THE EFFECT OF HOST GALAXIES ON TYPE Ia SUPERNOVAE IN THE SDSS-II SUPERNOVA SURVEY
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Adam G. Riess | Robert C. Nichol | Saurabh W. Jha | Jesper Sollerman | Myungshin Im | Ramon Miquel | Ariel Goobar | Jakob Nordin | Donald P. Schneider | Masao Sako | Bruce Bassett | John Marriner | David Cinabro | Benjamin Dilday | Joshua A. Frieman | R. Nichol | J. Frieman | J. Sollerman | A. Riess | S. Jha | M. Sako | R. Miquel | R. Foley | B. Bassett | H. Lampeitl | Mathew Smith | M. Stritzinger | J. Marriner | D. Cinabro | B. Dilday | P. Garnavich | A. Goobar | J. Nordin | M. Im | Ryan J. Foley | Mathew Smith | Peter M. Garnavich | Maximilian Stritzinger | Hubert Lampeitl | Linda Ostman | L. Östman | D. Schneider | D. Schneider
[1] M. S. Burns,et al. SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 < z < 1.12 AND THE UNION2 COMPILATION , 2010, 1004.1711.
[2] R. Nichol,et al. Measurements Of The Rate Of Type Ia Supernovae At Redshift Less Than Or Similar To 0.3 From The Sloan Digital Sky Survey II Supernova Survey , 2010 .
[3] M. Sullivan,et al. The dependence of Type Ia Supernovae luminosities on their host galaxies , 2010, 1003.5119.
[4] R. Nichol,et al. A MEASUREMENT OF THE RATE OF TYPE Ia SUPERNOVAE IN GALAXY CLUSTERS FROM THE SDSS-II SUPERNOVA SURVEY , 2010, 1003.1521.
[5] R. Nichol,et al. MEASUREMENTS OF THE RATE OF TYPE Ia SUPERNOVAE AT REDSHIFT ≲0.3 FROM THE SLOAN DIGITAL SKY SURVEY II SUPERNOVA SURVEY , 2010, 1001.4995.
[6] R. Kirshner,et al. HUBBLE RESIDUALS OF NEARBY TYPE Ia SUPERNOVAE ARE CORRELATED WITH HOST GALAXY MASSES , 2009, 0912.0929.
[7] J. Vanderplas,et al. First-year Sloan Digital Sky Survey-II supernova results: consistency and constraints with other intermediate-redshift data sets , 2009, 0910.2193.
[8] J. Vanderplas,et al. FIRST-YEAR SLOAN DIGITAL SKY SURVEY-II SUPERNOVA RESULTS: HUBBLE DIAGRAM AND COSMOLOGICAL PARAMETERS , 2009, 0908.4274.
[9] J. Vanderplas,et al. FIRST-YEAR SLOAN DIGITAL SKY SURVEY-II (SDSS-II) SUPERNOVA RESULTS: CONSTRAINTS ON NONSTANDARD COSMOLOGICAL MODELS , 2009, 0908.4276.
[10] Jake Vanderplas,et al. SNANA: A Public Software Package for Supernova Analysis , 2009, 0908.4280.
[11] R. Foley,et al. IMPROVED DISTANCES TO TYPE Ia SUPERNOVAE WITH TWO SPECTROSCOPIC SUBCLASSES , 2009, 0906.1616.
[12] Kevin Krisciunas,et al. THE CARNEGIE SUPERNOVA PROJECT: ANALYSIS OF THE FIRST SAMPLE OF LOW-REDSHIFT TYPE-Ia SUPERNOVAE , 2009, 0910.3317.
[13] Chris L. Fryer,et al. RATES AND DELAY TIMES OF TYPE Ia SUPERNOVAE , 2009, 0904.3108.
[14] Armin Rest,et al. IMPROVED DARK ENERGY CONSTRAINTS FROM ∼100 NEW CfA SUPERNOVA TYPE Ia LIGHT CURVES , 2009, 0901.4804.
[15] K. Abazajian,et al. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY , 2008, 0812.0649.
