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Title: The 2.4 μm Galaxy Luminosity Function as Measured Using WISE . II. Sample Selection

Abstract

The WISE satellite surveyed the entire sky multiple times in four infrared (IR) wavelengths (3.4, 4.6, 12, and 22 $μ$m). This all-sky IR photometric survey makes it possible to leverage many of the large publicly available spectroscopic redshift surveys to measure galaxy properties in the IR. While characterizing the cross-matching of WISE data to a single survey is a straightforward process, doing it with six different redshift surveys takes a fair amount of space to characterize adequately, because each survey has unique caveats and characteristics that need addressing. This work describes a data set that results from matching five public redshift surveys with the AllWISE data release, along with a reanalysis of the data described in Lake et al. The combined data set has an additional flux limit of 80 $μ$Jy (19.14 AB mag) in WISE's W1 filter, imposed in order to limit it to targets with high completeness and reliable photometry in the AllWISE data set. Consistent analysis of all of the data is only possible if the color bias discussed in Ilbert et al. is addressed (e.g., the techniques explored in Lake et al.). Finally, the sample defined herein is used in a companion paper in this seriesmore » to measure the luminosity function of galaxies at 2.4 μm rest-frame wavelength, and the selection process of the sample is optimized for this purpose.« less

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [4];  [5]; ORCiD logo [6]; ORCiD logo [7]
  1. Univ. of California, Los Angeles, CA (United States)
  2. Univ. Diego Portales, Santiago (Chile)
  3. Univ. of Cape Town (South Africa)
  4. NorthWest Research Associates, Redmond, WA (United States)
  5. Univ. of California, Davis, CA (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  6. California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Jet Propulsion Lab.
  7. Univ. of California, Los Angeles, CA (United States); California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Jet Propulsion Lab.
Publication Date:
Research Org.:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1545274
Grant/Contract Number:  
AC52-07NA27344
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 866; Journal Issue: 1; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; catalogs; galaxies: statistics; surveys

Citation Formats

Lake, S. E., Wright, E. L., Assef, R. J., Jarrett, T. H., Petty, S., Stanford, S. A., Stern, D., and Tsai, C. -W. The 2.4 μm Galaxy Luminosity Function as Measured Using WISE . II. Sample Selection. United States: N. p., 2018. Web. doi:10.3847/1538-4357/aae096.
Lake, S. E., Wright, E. L., Assef, R. J., Jarrett, T. H., Petty, S., Stanford, S. A., Stern, D., & Tsai, C. -W. The 2.4 μm Galaxy Luminosity Function as Measured Using WISE . II. Sample Selection. United States. doi:10.3847/1538-4357/aae096.
Lake, S. E., Wright, E. L., Assef, R. J., Jarrett, T. H., Petty, S., Stanford, S. A., Stern, D., and Tsai, C. -W. Wed . "The 2.4 μm Galaxy Luminosity Function as Measured Using WISE . II. Sample Selection". United States. doi:10.3847/1538-4357/aae096. https://www.osti.gov/servlets/purl/1545274.
@article{osti_1545274,
title = {The 2.4 μm Galaxy Luminosity Function as Measured Using WISE . II. Sample Selection},
author = {Lake, S. E. and Wright, E. L. and Assef, R. J. and Jarrett, T. H. and Petty, S. and Stanford, S. A. and Stern, D. and Tsai, C. -W.},
abstractNote = {The WISE satellite surveyed the entire sky multiple times in four infrared (IR) wavelengths (3.4, 4.6, 12, and 22 $μ$m). This all-sky IR photometric survey makes it possible to leverage many of the large publicly available spectroscopic redshift surveys to measure galaxy properties in the IR. While characterizing the cross-matching of WISE data to a single survey is a straightforward process, doing it with six different redshift surveys takes a fair amount of space to characterize adequately, because each survey has unique caveats and characteristics that need addressing. This work describes a data set that results from matching five public redshift surveys with the AllWISE data release, along with a reanalysis of the data described in Lake et al. The combined data set has an additional flux limit of 80 $μ$Jy (19.14 AB mag) in WISE's W1 filter, imposed in order to limit it to targets with high completeness and reliable photometry in the AllWISE data set. Consistent analysis of all of the data is only possible if the color bias discussed in Ilbert et al. is addressed (e.g., the techniques explored in Lake et al.). Finally, the sample defined herein is used in a companion paper in this series to measure the luminosity function of galaxies at 2.4 μm rest-frame wavelength, and the selection process of the sample is optimized for this purpose.},
doi = {10.3847/1538-4357/aae096},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 866,
place = {United States},
year = {2018},
month = {10}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Figures / Tables:

