Tomasz Bulik
University of Warsaw
780 Papers
12K Citations
Tomasz Bulik is an academic researcher from University of Warsaw. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 121, co-authored 698 publications. Previous affiliations of Tomasz Bulik include Jagiellonian University & Paris Observatory.
Chat about Author
Papers
The NoEMi (Noise Frequency Event Miner) framework
T. Accadia,Fausto Acernese,M. Agathos,P. Astone,G. Ballardin,Fabrizio Barone,M. Barsuglia,A. Basti,Th. S. Bauer,M. Bebronne,Michał Bejger,M. G. Beker,M. Bitossi,M. A. Bizouard,M. Blom,François Bondu,L. Bonelli,R. Bonnand,V. Boschi,L. Bosi,B. Bouhou,S. Braccini,C. Bradaschia,M. Branchesi,Gabriel Chardin T. Briant,A. Brillet,V. Brisson,Tomasz Bulik,H. J. Bulten,D. Buskulic,Christelle Lesvigne-Buy,Enrico Calloni,Benjamin Canuel,F. Carbognani,F. Cavalier,R. Cavalieri,G. Cella,Elena Cesarini,O. Chaibi,E. Chassande-Mottin,Andrea Chincarini,A. Chiummo,F. Cleva,E. Coccia,P. F. Cohadon,C. N. Colacino,J. Colas,A. Colla,M. Colombini,A. Conte,J.-P. Coulon,E. Cuoco,S. D'Antonio,V. Dattilo,M. Davier,R. Day,R. De Rosa,G. Debreczeni,W. Del Pozzo,L. Di Fiore,A. Di Lieto,M. Di Paolo Emilio,A. Di Virgilio,A. Dietz,M. Drago,G. Endroczi,V. Fafone,I. Ferrante,F. Fidecaro,I. Fiori,R. Flaminio,L. A. Forte,J.-D. Fournier,J. Franc,Stefaan Franco,S. Frasca,F. Frasconi,M. Galimberti,Luca Gammaitoni,F. Garufi,M. E. Gáspár,G. Gemme,E. Genin,A. Gennai,A. Giazotto,R. Gouaty,M. Granata,C. Greverie,G. M. Guidi,J.-F. Hayau,Antoine Heidmann,H. Heitmann,P. Hello,G. Hemming,Piotr Jaranowski,R. J. G. Jonker,M. Kasprzack,I. Kowalska,A. Królak,N. Leroy,N. Letendre,Tenglin Li,N. Liguori,M. Lorenzini,V. Loriette,G. Losurdo,Ettore Majorana,I. Maksimovic,V. Malvezzi,N. Man,M. Mantovani,Fabio Marchesoni,F. Marion,J. Marque,F. Martelli,A. Masserot,Christine Michel,Leopoldo Milano,Y. Minenkov,M. Mohan,N. Morgado,A. Morgia,S. Mosca,B. Mours,L. Naticchioni,F. Nocera,L. Palladino,C. Palomba,F. Paoletti,R. Paoletti,M. Parisi,A. Pasqualetti,R. Passaquieti,D. Passuello,Gianluca Persichetti,F. Piergiovanni,M. Pietka,L. Pinard,Rosa Poggiani,Mirko Prato,G. A. Prodi,M. Punturo,P. Puppo,D. S. Rabeling,István Rácz,P. Rapagnani,V. Re,T. Regimbau,F. Ricci,F. Robinet,A. Rocchi,L. Rolland,Rocco Romano,D. Rosińska,P. Ruggi,B. Sassolas,D. Sentenac,L. Sperandio,Riccardo Sturani,B. L. Swinkels,M. Tacca,L. Taffarello,A. P. M. ter Braack,Alessandra Toncelli,M. Tonelli,O. Torre,E. Tournefier,F. Travasso,G. Vajente,J. F. J. van den Brand,C. Van Den Broeck,S. Van Der Putten,M. Vasúth,M. Vavoulidis,G. Vedovato,D. Verkindt,F. Vetrano,A. Viceré,J. Y. Vinet,S. Vitale,H. Vocca,R. L. Ward,M. Was,Kazuhiro Yamamoto,M. Yvert,A. Zadroźny,J. P. Zendri +186 more
- 01 Jun 2012
TL;DR: The NoEMi (Noise Frequency Event Miner) framework as mentioned in this paper exploits some of the algorithms implemented for the continuous gravitational wave (CW) studies to identify, on a daily basis, the frequency lines observed in the Virgo science data and in a subset of the environmental sensors, looking for lines that match in frequency.
