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We present the first measurement of the rate of Type Ia supernovae at high redshift. The result is derived using a large subset of data from the Supernova Cosmology Project. Three supernovae were discovered in a surveyed area of 1.7 square…

We present extensive optical photometric and spectroscopic observations for the nearby Type Ia supernova (SN Ia) 2019ein, spanning the phases from $\sim 3$ days to $\sim 330$ days after the explosion. This SN Ia is characterized by…

We present optical light curves of five Type Ia supernovae (2002er, 2002fk, 2003cg, 2003du, 2003fk). The photometric observations were performed in a set of intermediate-band filters. SNe 2002er, 2003du appear to be normal SN Ia events with…

天体物理学 · 物理学 2007-05-23 Xiaofeng Wang , Xu Zhou , Tianmeng Zhang , Zongwei Li

Observations of the peculiar type Ia SN~1991bg in NGC~4374 collected at ESO--La Silla and Asiago are presented and discussed. The broad--band light curves in the early months have a narrower peak and a luminosity decline faster than other…

天体物理学 · 物理学 2015-06-24 M. Turatto , S. Benetti , E. Cappellaro , I. J. Danziger , M. Della Valle , C. Gouiffes , P. A. Mazzali , F. Patat

We present preliminary results of the observational campaign on SN 2002er carried out by the European Supernova Collaboration (ESC). For this supernova the optical coverage from epochs -11 days to +50 days is excellent, both in imaging and…

天体物理学 · 物理学 2007-05-23 G. Pignata , F. Patat , R. Kotak , P. Meikle , M. Stritzinger , W. Hillebrandt

The focus of this review is the work that has been done during the 1990s on using Type Ia supernovae (SNe Ia) to measure the Hubble constant ($H_0$). SNe Ia are well suited for measuring $H_0$. A straightforward maximum-light color…

天体物理学 · 物理学 2009-10-30 D. Branch

1991T-like supernovae are the luminous, slow-declining extreme of the Branch shallow-silicon (SS) subclass of Type Ia supernovae. They are distinguished by extremely weak Ca II H & K and Si II $\lambda6355$ and strong Fe III absorption…

We studied the spectral features of Si II $\lambda\lambda$4130, 5972, 6355 and S II W-trough for a large sample of Type Ia supernovae (SNe Ia). We find that in NV (Normal-Velocity) subclass of SNe Ia, these features tend to reach a maximum…

高能天体物理现象 · 物理学 2021-04-08 Xulin Zhao , Keiichi Maeda , Xiaofeng Wang , Hanna Sai

We present highly sampled photometry of the supernova (SN) 2023ixf, a Type II SN in M101, beginning 2 days before its first known detection. To gather these data, we enlisted the global Unistellar Network of citizen scientists. These 252…

高能天体物理现象 · 物理学 2023-07-28 Lauren A. Sgro , Thomas M. Esposito , Guillaume Blaclard , Sebastian Gomez , Franck Marchis , Alexei V. Filippenko , Daniel O'Conner Peluso , Stephen S. Lawrence , Aad Verveen , Andreas Wagner , Anouchka Nardi , Barbara Wiart , Benjamin Mirwald , Bill Christensen , Bob Eramia , Bruce Parker , Bruno Guillet , Byungki Kim , Chelsey A. Logan , Christopher C. M. Kyba , Christopher Toulmin , Claudio G. Vantaggiato , Dana Adhis , Dave Gary , Dave Goodey , David Dickinson , David Koster , Davy Martin , Eliud Bonilla , Enner Chung , Eric Miny , Fabrice Mortecrette , Fadi Saibi , Francois O. Gagnon , François Simard , Gary Vacon , Georges Simard , Gerrit Dreise , Hiromi Funakoshi , Janet Vacon , James Yaniz , Jean-Charles Le Tarnec , Jean-Marie Laugier , Jennifer L. W. Siders , Jim Sweitzer , Jiri Dvoracek , John Archer , John Deitz , John K. Bradley , Keiichi Fukui , Kendra Sibbernsen , Kevin Borrot , Kevin Cross , Kevin Heider , Koichi Yamaguchi , Lea A. Hirsch , Liouba Leroux , Mario Billiani , Markus Lorber , Martin J. Smallen , Masao Shimizu , Masayoshi Nishimura , Matthew Ryno , Michael Cunningham , Michael Gagnon , Michael Primm , Michael Rushton , Michael Sibbernsen , Mike Mitchell , Neil Yoblonsky , Niniane Leroux , Olivier Clerget , Ozren Stojanović , Patrice Unique , Patrick Huth , Raymund John Ang , Regis Santoni , Robert Foster , Roberto Poggiali , Ruyi Xu , Ryuichi Kukita , Sanja Šćepanović , Sophie Saibi , Stefan Will , Stephan Latour , Stephen Haythornthwaite , Sylvain Cadieux , Thoralf Müller , Tze Yang Chung , Yoshiya Watanabe , Yvan Arnaud

