Prospects for grb science with the fermi large area telescope

D. L. Band; M. Axelsson; L. Baldini; G. Barbiellini; M. G. Baring; D. Bastieri; M. Battelino; R. Bellazzini; E. Bissaldi; G. Bogaert; J. Bonnell; J. Chiang; J. Cohen-Tanugi; V. Connaughton; S. Cutini; F. De Palma; B. L. Dingus; E. Do Couto E Silva; G. Fishman; A. Galli; N. Gehrels; N. Giglietto; J. Granot; S. Guiriec; R. E. Hughes; T. Kamae; N. Komin; F. Kuehn; M. Kuss; F. Longo; P. Lubrano; R. M. Kippen; M. N. Mazziotta; J. E. McEnery; S. McGlynn; E. Moretti; T. Nakamori; J. P. Norris; M. Ohno; M. Olivo; N. Omodei; V. Pelassa; F. Piron; R. Preece; M. Razzano; J. J. Russell; F. Ryde; P. M. Saz Parkinson; J. D. Scargle; C. Sgrò; T. Shimokawabe; P. D. Smith; G. Spandre; P. Spinelli; M. Stamatikos; B. L. Winer; R. Yamazaki

doi:10.1088/0004-637X/701/2/1673

Prospects for grb science with the fermi large area telescope

D. L. Band, M. Axelsson, L. Baldini, G. Barbiellini, M. G. Baring, D. Bastieri, M. Battelino, R. Bellazzini, E. Bissaldi, G. Bogaert, J. Bonnell, J. Chiang, J. Cohen-Tanugi, V. Connaughton, S. Cutini, F. De Palma, B. L. Dingus, E. Do Couto E Silva, G. Fishman, A. GalliN. Gehrels, N. Giglietto, J. Granot, S. Guiriec, R. E. Hughes, T. Kamae, N. Komin, F. Kuehn, M. Kuss, F. Longo, P. Lubrano, R. M. Kippen, M. N. Mazziotta, J. E. McEnery, S. McGlynn, E. Moretti, T. Nakamori, J. P. Norris, M. Ohno, M. Olivo, N. Omodei, V. Pelassa, F. Piron, R. Preece, M. Razzano, J. J. Russell, F. Ryde, P. M. Saz Parkinson, J. D. Scargle, C. Sgrò, T. Shimokawabe, P. D. Smith, G. Spandre, P. Spinelli, M. Stamatikos, B. L. Winer, R. Yamazaki

نتاج البحث: نشر في مجلة › مقالة › مراجعة النظراء

ملخص

The 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.

اللغة الأصلية	الإنجليزيّة
الصفحات (من إلى)	1673-1694
عدد الصفحات	22
دورية	Astrophysical Journal
مستوى الصوت	701
رقم الإصدار	2
المعرِّفات الرقمية للأشياء	https://doi.org/10.1088/0004-637X/701/2/1673
حالة النشر	نُشِر - 2009
منشور خارجيًا	نعم

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10.1088/0004-637X/701/2/1673

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Link to publication in Scopus

قم بذكر هذا

Band, D. L., Axelsson, M., Baldini, L., Barbiellini, G., Baring, M. G., Bastieri, D., Battelino, M., Bellazzini, R., Bissaldi, E., Bogaert, G., Bonnell, J., Chiang, J., Cohen-Tanugi, J., Connaughton, V., Cutini, S., De Palma, F., Dingus, B. L., Do Couto E Silva, E., Fishman, G., ... Yamazaki, R. (2009). Prospects for grb science with the fermi large area telescope. Astrophysical Journal, 701(2), 1673-1694. https://doi.org/10.1088/0004-637X/701/2/1673

