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Article: Prospects for grb science with the fermi large area telescope

TitleProspects for grb science with the fermi large area telescope
Authors
Band, DLAxelsson, MBaldini, LBarbiellini, GBaring, MGBastieri, DBattelino, MBellazzini, RBissaldi, EBogaert, GBonnell, JChiang, JCohenTanugi, JConnaughton, VCutini, SDe Palma, FDingus, BLDo Couto E Silva, EFishman, GGalli, AGehrels, NGiglietto, NGranot, JGuiriec, SHughes, REKamae, TKomin, NKuehn, FKuss, MLongo, FLubrano, PKippen, RMMazziotta, MNMcenery, JEMcglynn, SMoretti, ENakamori, TNorris, JPOhno, MOlivo, MOmodei, NPelassa, VPiron, FPreece, RRazzano, MRussell, JJRyde, FSaz Parkinson, PMScargle, JDSgrò, CShimokawabe, TSmith, PDSpandre, GSpinelli, PStamatikos, MWiner, BLYamazaki, R
KeywordsGamma Rays: Bursts
Issue Date2009
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2009, v. 701 n. 2, p. 1673-1694 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/701/2/1673
AbstractThe Large Area Telescope (LAT) instrument on the Fermi mission will reveal the rich spectral and temporal gamma-ray burst (GRB) phenomena in the >100 MeV band. The synergy with Fermi's Gamma-ray Burst Monitor detectors will link these observations to those in the well explored 10-1000keV range; the addition of the >100 MeV band observations will resolve theoretical uncertainties about burst emission in both the prompt and afterglow phases. Trigger algorithms will be applied to the LAT data both onboard the spacecraft and on the ground. The sensitivity of these triggers will differ because of the available computing resources onboard and on the ground. Here we present the LAT's burst detection methodologies and the instrument's GRB capabilities. © 2009 The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188369
ISSN
2041-8205
2021 Impact Factor: 8.811
2020 SCImago Journal Rankings: 3.639
ISI Accession Number ID
WOS:000268761500062
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorBand, DLen_US
dc.contributor.authorAxelsson, Men_US
dc.contributor.authorBaldini, Len_US
dc.contributor.authorBarbiellini, Gen_US
dc.contributor.authorBaring, MGen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorBattelino, Men_US
dc.contributor.authorBellazzini, Ren_US
dc.contributor.authorBissaldi, Een_US
dc.contributor.authorBogaert, Gen_US
dc.contributor.authorBonnell, Jen_US
dc.contributor.authorChiang, Jen_US
dc.contributor.authorCohenTanugi, Jen_US
dc.contributor.authorConnaughton, Ven_US
dc.contributor.authorCutini, Sen_US
dc.contributor.authorDe Palma, Fen_US
dc.contributor.authorDingus, BLen_US
dc.contributor.authorDo Couto E Silva, Een_US
dc.contributor.authorFishman, Gen_US
dc.contributor.authorGalli, Aen_US
dc.contributor.authorGehrels, Nen_US
dc.contributor.authorGiglietto, Nen_US
dc.contributor.authorGranot, Jen_US
dc.contributor.authorGuiriec, Sen_US
dc.contributor.authorHughes, REen_US
dc.contributor.authorKamae, Ten_US
dc.contributor.authorKomin, Nen_US
dc.contributor.authorKuehn, Fen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLubrano, Pen_US
dc.contributor.authorKippen, RMen_US
dc.contributor.authorMazziotta, MNen_US
dc.contributor.authorMcenery, JEen_US
dc.contributor.authorMcglynn, Sen_US
dc.contributor.authorMoretti, Een_US
dc.contributor.authorNakamori, Ten_US
dc.contributor.authorNorris, JPen_US
dc.contributor.authorOhno, Men_US
dc.contributor.authorOlivo, Men_US
dc.contributor.authorOmodei, Nen_US
dc.contributor.authorPelassa, Ven_US
dc.contributor.authorPiron, Fen_US
dc.contributor.authorPreece, Ren_US
dc.contributor.authorRazzano, Men_US
dc.contributor.authorRussell, JJen_US
dc.contributor.authorRyde, Fen_US
dc.contributor.authorSaz Parkinson, PMen_US
dc.contributor.authorScargle, JDen_US
dc.contributor.authorSgrò, Cen_US
dc.contributor.authorShimokawabe, Ten_US
dc.contributor.authorSmith, PDen_US
dc.contributor.authorSpandre, Gen_US
dc.contributor.authorSpinelli, Pen_US
dc.contributor.authorStamatikos, Men_US
dc.contributor.authorWiner, BLen_US
dc.contributor.authorYamazaki, Ren_US
dc.date.accessioned2013-09-03T04:04:04Z-
dc.date.available2013-09-03T04:04:04Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 701 n. 2, p. 1673-1694en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188369-
dc.description.abstractThe Large Area Telescope (LAT) instrument on the Fermi mission will reveal the rich spectral and temporal gamma-ray burst (GRB) phenomena in the >100 MeV band. The synergy with Fermi's Gamma-ray Burst Monitor detectors will link these observations to those in the well explored 10-1000keV range; the addition of the >100 MeV band observations will resolve theoretical uncertainties about burst emission in both the prompt and afterglow phases. Trigger algorithms will be applied to the LAT data both onboard the spacecraft and on the ground. The sensitivity of these triggers will differ because of the available computing resources onboard and on the ground. Here we present the LAT's burst detection methodologies and the instrument's GRB capabilities. © 2009 The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectGamma Rays: Burstsen_US
dc.titleProspects for grb science with the fermi large area telescopeen_US
dc.typeArticleen_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1088/0004-637X/701/2/1673en_US
dc.identifier.scopuseid_2-s2.0-70549100101en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-70549100101&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume701en_US
dc.identifier.issue2en_US
dc.identifier.spage1673en_US
dc.identifier.epage1694en_US
dc.identifier.isiWOS:000268761500062-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridBand, DL=34567640300en_US
dc.identifier.scopusauthoridAxelsson, M=8670342300en_US
dc.identifier.scopusauthoridBaldini, L=35748339500en_US
dc.identifier.scopusauthoridBarbiellini, G=7103354697en_US
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dc.identifier.scopusauthoridBellazzini, R=12758801700en_US
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dc.identifier.scopusauthoridDe Palma, F=25724295700en_US
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dc.identifier.scopusauthoridDo Couto E Silva, E=35228200800en_US
dc.identifier.scopusauthoridFishman, G=7103365769en_US
dc.identifier.scopusauthoridGalli, A=34567640300en_US
dc.identifier.scopusauthoridGehrels, N=8670342300en_US
dc.identifier.scopusauthoridGiglietto, N=35748339500en_US
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dc.identifier.scopusauthoridHughes, RE=8540124100en_US
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dc.identifier.scopusauthoridLongo, F=7004358647en_US
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dc.identifier.scopusauthoridKippen, RM=8395348400en_US
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dc.identifier.scopusauthoridPelassa, V=7003464210en_US
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dc.identifier.scopusauthoridSaz Parkinson, PM=15755916900en_US
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dc.identifier.scopusauthoridYamazaki, R=25948722900en_US
dc.identifier.issnl2041-8205-

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