{sup -1} pc{sup 2}){sup -1}, which are consistent with those found for local ultraluminous infrared galaxies (ULIRGs) and other high-redshift SMGs. From analysis of published data, we find no evidence for enhanced L(IR)/L'(CO(1-0)) ratios for the SMG population in comparison to local ULIRGs. The GBT results highlight the power of using the CO lines to derive blind redshifts, which is challenging for the SMGs at optical wavelengths given their high obscuration.

  14. 70 Gy Versus 80 Gy in Localized Prostate Cancer: 5-Year Results of GETUG 06 Randomized Trial;Prostate cancer; Dose escalation; Conformal radiotherapy; Randomized trial

    SciTech Connect (OSTI)

    Beckendorf, Veronique; Guerif, Stephane; Le Prise, Elisabeth; Cosset, Jean-Marc; Bougnoux, Agnes; Chauvet, Bruno; Salem, Naji; Chapet, Olivier; Bourdain, Sylvain; Bachaud, Jean-Marc; Maingon, Philippe; Hannoun-Levi, Jean-Michel; Malissard, Luc; Simon, Jean-Marc; Pommier, Pascal; Hay, Men; Dubray, Bernard; Lagrange, Jean-Leon; Luporsi, Elisabeth; Bey, Pierre

    2011-07-15

    Purpose: To perform a randomized trial comparing 70 and 80 Gy radiotherapy for prostate cancer. Patients and Methods: A total of 306 patients with localized prostate cancer were randomized. No androgen deprivation was allowed. The primary endpoint was biochemical relapse according to the modified 1997-American Society for Therapeutic Radiology and Oncology and Phoenix definitions. Toxicity was graded using the Radiation Therapy Oncology Group 1991 criteria and the late effects on normal tissues-subjective, objective, management, analytic scales (LENT-SOMA) scales. The patients' quality of life was scored using the European Organization for Research and Treatment of Cancer Quality of Life Questionnaire 30-item cancer-specific and 25-item prostate-specific modules. Results: The median follow-up was 61 months. According to the 1997-American Society for Therapeutic Radiology and Oncology definition, the 5-year biochemical relapse rate was 39% and 28% in the 70- and 80-Gy arms, respectively (p = .036). Using the Phoenix definition, the 5-year biochemical relapse rate was 32% and 23.5%, respectively (p = .09). The subgroup analysis showed a better biochemical outcome for the higher dose group with an initial prostate-specific antigen level >15 ng/mL. At the last follow-up date, 26 patients had died, 10 of their disease and none of toxicity, with no differences between the two arms. According to the Radiation Therapy Oncology Group scale, the Grade 2 or greater rectal toxicity rate was 14% and 19.5% for the 70- and 80-Gy arms (p = .22), respectively. The Grade 2 or greater urinary toxicity was 10% at 70 Gy and 17.5% at 80 Gy (p = .046). Similar results were observed using the LENT-SOMA scale. Bladder toxicity was more frequent at 80 Gy than at 70 Gy (p = .039). The quality-of-life questionnaire results before and 5 years after treatment were available for 103 patients with no differences found between the 70- and 80-Gy arms. Conclusion: High-dose radiotherapy provided a

  15. Submillimeter galaxies as progenitors of compact quiescent galaxies

    SciTech Connect (OSTI)

    Toft, S.; Zirm, A.; Krogager, J.-K.; Man, A. W. S.; Smol?i?, V.; Krpan, J.; Magnelli, B.; Karim, A.; Michalowski, M.; Capak, P.; Sheth, K.; Schawinski, K.; Wuyts, S.; Lutz, D.; Staguhn, J.; Berta, S.; Sanders, D.; Mccracken, H.; Riechers, D.

    2014-02-20

    Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were already old, quiescent systems with little to no residual star formation and extremely compact with stellar mass densities at least an order of magnitude larger than in low-redshift ellipticals, their descendants. Little is known about how they formed, but their evolved, dense stellar populations suggest formation within intense, compact starbursts 1-2 Gyr earlier (at 3 < z < 6). Simulations show that gas-rich major mergers can give rise to such starbursts, which produce dense remnants. Submillimeter-selected galaxies (SMGs) are prime examples of intense, gas-rich starbursts. With a new, representative spectroscopic sample of compact, quiescent galaxies at z = 2 and a statistically well-understood sample of SMGs, we show that z = 3-6 SMGs are consistent with being the progenitors of z = 2 quiescent galaxies, matching their formation redshifts and their distributions of sizes, stellar masses, and internal velocities. Assuming an evolutionary connection, their space densities also match if the mean duty cycle of SMG starbursts is 42{sub ?29}{sup +40} Myr (consistent with independent estimates), which indicates that the bulk of stars in these massive galaxies were formed in a major, early surge of star formation. These results suggest a coherent picture of the formation history of the most massive galaxies in the universe, from their initial burst of violent star formation through their appearance as high stellar-density galaxy cores and to their ultimate fate as giant ellipticals.

