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Title: The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0

Abstract

The All-Sky Automated Survey for Supernovae (ASAS-SN) is working toward imaging the entire visible sky every night to a depth of $$V\sim 17$$ mag. The present data covers the sky and spans ~2–5 years with ~100–400 epochs of observation. The data should contain some ~1 million variable sources, and the ultimate goal is to have a database of these observations publicly accessible. We describe here a first step, a simple but unprecedented web interface https://asas-sn.osu.edu/ that provides an up to date aperture photometry light curve for any user-selected sky coordinate. The V band photometry is obtained using a two-pixel (16farcs0) radius aperture and is calibrated against the APASS catalog. Because the light curves are produced in real time, this web tool is relatively slow and can only be used for small samples of objects. However, it also imposes no selection bias on the part of the ASAS-SN team, allowing the user to obtain a light curve for any point on the celestial sphere. We present the tool, describe its capabilities, limitations, and known issues, and provide a few illustrative examples.

Authors:
ORCiD logo; ; ; ; ; ; ; ; ; ; ;
Publication Date:
Research Org.:
Krell Institute, Ames, IA (United States)
Sponsoring Org.:
USDOE; Gordon and Betty Moore Foundation (GBMF); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA)
OSTI Identifier:
1376265
Alternate Identifier(s):
OSTI ID: 1499899
Grant/Contract Number:  
FG02-97ER25308; GBMF5490; AST-1515927; AST-0908816; AST-1515876; HST-HF-51348.001; NAS 5-26555; IC120009
Resource Type:
Published Article
Journal Name:
Publications of the Astronomical Society of the Pacific
Additional Journal Information:
Journal Name: Publications of the Astronomical Society of the Pacific Journal Volume: 129 Journal Issue: 980; Journal ID: ISSN 0004-6280
Publisher:
IOP Publishing
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Kochanek, C. S., Shappee, B. J., Stanek, K. Z., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Shields, J. V., Will, D., Britt, C., Perzanowski, D., and Pojmański, G. The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0. United States: N. p., 2017. Web. doi:10.1088/1538-3873/aa80d9.
Kochanek, C. S., Shappee, B. J., Stanek, K. Z., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Shields, J. V., Will, D., Britt, C., Perzanowski, D., & Pojmański, G. The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0. United States. https://doi.org/10.1088/1538-3873/aa80d9
Kochanek, C. S., Shappee, B. J., Stanek, K. Z., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Shields, J. V., Will, D., Britt, C., Perzanowski, D., and Pojmański, G. Wed . "The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0". United States. https://doi.org/10.1088/1538-3873/aa80d9.
@article{osti_1376265,
title = {The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0},
author = {Kochanek, C. S. and Shappee, B. J. and Stanek, K. Z. and Holoien, T. W. -S. and Thompson, Todd A. and Prieto, J. L. and Dong, Subo and Shields, J. V. and Will, D. and Britt, C. and Perzanowski, D. and Pojmański, G.},
abstractNote = {The All-Sky Automated Survey for Supernovae (ASAS-SN) is working toward imaging the entire visible sky every night to a depth of $V\sim 17$ mag. The present data covers the sky and spans ~2–5 years with ~100–400 epochs of observation. The data should contain some ~1 million variable sources, and the ultimate goal is to have a database of these observations publicly accessible. We describe here a first step, a simple but unprecedented web interface https://asas-sn.osu.edu/ that provides an up to date aperture photometry light curve for any user-selected sky coordinate. The V band photometry is obtained using a two-pixel (16farcs0) radius aperture and is calibrated against the APASS catalog. Because the light curves are produced in real time, this web tool is relatively slow and can only be used for small samples of objects. However, it also imposes no selection bias on the part of the ASAS-SN team, allowing the user to obtain a light curve for any point on the celestial sphere. We present the tool, describe its capabilities, limitations, and known issues, and provide a few illustrative examples.},
doi = {10.1088/1538-3873/aa80d9},
journal = {Publications of the Astronomical Society of the Pacific},
number = 980,
volume = 129,
place = {United States},
year = {Wed Aug 23 00:00:00 EDT 2017},
month = {Wed Aug 23 00:00:00 EDT 2017}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1088/1538-3873/aa80d9

Citation Metrics:
Cited by: 591 works
Citation information provided by
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Figures / Tables:

Figure 1 Figure 1: Equatorial projection of the number of available ASAS-SN epochs. There are some artifacts because of historical details as ASAS-SN built up to two complete stations. There are, on average, 2.6 images for each epoch. (A color version of this figure is available in the online journal.)

