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2009CBET.1988....1Y - Central Bureau Electronic Telegrams, 1988, 1 (2009/October-0)
Supernovae 2009kb-2009kj.
YOUNG D., VALENTI S., REST A., NARAYAN G., HUBER M., GEZARI S., RODNEY S., TRUNDLE C., SMITH K., SMARTT S., PRICE P., STUBBS C., TONRY J., RIESS A., WOOD-VASEY W.M., BOTTICELLA M.T., PASTORELLO A., KOTAK R., FRASER M., HUNTER D., MAGUIRE K. and FOLEY R.
Abstract (from CDS):
Each object was detected on three or more nights in multiple (two to ten), dithered, 240-s g-, r-, i-, and z-band exposures on any one night, spanning 3-18 days. Deep, stacked images taken during May-June 2009 were used as templates in the subtractions, and no sign of the objects are visible on those pre-discovery images (to limiting r magnitude 24). This field lies within the SDSS DR7 footprint, and these pre-discovery images confirm no sign of the supernovae. Images from April 2009 also showed no detection of the transients to r-band magnitudes of about 24.
---------------------------------------------------------------------------— SN 2009 UT R.A. (2000.0) Decl. Mag. z Offset ---------------------------------------------------------------------------— 2009kb May 12.54 16 12 08.54 +55 07 41.3 21.2 0.44* 1".44 E, 1".35 S 2009kc June 10.85 12 23 20.35 +46 18 14.4 21.9 0.31* – 2009kd June 10.85 12 25 08.49 +46 59 44.2 22.0 0.28* – 2009ke June 10.95 16 07 24.69 +54 00 17.9 21.3 – 2009kf June 10.95 16 12 54.00 +55 38 13.8 21.8 0.182 1".10 W, 0".99 S 2009kg June 10.95 16 17 56.05 +54 58 01.3 21.9 0.34* 1".78 E, 0".84 S 2009kh June 10.96 16 13 20.25 +53 58 42.2 21.7 0.49* 1".60 W, 0".61 N 2009ki June 14.46 16 14 08.64 +55 41 41.9 21.0 0.107 0".06 E, 0".23 S 2009kj June 16.90 14 13 25.21 +52 51 31.0 21.0 0.60* 1".60 W, 1".00 S ---------------------------------------------------------------------------—
Those redshifts, z, with an asterisk tabulated above denote the SDSS photometric redshift of the presumed host galaxy. Supernovae 2009kc, 2009kd, and 2009ke are coincident with faint apparent host galaxies.
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Journal keyword(s):
Simbad objects: 9
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