  16. SEARCHING FOR THE HIGHEST REDSHIFT SOURCES IN 250-500 {mu}m SUBMILLIMETER SURVEYS

    SciTech Connect (OSTI)

    Pope, Alexandra; Chary, Ranga-Ram

    2010-06-01

    We explore a technique for identifying the highest redshift (z>4) sources in Herschel/SPIRE and BLAST submillimeter surveys by localizing the position of the far-infrared dust peak. Just as Spitzer/IRAC was used to identify stellar 'bump' sources, the far-IR peak is also a redshift indicator; although the latter also depends on the average dust temperature. We demonstrate the wide range of allowable redshifts for a reasonable range of dust temperatures and show that it is impossible to constraint the redshift of individual objects using solely the position of the far-IR peak. By fitting spectral energy distribution models to simulated Herschel/SPIRE photometry we show the utility of radio and/or far-infrared data in breaking this degeneracy. With prior knowledge of the dust temperature distribution it is possible to obtain statistical samples of high redshift submillimeter galaxy (SMG) candidates. We apply this technique to the BLAST survey of ECDFS to constrain the number of dusty galaxies at z>4. We find 8 {+-} 2 galaxies with flux density ratios of S {sub 500}>S {sub 350}; this sets an upper limit of 17 {+-} 4 deg{sup -2} if we assume all are at z>4. This is <35 % of all 500 {mu}m-selected galaxies down to S {sub 500}>45 mJy (L {sub IR}>2 x 10{sup 13} L {sub sun} for z>4). Modeling with conventional temperature and redshift distributions estimates the percentage of these 500 {mu}m peak galaxies at z>4 to be between 10% and 85%. Our results are consistent with other estimates of the number density of very high redshift SMGs and follow the decline in the star formation rate density at z>4.

  17. Concordant plutonium-241-americium-241 dating of environmental samples: results from forest fire ash

    SciTech Connect (OSTI)

    Goldstein, Steven J; Oldham, Warren J; Murrell, Michael T; Katzman, Danny

    2010-12-07

    We have measured the Pu, {sup 237}Np, {sup 241}Am, and {sup 151}Sm isotopic systematics for a set of forest fire ash samples from various locations in the western U.S. including Montana, Wyoming, Idaho, and New Mexico. The goal of this study is to develop a concordant {sup 241}Pu (t{sub 1/2} = 14.4 y)-{sup 241}Am dating method for environmental collections. Environmental samples often contain mixtures of components including global fallout. There are a number of approaches for subtracting the global fallout component for such samples. One approach is to use {sup 242}/{sup 239}Pu as a normalizing isotope ratio in a three-isotope plot, where this ratio for the nonglobal fallout component can be estimated or assumed to be small. This study investigates a new, complementary method of normalization using the long-lived fission product, {sup 151}Sm (t{sub 1/2} = 90 y). We find that forest fire ash concentrates actinides and fission products with {approx}1E10 atoms {sup 239}Pu/g and {approx}1E8 atoms {sup 151}Sm/g, allowing us to measure these nuclides by mass spectrometric (MIC-TIMS) and radiometric (liquid scintillation counting) methods. The forest fire ash samples are characterized by a western U.S. regional isotopic signature representing varying mixtures of global fallout with a local component from atmospheric testing of nuclear weapons at the Nevada Test Site (NTS). Our results also show that {sup 151}Sm is well correlated with the Pu nuclides in the forest fire ash, suggesting that these nuclides have similar geochemical behavior in the environment. Results of this correlation indicate that the {sup 151}Sm/{sup 239}Pu atom ratio for global fallout is {approx}0.164, in agreement with an independent estimate of 0.165 based on {sup 137}Cs fission yields for atmospheric weapons tests at the NTS. {sup 241}Pu-{sup 241}Am dating of the non-global fallout component in the forest fire ash samples yield ages in the late 1950's-early 1960's, consistent with a peak in NTS

  18. THE LARGE APEX BOLOMETER CAMERA SURVEY OF THE EXTENDED CHANDRA DEEP FIELD SOUTH

    SciTech Connect (OSTI)

    Weiss, A.; Kovacs, A.; Menten, K. M.; Coppin, K.; Smail, Ian; Greve, T. R.; Walter, F.; Dannerbauer, H.; Dunlop, J. S.; Ivison, R. J.; Knudsen, K. K.; Bertoldi, F.; Alexander, D. M.; Brandt, W. N.; Chapman, S. C.; Cox, P.; De Breuck, C.; Gawiser, E.; Lutz, D.; Koekemoer, A. M.