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An UXor among FUors: Extinction-related Brightness Variations of the Young Eruptive Star V582 Aur
journal, January 2018


Wolf 1130: A Nearby Triple System Containing a Cool, Ultramassive White Dwarf
journal, February 2018

  • Mace, Gregory N.; Mann, Andrew W.; Skiff, Brian A.
  • The Astrophysical Journal, Vol. 854, Issue 2
  • DOI: 10.3847/1538-4357/aaa8dd

Occultations from an Active Accretion Disk in a 72-day Detached Post-Algol System Detected by K 2
journal, February 2018


Multiple Stellar Flybys Sculpting the Circumstellar Architecture in RW Aurigae
journal, June 2018

  • Rodriguez, Joseph E.; Loomis, Ryan; Cabrit, Sylvie
  • The Astrophysical Journal, Vol. 859, Issue 2
  • DOI: 10.3847/1538-4357/aac08f

Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
journal, July 2018

  • Riess, Adam G.; Casertano, Stefano; Yuan, Wenlong
  • The Astrophysical Journal, Vol. 861, Issue 2
  • DOI: 10.3847/1538-4357/aac82e

Spots, Flares, Accretion, and Obscuration in the Pre-main-sequence Binary DQ Tau
journal, July 2018


NICER and Fermi GBM Observations of the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124
journal, August 2018

  • Wilson-Hodge, Colleen A.; Malacaria, Christian; Jenke, Peter A.
  • The Astrophysical Journal, Vol. 863, Issue 1
  • DOI: 10.3847/1538-4357/aace60

Monitoring AGNs with H β Asymmetry. I. First Results: Velocity-resolved Reverberation Mapping
journal, December 2018


First Resolution of Microlensed Images
journal, January 2019

  • Dong, Subo; Mérand, A.; Delplancke-Ströbele, F.
  • The Astrophysical Journal, Vol. 871, Issue 1
  • DOI: 10.3847/1538-4357/aaeffb

Kinematics of the Broad-line Region of 3C 273 from a 10 yr Reverberation Mapping Campaign
journal, May 2019


Imaging Polarimetry of the Type I Superluminous Supernova 2018hti
journal, April 2019


Absolute Dimensions of the Early F-type Eclipsing Binary V506 Ophiuchi
journal, May 2019

  • Torres, Guillermo; Sandberg Lacy, Claud H.; Fekel, Francis C.
  • The Astrophysical Journal, Vol. 876, Issue 1
  • DOI: 10.3847/1538-4357/ab1487

Reverberation Mapping of the Narrow-line Seyfert 1 Galaxy I Zwicky 1: Black Hole Mass
journal, May 2019


Inferring Explosion Properties from Type II-Plateau Supernova Light Curves
journal, June 2019

  • Goldberg, Jared A.; Bildsten, Lars; Paxton, Bill
  • The Astrophysical Journal, Vol. 879, Issue 1
  • DOI: 10.3847/1538-4357/ab22b6

Fast-cadence TESS Photometry and Doppler Tomography of the Asynchronous Polar CD Ind: A Revised Accretion Geometry from Newly Proposed Spin and Orbital Periods
journal, August 2019

  • Littlefield, Colin; Garnavich, Peter; Mukai, Koji
  • The Astrophysical Journal, Vol. 881, Issue 2
  • DOI: 10.3847/1538-4357/ab2a17

PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk
journal, August 2019

  • Holoien, T. W. -S.; Huber, M. E.; Shappee, B. J.
  • The Astrophysical Journal, Vol. 880, Issue 2
  • DOI: 10.3847/1538-4357/ab2ae1

Compact Disks in a High-resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud
journal, August 2019

