A strong ultraviolet pulse from a newborn type Ia supernova

[1]  D. Alter PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC , 2016 .

[2]  Daniela I. Moody,et al.  Automated variability selection in time-domain imaging surveys using sparse representations with learned dictionaries , 2015, 2015 IEEE Applied Imagery Pattern Recognition Workshop (AIPR).

[3]  Peter E. Nugent,et al.  SLOW-SPEED SUPERNOVAE FROM THE PALOMAR TRANSIENT FACTORY: TWO CHANNELS , 2014, 1405.7409.

[4]  R. B. Barreiro,et al.  Planck 2013 results , 2014 .

[5]  S. Jha,et al.  POSSIBLE DETECTION OF THE STELLAR DONOR OR REMNANT FOR THE TYPE Iax SUPERNOVA 2008ha , 2014, 1408.1091.

[6]  A. Riess,et al.  A luminous, blue progenitor system for the type Iax supernova 2012Z , 2014, Nature.

[7]  Xiaofeng Wang,et al.  Spectroscopic Classification of ASASSN-14ad , 2014 .

[8]  J. Prieto,et al.  ASAS-SN Discoveries of a Probable Supernova in IC 0831 and a Possible Extreme (delta V > 6.6 mag) M-dwarf Flare , 2014 .

[9]  F. Förster,et al.  PERSISTENT C ii ABSORPTION IN THE NORMAL TYPE Ia SUPERNOVA 2002fk , 2013, 1312.3342.

[10]  Filippo Mannucci,et al.  Observational Clues to the Progenitors of Type Ia Supernovae , 2013, 1312.0628.

[11]  E. Phinney,et al.  SCIENCE WITH A WIDE-FIELD UV TRANSIENT EXPLORER , 2013, 1303.6194.

[12]  C. A. Oxborrow,et al.  Planck 2013 results. XVI. Cosmological parameters , 2013, 1303.5076.

[13]  K. Wagstaff,et al.  ASTRONOMICAL DATA TRIAGE FOR RAPID SCIENCE RETURN , 2014 .

[14]  M. Wainwright,et al.  Using machine learning for discovery in synoptic survey imaging data , 2012, 1209.3775.

[15]  S. E. Persson,et al.  TYPE Iax SUPERNOVAE: A NEW CLASS OF STELLAR EXPLOSION , 2012, 1212.2209.

[16]  J. G. Hernández,et al.  No surviving evolved companions of the progenitor of SN 1006 , 2012, Nature.

[17]  M. A. Strauss,et al.  SPECTRAL CLASSIFICATION AND REDSHIFT MEASUREMENT FOR THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY , 2012, 1207.7326.

[18]  J. Wheeler,et al.  Testing supernovae Ia distance measurement methods with SN 2011fe , 2012, 1207.4310.

[19]  E. Ofek,et al.  ANALYSIS OF THE EARLY-TIME OPTICAL SPECTRA OF SN 2011fe IN M101 , 2012, 1205.6011.

[20]  A. Gal-yam,et al.  WISeREP—An Interactive Supernova Data Repository , 2012, 1204.1891.

[21]  P. Brown,et al.  CONSTRAINTS ON TYPE Ia SUPERNOVA PROGENITOR COMPANIONS FROM EARLY ULTRAVIOLET OBSERVATIONS WITH SWIFT , 2012, 1203.5315.

[22]  P. Ricker,et al.  IMPACT OF TYPE Ia SUPERNOVA EJECTA ON BINARY COMPANIONS IN THE SINGLE-DEGENERATE SCENARIO , 2012, 1203.1932.

[23]  A. Filippenko,et al.  Berkeley Supernova Ia Program – IV. Carbon detection in early-time optical spectra of Type Ia supernovae , 2012, 1202.3788.

[24]  R. Kirshner,et al.  THE LOW-VELOCITY, RAPIDLY FADING TYPE Ia SUPERNOVA 2002es , 2012, 1202.3140.

[25]  P. Brown,et al.  A SWIFT LOOK AT SN 2011fe: THE EARLIEST ULTRAVIOLET OBSERVATIONS OF A TYPE Ia SUPERNOVA , 2011, 1110.2538.

[26]  Emilio Falco,et al.  THE 2MASS REDSHIFT SURVEY—DESCRIPTION AND DATA RELEASE , 2011, 1108.0669.

[27]  M. Sullivan,et al.  The Palomar Transient Factory Photometric Calibration , 2011, 1112.4851.

[28]  Nathaniel R. Butler,et al.  Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe , 2011, Nature.

[29]  Federica B. Bianco,et al.  Supernova SN 2011fe from an exploding carbon–oxygen white dwarf star , 2011, Nature.

[30]  C. Tao,et al.  TYPE Ia SUPERNOVA CARBON FOOTPRINTS , 2011, 1109.1312.

[31]  R. Beaton,et al.  VERY EARLY ULTRAVIOLET AND OPTICAL OBSERVATIONS OF THE TYPE Ia SUPERNOVA 2009ig , 2011, 1109.0987.

[32]  I. Hook,et al.  CONSTRAINING TYPE Ia SUPERNOVAE PROGENITORS FROM THREE YEARS OF SUPERNOVA LEGACY SURVEY DATA , 2011, 1106.4008.

[33]  Richard Walters,et al.  REAL-TIME DETECTION AND RAPID MULTIWAVELENGTH FOLLOW-UP OBSERVATIONS OF A HIGHLY SUBLUMINOUS TYPE II-P SUPERNOVA FROM THE PALOMAR TRANSIENT FACTORY SURVEY , 2011, 1106.0400.

