NAOC Open IR
GRB 140102A: insight into prompt spectral evolution and early optical afterglow emission
Gupta, Rahul1,2; Oates, S. R.3; Pandey, S. B.1; Castro-Tirado, A. J.4,5; Joshi, Jagdish C.6,7; Hu, Y-D4,8; Valeev, A. F.9,10; Zhang, B. B.6,7; Zhang, Z.6; Kumar, Amit1,11; Aryan, A.1,2; Lien, A.12,13,14; Kumar, B.1; Cui, Ch15; Wang, Ch16; Dimple1,2; Bhattacharya, D.17; Sonbas, E.18; Bai, J.16; Tello, J. C.4; Gorosabel, J.4,19,20; Ceron, J. M. Castro21; Porto, J. R. F.22; Misra, K.1; De Pasquale, M.23; Caballero-Garcia, M. D.4; Jelinek, M.4,24; Kubanek, P.25; Minaev, P. Yu26; Cunniffe, R.4; Sanchez-Ramirez, R.27; Guziy, S.28,29; Jeong, S.4; Tiwari, S. N.2; Razzaque, S.30,31; Bhalerao, V32; Pintado, V. C.33; Sokolov, V. V.9; Zhao, X.16; Fan, Y.16; Xin, Y.16
2021-08-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume505Issue:3Pages:4086-4105
AbstractWe present and perform a detailed analysis of multiwavelength observations of GRB 140102A, an optical bright GRB with an observed reverse shock (RS) signature. Observations of this GRB were acquired with the BOOTES-4 robotic telescope, the Fermi, and the Swift missions. Time-resolved spectroscopy of the prompt emission shows that changes to the peak energy (E-p) tracks intensity and the low-energy spectral index seems to follow the intensity for the first episode, whereas this tracking behaviour is less clear during the second episode. The fit to the afterglow light curves shows that the early optical afterglow can be described with RS emission and is consistent with the thin shell scenario of the constant ambient medium. The late time afterglow decay is also consistent with the prediction of the external forward shock model. We determine the properties of the shocks, Lorentz factor, magnetization parameters, and ambient density of GRB 140102A, and compare these parameters with another 12 GRBs, consistent with having RS produced by thin shells in an interstellar medium like medium. The value of the magnetization parameter (R-B approximate to 18) indicates a moderately magnetized baryonic dominant jet composition for GRB 140102A. We also report the host galaxy photometric observations of GRB 140102A obtained with 10.4m GTC, 3.5 m Calar Alto Astronomical Observatory, and 3.6m Devasthal optical telescope and find the host (photo z = 2.8(-0.9)(+0.7)) to be a high-mass, star-forming galaxy with a star formation rate of 20 +/- 10 M(circle dot)yr(-1).
Keywordshock waves gamma-ray burst: general gamma-ray burst: individual: GRB 140102A methods: observational
Funding OrganizationDepartment of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE ; Department of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE ; Department of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE ; Department of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE
DOI10.1093/mnras/stab1573
WOS KeywordGAMMA-RAY BURST ; REVERSE-SHOCK EMISSION ; LIGHT CURVES ; FERMI-LAT ; PEAK LUMINOSITY ; COMPLETE SAMPLE ; STAR-FORMATION ; HOST GALAXIES ; SWIFT ; LONG
Language英语
Funding ProjectDepartment of Science and Technology (DST), India[DST/IMRCD/BRICS/PilotCall1/ProFCheap/2017(G)] ; Council of Scientific & Industrial Research (CSIR), India ; RFBR[19-02-00311A] ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; DOE[DE-AC02-76SF00515] ; [AYA2012-39727-C03-01]
Funding OrganizationDepartment of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE ; Department of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE ; Department of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE ; Department of Science and Technology (DST), India ; Department of Science and Technology (DST), India ; Council of Scientific & Industrial Research (CSIR), India ; Council of Scientific & Industrial Research (CSIR), India ; RFBR ; RFBR ; Istituto Nazionale di Astrofisica in Italy ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; Centre National d'Etudes Spatiales in France ; DOE ; DOE
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000671481700068
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/76529
Collection中国科学院国家天文台
Corresponding AuthorGupta, Rahul; Pandey, S. B.
