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相关论文: Swift Observations of X-ray supernovae

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The Ultra-Violet Optical Telescope on the Swift spacecraft has observed hundreds of supernovae, covering all major types and most subtypes. Here we introduce the Swift Optical/Ultraviolet Supernova Archive (SOUSA), which will contain all of…

高能天体物理现象 · 物理学 2015-06-22 Peter J. Brown , Alice A. Breeveld , Stephen Holland , Paul Kuin , Tyler Pritchard

We report on new VLT optical spectroscopic and multi-wavelength archival observations of SN1996cr, a previously identified ULX known as Circinus Galaxy X-2. Our optical spectrum confirms SN1996cr as a bona fide type IIn SN, while archival…

天体物理学 · 物理学 2009-11-13 F. E. Bauer , V. V. Dwarkadas , W. N. Brandt , S. Immler , S. Smartt , N. Bartel , M. F. Bietenholz

The Sloan Digital Sky Survey-II (SDSS-II) has embarked on a multi-year project to identify and measure light curves for intermediate-redshift (0.05 < z < 0.35) Type Ia supernovae (SNe Ia) using repeated five-band (ugriz) imaging over an…

Context. The SDSS-II Supernova Survey, conducted between 2005 and 2007, was designed to detect a large number of Type Ia supernovae (SNe Ia) around z~0.2, the redshift "gap" between low-z and high-z SN searches. The survey has provided…

We describe the observing strategy, data reduction tools and early results of a supernova (SN) search project, named SUDARE, conducted with the ESO VST telescope aimed at measuring the rate of the different types of SNe in the redshift…

SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and…

高能天体物理现象 · 物理学 2015-05-27 IceCube Collaboration , R. Abbasi , Y. Abdou , T. Abu-Zayyad , J. Adams , J. A. Aguilar , M. Ahlers , K. Andeen , J. Auffenberg , X. Bai , M. Baker , S. W. Barwick , R. Bay , J. L. Bazo Alba , K. Beattie , J. J. Beatty , S. Bechet , J. K. Becker , K. -H. Becker , M. L. Benabderrahmane , S. BenZvi , J. Berdermann , P. Berghaus , D. Berley , E. Bernardini , D. Bertrand , D. Z. Besson , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , D. Bose , S. Boser , O. Botner , J. Braun , S. Buitink , M. Carson , D. Chirkin , B. Christy , J. Clem , F. Clevermann , S. Cohen , C. Colnard , D. F. Cowen , M. V. D'Agostino , M. Danninger , J. C. Davis , C. De Clercq , L. Demirors , O. Depaepe , F. Descamps , P. Desiati , G. de Vries-Uiterweerd , T. DeYoung , J. C. D\?iaz-Velez , M. Dierckxsens , J. Dreyer , J. P. Dumm , M. R. Duvoort , R. Ehrlich , J. Eisch , R. W. Ellsworth , O. Engdegård , S. Euler , P. A. Evenson , O. Fadiran , A. R. Fazely , A. Fedynitch , T. Feusels , K. Filimonov , C. Finley , M. M. Foerster , B. D. Fox , A. Franckowiak , R. Franke , T. K. Gaisser , J. Gallagher , M. Geisler , L. Gerhardt 9 , L. Gladstone , T. Glusenkamp , A. Goldschmidt , J. A. Goodman , D. Grant , T. Griesel , A. Groß , S. Grullon , M. Gurtner , C. Ha , A. Hallgren , F. Halzen , K. Han , K. Hanson , K. Helbing , P. Herquet , S. Hickford , G. C. Hill , K. D. Hoffman , A. Homeier , K. Hoshina , D. Hubert , W. Huelsnitz , J. -P. Hülß , P. O. Hulth , K. Hultqvist , S. Hussain , A. Ishihara , J. Jacobsen , G. S. Japaridze , H. Johansson , J. M. Joseph , K. -H. Kampert , A. Kappes , T. Karg , A. Karle , J. L. Kelley , N. Kemming , P. Kenny , J. Kiryluk , F. Kislat , S. R. Klein , J. -H. Kohne , G. Kohnen , H. Kolanoski , L. Köpke , D. J. Koskinen , M. Kowalski , T. Kowarik , M. Krasberg , T. Krings , G. Kroll , K. Kuehn , T. Kuwabara , M. Labare , S. Lafebre , K. Laihem , H. Landsman , M. J. Larson , R. Lauer , R. Lehmann , J. Lunemann , J. Madsen , P. Majumdar , A. Marotta , R. Maruyama , K. Mase , H. S. Matis , M. Matusik , K. Meagher , M. Merck , P. Mészaros , T. Meures , E. Middell , N. Milke , J. Miller , T. Montaruli , R. Morse , S. M. Movit , R. Nahnhauer , J. W. Nam , U. Naumann , P. Nießen , D. R. Nygren , S. Odrowski , A. Olivas , M. Olivo , A. O'Murchadha , M. Ono , S. Panknin , L. Paul18 , C. Perez de los Heros , J. Petrovic , A. Piegsa , D. Pieloth , R. Porrata , J. Posselt , P. B. Price , M. Prikockis , G. T. Przybylski , K. Rawlins , P. Redl , E. Resconi , W. Rhode , M. Ribordy , A. Rizzo , J. P. Rodrigues , P. Roth , F. Rothmaier , C. Rott , T. Ruhe , D. Rutledge , B. Ruzybayev , D. Ryckbosch , H. -G. Sander , M. Santander , S. Sarkar , K. Schatto , S. Schlenstedt , T. Schmidt , A. Schukraft , A. Schultes , O. Schulz , M. Schunck , D. Seckel , B. Semburg , S. H. Seo , Y. Sestayo , S. Seunarine , A. Silvestri , K. Singh , A. Slipak , G. M. Spiczak , C. Spiering , M. Stamatikos , T. Stanev , G. Stephens , T. Stezelberger , R. G. Stokstad , S. Stoyanov , E. A. Strahler 20 , T. Straszheim16 , G. W. Sullivan16 , Q. Swillens , H. Taavola , I. Taboada , A. Tamburro , O. Tarasova , A. Tepe , S. Ter-Antonyan , S. Tilav , P. A. Toale , S. Toscano , D. Tosi , D. Turcan , N. van Eijndhoven , J. Vandenbroucke , A. Van Overloop , J. van Santen , M. Voge , B. Voigt , C. Walck , T. Waldenmaier , M. Wallraff , M. Walter , Ch. Weaver , C. Wendt1 , S. Westerhoff , N. Whitehorn , K. Wiebe , C. H. Wiebusch , G. Wikstrom , D. R. Williams , R. Wischnewski , H. Wissing , M. Wolf , K. Woschnagg , C. Xu , X. W. Xu , G. Yodh , S. Yoshida , P. Zarzhitsky

Type Ibn/Icn supernovae (SNe Ibn/Icn), which are characterized by narrow helium or carbon lines originated in hydrogen-poor dense circumstellar medium (CSM), provide new insights into the final evolution of massive stars. While SNe Ibn/Icn…

高能天体物理现象 · 物理学 2025-02-07 Yusuke Inoue , Keiichi Maeda

Wide field surveys will soon be discovering Type Ia supernovae (SNe) at rates of several thousand per year. Spectroscopic follow-up can only scratch the surface for such enormous samples, so these extensive data sets will only be useful to…

宇宙学与河外天体物理 · 物理学 2015-05-18 Steven A. Rodney , John L. Tonry

We present two supernovae (SNe) discovered with the Hubble Space Telescope (HST) in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), an HST multi-cycle treasury program. We classify both objects as Type Ia SNe…

Supernova (SN) rates serve as an important probe of star-formation models and initial mass functions. Near-infrared seeing-limited ground-based surveys typically discover a factor of 3-10 fewer SNe than predicted from far-infrared (FIR)…

We present BVRI and unfiltered Clear light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search (LOSS) follow-up program. Our SESN sample consists of 19…

