English
Related papers

Related papers: Supernova Discoveries 2010-2011: Statistics and Tr…

200 papers

The Catalina Real-time Transient Survey (CRTS) carried out a public survey for optical transients between 2007 and 2019, discovering more than 16,000 transient candidates. Here we present the spectra and highlight the results of the…

High Energy Astrophysical Phenomena · Physics 2025-10-27 A. J. Drake , S. G. Djorgovski , M. J. Graham , D. Stern , A. A. Mahabal , M. Catelan , J. L. Prieto , S. Larson

We present photometric properties and distance measurements of 252 high redshift Type Ia supernovae (0.15 < z < 1.1) discovered during the first three years of the Supernova Legacy Survey (SNLS). These events were detected and their…

The IceCube neutrino observatory pursues a follow-up program selecting interesting neutrino events in real-time and issuing alerts for electromagnetic follow-up observations. In March 2012, the most significant neutrino alert during the…

High Energy Astrophysical Phenomena · Physics 2019-08-16 M. G. Aartsen , K. Abraham , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , T. Anderson , M. Archinger , C. Arguelles , T. C. Arlen , J. Auffenberg , X. Bai , S. W. Barwick , V. Baum , R. Bay , J. J. Beatty , J. Becker Tjus , K. -H. Becker , E. Beiser , S. BenZvi , P. Berghaus , D. Berley , E. Bernardini , A. Bernhard , D. Z. Besson , G. Binder , D. Bindig , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , M. Börner , F. Bos , D. Bose , S. Böser , O. Botner , J. Braun , L. Brayeur , H. -P. Bretz , A. M. Brown , N. Buzinsky , J. Casey , M. Casier , E. Cheung , D. Chirkin , A. Christov , B. Christy , K. Clark , L. Classen , S. Coenders , D. F. Cowen , A. H. Cruz Silva , J. Daughhetee , J. C. Davis , M. Day , J. P. A. M. de André , C. De Clercq , H. Dembinski , S. De Ridder , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , J. C. Díaz-Vélez , J. P. Dumm , M. Dunkman , R. Eagan , B. Eberhardt , T. Ehrhardt , B. Eichmann , S. Euler , P. A. Evenson , O. Fadiran , S. Fahey , A. R. Fazely , A. Fedynitch , J. Feintzeig , J. Felde , K. Filimonov , C. Finley , T. Fischer-Wasels , S. Flis , T. Fuchs , M. Glagla , T. K. Gaisser , R. Gaior , J. Gallagher , L. Gerhardt , K. Ghorbani , D. Gier , L. Gladstone , T. Glüsenkamp , A. Goldschmidt , G. Golup , J. G. Gonzalez , D. Góra , D. Grant , P. Gretskov , J. C. Groh , A. Groß , C. Ha , C. Haack , A. Haj Ismail , A. Hallgren , F. Halzen , B. Hansmann , K. Hanson , D. Hebecker , D. Heereman , K. Helbing , R. Hellauer , D. Hellwig , S. Hickford , J. Hignight , G. C. Hill , K. D. Hoffman , R. Hoffmann , K. Holzapfe , A. Homeier , K. Hoshina , F. Huang , M. Huber , W. Huelsnitz , P. O. Hulth , K. Hultqvist , S. In , A. Ishihara , E. Jacobi , G. S. Japaridze , K. Jero , M. Jurkovic , B. Kaminsky , A. Kappes , T. Karg , A. Karle , M. Kauer , A. Keivani , J. L. Kelley , J. Kemp , A. Kheirandish , J. Kiryluk , J. Kläs , S. R. Klein , G. Kohnen , R. Koirala , H. Kolanoski , R. Konietz , A. Koob , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , M. Kowalski , K. Krings , G. Kroll , M. Kroll , J. Kunnen , N. Kurahashi , T. Kuwabara , M. Labare , J. L. Lanfranchi , M. J. Larson , M. Lesiak-Bzdak , M. Leuermann , J. Leuner , J. Lünemann , J. Madsen , G. Maggi , K. B. M. Mahn , R. Maruyama , K. Mase , H. S. Matis , R. Maunu , F. McNally , K. Meagher , M. Medici , A. Meli , T. Menne , G. Merino , T. Meures , S. Miarecki , E. Middell , E. Middlemas , J. Miller , L. Mohrmann , T. Montaruli , R. Morse , R. Nahnhauer , U. Naumann , H. Niederhausen , S. C. Nowicki , D. R. Nygren , A. Obertacke , A. Olivas , A. Omairat , A. O'Murchadha , T. Palczewski , H. Pandya , L. Paul , J. A. Pepper , C. Pérez de los Heros , C. Pfendner , D. Pieloth , E. Pinat , J. Posselt , P. B. Price , G. T. Przybylski , J. Pütz , M. Quinnan , L. Rädel , M. Rameez , K. Rawlins , P. Redl , R. Reimann , M. Relich , E. Resconi , W. Rhode , M. Richman , S. Richter , B. Riedel , S. Robertson , M. Rongen , C. Rott , T. Ruhe , D. Ryckbosch , S. M. Saba , L. Sabbatini , H. -G. Sander , A. Sandrock , J. Sandroos , S. Sarkar , K. Schatto , F. Scheriau , M. Schimp , T. Schmidt , M. Schmitz , S. Schoenen , S. Schöneberg , A. Schönwald , A. Schukraft , L. Schulte , D. Seckel , S. Seunarine , R. Shanidze , M. W. E. Smith , D. Soldin , G. M. Spiczak , C. Spiering , M. Stahlberg , M. Stamatikos , T. Stanev , N. A. Stanisha , A. Stasik , T. Stezelberger , R. G. Stokstad , A. Stößl , E. A. Strahler , R. Ström , N. L. Strotjohann , G. W. Sullivan , M. Sutherland , H. Taavola , I. Taboada , S. Ter-Antonyan , A. Terliuk , G. Tešić , S. Tilav , P. A. Toale , M. N. Tobin , D. Tosi , M. Tselengidou , A. Turcati , E. Unger , M. Usner , S. Vallecorsa , N. van Eijndhoven , J. Vandenbroucke , J. van Santen , S. Vanheule , J. Veenkamp , M. Vehring , M. Voge , M. Vraeghe , C. Walck , M. Wallraff , N. Wandkowsky , Ch. Weaver , C. Wendt , S. Westerhoff , B. J. Whelan , N. Whitehorn , C. Wichary , K. Wiebe , C. H. Wiebusch , L. Wille , D. R. Williams , H. Wissing , M. Wolf , T. R. Wood , K. Woschnagg , D. L. Xu , X. W. Xu , Y. Xu , J. P. Yanez , G. Yodh , S. Yoshida , P. Zarzhitsky , M. Zoll , Eran O. Ofek , Mansi M. Kasliwal , Peter E. Nugent , Iair Arcavi , Joshua S. Bloom , Shrinivas R. Kulkarni , Daniel A. Perley , Tom Barlow , Assaf Horesh , Avishay Gal-Yam , D. A. Howell , Ben Dilday , Phil A. Evans , Jamie A. Kennea , W. S. Burgett , K. C. Chambers , N. Kaiser , C. Waters , H. Flewelling , J. L. Tonry , A. Rest , S. J. Smartt