[16] Mamoru Doi,et al. THE SLOAN DIGITAL SKY SURVEY-II: PHOTOMETRY AND SUPERNOVA IA LIGHT CURVES FROM THE 2005 DATA , 2008, 0908.4277.
[17] R. Bender,et al. Absorption line indices in the UV. I. Empirical and theoretical stellar population models , 2008, 0811.0619.
[18] Ariel Goobar,et al. Low RV from Circumstellar Dust around Supernovae , 2008, 0809.1094.
[19] S. Jha,et al. Supernovae in Early-Type Galaxies: Directly Connecting Age and Metallicity with Type Ia Luminosity , 2008, 0805.4360.
[20] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[21] A. Goobar,et al. The colour-lightcurve shape relation of type Ia supernovae and the reddening law , 2007, 0712.1155.
[22] N. B. Suntzeff,et al. Constraining Cosmic Evolution of Type Ia Supernovae , 2007, 0710.2338.
[23] J. Prieto,et al. THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY: SEARCH ALGORITHM AND FOLLOW-UP OBSERVATIONS , 2007, 0708.2750.
[24] J. Kaplan,et al. THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY: TECHNICAL SUMMARY , 2007, 0708.2749.
[25] M. Sullivan,et al. Is There Evidence for a Hubble Bubble? The Nature of Type Ia Supernova Colors and Dust in External Galaxies , 2007, 0705.0367.
[26] M. Sullivan,et al. SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators , 2007, astro-ph/0701828.
[27] W. M. Wood-Vasey,et al. Observational Constraints on the Nature of Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey , 2007, astro-ph/0701041.
[28] A. Riess,et al. Improved Distances to Type Ia Supernovae with Multicolor Light-Curve Shapes: MLCS2k2 , 2006, astro-ph/0612666.
[29] J. Neill,et al. Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies , 2006, astro-ph/0605455.
[30] A. Fontana,et al. The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field , , 2006, astro-ph/0603094.
[31] Walter A. Siegmund,et al. # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE 2.5 m TELESCOPE OF THE SLOAN DIGITAL SKY SURVEY , 2005 .
[32] Wendy L. Freedman,et al. The Carnegie Supernova Project: The Low‐Redshift Survey , 2005, astro-ph/0512039.
[33] Lifan Wang. Dust around Type Ia Supernovae , 2005, astro-ph/0511003.
[34] R. Nichol,et al. The Fourth Data Release of the Sloan Digital Sky Survey , 2005 .
[35] F. Mannucci,et al. The Supernova rate per unit mass , 2004, astro-ph/0411450.
[36] I. Hook,et al. A high abundance of massive galaxies 3–6 billion years after the Big Bang , 2004, Nature.
[37] J. Brinkmann,et al. The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey , 2004, astro-ph/0405537.
[38] J. Brinkmann,et al. The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies , 2004, astro-ph/0402030.
[39] Andrew R. Liddle,et al. How many cosmological parameters , 2004, astro-ph/0401198.
[40] M. S. Burns,et al. The Hubble diagram of type Ia supernovae as a function of host galaxy morphology , 2002, astro-ph/0211444.
[41] D. Borgne,et al. Photometric redshifts from evolutionary synthesis with PÉGASE: The code Z-PEG and the z=0 age constraint , 2002, astro-ph/0202359.
[42] V. Narayanan,et al. Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data , 2001, astro-ph/0107201.
[43] P. Kroupa. On the variation of the initial mass function , 2000, astro-ph/0009005.
[44] Walter A. Siegmund,et al. The Sloan Digital Sky Survey: Technical Summary , 2000, astro-ph/0006396.
[45] W. Hillebrandt,et al. Type IA Supernova Explosion Models , 2000, astro-ph/0006305.
[46] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[47] S. Bergh. THE FREQUENCY OF SN IA IN GALAXIES OF DIFFERING HUBBLE TYPE , 1990 .
[48] J. Mathis,et al. The relationship between infrared, optical, and ultraviolet extinction , 1989 .
[49] A. Oemler,et al. Type I supernovae come from short-lived stars , 1979 .
[50] J. Whelan,et al. Binaries and Supernovae of Type I , 1973 .