T. Ch
1 Papers
T. Ch is an academic researcher. The author has contributed to research in topics: Pulsar & Electromagnetic spectrum. The author has an hindex of 1, co-authored 1 publications.
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Papers
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Resolving the Crab pulsar wind nebula at teraelectronvolt energies
H. Abdalla,Felix Aharonian,F. Ait Benkhali,E. O. Angüner,Masanori Arakawa,C. Arcaro,Michael Backes,Monica Barnard,Yvonne Becherini,J. Becker Tjus,D. Berge,Konrad Bernlöhr,R. Blackwell,Markus Böttcher,Catherine Boisson,J. Bolmont,S. Bonnefoy,P. Bordas,J. Bregeon,Francois Brun,Pierre Brun,M. Bryan,M. Büchele,Tomasz Bulik,T. Bylund,M. Capasso,S. Caroff,A. Carosi,Sabrina Casanova,Matteo Cerruti,Nachiketa Chakraborty,T. Ch,S. Ch,R. C. G. Chaves,A. W. Chen,S. Colafrancesco,B. Condon,I.D. Davids,Christoph Deil,J. Devin,P. deWilt,L. Dirson,A. Djannati-Ataï,A. Dmytriiev,Axel Donath,Victor Doroshenko,L. O'c. Drury,J. Dyks,K. Egberts,G. Emery,J.-P. Ernenwein,S. Eschbach,S. Fegan,A. Fiasson,G. Fontaine,Stefan Funk,M. Füßling,S. Gabici,Y.A. Gallant,F. Gaté,Gianluca Giavitto,D. Glawion,J.F. Glicenstein,D. Gottschall,M.-H. Grondin,J. Hahn,M. Haupt,G. Heinzelmann,G. Henri,G. Hermann,Jim Hinton,Werner Hofmann,C. Hoischen,Tim Holch,M. Holler,Dieter Horns,D. Huber,H. Iwasaki,A. Jacholkowska,Marek Jamrozy,D. Jankowsky,F. Jankowsky,Léa Jouvin,I. Jung-Richardt,M.A. Kastendieck,K. Katarzyński,M. Katsuragawa,U. Katz,Dmitry Khangulyan,B. Khélifi,J. King,S. Klepser,W. Kluźniak,Nu. Komin,K. Kosack,M. Kraus,G. Lamanna,J. Lau,Julien Lefaucheur,A. Lemière,M. Lemoine-Goumard,J.-P. Lenain,E. Leser,T. Lohse,R. López-Coto,I. Lypova,Denys Malyshev,V. Mar,A. Marcowith,C. Mariaud,G. Martí-Devesa,R. Marx,G. Maurin,P.J. Meintjes,Alison Mitchell,R. Moderski,M. Mohamed,L. Mohrmann,Christopher J. Moore,E. Moulin,Thomas Murach,S. Nakashima,M. de Naurois,H. Ndiyavala,F. Niederwanger,Jacek Niemiec,L. Oakes,P. T. O'Brien,H. Odaka,Stefan Ohm,M. Ostrowski,I. Oya,M. Panter,R. D. Parsons,C. Perennes,P.-O. Petrucci,B. Peyaud,Q. Piel,S. Pita,V. Poireau,A. Priyana Noel,D. A. Prokhorov,Heike Prokoph,G. Pühlhofer,Michael Punch,Andreas Quirrenbach,S. Raab,R. Rauth,A. Reimer,Olaf Reimer,M. Renaud,Frank M. Rieger,L. Rinchiuso,Carlo Romoli,Gavin Rowell,B. Rudak,E. Ruiz-Velasco,V. Sahakian,S. Saito,D. A. Sanchez,Andrea Santangelo,Manami Sasaki,Reinhard Schlickeiser,F. Schüssler,A. Schulz,H. M. Schutte,Ullrich Schwanke,S. Schwemmer,M. Seglar-Arroyo,Mohanraj Senniappan,A.S. Seyffert,N. Shafi,I. Shilon,K. Shiningayamwe,R. Simoni,Atreyee Sinha,Helene Sol,A. Specovius,M. Spir-Jacob,Ł. Stawarz,R. Steenkamp,C. Stegmann,C. Steppa,T. Takahashi,J.-P. Tavernet,T. Tavernier,A.M. Taylor,Regis Terrier,D. Tiziani,M. Tluczykont,C. Trichard,M. Tsirou,N. Tsuji,R. Tuffs,Yasunobu Uchiyama,D. J. van der Walt,C. van Eldik,C. van Rensburg,B. van Soelen,G. Vasileiadis,J. Veh,Christo Venter,P. Vincent,Jacco Vink,F. Voisin,Heinrich J. Völk,T. Vuillaume,Zorawar Wadiasingh,Stefan Wagner,Robert Wagner,R. J. White,A. Wierzcholska,Ruizhi Yang,H. Yoneda,D. Zaborov,M. Zacharias,R. Zanin,A.A. Zdziarski,A. Zech,A. Ziegler,J. Zorn,Natalia Żywucka +221 more
TL;DR: In this article, it was shown that the Crab nebula has an angular extension at gamma-ray energies of 52 arcseconds (assuming a Gaussian source width), significantly larger than at X-ray energy.