@article{77ca557e11fe4c2884ea270995df3edc,

title = "Prospects for grb science with the fermi large area telescope",

abstract = "The 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.",

keywords = "Gamma rays: bursts",

author = "Band, {D. L.} and M. Axelsson and L. Baldini and G. Barbiellini and Baring, {M. G.} and D. Bastieri and M. Battelino and R. Bellazzini and E. Bissaldi and G. Bogaert and J. Bonnell and J. Chiang and J. Cohen-Tanugi and V. Connaughton and S. Cutini and {De Palma}, F. and Dingus, {B. L.} and {Do Couto E Silva}, E. and G. Fishman and A. Galli and N. Gehrels and N. Giglietto and J. Granot and S. Guiriec and Hughes, {R. E.} and T. Kamae and N. Komin and F. Kuehn and M. Kuss and F. Longo and P. Lubrano and Kippen, {R. M.} and Mazziotta, {M. N.} and McEnery, {J. E.} and S. McGlynn and E. Moretti and T. Nakamori and Norris, {J. P.} and M. Ohno and M. Olivo and N. Omodei and V. Pelassa and F. Piron and R. Preece and M. Razzano and Russell, {J. J.} and F. Ryde and {Saz Parkinson}, {P. M.} and Scargle, {J. D.} and C. Sgr{\`o} and T. Shimokawabe and Smith, {P. D.} and G. Spandre and P. Spinelli and M. Stamatikos and Winer, {B. L.} and R. Yamazaki",

year = "2009",

doi = "10.1088/0004-637X/701/2/1673",

language = "אנגלית",

volume = "701",

pages = "1673--1694",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "2",

}

Band, DL, Axelsson, M, Baldini, L, Barbiellini, G, Baring, MG, Bastieri, D, Battelino, M, Bellazzini, R, Bissaldi, E, Bogaert, G, Bonnell, J, Chiang, J, Cohen-Tanugi, J, Connaughton, V, Cutini, S, De Palma, F, Dingus, BL, Do Couto E Silva, E, Fishman, G, Galli, A, Gehrels, N, Giglietto, N, Granot, J, Guiriec, S, Hughes, RE, Kamae, T, Komin, N, Kuehn, F, Kuss, M, Longo, F, Lubrano, P, Kippen, RM, Mazziotta, MN, McEnery, JE, McGlynn, S, Moretti, E, Nakamori, T, Norris, JP, Ohno, M, Olivo, M, Omodei, N, Pelassa, V, Piron, F, Preece, R, Razzano, M, Russell, JJ, Ryde, F, Saz Parkinson, PM, Scargle, JD, Sgrò, C, Shimokawabe, T, Smith, PD, Spandre, G, Spinelli, P, Stamatikos, M, Winer, BL & Yamazaki, R 2009, 'Prospects for grb science with the fermi large area telescope', Astrophysical Journal, المجلد 701, رقم 2, الصفحات 1673-1694. https://doi.org/10.1088/0004-637X/701/2/1673

TY - JOUR

T1 - Prospects for grb science with the fermi large area telescope

AU - Band, D. L.

AU - Axelsson, M.

AU - Baldini, L.

AU - Barbiellini, G.

AU - Baring, M. G.

AU - Bastieri, D.

AU - Battelino, M.

AU - Bellazzini, R.

AU - Bissaldi, E.

AU - Bogaert, G.

AU - Bonnell, J.

AU - Chiang, J.

AU - Cohen-Tanugi, J.

AU - Connaughton, V.

AU - Cutini, S.

AU - De Palma, F.

AU - Dingus, B. L.

AU - Do Couto E Silva, E.

AU - Fishman, G.

AU - Galli, A.

AU - Gehrels, N.

AU - Giglietto, N.

AU - Granot, J.

AU - Guiriec, S.

AU - Hughes, R. E.

AU - Kamae, T.

AU - Komin, N.

AU - Kuehn, F.

AU - Kuss, M.

AU - Longo, F.

AU - Lubrano, P.

AU - Kippen, R. M.

AU - Mazziotta, M. N.

AU - McEnery, J. E.

AU - McGlynn, S.

AU - Moretti, E.

AU - Nakamori, T.

AU - Norris, J. P.

AU - Ohno, M.

AU - Olivo, M.

AU - Omodei, N.

AU - Pelassa, V.

AU - Piron, F.

AU - Preece, R.

AU - Razzano, M.

AU - Russell, J. J.

AU - Ryde, F.

AU - Saz Parkinson, P. M.

AU - Scargle, J. D.

AU - Sgrò, C.

AU - Shimokawabe, T.

AU - Smith, P. D.

AU - Spandre, G.

AU - Spinelli, P.

AU - Stamatikos, M.

AU - Winer, B. L.

AU - Yamazaki, R.

PY - 2009

Y1 - 2009

N2 - The 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.

AB - The 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.

KW - Gamma rays: bursts

UR - http://www.scopus.com/inward/record.url?scp=70549100101&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/701/2/1673

DO - 10.1088/0004-637X/701/2/1673

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:70549100101

SN - 0004-637X

VL - 701

SP - 1673

EP - 1694

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

ER -

Prospects for grb science with the fermi large area telescope

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