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Revealing the characteristics of the dark GRB 150309A : Dust extinguished or high-z?

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  • معلومة اضافية
    • Contributors:
      Department of Physics
    • بيانات النشر:
      EDP sciences
    • الموضوع:
      2024
    • Collection:
      Helsingfors Universitet: HELDA – Helsingin yliopiston digitaalinen arkisto
    • نبذة مختصرة :
      Peer reviewed
    • File Description:
      application/pdf
    • Relation:
      We thank the anonymous referee for providing constructive and positive comments. This work is based partly on observations carried out with the 10.4 m Gran Telescopio Canarias (GTC) at the Spanish island of La Palma. This work has partially made use of data products from the Two Micron All Sky Survey (2MASS), which is a joint project of the Univ. of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of data obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC) and the Leicester Database and Archive Service (LEDAS), provided by NASA’s Goddard Space Flight Center and the Department of Physics and Astronomy, Leicester University, UK, respectively. R.G. and S.B.P. acknowledge the financial support of ISRO under AstroSat archival Data utilisation program (DS_2B-13013(2)/1/2021-Sec.2). A.J.C.T. acknowledges support from the Spanish Ministry project PID2020-118491GB-I00/AEI/10.13039/501100011033 and Junta de Andalucia grant P20_010168 and from the Severo Ochoa grant CEX2021-001131-S funded by MCIN/AEI/ 10.13039/501100011033. M.C.G. acknowledges support from the Ramón y Cajal Fellowship RYC2019-026465-I (funded by the MCIN/AEI /10.13039/501100011033 and the European Social Funding). Y.D.H. acknowledges support under the additional funding from the RYC2019-026465-I. R.S.-R. acknowledges support under the CSIC-MURALES project with reference 20215AT009. M.G. acknowledges the Academy of Finland project No. 325806. V.A.F. was supported by 075-15-2022-262 (13.MNPMU.21.0003) grant. Research in UrFU is supported by the Program of Development within the Priority-2030.; Castro-Tirado , A J , Gupta , R , Pandey , S B , Guelbenzu , A N , Eikenberry , S , Ackley , K , Gerarts , A , Valeev , A F , Jeong , S , Park , I H , Oates , S R , Zhang , B-B , Sánchez-Ramírez , R , Martín-Carrillo , A , Tello , J C , Jelínek , M , Hu , Y-D , Cunniffe , R , Sokolov , V V , Guziy , S , Ferrero , P , Caballero-García , M D , Ror , A K , Aryan , A , Castro Tirado , M A , Fernández-García , E , Gritsevich , M , Olivares , I , Pérez-García , I , Castro Cerón , J M & Cepa , J 2024 , ' Revealing the characteristics of the dark GRB 150309A : Dust extinguished or high-z? ' , Astronomy and Astrophysics , vol. 683 , A55 . https://doi.org/10.1051/0004-6361/202346042; ORCID: /0000-0003-4268-6277/work/159904011; http://hdl.handle.net/10138/575592; d64192aa-74cb-44ca-b892-6e3381f561b8; 85187136316; 001179670200010
    • Rights:
      cc_by ; info:eu-repo/semantics/openAccess ; openAccess
    • الرقم المعرف:
      edsbas.86DC08B2