We present new estimates of the observed rates of SNe determined with the {\em control time} method applied to the files of observations of two long term, photographic SN searches carried out at the Asiago and Sternberg Observatories. Our…

Astrophysics · Physics 2007-05-23 E. Cappellaro , M. Turatto , Benetti , D. Yu. Tsvetkov , O. S. Bartunov , I. N. Makarova

The Sloan Digital Sky Survey-II Supernova Survey has identified a large number of new transient sources in a 300 sq. deg. region along the celestial equator during its first two seasons of a three-season campaign. Multi-band (ugriz) light…

The detection of obscured supernovae (SNe) in near-infrared monitoring campaigns of starburst galaxies has shown that a significant fraction of SNe is missed by optical surveys. However, the number of SNe detected in ground-based near-IR…

Astrophysics · Physics 2009-11-11 G. Cresci , F. Mannucci , M. Della Valle , R. Maiolino

Based on the database compiled in the first article of this series, with 56 SN events discovered in 3838 galaxies of the southern hemisphere, we compute the rate of supernovae (SNe) of different types along the Hubble sequence normalized to…

Cosmology and Nongalactic Astrophysics · Physics 2012-01-17 A. A. Hakobyan , A. R. Petrosian , G. A. Mamon , B. McLean , D. Kunth , M. Turatto , E. Cappellaro , F. Mannucci , R. J. Allen , N. Panagia , M. Della Valle

We calculate the rate per unit volume of hydrogen-poor superluminous supernovae (SLSNe-I) based on the 17 events discovered with the Pan-STARRS1 Medium Deep Survey (PS1 MDS). Two forms of the luminosity function (LF) are assumed : a…

High Energy Astrophysical Phenomena · Physics 2020-09-30 Wen-Chang Zhao , Xiao-Xin Xue , Xiao-Feng Cao

We propose a new strategy of finding strongly-lensed supernovae (SNe) by monitoring known galaxy-scale strong-lens systems. Strongly lensed SNe are potentially powerful tools for the study of cosmology, galaxy evolution, and stellar…

Astrophysics of Galaxies · Physics 2018-09-19 Yiping Shu , Adam S. Bolton , Shude Mao , Xi Kang , Guoliang Li , Monika Soraisam

Near-infrared and radio searches for core-collapse supernovae (CC SNe) in the local universe have shown that the vast majority of the events occurring in massive starburst are missed by the current optical searches as they explode in very…

Astrophysics · Physics 2008-11-26 F. Mannucci , M. Della Valle , N. Panagia

By cross matching blue objects from SDSS with GALEX and the astrometric catalogues USNO-B1.0, GSC2.3 and CMC14, 64 new dwarf nova candidates with one or more observed outbursts have been identified. 14 of these systems are confirmed as…

Solar and Stellar Astrophysics · Physics 2014-11-20 Patrick Wils , Boris T. Gaensicke , Andrew J. Drake , John Southworth

The statistics of SN discoveries is used to reveal selection biases of past and current SN searches and to gain insight on the progenitor scenarios for the different SN types. We also report estimates of the SN rate per unit mass in…

Astrophysics · Physics 2007-05-23 Enrico Cappellaro , Roberto Barbon , Massimo Turatto

Supernovae that are strongly gravitationally lensed (gLSNe) by galaxies are powerful probes of astrophysics and cosmology that will be discovered systematically by next-generation wide-field, high-cadence imaging surveys such as the Zwicky…

Astrophysics of Galaxies · Physics 2019-07-10 Daniel A. Goldstein , Peter E. Nugent , Ariel Goobar

The Pan-STARRS1 (PS1) survey has obtained imaging in 5 bands (grizy_P1) over 10 Medium Deep Survey (MDS) fields covering a total of 70 square degrees. This paper describes the search for apparently hostless supernovae (SNe) within the first…

A search is performed for supernova-like neutrino interactions coincident with 76 gravitational wave events detected by the LIGO/Virgo Collaboration. For 40 of these events, full readout of the time around the gravitational wave is…