•Journal Article
Rapidly rotating compact strange stars
Dorota Gondek-Rosińska,Tomasz Bulik,Eric Gourgoulhon,Jishnu Dey,Subharthi Ray,L. Zdunik,Mira Dey +6 more
TL;DR: In this article, Dey et al. compute numerical, relativistic models of uni-formly rotating stars for the recently proposed QCD-based equation of state (EOS) of strange quark matter.
H.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloud
A. Abramowski,Felix Aharonian,Felix Aharonian,Felix Aharonian,F. Ait Benkhali,A. G. Akhperjanian,A. G. Akhperjanian,E. O. Angüner,Michael Backes,S. Balenderan,A. Balzer,Anna Barnacka,Anna Barnacka,Yvonne Becherini,J. Becker Tjus,David Berge,S. Bernhard,Konrad Bernlöhr,Konrad Bernlöhr,E. Birsin,J. Biteau,J. Biteau,Markus Böttcher,Catherine Boisson,J. Bolmont,Pol Bordas,Johan Bregeon,Francois Brun,Pierre Brun,M. Bryan,Tomasz Bulik,Svenja Carrigan,Sabrina Casanova,P. M. Chadwick,Nachiketa Chakraborty,R. Chalme-Calvet,R. C. G. Chaves,M. Chrétien,S. Colafrancesco,G. Cologna,Jan Conrad,C. Couturier,Y. Cui,I. D. Davids,I. D. Davids,B. Degrange,Christoph Deil,P. deWilt,A. Djannati-Ataï,W. Domainko,Axel Donath,L. O'c. Drury,Guillaume Dubus,K. Dutson,J. Dyks,Michal Dyrda,Tanya Edwards,Kathrin Egberts,Peter Eger,P. Espigat,C. Farnier,S. J. Fegan,F. Feinstein,M. V. Fernandes,D. Fernandez,A. Fiasson,G. Fontaine,A. Förster,M. Füßling,Stefano Gabici,M. Gajdus,Y. A. Gallant,T. Garrigoux,Gianluca Giavitto,B. Giebels,J. F. Glicenstein,D. Gottschall,M.-H. Grondin,M. Grudzińska,Daniela Hadasch,S. Häffner,Joachim Hahn,J. Harris,G. Heinzelmann,Gilles Henri,G. Hermann,Olivier Hervet,Andreas Hillert,Jim Hinton,Werner Hofmann,Petter Hofverberg,M. Holler,Dieter Horns,A. Ivascenko,A. Jacholkowska,C. Jahn,Marek Jamrozy,Mateusz Janiak,Felix Jankowsky,I. Jung-Richardt,M. A. Kastendieck,K. Katarzyński,Uli Katz,Sarah Kaufmann,B. Khélifi,M. Kieffer,S. Klepser,D. Klochkov,W. Kluźniak,D. Kolitzus,Nu. Komin,Karl Kosack,S. Krakau,F. Krayzel,P. P. Krüger,H. Laffon,G. Lamanna,Julien Lefaucheur,V. Lefranc,Anne Lemiere,Marianne Lemoine-Goumard,J.-P. Lenain,Thomas Lohse,A. Lopatin,Chia-Chun Lu,Vincent Marandon,Alexandre Marcowith,Ramin Marx,G. Maurin,N. Maxted,M. Mayer,T. J. L. McComb,J. Méhault,P. J. Meintjes,U. Menzler,Manuel Meyer,Alison Mitchell,R. Moderski,M. Mohamed,K. Morå,Emmanuel Moulin,Thomas Murach,M. de Naurois,Jacek Niemiec,S. J. Nolan,L. Oakes,H. Odaka,Stefan Ohm,B. Opitz,Michał Ostrowski,Igor Oya,M. Panter,R. D. Parsons,M. Paz Arribas,N. W. Pekeur,G. Pelletier,P.