The ASAS-SN bright supernova catalogue – I. 2013–2014

We present basic statistics for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during its first year-and-a-half of operations, spanning 2013 and 2014. We also present the same information for all other bright (mV ≤ 17), spectroscopically confirmed supernovae disco...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-09, Vol.464 (3)
Hauptverfasser:	Holoien, T. W. -S., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Brimacombe, J., Bersier, D., Bishop, D. W., Dong, Subo, Brown, J. S., Danilet, A. B., Simonian, G. V., Basu, U., Beacom, J. F., Falco, E., Pojmanski, G., Skowron, D. M., Woźniak, Przemyslaw R., Ávila, C. G., Conseil, E., Contreras, C., Cruz, I., Fernández, J. M., Koff, R. A., Guo, Zhen, Herczeg, G. J., Hissong, J., Hsiao, E. Y., Jose, J., Kiyota, S., Long, Feng, Monard, L. A. G., Nicholls, B., Nicolas, J., Wiethoff, W. S.
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Sprache:	eng
Schlagworte:	ASTRONOMY AND ASTROPHYSICS catalogues supernovae general surveys
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creator	Holoien, T. W. -S. Stanek, K. Z. Kochanek, C. S. Shappee, B. J. Prieto, J. L. Brimacombe, J. Bersier, D. Bishop, D. W. Dong, Subo Brown, J. S. Danilet, A. B. Simonian, G. V. Basu, U. Beacom, J. F. Falco, E. Pojmanski, G. Skowron, D. M. Woźniak, Przemyslaw R. Ávila, C. G. Conseil, E. Contreras, C. Cruz, I. Fernández, J. M. Koff, R. A. Guo, Zhen Herczeg, G. J. Hissong, J. Hsiao, E. Y. Jose, J. Kiyota, S. Long, Feng Monard, L. A. G. Nicholls, B. Nicolas, J. Wiethoff, W. S.
description	We present basic statistics for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during its first year-and-a-half of operations, spanning 2013 and 2014. We also present the same information for all other bright (mV ≤ 17), spectroscopically confirmed supernovae discovered from 2014 May 1 through the end of 2014, providing a comparison to the ASAS-SN sample starting from the point where ASAS-SN became operational in both hemispheres. In addition, we present collected redshifts and near-UV through IR magnitudes, where available, for all host galaxies of the bright supernovae in both samples. This work represents a comprehensive catalogue of bright supernovae and their hosts from multiple professional and amateur sources, allowing for population studies that were not previously possible because the all-sky emphasis of ASAS-SN redresses many previously existing biases. In particular, ASAS-SN systematically finds bright supernovae closer to the centres of host galaxies than either other professional surveys or amateurs, a remarkable result given ASAS-SN's poorer angular resolution. In conclusion, this is the first of a series of yearly papers on bright supernovae and their hosts that will be released by the ASAS-SN team.
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V. ; Basu, U. ; Beacom, J. F. ; Falco, E. ; Pojmanski, G. ; Skowron, D. M. ; Woźniak, Przemyslaw R. ; Ávila, C. G. ; Conseil, E. ; Contreras, C. ; Cruz, I. ; Fernández, J. M. ; Koff, R. A. ; Guo, Zhen ; Herczeg, G. J. ; Hissong, J. ; Hsiao, E. Y. ; Jose, J. ; Kiyota, S. ; Long, Feng ; Monard, L. A. G. ; Nicholls, B. ; Nicolas, J. ; Wiethoff, W. S.</creator><creatorcontrib>Holoien, T. W. -S. ; Stanek, K. Z. ; Kochanek, C. S. ; Shappee, B. J. ; Prieto, J. L. ; Brimacombe, J. ; Bersier, D. ; Bishop, D. W. ; Dong, Subo ; Brown, J. S. ; Danilet, A. B. ; Simonian, G. V. ; Basu, U. ; Beacom, J. F. ; Falco, E. ; Pojmanski, G. ; Skowron, D. M. ; Woźniak, Przemyslaw R. ; Ávila, C. G. ; Conseil, E. ; Contreras, C. ; Cruz, I. ; Fernández, J. M. ; Koff, R. A. ; Guo, Zhen ; Herczeg, G. J. ; Hissong, J. ; Hsiao, E. Y. ; Jose, J. ; Kiyota, S. ; Long, Feng ; Monard, L. A. G. ; Nicholls, B. ; Nicolas, J. ; Wiethoff, W. 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This work represents a comprehensive catalogue of bright supernovae and their hosts from multiple professional and amateur sources, allowing for population studies that were not previously possible because the all-sky emphasis of ASAS-SN redresses many previously existing biases. In particular, ASAS-SN systematically finds bright supernovae closer to the centres of host galaxies than either other professional surveys or amateurs, a remarkable result given ASAS-SN's poorer angular resolution. 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S.</creatorcontrib><creatorcontrib>Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)</creatorcontrib><title>The ASAS-SN bright supernova catalogue – I. 2013–2014</title><title>Monthly notices of the Royal Astronomical Society</title><description>We present basic statistics for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during its first year-and-a-half of operations, spanning 2013 and 2014. We also present the same information for all other bright (mV ≤ 17), spectroscopically confirmed supernovae discovered from 2014 May 1 through the end of 2014, providing a comparison to the ASAS-SN sample starting from the point where ASAS-SN became operational in both hemispheres. In addition, we present collected redshifts and near-UV through IR magnitudes, where available, for all host galaxies of the bright supernovae in both samples. This work represents a comprehensive catalogue of bright supernovae and their hosts from multiple professional and amateur sources, allowing for population studies that were not previously possible because the all-sky emphasis of ASAS-SN redresses many previously existing biases. In particular, ASAS-SN systematically finds bright supernovae closer to the centres of host galaxies than either other professional surveys or amateurs, a remarkable result given ASAS-SN's poorer angular resolution. 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title	The ASAS-SN bright supernova catalogue – I. 2013–2014
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