Por favor, use este identificador para citar o enlazar a este item:
http://hdl.handle.net/10261/211738
COMPARTIR / EXPORTAR:
SHARE CORE BASE | |
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE | |
Campo DC | Valor | Lengua/Idioma |
---|---|---|
dc.contributor.author | Zhao, Y. | - |
dc.contributor.author | Zhang, B. B. | - |
dc.contributor.author | Xiong, S.L. | - |
dc.contributor.author | Long, X. | - |
dc.contributor.author | Zhang, Q. | - |
dc.contributor.author | Song, L.M. | - |
dc.contributor.author | Sun, J.C. | - |
dc.contributor.author | Wang, Y.H. | - |
dc.contributor.author | Li, H.C. | - |
dc.contributor.author | Bu, Q.C. | - |
dc.contributor.author | Feng, M.Z. | - |
dc.contributor.author | Li, Z.H. | - |
dc.contributor.author | Wen, X. | - |
dc.contributor.author | Wu, B.B. | - |
dc.contributor.author | Zhang, L.Y. | - |
dc.contributor.author | Zhang, Y. J. | - |
dc.contributor.author | Zhang, S. N. | - |
dc.contributor.author | Shao, J. X. | - |
dc.date.accessioned | 2020-05-20T11:16:29Z | - |
dc.date.available | 2020-05-20T11:16:29Z | - |
dc.date.issued | 2018 | - |
dc.identifier | doi: 10.1088/1674-4527/18/5/57 | - |
dc.identifier | issn: 1674-4527 | - |
dc.identifier.citation | Research in Astronomy and Astrophysics 18(5): 5i (2018) | - |
dc.identifier.uri | http://hdl.handle.net/10261/211738 | - |
dc.description | 14 pages, 8 figures. The paper has been accepted by Research in Astronomy and Astrophysics (RAA) | - |
dc.description.abstract | Rapid response and short time latency are very important for Time Domain Astronomy, such as the observations of Gamma-ray Bursts (GRBs) and electromagnetic (EM) counterparts of gravitational waves (GWs). Based on near real-time Fermi/GBM data, we developed a low-latency pipeline to automatically calculate the temporal and spectral properties of GRBs. With this pipeline, some important parameters can be obtained, such as T and fluence, within ∼ 20 min after the GRB trigger. For ∼ 90% of GRBs, T and fluence are consistent with the GBM catalog results within 2σ errors. This pipeline has been used by the Gamma-ray Bursts Polarimeter (POLAR) and the Insight Hard X-ray Modulation Telescope (Insight-HXMT) to follow up the bursts of interest. For GRB 170817A, the first EM counterpart of GW events detected by Fermi/GBM and INTEGRAL/SPI-ACS, the pipeline gave T and spectral information 21 min after the GBM trigger, providing important information for POLAR and Insight-HXMT observations. © 2018 National Astronomical Observatories, CAS and IOP Publishing Ltd.. | - |
dc.description.sponsorship | We thank the anonymous reviewer for helpful comments and suggestions. This work is supported by the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDB23040400), the National Natural Science Foundation of China (Grant Nos. 11403026, 11503028 and 11673023) and the National Basic Research Program of China (973 program, Grant No. 2014CB845800). BBZ acknowledges support from the National Thousand Young Talents programof China. We gratefully acknowledge support from the collaboration team of POLAR, a project funded by China National Space Administration (CNSA), the Chinese Academy of Sciences (CAS) and the University of Geneva (UNIGE). The authors would also like to thank Jing Jin, Jinlu Qu, Xiaobo Li, Youli Tuo, Zijian Li, Mingyu Ge, Jinyuan Liao, Guangcheng Xiao, Yue Huang and Chengkui Li for their suggestions on data analysis and the revision of this paper. | - |
dc.language | eng | - |
dc.publisher | IOP Publishing | - |
dc.relation.isversionof | Postprint | - |
dc.rights | openAccess | - |
dc.subject | Gamma-ray bursts: general | - |
dc.subject | Polarization | - |
dc.subject | Radiation mechanisms: non-thermal | - |
dc.title | A low-latency pipeline for GRB light curve and spectrum using Fermi/GBM near real-time data | - |
dc.type | artículo | - |
dc.identifier.doi | 10.1088/1674-4527/18/5/57 | - |
dc.relation.publisherversion | http://dx.doi.org/10.1088/1674-4527/18/5/57 | - |
dc.date.updated | 2020-05-20T11:16:29Z | - |
dc.contributor.funder | Chinese Academy of Sciences | - |
dc.contributor.funder | National Basic Research Program (China) | - |
dc.contributor.funder | National Thousand Young Talents program of China | - |
dc.relation.csic | Sí | - |
dc.identifier.funder | http://dx.doi.org/10.13039/501100002367 | es_ES |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.openairetype | artículo | - |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
Aparece en las colecciones: | (IAA) Artículos |
Ficheros en este ítem:
Fichero | Descripción | Tamaño | Formato | |
---|---|---|---|---|
IAA_2018RAA_a_low-latency.pdf | 653,4 kB | Adobe PDF | Visualizar/Abrir |
CORE Recommender
SCOPUSTM
Citations
4
checked on 13-abr-2024
WEB OF SCIENCETM
Citations
3
checked on 18-feb-2024
Page view(s)
100
checked on 19-abr-2024
Download(s)
135
checked on 19-abr-2024
Google ScholarTM
Check
Altmetric
Altmetric
NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.