    2009-12-20

    We present a sensitive 870 mum survey of the Extended Chandra Deep Field South (ECDFS) combining 310 hr of observing time with the Large Apex BOlometer Camera (LABOCA) on the APEX telescope. The LABOCA ECDFS Submillimetre Survey (LESS) covers the full 30' x 30' field size of the ECDFS and has a uniform noise level of sigma{sub 870{sub m}}u{sub m} approx 1.2 mJy beam{sup -1}. LESS is thus the largest contiguous deep submillimeter survey undertaken to date. The noise properties of our map show clear evidence that we are beginning to be affected by confusion noise. We present a catalog of 126 submillimeter galaxies (SMGs) detected with a significance level above 3.7sigma, at which level we expect five false detections given our map area of 1260 arcmin{sup 2}. The ECDFS exhibits a deficit of bright SMGs relative to previously studied blank fields but not of normal star-forming galaxies that dominate the extragalactic background light (EBL). This is in line with the underdensities observed for optically defined high redshift source populations in the ECDFS (BzKs, DRGs, optically bright active galactic nucleus, and massive K-band-selected galaxies). The differential source counts in the full field are well described by a power law with a slope of alpha = -3.2, comparable to the results from other fields. We show that the shape of the source counts is not uniform across the field. Instead, it steepens in regions with low SMG density. Towards the highest overdensities we measure a source-count shape consistent with previous surveys. The integrated 870 mum flux densities of our source-count models down to S{sub 870{sub m}}u{sub m} = 0.5 mJy account for >65% of the estimated EBL from COBE measurements. We have investigated the clustering of SMGs in the ECDFS by means of a two-point correlation function and find evidence for strong clustering on angular scales <1' with a significance of 3.4sigma. Assuming a power-law dependence for the correlation function and a typical

  19. A MID-INFRARED IMAGING SURVEY OF SUBMILLIMETER-SELECTED GALAXIES WITH THE SPITZER SPACE TELESCOPE

    SciTech Connect (OSTI)

    Hainline, Laura J.; Blain, A. W.; Smail, Ian; Frayer, D. T.; Chapman, S. C.; Ivison, R. J.; Alexander, D. M. E-mail: ljh@astro.umd.edu

    2009-07-10

    We present Spitzer-IRAC and MIPS mid-IR observations of a sample of 73 radio-detected submillimeter-selected galaxies (SMGs) with spectroscopic redshifts, the largest such sample published to date. From our data, we find that IRAC colors of SMGs are much more uniform as compared with rest-frame UV and optical colors, and z>1.5 SMGs tend to be redder in their mid-IR colors than both field galaxies and lower-z SMGs. However, the IRAC colors of the SMGs overlap those of field galaxies sufficiently that color-magnitude and color-color selection criteria suggested in the literature to identify SMG counterparts produce ambiguous counterparts within an 8'' radius in 20%-35% of cases. We use a rest-frame J-H versus H-K color-color diagram and a S {sub 24}/S {sub 8.0} versus S {sub 8.0}/S {sub 4.5} color-color diagram to determine that 13%-19% of our sample are likely to contain active galactic nuclei which dominate their mid-IR emission. We observe in the rest-frame JHK colors of our sample that the rest-frame near-IR emission of SMGs does not resemble that of the compact nuclear starburst observed in local ultraluminous IR galaxies and is consistent with more widely distributed star formation. We take advantage of the fact that many high-z galaxy populations selected at different wavelengths are detected by Spitzer to carry out a brief comparison of mid-IR properties of SMGs to UV-selected high-z galaxies, 24 {mu}m-selected galaxies, and high-z radio galaxies, and find that SMGs have mid-IR fluxes and colors which are consistent with being more massive and more reddened than UV-selected galaxies, while the IRAC colors of SMGs are most similar to powerful high-z radio galaxies.

