UBVRILight Curves of 44 Type Ia Supernovae | Zendy

Saurabh W. Jha | Zendy; R. Kirshner | Zendy; Peter Challis | Zendy; P. Garnavich | Zendy; T. Matheson | Zendy; Alicia Soderberg | Zendy; Genevieve J. Graves | Zendy; M. Hicken | Zendy; J. Alves | Zendy; Héctor G. Arce | Zendy; Z. Balog | Zendy; P. Barmby | Zendy; E. J. Barton | Zendy; P. Berlind | Zendy; Ann Bragg | Zendy; César Briceño | Zendy; Warren R. Brown | Zendy; J. H. Buckley | Zendy; Nelson Caldwell | Zendy; M. Calkins | Zendy; Barbara J. Carter | Zendy; Kristi Dendy Concan | Zendy; Rich Donnelly | Zendy; Kristoffer A. Eriksen | Zendy; Daniel G. Fabricant | Zendy; E. Falco | Zendy; F. Fiore | Zendy; M. R. Garcia | Zendy; M. Gómez | Zendy; Norman A. Grogin | Zendy; Ted Groner | Zendy; P. Groot | Zendy; Karl E. Haisch | Zendy; Lee Hartmann | Zendy; C. W. Hergenrother | Zendy; M. J. Holman | Zendy; J. P. Huchra | Zendy; Ray Jayawardhana | Zendy; D. Jerius | Zendy; Sheila J. Kannappan | Zendy; Dong-Woo Kim | Zendy; Jan Kleyna | Zendy; C. S. Kochanek | Zendy; Daniel M. Koranyi | Zendy; M. Krockenberger | Zendy; C. J. Lada | Zendy; K. L. Luhman | Zendy; Jane Luu | Zendy; Lucas M. Macri | Zendy; J. Mader | Zendy; Andisheh Mahdavi | Zendy; M. Marengo | Zendy; B. G. Marsden | Zendy; B. A. McLeod | Zendy; B. R. McNamara | Zendy; S. T. Megeath | Zendy; Dan Moraru | Zendy; Amy E. Mossman | Zendy; August Muench | Zendy; J. A. Muñoz | Zendy; James Muzerolle | Zendy; O. Naranjo | Zendy; Kristin Nelson-Patel | Zendy; M. A. Pahre | Zendy; B. M. Patten | Zendy; J. Peters | Zendy; W. N. Peters | Zendy; J. C. Raymond | Zendy; Kenneth J. Rines | Zendy; Rudolph E. Schild | Zendy; Gregory J. Sobczak | Zendy; T. B. Spahr | Zendy; J. R. Stauffer | Zendy; R. P. Stefanik | Zendy; Andrew Szentgyorgyi | Zendy; E. V. Tollestrup | Zendy; P. Väisänen | Zendy; A. Vikhlinin | Zendy; Zhong Wang | Zendy; S. P. Willner | Zendy; S. J. Wolk | Zendy; Joseph Zajac | Zendy; Ping Zhao | Zendy; Krzysztof Z. Stanek | Zendy

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UBVRILight Curves of 44 Type Ia Supernovae

Author(s) -

Saurabh W. Jha,

R. Kirshner,

Peter Challis,

P. Garnavich,

T. Matheson,

Alicia Soderberg,

Genevieve J. Graves,

M. Hicken,

J. Alves,

Héctor G. Arce,

Z. Balog,

P. Barmby,

E. J. Barton,

P. Berlind,

Ann Bragg,

César Briceño,

Warren R. Brown,

J. H. Buckley,

Nelson Caldwell,

M. Calkins,

Barbara J. Carter,

Kristi Dendy Concan,

Rich Donnelly,

Kristoffer A. Eriksen,

Daniel G. Fabricant,

E. Falco,

F. Fiore,

M. R. Garcia,

M. Gómez,

Norman A. Grogin,

Ted Groner,

P. Groot,

Karl E. Haisch,

Lee Hartmann,

C. W. Hergenrother,

M. J. Holman,

J. P. Huchra,

Ray Jayawardhana,

D. Jerius,

Sheila J. Kannappan,

Dong-Woo Kim,

Jan Kleyna,

C. S. Kochanek,

Daniel M. Koranyi,

M. Krockenberger,

C. J. Lada,

K. L. Luhman,

Jane Luu,

Lucas M. Macri,

J. Mader,

Andisheh Mahdavi,

M. Marengo,

B. G. Marsden,

B. A. McLeod,

B. R. McNamara,

S. T. Megeath,

Dan Moraru,

Amy E. Mossman,

August Muench,

J. A. Muñoz,

James Muzerolle,

O. Naranjo,

Kristin Nelson-Patel,

M. A. Pahre,

B. M. Patten,

J. Peters,

W. N. Peters,

J. C. Raymond,

Kenneth J. Rines,

Rudolph E. Schild,

Gregory J. Sobczak,

T. B. Spahr,

J. R. Stauffer,

R. P. Stefanik,

Andrew Szentgyorgyi,

E. V. Tollestrup,

P. Väisänen,

A. Vikhlinin,

Zhong Wang,

S. P. Willner,

S. J. Wolk,

Joseph Zajac,

Ping Zhao,

Krzysztof Z. Stanek

Publication year - 2006

Publication title -

the astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.61

H-Index - 271

eISSN - 1538-3881

pISSN - 0004-6256

DOI - 10.1086/497989

Subject(s) - photometry (optics) , astrophysics , physics , supernova , light curve , observatory , astronomy , redshift , galaxy , stars

We present UBVRI photometry of 44 type-Ia supernovae (SN Ia) observed from1997 to 2001 as part of a continuing monitoring campaign at the Fred LawrenceWhipple Observatory of the Harvard-Smithsonian Center for Astrophysics. Thedata set comprises 2190 observations and is the largest homogeneously observedand reduced sample of SN Ia to date, nearly doubling the number ofwell-observed, nearby SN Ia with published multicolor CCD light curves. Thelarge sample of U-band photometry is a unique addition, with importantconnections to SN Ia observed at high redshift. The decline rate of SN IaU-band light curves correlates well with the decline rate in other bands, asdoes the U-B color at maximum light. However, the U-band peak magnitudes showan increased dispersion relative to other bands even after accounting forextinction and decline rate, amounting to an additional ~40% intrinsic scattercompared to B-band.

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