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Related papers: CfA4: Light Curves for 94 Type Ia Supernovae

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We present the optical (UBVRI) and ultraviolet (Swift-UVOT) photometry, and optical spectroscopy of Type Ia supernova SN 2017hpa. We study broadband UV+optical light curves and low resolution spectroscopy spanning from $-13.8$ to $+108$~d…

Solar and Stellar Astrophysics · Physics 2021-03-03 Anirban Dutta , Avinash Singh , G. C. Anupama , D. K. Sahu , Brajesh Kumar

Large planned photometric surveys will discover hundreds of thousands of supernovae (SNe), outstripping the resources available for spectroscopic follow-up and necessitating the development of purely photometric methods to exploit these…

We present 432 low-dispersion optical spectra of 32 Type Ia supernovae (SNe Ia) that also have well-calibrated light curves. The coverage ranges from 6 epochs to 36 epochs of spectroscopy. Most of the data were obtained with the 1.5m…

We present the discovery of a Type Ia supernova (SN) at redshift $z = 1.914$ from the CANDELS multi-cycle treasury program on the \textit{Hubble Space Telescope (HST)}. This SN was discovered in the infrared using the Wide-Field Camera 3,…

In this third paper in a series we compare spectral feature measurements to photometric properties of 108 low-redshift (z < 0.1) Type Ia supernovae (SNe Ia) with optical spectra within 5 d of maximum brightness. We find the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Jeffrey M. Silverman , Mohan Ganeshalingam , Weidong Li , Alexei V. Filippenko

We present an analysis of the Hubble diagram for 12 Type Ia supernovae (SNe Ia) observed in the near-infrared J and H bands. We select SNe exclusively from the redshift range 0.03 < z < 0.09 to reduce uncertainties coming from peculiar…

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

The Carnegie Supernova Project (CSP) was a five-year observational survey conducted at Las Campanas Observatory that obtained, among other things, high-quality light curves of ~100 low-redshift Type Ia supernovae (SNe Ia). Presented here is…

This is the first release of optical spectroscopic data of low-redshift Type Ia supernovae (SNe Ia) by the Carnegie Supernova Project including 604 previously unpublished spectra of 93 SNe Ia. The observations cover a range of phases from…

We analyze the three-year SDSS-II Superernova (SN) Survey data and identify a sample of 1070 photometric SN Ia candidates based on their multi-band light curve data. This sample consists of SN candidates with no spectroscopic confirmation,…

We present griz light curves of 146 spectroscopically confirmed Type Ia Supernovae ($0.03 < z <0.65$) discovered during the first 1.5 years of the Pan-STARRS1 Medium Deep Survey. The Pan-STARRS1 natural photometric system is determined by a…

Aims. We present and study the spectroscopic and photometric evolution of the type Ia supernova (SN Ia) 2010ev. Methods. We obtain and analyze multi-band optical light curves and optical-near-infrared spectroscopy at low and medium…

Early-time observations of Type Ia supernovae (SNe Ia) are essential to constrain their progenitor properties. In this paper, we present high-quality light curves of 127 SNe Ia discovered by the Zwicky Transient Facility (ZTF) in 2018. We…

A comparative study of near-maximum-light optical spectra of 24 Type Ia supernovae (SNe Ia) is presented. The spectra are quantified in two ways, and assigned to four groups. Seven "core-normal" SNe Ia have very similar spectra, except for…

Type Ia supernova (SN Ia) as a standard candle is an ideal tool to measure cosmic distance and expansion history of the Universe. Here we investigate the SN Ia photometric measurement in the China Space Station Telescope Ultra Deep Field…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-24 Minglin Wang , Yan Gong , Furen Deng , Haitao Miao , Xuelei Chen , Hu Zhan

A sample of 35 SNe Ia with good to excellent photometry in B and V, minimum internal absorption, and 1200 < v < \approx 30000 km/s is compiled from the literature. As far as their spectra are known they are all Branch-normal. For 29 of the…

Astrophysics · Physics 2009-02-16 B. R. Parodi , A. Saha , A. Sandage , G. A. Tammann

We present spectra of twelve Type Ia supernovae obtained in 1999 at the William Herschel Telescope and the Nordic Optical Telescope during a search for Type Ia supernovae (SN Ia) at intermediate redshift. The spectra range from z=0.178 to…

We present a new empirical method for fitting multicolor light curves of Type Ia supernovae. Our method combines elements from two widely used techniques in the literature: the delta_m15 template fitting method and the Multicolor…

Astrophysics · Physics 2008-11-26 Jose Luis Prieto , Armin Rest , Nicholas B. Suntzeff