  20. Late Patient-Reported Toxicity After Preoperative Radiotherapy or Chemoradiotherapy in Nonresectable Rectal Cancer: Results From a Randomized Phase III Study

    SciTech Connect (OSTI)

    Braendengen, Morten, E-mail: mortbrae@medisin.uio.no [Oslo University Hospital, Ulleval, Cancer Centre, Oslo (Norway); Department of Oncology and Pathology, Karolinska Institutet, Stockholm (Sweden); Tveit, Kjell Magne [Oslo University Hospital, Ulleval, Cancer Centre, Oslo (Norway); Faculty of Medicine, University of Oslo, Oslo (Norway); Bruheim, Kjersti [Oslo University Hospital, Ulleval, Cancer Centre, Oslo (Norway); Cvancarova, Milada [Department of Clinical Cancer Research, Oslo University Hospital, Radiumhospitalet, Oslo (Norway); Berglund, Ake [Department of Oncology, Radiology and Clinical Immunology, University of Uppsala, Uppsala (Sweden); Glimelius, Bengt [Department of Oncology and Pathology, Karolinska Institutet, Stockholm (Sweden); Department of Oncology, Radiology and Clinical Immunology, University of Uppsala, Uppsala (Sweden)

    2011-11-15

    Purpose: Preoperative chemoradiotherapy (CRT) is superior to radiotherapy (RT) in locally advanced rectal cancer, but the survival gain is limited. Late toxicity is, therefore, important. The aim was to compare late bowel, urinary, and sexual functions after CRT or RT. Methods and Materials: Patients (N = 207) with nonresectable rectal cancer were randomized to preoperative CRT or RT (2 Gy Multiplication-Sign 25 {+-} 5-fluorouracil/leucovorin). Extended surgery was often required. Self-reported late toxicity was scored according to the LENT SOMA criteria in a structured telephone interview and with questionnaires European Organisation for Research and Treatment of Cancer (EORTC) Quality of Life Questionnaire (QLQ-C30), International Index of Erectile Function (IIEF), and sexual function -vaginal changes questionnaire (SVQ). Results: Of the 105 patients alive in Norway and Sweden after 4 to 12 years of follow-up, 78 (74%) responded. More patients in the CRT group had received a stoma (73% vs. 52%, p = 0.09). Most patients without a stoma (7 of 12 in CRT group and 9 of 16 in RT group) had incontinence for liquid stools or gas. No stoma and good anal function were seen in 5 patients (11%) in the CRT group and in 11 (30%) in the RT group (p = 0.046). Of 44 patients in the CRT group, 12 (28%) had had bowel obstruction compared with 5 of 33 (15%) in the RT group (p = 0.27). One-quarter of the patients reported urinary incontinence. The majority of men had severe erectile dysfunction. Few women reported sexual activity during the previous month. However, the majority did not have concerns about their sex life. Conclusions: Fecal incontinence and erectile dysfunction are frequent after combined treatment for locally advanced rectal cancer. There was a clear tendency for the problems to be more common after CRT than after RT.

  1. Development of Advanced Continuum Models that Incorporate Nanomechanical Deformation into Engineering Analysis.

    SciTech Connect (OSTI)

    Zimmerman, Jonathan A.; Jones, Reese E.; Templeton, Jeremy Alan; McDowell, David L.; Mayeur, Jason R.; Tucker, Garritt J.; Bammann, Douglas J.; Gao, Huajian

    2008-09-01

    Materials with characteristic structures at nanoscale sizes exhibit significantly different mechani-cal responses from those predicted by conventional, macroscopic continuum theory. For example,nanocrystalline metals display an inverse Hall-Petch effect whereby the strength of the materialdecreases with decreasing grain size. The origin of this effect is believed to be a change in defor-mation mechanisms from dislocation motion across grains and pileup at grain boundaries at mi-croscopic grain sizes to rotation of grains and deformation within grain boundary interface regionsfor nanostructured materials. These rotational defects are represented by the mathematical conceptof disclinations. The ability to capture these effects within continuum theory, thereby connectingnanoscale materials phenomena and macroscale behavior, has eluded the research community.The goal of our project was to develop a consistent theory to model both the evolution ofdisclinations and their kinetics. Additionally, we sought to develop approaches to extract contin-uum mechanical information from nanoscale structure to verify any developed continuum theorythat includes dislocation and disclination behavior. These approaches yield engineering-scale ex-pressions to quantify elastic and inelastic deformation in all varieties of materials, even those thatpossess highly directional bonding within their molecular structures such as liquid crystals, cova-lent ceramics, polymers and biological materials. This level of accuracy is critical for engineeringdesign and thermo-mechanical analysis is performed in micro- and nanosystems. The researchproposed here innovates on how these nanoscale deformation mechanisms should be incorporatedinto a continuum mechanical formulation, and provides the foundation upon which to develop ameans for predicting the performance of advanced engineering materials.4 AcknowledgmentThe authors acknowledge helpful discussions with Farid F. Abraham, Youping Chen, Terry J

  2. An Integrated Solid-State LED Luminaire for General Lighting

    SciTech Connect (OSTI)