Affiliation1.Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263002, Nainital, India
2.Deen Dayal Upadhyaya Gorakhpur Univ, Dept Phys, Gorakhpur 273009, Uttar Pradesh, India
3.Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
4.Inst Astrofis Andalucia IAA CSIC, Glorieta Astron S-N, E-18008 Granada, Spain
5.Univ Malaga, Dept Ingn Sistemas & Automat, Escuela Ingn, C Dr Ortiz Ramos Sn, E-29071 Malaga, Spain
6.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
7.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Peoples R China
8.Univ Granada, Fac Ciencias, Campus Fuentenueva S-N, E-18071 Granada, Spain
9.Russian Acad Sci, Special Astrophys Observ, Nizhniy Arkhyz 369167, Russia
10.Russian Acad Sci, Crimean Astrophys Observ, Nauchnyi 298409, Russia
11.Pandit Ravishankar Shukla Univ, Sch Studies Phys & Astrophys, Raipur 492010, Madhya Pradesh, India
12.Ctr Res & Explorat Space Sci & Technol CRESST, Greenbelt, MD 20771 USA
13.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
14.Univ Maryland Baltimore Cty, Dept Phys, 1000 Hilltop Circle, Baltimore, MD 21250 USA
15.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
16.Chinese Acad Sci, Yunnan Natl Astron Observ, Phoenix Hill, Kunming 650011, Yunnan, Peoples R China
17.Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
18.Adiyaman Univ, Dept Phys, TR-02040 Adiyaman, Turkey
19.Univ Pais Vasco UPV EHU, Unidad Asociada Grp Ciencias Planetarias UPV EHU, Dept Fis Aplicada 1, ETS, E-48013 Bilbao, Spain
20.Basque Fdn Sci, Ikerbasque, E-48008 Bilbao, Spain
21.European Space Astron Ctr ESA ESAC, Camino Bajo del Castillo S-N, E-28692 Villanueva Dela Canada, Madrid, Spain
22.Univ Int Valenciana, Dept Sci, Valencia 46021, Spain
23.Istanbul Univ, Astron & Space Sci Dept, TR-34119 Istanbul, Turkey
24.Czech Acad Sci ASU CAS, Astron Inst, Fricova 298, CZ-25165 Ondrejov, Czech Republic
25.Fyzikalni Ustav AV CR, Na Slovance 2, CZ-18221 Prague 8, Czech Republic
26.Russian Acad Sci IKI, Space Res Inst, 84-32 Profsoyuznaya Str, Moscow 117997, Russia
27.Ist Astrofis & Planetol Spaziali, INAF, Via Fosso del Cavaliere 100, I-00133 Rome, Italy
28.Nikolaev Natl Univ, Nikolska 24, UA-54030 Nikolayev, Ukraine
29.Nikolaev Astron Observ, UA-54030 Nikolayev, Ukraine
30.Univ Johannesburg, Ctr Astroparticle Phys CAPP, POB 524, ZA-2006 Auckland Pk, South Africa
31.Univ Johannesburg, Dept Phys, POB 524, ZA-2006 Auckland Pk, South Africa
32.Indian Inst Technol, Dept Phys, Mumbai 400076, Maharashtra, India
33.Inst Educ Secundaria Beniajan, Dept Matemat, Avda Monteazahar 17, E-30570 Murcia, Spain
Recommended Citation
GB/T 7714
Gupta, Rahul,Oates, S. R.,Pandey, S. B.,et al. GRB 140102A: insight into prompt spectral evolution and early optical afterglow emission[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,505(3):4086-4105.
APA Gupta, Rahul.,Oates, S. R..,Pandey, S. B..,Castro-Tirado, A. J..,Joshi, Jagdish C..,...&Xin, Y..(2021).GRB 140102A: insight into prompt spectral evolution and early optical afterglow emission.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,505(3),4086-4105.
MLA Gupta, Rahul,et al."GRB 140102A: insight into prompt spectral evolution and early optical afterglow emission".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 505.3(2021):4086-4105.
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