TY - JOUR
T1 - Optical and infrared photometry of the unusual type Ia supernova 2000cx
AU - Candia, P.
AU - Krisciunas, K.
AU - Suntzeff, Nicholas B.
AU - González, D.
AU - Espinoza, J.
AU - Leiton, R.
AU - Rest, A.
AU - Smith, R. C.
AU - Cuadra, J.
AU - Tavenner, T.
AU - Logan, C.
AU - Snider, K.
AU - Thomas, M.
AU - West, A. A.
AU - González, G.
AU - González, S.
AU - Phillips, M. M.
AU - Hastings, N. C.
AU - McMillan, R.
PY - 2003
Y1 - 2003
N2 - We present optical and infrared photometry of the unusual Type la supernova 2000cx. With the data of Li et al. and Jha, this constitutes the largest data set ever assembled for a Type la SN, more than 600 points in UBVRIJHK. We confirm the finding of Li et al. regarding the unusually blue B-V colors as SN 2000cx entered the nebular phase. Its I-band secondary hump was extremely weak given its B-band decline rate. The V minus near-infrared colors likewise do not match loci based on other slowly declining Type la SNe, although V-K is the least "abnormal." In several ways, SN 2000cx resembles other slow decliners, given its B-band decline rate [Δm15(B) = 0.93], the appearance of Fe III lines and weakness of Si II in its premaximum spectrum, the V-K colors, and postmaximum V-H colors. If the distance modulus derived from surface brightness fluctuations of the host galaxy is correct, we find that the rate of light increase prior to maximum, the characteristics of the bolometric light curve, and the implied absolute magnitude at maximum are all consistent with a subluminous object with Δm15(B) ≈ 1.6-1.7 having a higher than normal kinetic energy.
AB - We present optical and infrared photometry of the unusual Type la supernova 2000cx. With the data of Li et al. and Jha, this constitutes the largest data set ever assembled for a Type la SN, more than 600 points in UBVRIJHK. We confirm the finding of Li et al. regarding the unusually blue B-V colors as SN 2000cx entered the nebular phase. Its I-band secondary hump was extremely weak given its B-band decline rate. The V minus near-infrared colors likewise do not match loci based on other slowly declining Type la SNe, although V-K is the least "abnormal." In several ways, SN 2000cx resembles other slow decliners, given its B-band decline rate [Δm15(B) = 0.93], the appearance of Fe III lines and weakness of Si II in its premaximum spectrum, the V-K colors, and postmaximum V-H colors. If the distance modulus derived from surface brightness fluctuations of the host galaxy is correct, we find that the rate of light increase prior to maximum, the characteristics of the bolometric light curve, and the implied absolute magnitude at maximum are all consistent with a subluminous object with Δm15(B) ≈ 1.6-1.7 having a higher than normal kinetic energy.
UR - http://www.scopus.com/inward/record.url?scp=0037220053&partnerID=8YFLogxK
U2 - 10.1086/368229
DO - 10.1086/368229
M3 - Article
AN - SCOPUS:0037220053
SN - 0004-6280
VL - 115
SP - 277
EP - 294
JO - Publications of the Astronomical Society of the Pacific
JF - Publications of the Astronomical Society of the Pacific
IS - 805
ER -