[34]  M. Sullivan,et al.  SNLS3: CONSTRAINTS ON DARK ENERGY COMBINING THE SUPERNOVA LEGACY SURVEY THREE-YEAR DATA WITH OTHER PROBES , 2011, 1104.1444.

[35]  Robert A. Fesen,et al.  A STUDY OF CARBON FEATURES IN TYPE Ia SUPERNOVA SPECTRA , 2011, 1103.1671.

[36]  A. Breeveld,et al.  An Updated Ultraviolet Calibration for the Swift/UVOT , 2011, 1102.4717.

[37]  Wendy L. Freedman,et al.  THE CARNEGIE SUPERNOVA PROJECT: LIGHT-CURVE FITTING WITH SNooPy , 2010, 1010.4040.

[38]  Robert C. Nichol,et al.  SINGLE OR DOUBLE DEGENERATE PROGENITORS? SEARCHING FOR SHOCK EMISSION IN THE SDSS-II TYPE Ia SUPERNOVAE , 2010, 1008.4797.

[39]  M. Phillips,et al.  NEAR-ULTRAVIOLET PROPERTIES OF A LARGE SAMPLE OF TYPE Ia SUPERNOVAE AS OBSERVED WITH THE Swift UVOT , 2010, 1007.5279.

[40]  W. Hillebrandt,et al.  DOUBLE-DETONATION SUB-CHANDRASEKHAR SUPERNOVAE: SYNTHETIC OBSERVABLES FOR MINIMUM HELIUM SHELL MASS MODELS , 2010, 1006.4489.

[41]  W. M. Wood-Vasey,et al.  EARLY- AND LATE-TIME OBSERVATIONS OF SN 2008ha: ADDITIONAL CONSTRAINTS FOR THE PROGENITOR AND EXPLOSION , 2009, 0912.0732.

[42]  Daniel Kasen,et al.  SEEING THE COLLISION OF A SUPERNOVA WITH ITS COMPANION STAR , 2009, 0909.0275.

[43]  Ernest E. Croner,et al.  The Palomar Transient Factory: System Overview, Performance, and First Results , 2009, 0906.5350.

[44]  M. Fukugita,et al.  LUMINOSITY FUNCTIONS OF TYPE Ia SUPERNOVAE AND THEIR HOST GALAXIES FROM THE SLOAN DIGITAL SKY SURVEY , 2009, 0905.4125.

[45]  Mark Sullivan,et al.  The Progenitors of Type Ia Supernovae , 2008, 0806.3729.

[46]  Oswald H. W. Siegmund,et al.  UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVIII , 2007 .

[47]  M. Sullivan,et al.  SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators , 2007, astro-ph/0701828.

[48]  W. B. Burton,et al.  The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI - Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections , 2005, astro-ph/0504140.

[49]  Alan A. Wells,et al.  The Swift Gamma-Ray Burst Mission , 2004, astro-ph/0405233.

[50]  I. Hook,et al.  The Gemini–North Multi‐Object Spectrograph: Performance in Imaging, Long‐Slit, and Multi‐Object Spectroscopic Modes , 2004 .

[51]  Peter W. A. Roming,et al.  The Swift Ultra-Violet/Optical Telescope , 2002, SPIE Optics + Photonics.

[52]  D. Watson,et al.  The Swift X-Ray Telescope , 1999, SPIE Optics + Photonics.

[53]  O. Lahav,et al.  Cosmological parameters , 2008 .

[54]  Alison L. Coil,et al.  The DEIMOS spectrograph for the Keck II Telescope: integration and testing , 2003, SPIE Astronomical Telescopes + Instrumentation.

[55]  Caltech,et al.  SN 2002cx: The Most Peculiar Known Type Ia Supernova , 2003, astro-ph/0301428.

[56]  A. Moorwood,et al.  Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, , 2003 .

[57]  A. Chtchelkanova,et al.  Supernovae : Simulations of the Deflagration Stage and Their Implications , 2018 .

[58]  D. Branch,et al.  Optical Spectra of Supernovae , 2001, astro-ph/0111573.

[59]  I. Hook,et al.  Measurements of Ω and Λ from 42 High-Redshift Supernovae , 1998, astro-ph/9812133.

[60]  M. Scodeggio,et al.  The Universality of the Fundamental Plane of E and S0 Galaxies: Sample Definition and I-Band Photometric Data , 1998, astro-ph/9809350.

[61]  A. G. Alexei,et al.  OBSERVATIONAL EVIDENCE FROM SUPERNOVAE FOR AN ACCELERATING UNIVERSE AND A COSMOLOGICAL CONSTANT , 1998 .

[62]  A. Riess,et al.  Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.

[63]  P. Nugent,et al.  Synthetic Spectra of Hydrodynamic Models of Type Ia Supernovae , 1996, astro-ph/9612044.

[64]  Harland W. Epps,et al.  THE KECK LOW-RESOLUTION IMAGING SPECTROMETER , 1995 .

[65]  M. Phillips,et al.  The Absolute Magnitudes of Type IA Supernovae , 1993 .

[66]  L. Ho,et al.  The subluminous spectroscopically peculiar type Ia supernova 1991bg in the elliptical galaxy NGC 4374 , 1992 .

[67]  James E. Gunn,et al.  AN EFFICIENT LOW RESOLUTION AND MODERATE RESOLUTION SPECTROGRAPH FOR THE HALE TELESCOPE , 1982 .

[68]  J. Whelan,et al.  Binaries and Supernovae of Type I , 1973 .