High Energy Physics - Experiment · Physics 2023-02-17 M. A. Acero , P. Adamson , L. Aliaga , N. Anfimov , A. Antoshkin , E. Arrieta-Diaz , L. Asquith , A. Aurisano , A. Back , C. Backhouse , M. Baird , N. Balashov , P. Baldi , B. A. Bambah , S. Bashar , K. Bays , R. Bernstein , V. Bhatnagar , B. Bhuyan , J. Bian , J. Blair , A. C. Booth , R. Bowles , C. Bromberg , N. Buchanan , A. Butkevich , S. Calvez , T. J. Carroll , E. Catano-Mur , B. C. Choudhary , A. Christensen , T. E. Coan , M. Colo , L. Corwin , L. Cremonesi , G. S. Davies , P. F. Derwent , P. Ding , Z. Djurcic , M. Dolce , D. Doyle , D. Dueñas Tonguino , E. C. Dukes , H. Duyang , S. Edayath , R. Ehrlich , M. Elkins , E. Ewart , G. J. Feldman , P. Filip , J. Franc , M. J. Frank , H. R. Gallagher , R. Gandrajula , F. Gao , A. Giri , R. A. Gomes , M. C. Goodman , V. Grichine , M. Groh , R. Group , B. Guo , A. Habig , F. Hakl , A. Hall , J. Hartnell , R. Hatcher , A. Hatzikoutelis , H. Hausner , K. Heller , V Hewes , A. Himmel , A. Holin , J. Huang , B. Jargowsky , J. Jarosz , F. Jediny , C. Johnson , M. Judah , I. Kakorin , D. Kalra , D. M. Kaplan , A. Kalitkina , R. Keloth , O. Klimov , L. W. Koerner , L. Kolupaeva , S. Kotelnikov , R. Kralik , Ch. Kullenberg , M. Kubu , A. Kumar , C. D. Kuruppu , V. Kus , T. Lackey , K. Lang , P. Lasorak , J. Lesmeister , S. Lin , A. Lister , J. Liu , M. Lokajicek , S. Magill , M. Manrique Plata , W. A. Mann , M. L. Marshak , M. Martinez-Casales , V. Matveev , B. Mayes , D. P. Méndez , M. D. Messier , H. Meyer , T. Miao , W. H. Miller , S. R. Mishra , A. Mislivec , R. Mohanta , A. Moren , A. Morozova , W. Mu , L. Mualem , M. Muether , S. Mufson , K. Mulder , D. Naples , N. Nayak , J. K. Nelson , R. Nichol , E. Niner , A. Norman , A. Norrick , T. Nosek , H. Oh , A. Olshevskiy , T. Olson , J. Ott , J. Paley , R. B. Patterson , G. Pawloski , O. Petrova , R. Petti , D. D. Phan , R. K. Plunkett , J. C. C. Porter , A. Rafique , F. Psihas , V. Raj , M. Rajaoalisoa , B. Ramson , B. Rebel , P. Rojas , V. Ryabov , O. Samoylov , M. C. Sanchez , S. Sánchez Falero , P. Shanahan , A. Sheshukov , P. Singh , V. Singh , E. Smith , J. Smolik , P. Snopok , N. Solomey , A. Sousa , K. Soustruznik , M. Strait , L. Suter , A. Sutton , S. Swain , C. Sweeney , B. Tapia Oregui , P. Tas , T. Thakore , R. B. Thayyullathil , J. Thomas , E. Tiras , J. Tripathi , J. Trokan-Tenorio , A. Tsaris , Y. Torun , J. Urheim , P. Vahle , Z. Vallari , J. Vasel , P. Vokac , T. Vrba , M. Wallbank , T. K. Warburton , M. Wetstein , D. Whittington , D. A. Wickremasinghe , S. G. Wojcicki , J. Wolcott , W. Wu , Y. Xiao , A. Yallappa Dombara , K. Yonehara , S. Yu , Y. Yu , S. Zadorozhnyy , J. Zalesak , Y. Zhang , R. Zwaska

Distant supernovae can now be detected routinely. To date 34 supernovae at $z > 0.1$ have been discovered. Among them are 12 Type~Ia supernovae confirmed spectroscopically and suited to measure the cosmic deceleration when appropriately…

Astrophysics · Physics 2007-05-23 B. Leibundgut , J. Spyromilio

The Milky Way hosts on average a few supernova explosions per century, yet in the past millennium only five supernovae have been identified confidently in the historical record. This deficit of naked-eye supernovae is at least partly due to…

Solar and Stellar Astrophysics · Physics 2021-09-08 C. Tanner Murphey , Jacob W. Hogan , Brian D. Fields , Gautham Narayan

This review presents a selection of the final results of searches for various exotic physics phenomena in proton-proton collisions at sqrt(s)=7 and 8 TeV delivered by the LHC and collected with the ATLAS and CMS detectors in 2011 (5 fb-1)…

High Energy Physics - Experiment · Physics 2013-01-14 Francesco Santanastasio

We study the detectability of neutrino bursts from nearby direct black hole-forming collapses (failed supernovae) at Megaton detectors. Due to their high energetics, these bursts could be identified - by the time coincidence of N >= 2 or N…

Cosmology and Nongalactic Astrophysics · Physics 2011-10-11 Lili Yang , Cecilia Lunardini

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…