-O. Petrucci,B. Peyaud,S. Pita,Helen Poon,G. Pühlhofer,Michael Punch,Andreas Quirrenbach,S. Raab,Ignasi Reichardt,A. Reimer,Olaf Reimer,M. Renaud,R. de los Reyes,Frank M. Rieger,C. Romoli,S. Rosier-Lees,Gavin Rowell,B. Rudak,C. B. Rulten,V. Sahakian,V. Sahakian,David Salek,D. A. Sanchez,Andrea Santangelo,Reinhard Schlickeiser,F. Schüssler,André Schulz,Ullrich Schwanke,S. Schwarzburg,S. Schwemmer,Helene Sol,Felix Spanier,G. Spengler,F. Spies,Łukasz Stawarz,R. Steenkamp,C. Stegmann,F. Stinzing,K. Stycz,Iurii Sushch,Iurii Sushch,J.-P. Tavernet,T. Tavernier,Andrew M. Taylor,Regis Terrier,M. Tluczykont,C. Trichard,K. Valerius,C. van Eldik,B. van Soelen,G. Vasileiadis,J. Veh,Christo Venter,Aion Viana,P. Vincent,Jacco Vink,Heinrich J. Völk,Francesca Volpe,M. J. Vorster,T. Vuillaume,Stefan Wagner,P. Wagner,Robert Wagner,Martin Ward,Matthias Weidinger,Quirin Weitzel,R. White,Alicja Wierzcholska,P. Willmann,A. Wörnlein,Denis Wouters,Ruizhi Yang,Victor Zabalza,Victor Zabalza,D. Zaborov,Michael Zacharias,A. A. Zdziarski,A. Zech,H.-S. Zechlin +234 more
TL;DR: In this article, a gamma-ray supernova remnant (G349.2) was detected at the distance of 11.5 kpc and observed across the entire electromagnetic spectrum from radio to high energy (HE; 0.7+0.1 GeV 100 GeV).
Initial Populations of Black Holes in Star Clusters
TL;DR: In this article, the formation and evolution of binary X-ray binaries in and around star clusters was investigated. But the authors focused on the formation of BH-BH binaries.
H.E.S.S. discovery of VHE γ-rays from the quasar PKS 1510−089
A. Abramowski,Fabio Acero,Felix Aharonian,Felix Aharonian,Felix Aharonian,A. G. Akhperjanian,A. G. Akhperjanian,Gisela Anton,S. Balenderan,A. Balzer,Anna Barnacka,Yvonne Becherini,Yvonne Becherini,J. Becker Tjus,B. Behera,Konrad Bernlöhr,Konrad Bernlöhr,E. Birsin,J. Biteau,A. Bochow,Catherine Boisson,J. Bolmont,Pol Bordas,J. Brucker,Francois Brun,Pierre Brun,Tomasz Bulik,Svenja Carrigan,Sabrina Casanova,Sabrina Casanova,Matteo Cerruti,P. M. Chadwick,R. C. G. Chaves,R. C. G. Chaves,A. Cheesebrough,S. Colafrancesco,G. Cologna,Jan Conrad,C. Couturier,M. Dalton,M. Dalton,M. K. Daniel,I. D. Davids,B. Degrange,Christoph Deil,P. deWilt,Hugh Dickinson,A. Djannati-Ataï,W. Domainko,L. O'c. Drury,Guillaume Dubus,K. Dutson,J. Dyks,Michal Dyrda,Kathrin