BVRI light curves for 22 Type Ia supernovae

被引：678

作者：

Riess, AG

Kirshner, RP

Schmidt, BP

Jha, S

Challis, P

Garnavich, PM

Esin, AA

Carpenter, C

Grashius, R

Schild, RE

Berlind, PL

Huchra, JP

Prosser, CF

Falco, EE

Benson, PJ

Briceño, C

Brown, WR

Caldwell, N

Dell'Antonio, IP

Filippenko, AV

Goodman, AA

Grogin, NA

Groner, T

Hughes, JP

Green, PJ

Jansen, RA

Kleyna, JT

Luu, JX

Macri, LM

McLeod, BA

McLeod, KK

McNamara, BR

McLean, B

Milone, AAE

Mohr, JJ

Moraru, D

Peng, C

Peters, J

Prestwich, AH

Stanek, KZ

Szentgyorgyi, A

Zhao, P

机构：

[1] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[3] Australian Natl Univ, Mt Stromlo & Siding Spring Observ, Weston, ACT 2611, Australia

[4] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA

[5] Natl Opt Astron Observ, Tucson, AZ 85726 USA

[6] Fred Lawrence Whipple Observ, Amado, AZ 85645 USA

[7] Wellesley Coll, Dept Astron, Whitin Observ, Wellesley, MA 02481 USA

[8] Lucent Technol, Bell Labs, Murray Hill, NJ 07974 USA

[9] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08855 USA

[10] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[11] Whipple Observ, Multiple Mirror Telescope Observ, Amado, AZ 85645 USA

[12] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA

[13] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA

[14] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

来源：

ASTRONOMICAL JOURNAL | 1999年 / 117卷 / 02期

关键词：

supernovae; general;

D O I：

10.1086/300738

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present 1210 Johnson/Cousins B, V, R, and I photometric observations of 22 recent Type Ia supernovae (SNe Ia): SNe 1993ac, 1993ae, 1994M, 1994S, 1994T, 1994Q, 1994ae, 1995D, 1995E, 1995al, 1995ac, 1995ak, 1995bd, 1996C, 1996X, 1996Z, 1996ab, 1996ai, 1996bk, 1996bl, 1996bo, and 1996bv. Most of the photometry was obtained at the Fred Lawrence Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics in a cooperative observing plan aimed at improving the database for SNe Ia. The redshifts of the sample range from cz = 1200 to 37,000 km s(-1) with a mean of ct = 7000 km s(-1).

引用

页码：707 / 724

页数：18

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