Keck Infrared Transient Survey Data Release 1
Authors/Creators
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Tinyanont, Samaporn1
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Foley, Ryan J2
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Taggart, Kirsty2
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Davis, Kyle W2
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LeBaron, Natalie3
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Andrews, Jennifer E4
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Bustamante-Rosell, Maria Jose2
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Camacho-Neves, Yssavo5
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Chornock, Ryan6
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Coulter, David A2
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Galbany, Lluís7
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Jha, Saurabh W5
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Kilpatrick, Charles D8
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Kwok, Lindsey A5
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Larison, Conor5
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Pierel, Justin R9
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Siebert, Matthew R10
- Aldering, Greg11
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Auchettl, Katie12
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Bloom, Josh S13
- Dhawan, S14
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Filippenko, Alex V6
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French, K Decker15
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Grayling, Matthew14
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Jacobson-Galán, Wynn V6
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Jones, David O4
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Macias, Phillip2
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Mandel, Kaisey S14
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McCully, Curtis16
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Rest, Armin17
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Rojas-Bravo, César2
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Skrutskie, Michael F18
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Thorp, Stephen19
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Wang, Qinan20
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Ward, Sam M14
- 1. National Astronomical Research Institute of Thailand, 260 Moo 4, Donkaew, Maerim, Chiang Mai, 50180, Thailand
- 2. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA
- 3. Department of Astronomy, University of California, Berkeley, CA 94720, USA
- 4. Gemini Observatory, NSF's NOIRLab, 670 N. A'ohoku Place, Hilo, Hawai'i, 96720, USA
- 5. Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA
- 6. Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA
- 7. Institute of Space Sciences (ICE-CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain; Institut d'Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain.
- 8. Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208, USA
- 9. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
- 10. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218-2410, USA
- 11. Physics Division, Lawrence Berkeley National Lab, 1 Cyclotron Rd, Berekely, CA 94720
- 12. School of Physics, The University of Melbourne, Parkville, VIC 3010, Australia; Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA
- 13. Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA; Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50B-4206, Berkeley, CA 94720, USA
- 14. Institute of Astronomy and Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
- 15. Department of Astronomy, University of Illinois, 1002 W. Green St., Urbana, IL 61801, USA
- 16. Las Cumbres Observatory 6740 Cortona Dr, Suite 102, Goleta CA 93117
- 17. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218-2410, USA; Physics and Astronomy Department, Johns Hopkins University, Baltimore, MD 21218, USA
- 18. Department of Astronomy University of Virginia 530 McCormick Road, Charlottesville, VA 22904, USA
- 19. he Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova University Centre, SE 106 91 Stockholm, Sweden; Institute of Astronomy and Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
- 20. Physics and Astronomy Department, Johns Hopkins University, Baltimore, MD 21218, USA
Description
We present the first data release from the Keck Infrared Transient Survey (KITS), a NASA Key Strategic Mission Support program to obtain near-infrared (NIR) spectra of astrophysical transients of all types. This data release consists of 105 NIR spectra of 50 transients. As we are entering a new era of infrared astronomy with the James Webb Space Telescope (JWST) and the upcoming Nancy Grace Roman Space Telescope (Roman), KITS provides a large, publicly available sample of IR spectroscopy for a wide range of transients. These data will be essential to search JWST images for stellar explosions of the first stars and to plan an effective Roman SN Ia cosmology survey, both key science objectives for mission success. The first data release represents the first semester, which is one third of the full survey. We systematically observed three samples: a flux-limited sample that includes all transients brighter than 17~mag in a red optical band (usually ZTF r or ATLAS o bands); a volume-limited sample including all transients within redshift z < 0.01; and an SN Ia sample targeting objects at phases and light-curve parameters that had scant existing NIR data in the literature. Please see the accompanying paper where we describe our observing procedures and data reduction using an automated pipeline pypeit with minimal human interaction to ensure reproducibility. In this dataset, we provide telluric-corrected spectra of the transient in CSV format. We also provide one-dimensional extracted spectra of transients and telluric standard stars in FITS format from pypeit. Users can use these intermediate data products to redo telluric correction if desired.
Files
KITS_DR1_data_Zenodo.zip
Files
(127.6 MB)
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