RECONSIDERING THE EFFECTS OF LOCAL STAR FORMATION ON TYPE Ia SUPERNOVA COSMOLOGY
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[1] C. Baltay,et al. Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local H$\alpha$ , 2013, 1309.1182.
[2] Mohan Ganeshalingam,et al. Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample , 2010, 1006.4612.
[3] Benjamin D. Johnson,et al. UV Star Formation Rates in the Local Universe , 2007, 0704.3611.
[4] Wendy L. Freedman,et al. THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE , 2010, 1108.3108.
[5] Constraints on the Progenitors of Type Ia Supernovae and Implications for the Cosmological Equation of State , 2001, astro-ph/0104257.
[6] Armin Rest,et al. IMPROVED DARK ENERGY CONSTRAINTS FROM ∼100 NEW CfA SUPERNOVA TYPE Ia LIGHT CURVES , 2009, 0901.4804.
[7] Douglas P. Finkbeiner,et al. MEASURING REDDENING WITH SLOAN DIGITAL SKY SURVEY STELLAR SPECTRA AND RECALIBRATING SFD , 2010, 1012.4804.
[8] Jake Vanderplas,et al. SNANA: A Public Software Package for Supernova Analysis , 2009, 0908.4280.
[9] M. Sullivan,et al. SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY , 2011, 1104.1443.
[10] D. Calzetti,et al. Measuring star formation with resolved observations: the test case of M 33 , 2015, 1502.01347.
[11] Nicholas B. Suntzeff,et al. The Hubble diagram of the Calan/Tololo type IA supernovae and the value of HO , 1996 .
[12] T. Pritchard,et al. RESULTS OF THE LICK OBSERVATORY SUPERNOVA SEARCH FOLLOW-UP PHOTOMETRY PROGRAM: BVRI LIGHT CURVES OF 165 TYPE Ia SUPERNOVAE , 2010 .
[13] A. Pastorello,et al. COSMOLOGICAL CONSTRAINTS FROM MEASUREMENTS OF TYPE Ia SUPERNOVAE DISCOVERED DURING THE FIRST 1.5 yr OF THE Pan-STARRS1 SURVEY , 2013, 1310.3828.
[14] R. Bacon,et al. Overview of the Nearby Supernova Factory , 2002, SPIE Astronomical Telescopes + Instrumentation.
[15] M. Sullivan,et al. SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators , 2007, astro-ph/0701828.
[16] Armin Rest,et al. CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA , 2009, 0901.4787.
[17] Armin Rest,et al. COLOR DISPERSION AND MILKY-WAY-LIKE REDDENING AMONG TYPE Ia SUPERNOVAE , 2013, 1306.4050.
[18] J. Mathis,et al. The relationship between infrared, optical, and ultraviolet extinction , 1989 .
[19] J. Neill,et al. THE LOCAL HOSTS OF TYPE Ia SUPERNOVAE , 2009, 0911.0690.
[20] R. Nichol,et al. THE FUNDAMENTAL METALLICITY RELATION REDUCES TYPE Ia SN HUBBLE RESIDUALS MORE THAN HOST MASS ALONE , 2012, 1212.4848.
[21] M. Sullivan,et al. Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples , 2014, 1401.4064.
[22] Streaming motions of galaxy clusters within 12 000 km s−1– V. The peculiar velocity field , 2004, astro-ph/0404386.
[23] Stefano Casertano,et al. A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3 , 2011, 1103.2976.
[24] Adam G. Riess,et al. THE EFFECT OF HOST GALAXIES ON TYPE Ia SUPERNOVAE IN THE SDSS-II SUPERNOVA SURVEY , 2010, 1005.4687.
[25] M. Sullivan,et al. The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints , , 2010, 1010.4743.
[26] Mohan Ganeshalingam,et al. Distances with <4% precision from type Ia supernovae in young star-forming environments , 2014, Science.
[27] Filippo Mannucci,et al. Observational Clues to the Progenitors of Type Ia Supernovae , 2013, 1312.0628.
[28] C. Wolf,et al. Ages of Type Ia supernovae over cosmic time , 2014, 1409.2951.
[29] M. Sullivan,et al. The dependence of Type Ia Supernovae luminosities on their host galaxies , 2010, 1003.5119.
[30] R. Ellis,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.
[31] HUBBLE RESIDUALS OF NEARBY TYPE Ia SUPERNOVAE ARE CORRELATED WITH HOST GALAXY MASSES , 2009, 0912.0929.
[32] C. Baltay,et al. CONFIRMATION OF A STAR FORMATION BIAS IN TYPE Ia SUPERNOVA DISTANCES AND ITS EFFECT ON THE MEASUREMENT OF THE HUBBLE CONSTANT , 2014, 1412.6501.
[33] P. E. Nugent,et al. K-corrections and spectral templates of Type Ia supernovae , 2007 .
[34] J. Vanderplas,et al. FIRST-YEAR SLOAN DIGITAL SKY SURVEY-II SUPERNOVA RESULTS: HUBBLE DIAGRAM AND COSMOLOGICAL PARAMETERS , 2009, 0908.4274.
[35] J. Neill,et al. The Peculiar Velocities of Local Type Ia Supernovae and Their Impact on Cosmology , 2007, 0704.1654.
[36] W. Wood-Vasey,et al. CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE , 2012, 1205.4493.
[37] Wendy L. Freedman,et al. THE CARNEGIE SUPERNOVA PROJECT: INTRINSIC COLORS OF TYPE Ia SUPERNOVAE , 2014, 1405.3934.
[38] Adam G. Riess,et al. Improved Distances to Type Ia Supernovae with Multicolor Light-Curve Shapes: MLCS2k2 , 2006 .
[39] R. Nichol,et al. SN Ia host galaxy properties from Sloan Digital Sky Survey-II spectroscopy , 2012, 1211.1386.
[40] et al,et al. UBVRI Light Curves of 44 Type Ia Supernovae , 2005 .
[41] Adam G. Riess,et al. BVRI Light Curves for 22 Type Ia Supernovae , 1998 .
[42] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[43] William Press,et al. A Precise Distance Indicator: Type Ia Supernova Multicolor Light-Curve Shapes , 1996, astro-ph/9604143.
[44] E. Bertin,et al. SExtractor: Software for source extraction , 1996 .
[45] A. Pastorello,et al. SYSTEMATIC UNCERTAINTIES ASSOCIATED WITH THE COSMOLOGICAL ANALYSIS OF THE FIRST PAN-STARRS1 TYPE Ia SUPERNOVA SAMPLE , 2013, 1310.3824.
[46] C. Tao,et al. HOST GALAXY PROPERTIES AND HUBBLE RESIDUALS OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY , 2013, 1304.4720.
[47] Wendy L. Freedman,et al. The Carnegie Supernova Project: The Low‐Redshift Survey , 2005, astro-ph/0512039.
[48] M. Hudson,et al. Cosmological Parameters from the Comparison of the 2MASS Gravity Field with Peculiar Velocity Surveys , 2005, astro-ph/0511012.