    Kevin Dowling; Fritz Morgan Ihor Lys; Mike Datta; Bernd Keller; Thomas Yuan

    2009-03-31

    A strong systems approach to designing and building practical LED-based replacement lamps is lacking. The general method of taking high-performance LEDs and marrying them to standard printed circuit boards, drivers and a heat sink has fallen short of the promise of LED lighting. In this program, a top-down assessment of requirements and a bottom-up reinvention of LED sources, electronics, optics and mechanics have resulted in the highest performance lamp possible. The team, comprised of Color Kinetics, the leaders in LED lighting and Cree, the leaders in LED devices took an approach to reinvent the package, the driver and the overall form and aesthetic of a replacement source. The challenge was to create a new benchmark in LED lighting - the resultant lamp, a PAR38 equivalent, met the light output, color, color quality and efficacy marks set out in the program as well as being dimmable, which is important for market acceptance. The approach combined the use of multiple source die, a chip-on-board approach, a very efficient driver topology, the use of both direct emission and phosphor conversion, and a unique faceted optic to avoid the losses, artifacts and hotspots of lensed approaches. The integral heat sink provided a mechanical base and airflow using a chimney-effect for use in a wide variety of locations and orientations. These research results led to a much better understanding of the system effects of component level technologies. It was clear that best-of-breed sub-system results do not necessarily result in the best end result for the complete system. In doing this work, we did not neglect the practical aspects of these systems. These were not rarified results and commercially impractical but lent themselves to eventual commercial products in the marketplace. The end result - a high performance replacement lamp - will save significant energy while providing a high-quality light source.

  3. Final Project Report for project titled "Fluoroalkylphosphonic-acid-based proton conductors"

    SciTech Connect (OSTI)

    Stephen Creager

    2011-12-08

    unexpected polymer crosslinking effect of acidic groups having two P-OH groups. The project has lent insight into how FPA groups transport protons in both liquid and polymeric forms, which provides guidance to future efforts to design and prepare future generations of proton-conducting polymer electrolytes for hydrogen fuel cells and other types of electrochemical energy conversion and storage devices.

  4. Rectal wall sparing by dosimetric effect of rectal balloon used during Intensity-Modulated Radiation Therapy (IMRT) for prostate cancer

    SciTech Connect (OSTI)

    Teh, Bin S.

    2005-03-31

    The use of an air-filled rectal balloon has been shown to decrease prostate motion during prostate radiotherapy. However, the perturbation of radiation dose near the air-tissue interfaces has raised clinical concerns of underdosing the prostate gland. The aim of this study was to investigate the dosimetric effects of an air-filled rectal balloon on the rectal wall/mucosa and prostate gland. Clinical rectal toxicity and dose-volume histogram (DVH) were also assessed to evaluate for any correlation. A film phantom was constructed to simulate the 4-cm diameter air cavity created by a rectal balloon. Kodak XV2 films were utilized to measure and compare dose distribution with and without air cavity. To study the effect in a typical clinical situation, the phantom was computed tomography (CT) scanned on a Siemens DR CT scanner for intensity-modulated radiation therapy (IMRT) treatment planning. A target object was drawn on the phantom CT images to simulate the treatment of prostate cancer. Because patients were treated in prone position, the air cavity was situated superiorly to the target. The treatment used a serial tomotherapy technique with the Multivane Intensity Modulating Collimator (MIMiC) in arc treatment mode. Rectal toxicity was assessed in 116 patients treated with IMRT to a mean dose of 76 Gy over 35 fractions (2.17-Gy fraction size). They were treated in the prone position, immobilized using a Vac-LokTM bag and carrier-box system. Rectal balloon inflated with 100 cc of air was used for prostate gland immobilization during daily treatment. Rectal toxicity was assessed using modifications of the Radiation Therapy Oncology Group (RTOG) and late effects Normal Tissue Task Force (LENT) scales systems. DVH of the rectum was also evaluated. From film dosimetry, there was a dose reduction at the distal air-tissue interface as much as 60% compared with the same geometry without the air cavity for 15-MV photon beam and 2 x 2-cm field size. The dose beyond the

  5. Geothermal Exploration in Hot Springs, Montana

    SciTech Connect (OSTI)

    Toby McIntosh, Jackola Engineering

    2012-09-26

    ‚ of the hottest water within the gravel aquifer. This lent i t sel f as a logical and economical location to continue the exploration within the existing well. Faced with budget constraints due to unanticipated costs, changing dril l ing techniques stretched the limited project resources to maximize the overa l l well depth which f e l l short of original project goals. The project goal of finding 165°F or hotter water was not achieved; however the project provides additional information and understanding of the Camp Aqua area that could prove valuable in future exploration efforts