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相关论文: SN 2002cx: The Most Peculiar Known Type Ia Superno…

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We present Keck optical spectra of SN 2002cx, the most peculiar known Type Ia supernova (SN Ia), taken 227 and 277 days past maximum light. Astonishingly, the spectra are not dominated by the forbidden emission lines of iron that are a…

We present extensive photometric and spectroscopic observations of the Type Ia supernova (SN Ia) 2000cx in the S0 galaxy NGC 524, which reveal it to be peculiar. Photometrically, SN 2000cx is different from all known SNe Ia, and its light…

In spite of the apparent lack of Si II and S II features in its spectra, SN 2002cx was classified as a peculiar Type Ia supernova (SN Ia) on the basis of its overall photometric and spectroscopic behavior. Spectra obtained near maximum…

天体物理学 · 物理学 2009-11-10 David Branch , E. Baron , R. C. Thomas , D. Kasen , Weidong Li , Alexei V. Filippenko

The Type Ia supernova (SN Ia) SN 2000cx was one of the most peculiar transients ever discovered, with a rise to maximum brightness typical of a SN Ia, but a slower decline and a higher photospheric temperature. Thirteen years later SN…

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…

We present extensive photometric and spectroscopic observations of the peculiar Type Ia supernova (SN Ia) 2022vqz. It shares many similarities with the SN 2002es-like SNe Ia, such as low luminosity ($M_{B,\rm max}=-18.11\pm0.16$ mag) and…

SN 2002es is a peculiar subluminous Type Ia supernova (SN Ia) with a combination of observed characteristics never before seen in a SN Ia. At maximum light, SN 2002es shares spectroscopic properties with the underluminous SN 1991bg subclass…

We present optical spectroscopic and photometric observations of Type Ia supernova (SN) 2006X from --10 to +91 days after the $B$-band maximum. This SN exhibits one of the highest expansion velocity ever published for SNe Ia. At premaximum…

We present multi-band photometry and multi-epoch spectroscopy of the peculiar Type Ia supernova (SN Ia) 2007qd, discovered by the SDSS-II Supernova Survey. It possesses physical properties intermediate to those of the peculiar SN 2002cx and…

We present optical and infrared photometry of the unusual Type Ia supernova 2000cx. With the data of Li et al. (2001) and Jha (2002), this comprises the largest dataset ever assembled for a Type Ia SN, more than 600 points in UBVRIJHK. We…

We present Keck spectropolarimetry of the unusual type Ia supernova (SN Ia) 2005hk several days before maximum light. An analysis of the high signal-to-noise-ratio total-flux spectrum shows the object's extreme similarity to the peculiar SN…

天体物理学 · 物理学 2009-02-10 Ryan Chornock , Alexei V. Filippenko , David Branch , Ryan J. Foley , Saurabh Jha , Weidong Li

As part of the European Supernova Collaboration we obtained extensive photometry and spectroscopy of the type Ia SN 2002dj covering epochs from 11 days before to nearly two years after maximum. Detailed optical and near-infrared…

We present a preliminary analysis of an extensive set of optical observations of the Type Ia SN 2005hk. We show that the evolution of SN 2005hk closely follows that of the peculiar SN 2002cx. SN 2005hk is more luminous than SN 2002cx, while…

The Type Ia SN 2000cx exhibited multiple peculiarities, including a lopsided B-band light-curve peak that does not conform to current methods for using shapes of light curves to standardize SN Ia luminosities. We use the parameterized…

天体物理学 · 物理学 2009-11-10 D. Branch , R. C. Thomas , E. Baron , D. Kasen , K. Hatano , K. Nomoto , A. V. Filippenko , W. Li , R. J. Rudy

We present a comprehensive set of optical and near-infrared photometric and spectroscopic observations for SN 2014ck, extending from pre-maximum to six months later. These data indicate that SN 2014ck is photometrically nearly identical to…

We present extensive optical (UBVRI), near-infrared (JK) light curves and optical spectroscopy of the Type Ia supernova (SN) 2006X in the nearby galaxy NGC 4321 (M100). Our observations suggest that either SN 2006X has an intrinsically…

We present optical, infrared, ultraviolet, and radio observations of SN 2022xkq, an underluminous fast-declining type Ia supernova (SN Ia) in NGC 1784 ($\mathrm{D}\approx31$ Mpc), from $<1$ to 180 days after explosion. The high-cadence…

高能天体物理现象 · 物理学 2023-10-10 Jeniveve Pearson , David J. Sand , Peter Lundqvist , Lluís Galbany , Jennifer E. Andrews , K. Azalee Bostroem , Yize Dong , Emily Hoang , Griffin Hosseinzadeh , Daryl Janzen , Jacob E. Jencson , Michael J. Lundquist , Darshana Mehta , Nicolás Meza Retamal , Manisha Shrestha , Stefano Valenti , Samuel Wyatt , Joseph P. Anderson , Chris Ashall , Katie Auchettl , Eddie Baron , Stéphane Blondin , Christopher R. Burns , Yongzhi Cai , Ting-Wan Chen , Laura Chomiuk , David A. Coulter , Dane Cross , Kyle W. Davis , Thomas de Jaeger , James M. DerKacy , Dhvanil D. Desai , Georgios Dimitriadis , Aaron Do , Joseph R. Farah , Ryan J. Foley , Mariusz Gromadzki , Claudia P. Gutiérrez , Joshua Haislip , Jonay I. González Hernández , Jason T. Hinkle , Willem B. Hoogendam , D. Andrew Howell , Peter Hoeflich , Eric Hsiao , Mark E. Huber , Saurabh W. Jha , Cristina Jiménez Palau , Charles D. Kilpatrick , Vladimir Kouprianov , Sahana Kumar , Lindsey A. Kwok , Conor Larison , Natalie LeBaron , Xavier Le Saux , Jing Lu , Curtis McCully , Tycho Mera Evans , Peter Milne , Maryam Modjaz , Nidia Morrell , Tomás E. Müller-Bravo , Megan Newsome , Matt Nicholl , Estefania Padilla Gonzalez , Anna V. Payne , Craig Pellegrino , Kim Phan , Jonathan Pineda-García , Anthony L. Piro , Lara Piscarreta , Abigail Polin , Daniel E. Reichart , César Rojas-Bravo , Stuart D. Ryder , Irene Salmaso , Michaela Schwab , Melissa Shahbandeh , Benjamin J. Shappee , Matthew R. Siebert , Nathan Smith , Jay Strader , Kirsty Taggart , Giacomo Terreran , Samaporn Tinyanont , M. A. Tucker , Giorgio Valerin , D. R. Young

We present optical photometric and spectroscopic observations of the peculiar Type Ia supernova ASASSN-20jq/SN 2020qxp. It is a low-luminosity object with a peak absolute magnitude of $M_B=-17.1\pm0.5$ mag. Despite its low luminosity, its…

We present extensive u'g'r'i'BVRIYJHKs photometry and optical spectroscopy of SN 2005hk. These data reveal that SN 2005hk was nearly identical in its observed properties to SN 2002cx, which has been called ``the most peculiar known type Ia…

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