FIRST-YEAR SPECTROSCOPY FOR THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY
Autor: | Steven M. Kahn, Jennifer L. Marshall, Mamoru Doi, Changsu Choi, Roger W. Romani, John R. Lucey, Hubert Lampeitl, S. J. Kleinman, Dan Long, D. Cinabro, Jesper Sollerman, Naoki Yasuda, John Marriner, Bruce A. Bassett, Chris A. Collins, Gajus Miknaitis, John C. Barentine, Shannon Watters, Joshua A. Frieman, K. Schlesinger, F. DeJongh, Chen Zheng, Andrew C. Becker, Giorgos Leloudas, Craig J. Hogan, Ryan J. Foley, Darren L. DePoy, Naohiro Takanashi, Tomoki Morokuma, Stephanie A. Snedden, Viktor Malanushenko, Peter M. Garnavich, Yutaka Ihara, Richard Kessler, Linda C. Watson, Roberto J. Assef, Saurabh Jha, Kaike Pan, Kouichi Tokita, Jurek Krzesinski, Ralf Bender, Mathew Smith, Ed Elson, Stephan Frank, Ben Dilday, Linda Ostman, Ulrich Hopp, Atsuko Nitta, Alastair C. Edge, Donald P. Schneider, Christopher W. Morgan, G. Saurage, Robert C. Nichol, A. Kathy Romer, Wolfram Kollatschny, Jon A. Holtzman, Adam G. Riess, Michael Richmond, Arlin P. S. Crotts, D. McGinnis, Russet McMillan, Jack Dembicky, Howard Brewington, Donald G. York, Roger Blandford, Jason D. Eastman, J. Craig Wheeler, J. L. Prieto, Elena Malanushenko, Malcolm N. Bremer, Masao Sako, Kohki Konishi, William Ketzeback, Alexei V. Filippenko, Kurt van der Heyden, Michael E. Eyler, Michael Harvanek, Myungshin Im, Maximilian Stritzinger, Ariel Goobar |
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Rok vydání: | 2008 |
Předmět: |
Cosmology and Gravitation
Astrophysics::High Energy Astrophysical Phenomena media_common.quotation_subject Population Data analysis Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Surveys 01 natural sciences 0103 physical sciences Methods Astrophysics::Solar and Stellar Astrophysics Spectroscopy education 010303 astronomy & astrophysics Observations Astrophysics::Galaxy Astrophysics media_common Physics education.field_of_study 010308 nuclear & particles physics Astronomy and Astrophysics Light curve Techniques Redshift Galaxy Cosmology Supernova Supernovae Spectroscopic 13. Climate action Space and Planetary Science Sky Dark energy |
Zdroj: | Zheng, C, Romani, R W, Sako, M, Marriner, J P, Bassett, B A, Becker, A C, Choi, C, Cinabro, D, Dejongh, F, Depoy, D L, Dilday, B, Doi, M, Frieman, J A, Garnavich, P M, Hogan, C J, Holtzman, J A, Im, M, Jha, S W, Kessler, R, Konishi, K, Lampeitl, H, Marshall, J L, McGinnis, D, Miknaitis, G, Nichol, R C, Prieto, J L, Riess, A G, Richmond, M W, Schneider, D P, Smith, M, Takanashi, N, Tokita, K, van der Heyden, K J, Yasuda, N, Assef, R J, Barentine, J C, Bender, R, Blandford, R D, Bremer, M, Brewington, H J, Collins, C A, Crotts, A, Dembicky, J, Eastman, J, Edge, A C, Elson, E, Eyler, M E, Filippenko, A V, Foley, R J, Frank, S, Goobar, A, Harvanek, M, Hopp, U, Ihara, Y, Kahn, S, Ketzeback, W, Kleinman, S J, Kollatschny, W, Krzesinski, J, Leloudas, G, Long, D C, Lucey, J, Malanushenko, E, Malanushenko, V, McMillan, R J, Morgan, C W, Morokuma, T, Nitta, A, Ostman, L, Pan, K, Romer, A K, Saurage, G, Schlesinger, K J, Snedden, S A, Sollerman, J, Stritzinger, M D, Watson, L C, Watters, S, Wheeler, J C & York, D G 2008, ' First-year spectroscopy for the Sloan Digital Sky Survey-II supernova survey ', The Astronomical Journal, vol. 135, no. 5, pp. 1766-1784 . https://doi.org/10.1088/0004-6256/135/5/1766 Astronomical journal, 2008, Vol.135(5), pp.1766-1784 [Peer Reviewed Journal] |
ISSN: | 1538-3881 0004-6256 |
DOI: | 10.1088/0004-6256/135/5/1766 |
Popis: | This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital Sky Survey-II Supernova Survey. This program searches for and measures multi-band light curves of supernovae in the redshift range z = 0.05 - 0.4, complementing existing surveys at lower and higher redshifts. Our goal is to better characterize the supernova population, with a particular focus on SNe Ia, improving their utility as cosmological distance indicators and as probes of dark energy. Our supernova spectroscopy program features rapid-response observations using telescopes of a range of apertures, and provides confirmation of the supernova and host-galaxy types as well as precise redshifts. We describe here the target identification and prioritization, data reduction, redshift measurement, and classification of 129 SNe Ia, 16 spectroscopically probable SNe Ia, 7 SNe Ib/c, and 11 SNe II from the first season. We also describe our efforts to measure and remove the substantial host galaxy contamination existing in the majority of our SN spectra. |
Databáze: | OpenAIRE |
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