  • Long, Feng; Herczeg, Gregory J.; Harsono, Daniel
  • The Astrophysical Journal, Vol. 882, Issue 1
  • DOI: 10.3847/1538-4357/ab2d2d

A New Class of Changing-look LINERs
journal, September 2019

  • Frederick, Sara; Gezari, Suvi; Graham, Matthew J.
  • The Astrophysical Journal, Vol. 883, Issue 1
  • DOI: 10.3847/1538-4357/ab3a38

Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS
journal, September 2019

  • Holoien, Thomas W. -S.; Vallely, Patrick J.; Auchettl, Katie
  • The Astrophysical Journal, Vol. 883, Issue 2
  • DOI: 10.3847/1538-4357/ab3c66

Supermassive Black Hole Binary Candidates from the Pan-STARRS1 Medium Deep Survey
journal, October 2019


Monitoring the Superorbital Period Variation and Spin Period Evolution of SMC X-1
journal, November 2019

  • Hu, Chin-Ping; Mihara, Tatehiro; Sugizaki, Mutsumi
  • The Astrophysical Journal, Vol. 885, Issue 2
  • DOI: 10.3847/1538-4357/ab48e4

Spectral Evolution and Radial Dust Transport in the Prototype Young Eruptive System EX Lup
journal, December 2019


OGLE-ing the Magellanic System: Cepheids in the Bridge
journal, January 2020

  • Jacyszyn-Dobrzeniecka, Anna M.; Soszyński, Igor; Udalski, Andrzej
  • The Astrophysical Journal, Vol. 889, Issue 1
  • DOI: 10.3847/1538-4357/ab61f1

A Neutral Beam Model for High-energy Neutrino Emission from the Blazar TXS 0506+056
journal, January 2020

  • Zhang, B. Theodore; Petropoulou, Maria; Murase, Kohta
  • The Astrophysical Journal, Vol. 889, Issue 2
  • DOI: 10.3847/1538-4357/ab659a

A Possible ∼20 yr Periodicity in Long-term Optical Photometric and Spectral Variations of the Nearby Radio-quiet Active Galactic Nucleus Ark 120
journal, April 2019

  • Li, Yan-Rong; Wang, Jian-Min; Zhang, Zhi-Xiang
  • The Astrophysical Journal Supplement Series, Vol. 241, Issue 2
  • DOI: 10.3847/1538-4365/ab0ec5

On the Chemical Abundances of Miras in Clusters: V1 in the Metal-rich Globular NGC 5927
journal, March 2018


Variable Warm Dust around the Herbig Ae Star HD 169142: Birth of a Ring?
journal, December 2019

  • Chen, Lei; Moór, Attila; Kreplin, Alexander
  • The Astrophysical Journal, Vol. 887, Issue 2
  • DOI: 10.3847/2041-8213/ab59dd

ASAS-SN Identification of a Detached Eclipsing Binary System with a ∼ 7.3 Year Period
journal, July 2018

  • Jayasinghe, T.; Stanek, K. Z.; Kochanek, C. S.
  • Research Notes of the AAS, Vol. 2, Issue 3
  • DOI: 10.3847/2515-5172/aad287

Spectroscopic Classification of Nine Cataclysmic Variable Candidates with the Liverpool Telescope
journal, July 2018

  • Smith, H. L.; Upsdell, E. W.; Copperwheat, C. M.
  • Research Notes of the AAS, Vol. 2, Issue 3
  • DOI: 10.3847/2515-5172/aae154

ASAS-SN Identification of FY Sct as a Detached Eclipsing Binary System with a 2.6 Years Period
journal, July 2018

  • Jayasinghe, T.; Stanek, K. Z.; Kochanek, C. S.
  • Research Notes of the AAS, Vol. 2, Issue 3
  • DOI: 10.3847/2515-5172/aae433

Spectroscopic Observations of Nine Candidate Cataclysmic Variables with the Liverpool Telescope
journal, October 2018


Improved Observational Data for V54, A Recently Discovered RR Lyrae Star in M13
journal, February 2020

  • Layden, Andrew; Osborn, Wayne; Pritzl, Barton J.
  • Research Notes of the AAS, Vol. 4, Issue 2
  • DOI: 10.3847/2515-5172/ab7242

Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.