Table 1 Table 1: Summary of Spectroscopic Surveys Used

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Works referenced in this record:

The Seventh data Release of the Sloan Digital sky Survey
journal, May 2009

  • Abazajian, Kevork N.; Adelman-McCarthy, Jennifer K.; Agüeros, Marcel A.
  • The Astrophysical Journal Supplement Series, Vol. 182, Issue 2
  • DOI: 10.1088/0067-0049/182/2/543

The Tenth data Release of the Sloan Digital sky Survey: First Spectroscopic data from the Sdss-Iii Apache Point Observatory Galactic Evolution Experiment
journal, March 2014

  • Ahn, Christopher P.; Alexandroff, Rachael; Allende Prieto, Carlos
  • The Astrophysical Journal Supplement Series, Vol. 211, Issue 2
  • DOI: 10.1088/0067-0049/211/2/17

THE SPITZER DEEP, WIDE-FIELD SURVEY
journal, July 2009


LOW-RESOLUTION SPECTRAL TEMPLATES FOR ACTIVE GALACTIC NUCLEI AND GALAXIES FROM 0.03 TO 30 μm
journal, March 2010


Galaxy And Mass Assembly (GAMA): the input catalogue and star-galaxy separation
journal, February 2010


Estimating Fixed-Frame Galaxy Magnitudes in the Sloan Digital Sky Survey
journal, May 2003

  • Blanton, Michael R.; Brinkmann, J.; Csabai, Istvn
  • The Astronomical Journal, Vol. 125, Issue 5
  • DOI: 10.1086/342935

The Galaxy Luminosity Function and Luminosity Density at Redshift z = 0.1
journal, August 2003

  • Blanton, Michael R.; Hogg, David W.; Bahcall, Neta A.
  • The Astrophysical Journal, Vol. 592, Issue 2
  • DOI: 10.1086/375776

The First Release COSMOS Optical and Near‐IR Data and Catalog
journal, September 2007

  • Capak, P.; Aussel, H.; Ajiki, M.
  • The Astrophysical Journal Supplement Series, Vol. 172, Issue 1
  • DOI: 10.1086/519081

Mid-Infrared Galaxy Luminosity Functions from the agn and Galaxy Evolution Survey
journal, May 2009


Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release: GAMA
journal, March 2011


Quantifying cosmic variance: Cosmic variance
journal, September 2010


Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
journal, November 2001

  • Eisenstein, Daniel J.; Annis, James; Gunn, James E.
  • The Astronomical Journal, Vol. 122, Issue 5
  • DOI: 10.1086/323717

The DEIMOS spectrograph for the Keck II Telescope: integration and testing
conference, March 2003

  • Faber, Sandra M.; Phillips, Andrew C.; Kibrick, Robert I.
  • Astronomical Telescopes and Instrumentation, SPIE Proceedings
  • DOI: 10.1117/12.460346

NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
journal, September 2013

  • Hinshaw, G.; Larson, D.; Komatsu, E.
  • The Astrophysical Journal Supplement Series, Vol. 208, Issue 2
  • DOI: 10.1088/0067-0049/208/2/19

Bias in the estimation of global luminosity functions
journal, June 2004


The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures
journal, October 2009


The 6dF Galaxy Survey: samples, observational techniques and the first data release
journal, December 2004


THE zCOSMOS 20k GROUP CATALOG
journal, June 2012


Ages: the agn and Galaxy Evolution Survey
journal, May 2012

  • Kochanek, C. S.; Eisenstein, D. J.; Cool, R. J.
  • The Astrophysical Journal Supplement Series, Vol. 200, Issue 1
  • DOI: 10.1088/0067-0049/200/1/8