高能天体物理现象 · 物理学 2022-03-30 WeiKang Zheng , Benjamin E. Stahl , Thomas de Jaeger , Alexei V. Filippenko , Shan-Qin Wang , Wen-Pei Gan , Thomas G. Brink , Ivan Altunin , Raphael Baer-Way , Andrew Bigley , Kyle Blanchard , Peter K. Blanchard , James Bradley , Samantha K. Cargill , Chadwick Casper , Teagan Chapman , Vidhi Chander , Sanyum Channa , Byung Yun Choi , Nick Choksi , Matthew Chu , Kelsey I. Clubb , Daniel P. Cohen , Paul A. Dalba , Asia deGraw , Maxime de Kouchkovsky , Michael Ellison , Edward Falcon , Ori D. Fox , Kiera Fuller , Mohan Ganeshalingam , Nachiket Girish , Carolina Gould , Goni Halevi , Andrew Halle , Kevin T. Hayakawa , Romain Hardy , Julia Hestenes , Andrew M. Hoffman , Michael Hyland , Benjamin T. Jeffers , Connor Jennings , Michael T. Kandrashoff , Anthony Khodanian , Minkyu Kim , Haejung Kim , Michelle E. Kislak , Daniel Krishnan , Sahana Kumar , Snehaa Ganesh Kumar , Joel Leja , Erin J. Leonard , Gary Z. Li , Weidong Li , Ji-Shun Lian , Evelyn Liu , Thomas B. Lowe , Philip Lu , Emily Ma , Michelle N. Mason , Michael May , Kyle McAllister , Emma McGinness , Shaunak Modak , Jeffrey Molloy , Yukei S. Murakami , Omnarayani Nayak , Derek Perera , Kenia Pina , Druv Punjabi , Andrew Rikhter , Timothy W. Ross , Jackson Sipple , Costas Soler , Samantha Stegman , Haynes Stephens , James Sunseri , Kevin Tang , Stephen Taylor , Patrick Thrasher , Schuyler D. Van Dyk , Xiang-Gao Wang , Jeremy Wayland , Andrew Wilkins , Abel Yagubyan , Heechan Yuk , Sameen Yunus , Keto D. Zhang

Short supersoft X-ray source (SSS) states (durations < 100 days) of classical novae (CNe) indicate massive white dwarfs that are candidate progenitors of supernovae type Ia. We carry out a dedicated optical and X-ray monitoring program of…

Classical novae (CNe) have recently been reported to represent the major class of supersoft X-ray sources (SSSs) in the central area of our neighbouring galaxy M 31. This paper presents a review of results from recent X-ray observations of…

高能天体物理现象 · 物理学 2015-05-14 M. Henze , W. Pietsch , F. Haberl , G. Sala , M. Hernanz , D. Hatzidimitriou , A. Rau , D. H. Hartmann , J. Greiner , M. Orio , H. Stiele , M. J. Freyberg

Core-collapse supernovae (CC SNe), especially those of type II-plateau (II-P), are thought to be important contributors to cosmic dust production. The most obvious indicator of the presence of newly-formed and/or pre-existing dust is the…

太阳与恒星天体物理 · 物理学 2015-06-12 T. Szalai , J. Vinkó

We present a systematic study of mid-infrared (mid-IR) emission from 141 nearby supernovae (SNe) observed with the InfraRed Array Camera (IRAC) on Spitzer.These SNe reside in one of the 190 galaxies within 20 Mpc drawn from the ongoing…

The super-massive black-holes in the centers of Active Galactic Nuclei (AGNs) are surrounded by obscuring matter that can block the nuclear radiation. Depending on the amount of blocked radiation, the flux from the AGN can be too faint to…

高能天体物理现象 · 物理学 2012-08-06 Eugenio Bottacini , Marco Ajello , Jochen Greiner

Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources:…

高能天体物理现象 · 物理学 2016-10-05 P. Romano , E. Bozzo , P. Esposito , B. Sbarufatti , F. Haberl , G. Ponti , P. D'Avanzo , L. Ducci , A. Segreto , C. Jin , N. Masetti , M. Del Santo , S. Campana , V. Mangano

We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST). By targeting massive galaxy clusters at 0.9<z<1.5, we obtain a twofold improvement in the efficiency of…