Aims: Spectroscopic observations of Type Ia supernovae obtained at the New Technology Telescope (NTT) and the Nordic Optical Telescope (NOT), in conjunction with the SDSS-II Supernova Survey, are analysed. We use spectral indicators…

We present a set of photometric and spectroscopic observations of a bright Type Ib supernova SN 2012au from -6d until ~+150d after maximum. The shape of its early R-band light curve is similar to that of an average Type Ib/c supernova. The…

We present 32 epochs of optical (3300-9700 \AA) spectrophotometric observations of the nearby quintessential "normal" type Ia supernova (SN Ia) SN 2011fe in the galaxy M101, extending from -15 to +97 d with respect to B-band maximum,…

We present photometric and spectroscopic observations of the nearby Type Ia SN 2019yvq, from its discovery $\sim$1 day after explosion to $\sim$100 days after its peak brightness. This SN exhibits several unusual features, most notably an…

We present 2603 spectra of 462 nearby Type Ia supernovae (SN Ia) obtained during 1993-2008 through the Center for Astrophysics Supernova Program. Most of the spectra were obtained with the FAST spectrograph at the FLWO 1.5m telescope and…

We present optical and near-infrared photometry and spectroscopy of the Type Ia SN 2003cg, which exploded in the nearby galaxy NGC 3169. The observations cover a period between -8.5 and +414 days post-maximum. SN 2003cg is a normal but…

The spectacular success of type Ia supernovae (SNe Ia) in SN-cosmology is based on the assumption that their photometric and spectroscopic properties are invariant with redshift. However, this fundamental assumption needs to be tested with…

高能天体物理现象 · 物理学 2017-12-13 Zach Cano , Jonatan Selsing , Jens Hjorth , Antonio de Ugarte Postigo , Lise Christensen , Christa Gall , D. A. Kann

SN 1998bw holds the record for the most energetic Type Ic explosion, one of the brightest radio supenovae and probably the first supernova associated with a gamma-ray burst. In this paper we present spectral observations of SN 1998bw…

We present optical photometry and spectroscopy of SN\,2019stc (=ZTF19acbonaa), an unusual Type Ic supernova (SN Ic) at a redshift of $z=0.117$. SN\,2019stc exhibits a broad double-peaked light curve, with the first peak having an absolute…

高能天体物理现象 · 物理学 2021-07-30 Sebastian Gomez , Edo Berger , Griffin Hosseinzadeh , Peter K. Blanchard , Matt Nicholl , V. Ashley Villar

We present optical observations of supernova (SN) 2014ek discovered during the Tsinghua-NAOC Transient Survey (TNTS), which shows properties that are consistent with those of SN 2002cx-like events (dubbed as SNe Iax). The photometry…

Ultraviolet, optical, and near-infrared photometry and optical spectroscopy of the broad-lined Type Ic supernova (SN) 2009bb are presented, following the flux evolution from -10 to +285 days past B-band maximum. Thanks to the very early…