/ftp/cats/aliases/P/PMY2007



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J/MNRAS/382/1169    Supernovae in the Subaru Deep Field      (Poznanski+, 2007)
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	table1.dat table2.dat table3.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/382/1169
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Beginning of ReadMe : J/MNRAS/382/1169 Supernovae in the Subaru Deep Field (Poznanski+, 2007) ================================================================================ Supernovae in the Subaru Deep Field: an initial sample and Type Ia rate out to redshift 1.6. Poznanski D., Maoz D., Yasuda N., Foley R.J., Doi M., Filippenko A.V., Fukugita M., Gal-Yam A., Jannuzi B.T., Morokuma T., Oda T., Schweiker H., Sharon K., Silverman J.M., Totani T. <Mon. Not. R. Astron. Soc., 382, 1169-1186 (2007)> =2007MNRAS.382.1169P ================================================================================ ADC_Keywords: Surveys ; Supernovae ; Photometry ; Redshifts Keywords: surveys - supernovae: general - cosmology: miscellaneous - cosmology: observations Abstract: Large samples of high-redshift supernovae (SNe) are potentially powerful probes of cosmic star formation, metal enrichment and SN physics. We present initial results from a new deep SN survey, based on re-imaging in the R, i', z' bands, of the 0.25deg^2^ Subaru Deep Field (SDF), with the 8.2-m Subaru telescope and Suprime-Cam. In a single new epoch consisting of two nights of observations, we have discovered 33 candidate SNe, down to a z'-band magnitude of 26.3 (AB). We have measured the photometric redshifts of the SN host galaxies, obtained Keck spectroscopic redshifts for 17 of the host galaxies and classified the SNe using the Bayesian photometric algorithm of Poznanski et al. (2007AJ....134.1285P) that relies on template matching. Description: Our SN survey is carried out in the SDF (RA=13:24:39, DE=+27:29:26; J2000). The reference images for this field, obtained with the Suprime-Cam camera on the Subaru 8.2-m telescope on Mauna Kea, Hawaii, are described by Kashikawa et al. (2004PASJ...56.1011K). The imaging for the reference SDF epoch was carried out between 2002 April and 2003 April, with some preliminary data collected in 2001, as described by Kashikawa et al. (2004PASJ...56.1011K). We re-imaged the field on 2005 March 5 and 6 (ut dates are used throughout this paper), in the three reddest Suprime-Cam broad bands: R, i' and z'. We also observed the field with the MOSAIC-I wide field imager on the Kitt Peak National Observatory (KPNO) 4-m Mayall telescope on 2005 March 2, April 5 and June 8, and on 2006 June 19.