Supernova rates from STRESS (Botticella+, 2008)

Details Supernova rates from STRESS (Botticella+, 2008) Supernova rates from STRESS (Botticella+, 2008)

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34790049b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/479/49. Originally published in: 2008A&A...479...49B

Physics

Supernovae, Redshifts

Scientific paper

Observations were carried out using the Wide Field Imager (WFI) at the 2.2m MPG/ESO telescope at La Silla, Chile. WFI is a mosaic camera consisting of 2x4 CCDs, each of 2048x4096 pixels, with a pixel scale of 0.238arcsec and a field of view of 34x33arcmin2. The individual chips are separated by gaps of 23.8arcsec and 14.3arcsec along right ascension and declination respectively, for a resulting filling factor of 95.9%.
We performed observations in the B,V,R,I bands using the following ESO/WFI broad-band filters: B/99, B/123, V/89, Rc/162, Ic/lwp.
The observing programme was distributed over a period of 6 years, from 1999 to 2005.
(3 data files).

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