J/other/Nat/491.228    Light curves of 2 superluminous supernovae (Cooke+, 2012)

Superluminous supernovae at redshifts of 2.05 and 3.90. Cooke J., Sullivan M., Gal-Yam A., Barton E.J., Carlberg R.G., Ryan-Weber E.V., Horst C., Omori Y., Diaz G. <Nature, 491, 228-231 (2012)> =2012Natur.491..228C 2012Natur.491..228C
ADC_Keywords: Supernovae ; Photometry, SDSS Abstract: A rare class of 'superluminous' supernovae that are about ten or more times more luminous at their peaks than other types of luminous supernova has recently been found at low to intermediate redshifts. A small subset of these events have luminosities that evolve slowly and result in radiated energies of up to about 1051ergs. Therefore, they are probably examples of 'pair-instability' or 'pulsational pair-instability' supernovae with estimated progenitor masses of 100 to 250 times that of the Sun. These events are exceedingly rare at low redshift, but are expected to be more common at high redshift because the mass distribution of the earliest stars was probably skewed to high values. Here we report the detection of two superluminous supernovae, at redshifts of 2.05 and 3.90, that have slowly evolving light curves. We estimate the rate of events at redshifts of 2 and 4 to be approximately ten times higher than the rate at low redshift. The extreme luminosities of superluminous supernovae extend the redshift limit for supernova detection using present technology, previously 2.36, and provide a way of investigating the deaths of the first generation of stars to form after the Big Bang. Objects: ----------------------------------------------------------------------- RA (2000) DE Designation(s) (z) (files) ----------------------------------------------------------------------- 22 13 39.970 -17 45 24.486 (2.0458) = SN 2213-1745 (tablef1.dat) 10 00 05.872 +02 16 23.621 (3.8993) = SN 1000+0216 (tablef2.dat) ----------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablef1.dat 50 50 SN2213-1745 g'r'i' magnitudes for 2005 and 2006 tablef2.dat 50 53 SN1000+0216 g'r'i' magnitudes for 2006 and 2007 -------------------------------------------------------------------------------- See also: J/A+A/506/999 : Photometric Calibration of SNLS (Regnault+, 2009) Byte-by-byte Description of file: tablef1.dat tablef2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 d MJDg' ? MJD for g' band 7- 11 F5.2 mag g'mag ? g' magnitude 13- 16 F4.2 mag e_g'mag ? rms uncertainty on g'mag 18- 22 I5 d MJDr' ? MJD for r' band 24- 28 F5.2 mag r'mag ? r' magnitude 30- 33 F4.2 mag e_r'mag ? rms uncertainty on r'mag 35- 39 I5 d MJDi' ? MJD for i' band 41- 45 F5.2 mag i'mag ? i' magnitude 47- 50 F4.2 mag e_i'mag ? rms uncertainty on i'mag -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 27-Dec-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line