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Related papers: Using Spectral Flux Ratios to Standardize SN Ia Lu…

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We present the analysis of the first set of low-redshift Type Ia supernovae (SNe Ia) by the Carnegie Supernova Project. Well-sampled, high-precision optical (ugriBV) and near-infrared (NIR; YJHKs) light curves obtained in a well-understood…

Measurements of Type Ia Supernovae (SNe Ia) in the near-infrared (NIR) have been used both as an alternate path to cosmology compared to optical measurements and as a method of constraining key systematics for the larger optical studies.…

Type Ia supernovae (SNe Ia) are more precise standardizable candles when measured in the near-infrared (NIR) than in the optical. With this motivation, from 2012-2017 we embarked on the RAISIN program with the Hubble Space Telescope (HST)…

We present an empirical method which measures the distance to a Type Ia supernova (SN Ia) with a precision of ~ 10% from a single night's data. This method measures the supernova's age and luminosity/light-curve parameter from a spectrum,…

We study the properties of Type Ia Supernovae (SNe Ia) as functions of the radial distance from their host galaxy centers. Using a sample of 62 SNe Ia with reliable luminosity, reddening, and decline rate determinations, we find no…

Astrophysics · Physics 2009-10-31 Valentin D. Ivanov , Mario Hamuy , Philip A. Pinto

Strongly lensed type Ia supernovae (SNe Ia) provide a unique cosmological probe to address the Hubble tension problem in cosmology. In addition to the sensitivity of the time delays to the value of the Hubble constant, the transient and…

Cosmology and Nongalactic Astrophysics · Physics 2025-06-27 Prajakta Mane , Anupreeta More , Surhud More

Ultraviolet (UV) observations of Type Ia supernovae (SNe Ia) are crucial for constraining the properties of their progenitor systems. Theoretical studies predicted that the UV spectra, which probe the outermost layers of a SN, should be…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Y. -C. Pan , R. J. Foley , D. O. Jones , A. V. Filippenko , N. P. M. Kuin

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. To perform such measurements the luminosity and cosmological redshift ($z$) of the SNe Ia have to be determined. The uncertainty on $z$ includes an…

We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.45 from the Hubble Space Telescope (HST) Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe.…

With the advent of large dedicated Type Ia supernova (SN Ia) surveys, K-corrections of SNe Ia and their uncertainties have become especially important in the determination of cosmological parameters. While K-corrections are largely driven…

We present the first maximum-light ultraviolet (UV) through near-infrared (NIR) Type Ia supernova (SN Ia) spectrum. This spectrum of SN 2011iv was obtained nearly simultaneously by the Hubble Space Telescope at UV/optical wavelengths and…

We present ultraviolet (UV) spectroscopy and photometry of four Type Ia supernovae (SNe 2004dt, 2004ef, 2005M, and 2005cf) obtained with the UV prism of the Advanced Camera for Surveys on the Hubble Space Telescope. This dataset provides…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Xiaofeng Wang , Lifan Wang , Alexei V. Filippenko , Eddie Baron , Markus Kromer , Dennis Jack , Tianmeng Zhang , Greg Aldering , Pierre Antilogus , David Arnett , Dietrich Baade , Brian J. Barris , Stefano Benetti , Patrice Bouchet , Adam S. Burrows , Ramon Canal , Enrico Cappellaro , Raymond Carlberg , Elisa di Carlo , Peter Challis , Arlin Crotts , John I. Danziger , Massimo Della Valle , Michael Fink , Ryan J. Foley , Claes Fransson , Avishay Gal-Yam , Peter Garnavich , Chris L. Gerardy , Gerson Goldhaber , Mario Hamuy , Wolfgang Hillebrandt , Peter A. Hoeflich , Stephen T. Holland , Daniel E. Holz , John P. Hughes , David J. Jeffery , Saurabh W. Jha , Dan Kasen , Alexei M. Khokhlov , Robert P. Kirshner , Robert Knop , Cecilia Kozma , Kevin Krisciunas , Brian C. Lee , Bruno Leibundgut , Eric J. Lentz , Douglas C. Leonard , Walter H. G. Lewin , Weidong Li , Mario Livio , Peter Lundqvist , Dan Maoz , Thomas Matheson , Paolo Mazzali , Peter Meikle , Gajus Miknaitis , Peter Milne , Stefan Mochnacki , Ken'Ichi Nomoto , Peter E. Nugent , Elaine Oran , Nino Panagia , Saul Perlmutter , Mark M. Phillips , Philip Pinto , Dovi Poznanski , Christopher J. Pritchet , Martin Reinecke , Adam Riess , Pilar Ruiz-Lapuente , Richard Scalzo , Eric M. Schlegel , Brian Schmidt , James Siegrist , Alicia M. Soderberg , Jesper Sollerman , George Sonneborn , Anthony Spadafora , Jason Spyromilio , Richard A. Sramek , Sumner G. Starrfield , Louis G. Strolger , Nicholas B. Suntzeff , Rollin Thomas , John L. Tonry , Amedeo Tornambe , James W. Truran , Massimo Turatto , Michael Turner , Schuyler D. Van Dyk , Kurt Weiler , J. Craig Wheeler , Michael Wood-Vasey , Stan Woosley , Hitoshi Yamaoka

Ultraviolet (UV) observations of Type Ia supernovae (SNe Ia) probe the outermost layers of the explosion, and UV spectra of SNe Ia are expected to be extremely sensitive to differences in progenitor composition and the details of the…

This is the third paper of a series in which we present new measurements of the observed rates of supernovae (SNe) in the local Universe, determined from the Lick Observatory Supernova Search (LOSS). We have considered a sample of about…

Having two "sibling" Type Ia supernovae (SNe Ia) in the same galaxy offers additional advantages in reducing a variety of systematic errors involved in estimating the Hubble constant, $H_{0}$. NGC 4414 is a nearby galaxy included in the…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-05 Eulalia Gallego-Cano , Luca Izzo , Carlos Dominguez-Tagle , Francisco Prada , Enrique Pérez , Nandita Khetan , In Sung Jang

We compare the observed correlations between the maximum brightness, postmaximum decline rate and color at maximum light of Type Ia supernovae (SN Ia) with model predictions. The observations are based on a total of 40 SN Ia with 29 SN of…

Astrophysics · Physics 2016-08-30 P. Höflich , A. Khokhlov , J. C. Wheeler , M. Hamuy , M. M. Phillips , N. B. Suntzeff

We improve estimates of stellar mass and mass-weighted average age of Type Ia supernova (SN Ia) host galaxies by combining UV and near-IR photometry with optical photometry in our analysis. Using 206 SNe Ia drawn from the full three-year…