H.E.S.S. Observations of the Gamma-ray Binary LMC P3 Leonard Everett Fisher , F. Aharonian , Faical Ait-Benkhali , Attila Alkan , Jann Aschersleben , Halim Ashkar , Michael Backes , Ali Baktash , Victor Barbosa Martins , A. Barnacka , Joleen Barnard , Rowan William Batzofin , Y. Becherini , Geoffrey Beck , D. Berge , K. Bernloehr , Baiyang Bi , Markus Boettcher , C. Boisson , J. Bolmont , Mathieu Bony , Jowita Borowska , Makarim Bouyahiaoui , Federica Bradascio , M. Breuhaus , Robert Brose , A. M. Brown , F. Brun , Benedetta Bruno , T. Bulik , Christopher Burger-Scheidlin , Thomas Bylund , F. Cangemi , Sami Caroff , S. Casanova , Rahul Cecil , Jelena Celic , M. Cerruti , Pauline Chambéry , T. Chand , S. Chandra , Andrew Chen , James O. Chibueze , Ogochukwu Chibueze , Tiffany Collins , G. Cotter , Pierre Cristofari , J. Damascene Mbarubucyeye , I. D. Davids , J. Davies , Laenita de Jonge , J. Devin , A. Djannati-Ataı̈ , A. Dmytriiev , Victor Doroshenko , Lenté Dreyer , Louis Du Plessis , K. Egberts , S. Einecke , J.-P. Ernenwein , S. J. Fegan , Kirsty Feijen , Gaëtan Fichet de Clairfontaine , G. Fontaine , Lott Frans , Matthias Fuessling , S. Funk , S. Gabici , Y. A. Gallant , Shahede Ghafourizadeh , G. Giavitto , Luca Giunti , D. Glawion , J. F. Glicenstein , Jonas Glombitza , Pranjupriya Goswami , Guillaume Grolleron , M.-H. Grondin , Lucia Haerer , Sumari Hattingh , M. Haupt , G. Hermann , J. A. Hinton , W. Hofmann , T.L. Holch , M. Holler , D. Horns , Zhiqiu Huang , Annanay Jaitly , M. Jamrozy , F. Jankowsky , A. Jardin-Blicq , Vikas Joshi , I. Jung-Richardt , E. Kasai , K. Katarzyński , Hiiko Katjaita , D. Khangulyan , Rukaiya Khatoon , B. Khélifi , S. Klepser , W. Kluźniak , Nu. Komin , Ruslan Konno , K. Kosack , D. Kostunin , A. Kundu , G. Lamanna , Rodrigo Guedes Lang , S. Le Stum , V. Lefranc , Franziska Leitl , A. Lemière , M. Lemoine‐Goumard , Jean-Philippe Lenain , Fabian Leuschner , Anna Luashvili , I. Lypova , Jonathan Mackey , Denys Malyshev , Dmitry Malyshev , V. Marandon , A. Marcowith , Peter David Marinos , Guillem Marti'i-Devesa , R. Marx , G. Maurin , Abhay Mehta , Pieter Meintjes , Manuel Meyer , Alison Mitchell , R. Moderski , L. Mohrmann , A. Montanari , Chris Moore , Emmanuel Moulin , T. Murach , Kaori Nakashima , M. de Naurois , H. Ndiyavala , J. Niemiec , A. Priyana Noel , P. T. O’Brien , S. Ohm , Laura Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , Enzo Oukacha , Sebastian Panny , M. Panter , D. R. Parsons , Ugo Pensec , Giada Peron , S. Pita , V. Poireau , Dmitry Prokhorov , H. Prokoph , G. Puehlhofer , M. Punch , A. Quirrenbach , Maxime Regeard , Patrick Reichherzer , O. Reimer , Igor Adriano de Oliveira Reis , Quentin Rémy , Helena X. Ren , M. Renaud , Brian Reville , Frank Rieger , Gerrit Roellinghoff , E. Rol , Gavin Rowell , B. Rudak , Hector Rueda Ricarte , Edna Ruiz Velasco , Karim Sabri , V. Sahakian , Simon Sailer , Heiko Salzmann , David Sánchez , A. Santangelo , M. Sasaki , Johannes Schaefer , F. Schuessler , Hester Schutte , M. Senniappan , Jimmy N.S. Shapopi , Sigrid Shilunga , K. Shiningayamwe , H. Sol , Hugh Spackman , Andreas Specovius , S. Spencer , Ł. Stawarz , R. Steenkamp , C. Stegmann , Simon Steinmassl , C. Steppa , Katrin Streil , I. Sushch , Hiromasa Suzuki , Tadayuki Takahashi , Takaaki Tanaka , T. Tavernier , Andrew M. Taylor , R. Terrier , Adnaan Thakur , Hannes Thiersen , Charles Thorpe-Morgan , M. Tluczykont , M. Tsirou , Naomi Tsuji , R. Tuffs , Y. Uchiyama , Marion Ullmo , Tim Unbehaun , Pieter van der Merwe , C. van Eldik , B. van Soelen , G. Vasileiadis , M. Vecchi , J. Veh , C. Venter , Jacco Vink , H. J. Voêlk , Naomi Vogel , Tina Wach , S. J. Wagner , Félix Werner , R. White , A. Wierzcholska , Yu Wun Wong , Hend Mahmoud Yassin , M. Zacharias , Davit Zargaryan , Andrzej Zdziarski , A. Zech , Sylvia Zhu , Andreas Zmija , Samuel Zouari , Natalia Żywucka openalex（2023）
摘要
LMC P3 is a gamma-ray binary comprising of an unconfirmed compact object and an O-star and is located in the Large Magellanic Cloud.Initially discovered in Fermi-LAT data, it shows an orbital period of 10.3 days.H.E.S.S. has reported the detected VHE gamma-ray emission during only 20% of the orbit, between orbital phases 0.2 and 0.4, which roughly corresponds to the inferior conjunction of the compact object.H.E.S.S. has continued the observations of this object since then.Here we will present new results obtained with a much deeper data set.The new data allow a more precise measurement of the location of the VHE gamma-ray peak along the orbit of the system to be made.We will interpret these results with respect to emission and absorption mechanisms in gamma-ray binary systems.
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