[IAUC] CBET 2567: 20101207 : SUPERNOVAE 2010kl AND 2010km
quai en eps.harvard.edu
quai en eps.harvard.edu
Mie Sep 14 16:19:23 ART 2011
Electronic Telegram No. 2567
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
CBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University;
20 Oxford St.; Cambridge, MA 02138; U.S.A.
e-mail: cbatiau en eps.harvard.edu (alternate cbat en iau.org)
URL http://www.cbat.eps.harvard.edu/index.html
Prepared using the Tamkin Foundation Computer Network
SUPERNOVAE 2010kl AND 2010km
S. Howerton, Arkansas City, KS, U.S.A.; A. J. Drake, S. G. Djorgovski, A.
Mahabal, M. J. Graham, and R. Williams, California Institute of Technology;
J. L. Prieto, Carnegie Observatories; M. Catelan, Pontificia Universidad
Catolica de Chile; E. C. Beshore and S. M. Larson, Lunar and Planetary
Laboratory, University of Arizona; and E. Christensen, Gemini Observatory,
report the CRTS discovery of two apparent supernovae in public images from
the Catalina Sky Survey (CSS) 1.5-m telescope.
SN 2010 UT R.A. (2000.0) Decl. Mag. Offset
2010kl Nov. 16.47 11 27 17.48 + 3 45 33.3 18.9 0".3 W, 10".0 N
2010km Dec. 4.33 2 55 12.81 +24 38 13.1 18.8 9".1 E, 3".3 N
SN 2010kl is not seen co-added Mt. Lemmon Survey (MLS) images reaching mag
22.5 or in Sloan Digital Sky Survey DR7 images reaching a similar depth; its
presumed host galaxy (CGCG 39-184) has redshift z = 0.035. Further magnitudes
for 2010kl: May 5.15 UT, [20.5 (MLS); Dec. 1.45, 19.2 (CSS). SN 2010km is
not seen in MLS co-added images reaching mag 22.0; its presumed host galaxy
(CGCG 484-24) has redshift z = 0.023. Further magnitudes for 2010km: Nov.
17.19 [19.5 (CSS); Nov. 28.35, 19.2 (CSS); Dec. 5.31, 18.7 (MLS).
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2010 CBAT
2010 December 7 (CBET 2567) Daniel W. E. Green
Más información sobre la lista de distribución Iauc