Egberts,Peter Eger,P. Espigat,L. Fallon,C. Farnier,S. J. Fegan,F. Feinstein,M. V. Fernandes,D. Fernandez,A. Fiasson,G. Fontaine,A. Förster,M. Füßling,M. Gajdus,Y. A. Gallant,T. Garrigoux,Henning Gast,B. Giebels,J. F. Glicenstein,B. Glück,D. Göring,M. H. Grondin,M. H. Grondin,M. Grudzińska,S. Häffner,J. D. Hague,Joachim Hahn,D. Hampf,J. Harris,M. Hauser,S. Heinz,G. Heinzelmann,Gilles Henri,G. Hermann,Andreas Hillert,Jim Hinton,Werner Hofmann,Petter Hofverberg,M. Holler,Dieter Horns,A. Jacholkowska,C. Jahn,Marek Jamrozy,I. Jung,M. A. Kastendieck,K. Katarzyński,U. F. Katz,S. Kaufmann,B. Khélifi,S. Klepser,D. Klochkov,W. Kluźniak,T. Kneiske,D. Kolitzus,Nu. Komin,Karl Kosack,R. Kossakowski,F. Krayzel,P.P. Krüger,P.P. Krüger,H. Laffon,G. Lamanna,Julien Lefaucheur,Marianne Lemoine-Goumard,J.-P. Lenain,Dirk Lennarz,Thomas Lohse,A. Lopatin,Chia-Chun Lu,Vincent Marandon,Alexandre Marcowith,Julien Masbou,G. Maurin,N. Maxted,M. Mayer,T. J. L. McComb,M. C. Medina,J. Mehault,J. Mehault,U. Menzler,R. Moderski,M. Mohamed,Emmanuel Moulin,C. L. Naumann,M. Naumann-Godo,M. de Naurois,D. Nedbal,N. Nguyen,Jacek Niemiec,S. J. Nolan,Stefan Ohm,Stefan Ohm,E. de Oña Wilhelmi,B. Opitz,Michał Ostrowski,I. Oya,M. Panter,R. D. Parsons,M. Paz Arribas,N. W. Pekeur,Guy Pelletier,J. Perez,Pierre-Olivier Petrucci,B. Peyaud,S. Pita,G. Pühlhofer,Michael Punch,Andreas Quirrenbach,S. Raab,Martin Raue,A. Reimer,Olaf Reimer,M. Renaud,R. de los Reyes,Frank M. Rieger,Joachim Ripken,L. Rob,S. Rosier-Lees,Gavin Rowell,B. Rudak,Cameron B Rulten,V. Sahakian,V. Sahakian,Daniel Sánchez,Andrea Santangelo,Reinhard Schlickeiser,André Schulz,Ullrich Schwanke,S. Schwarzburg,S. Schwemmer,F. Sheidaei,F. Sheidaei,J. L. Skilton,Helene Sol,G. Spengler,Łukasz Stawarz,R. Steenkamp,C. Stegmann,F. Stinzing,K. Stycz,Iurii Sushch,Anna Szostek,J.-P. Tavernet,Regis Terrier,M. Tluczykont,C. Trichard,K. Valerius,C. van Eldik,C. van Eldik,G. Vasileiadis,Christo Venter,A. Viana,A. Viana,P. Vincent,Heinrich J. Völk,Francesca Volpe,S. Vorobiov,M. J. Vorster,Stefan Wagner,Martin Ward,R. White,Alicja Wierzcholska,Denis Wouters,Michael Zacharias,Anna Zajczyk,A. A. Zdziarski,A. Zech,H.-S. Zechlin +221 more
TL;DR: In this article, a very high energy (VHE) emission from the quasar PKS 1510−089 (z = 0.361) was detected with a statistical significance of 9.2 standard deviations in 15.8 h of H.E.S. data taken during March and April 2009.