K-Corrections: an Examination of Their Contribution to the Uncertainty of Luminosity Measurements
journal, October 2016


OPTICAL SPECTROSCOPIC SURVEY OF HIGH-LATITUDE WISE -SELECTED SOURCES
journal, December 2011


The 2.4 μ m Galaxy Luminosity Function As Measured Using WISE . I. Measurement Techniques
journal, March 2017


The UKIRT Infrared Deep Sky Survey (UKIDSS)
journal, August 2007


THE zCOSMOS 10k-BRIGHT SPECTROSCOPIC SAMPLE
journal, September 2009

  • Lilly, Simon J.; Le Brun, Vincent; Maier, Christian
  • The Astrophysical Journal Supplement Series, Vol. 184, Issue 2
  • DOI: 10.1088/0067-0049/184/2/218

Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
journal, July 2015

  • Liske, J.; Baldry, I. K.; Driver, S. P.
  • Monthly Notices of the Royal Astronomical Society, Vol. 452, Issue 2
  • DOI: 10.1093/mnras/stv1436

The Galaxy Evolution Explorer : A Space Ultraviolet Survey Mission
journal, January 2005

  • Martin, D. Christopher; Fanson, James; Schiminovich, David
  • The Astrophysical Journal, Vol. 619, Issue 1
  • DOI: 10.1086/426387

SpecPro: An Interactive IDL Program for Viewing and Analyzing Astronomical Spectra
journal, May 2011

  • Masters, D.; Capak, P.
  • Publications of the Astronomical Society of the Pacific, Vol. 123, Issue 903
  • DOI: 10.1086/660023

The Deep2 Galaxy Redshift Survey: Design, Observations, data Reduction, and Redshifts
journal, August 2013

  • Newman, Jeffrey A.; Cooper, Michael C.; Davis, Marc
  • The Astrophysical Journal Supplement Series, Vol. 208, Issue 1
  • DOI: 10.1088/0067-0049/208/1/5

Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
journal, June 2002

  • Richards, Gordon T.; Fan, Xiaohui; Newberg, Heidi Jo
  • The Astronomical Journal, Vol. 123, Issue 6
  • DOI: 10.1086/340187

S‐COSMOS: The Spitzer Legacy Survey of the Hubble Space Telescope ACS 2 deg 2 COSMOS Field I: Survey Strategy and First Analysis
journal, September 2007

  • Sanders, D. B.; Salvato, M.; Aussel, H.
  • The Astrophysical Journal Supplement Series, Vol. 172, Issue 1
  • DOI: 10.1086/517885

Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
journal, June 1998

  • Schlegel, David J.; Finkbeiner, Douglas P.; Davis, Marc
  • The Astrophysical Journal, Vol. 500, Issue 2
  • DOI: 10.1086/305772

The Cosmic Evolution Survey (COSMOS): Overview
journal, September 2007

  • Scoville, N.; Aussel, H.; Brusa, M.
  • The Astrophysical Journal Supplement Series, Vol. 172, Issue 1
  • DOI: 10.1086/516585

The Two Micron All Sky Survey (2MASS)
journal, February 2006

  • Skrutskie, M. F.; Cutri, R. M.; Stiening, R.
  • The Astronomical Journal, Vol. 131, Issue 2
  • DOI: 10.1086/498708

Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
journal, September 2002

  • Strauss, Michael A.; Weinberg, David H.; Lupton, Robert H.
  • The Astronomical Journal, Vol. 124, Issue 3
  • DOI: 10.1086/342343

The Wide-Field Infrared Survey Explorer (Wise): Mission Description and Initial On-Orbit Performance
journal, November 2010


The Seventh Data Release of the Sloan Digital Sky Survey
text, January 2009

  • Abazajian, Kevork N.; Adelman-McCarthy, Jennifer K.; Agüeros, Marcel Andre
  • Columbia University
  • DOI: 10.7916/d8n879qg