Fermi-GBM Analysis of GRB 221009A

S. Lesage; P. Veres; M. S. Briggs; A. Goldstein; D. Kocevski; E. Burns; C. A. Wilson-Hodge; P. Veres; P. N. Bhat; D. Huppenkothen; C. L. Fryer; R. Hamburg; J. Racusin; E. Bissaldi; W. H. Cleveland; S. Dalessi; C. Fletcher; M. M. Giles; B. A. Hristov; C. M. Hui; B. Mailyan; C. Malacaria; S. Poolakkil; O. J. Roberts; A. von Kienlin; J. Wood; M. Ajello; M. Arimoto; L. Baldini; J. Ballet; M. G. Baring; D. Bastieri; J. Becerra Gonzalez; R. Bellazzini; R. D. Blandford; R. Bonino; P. Bruel; S. Buson; R. A. Cameron; R. Caputo; P. A. Caraveo; E. Cavazzuti; G. Chiaro; N. Cibrario; S. Ciprini; P. Cristarella Orestano; M. Crnogorcevic; A. Cuoco; S. Cutini; F. D’Ammando; S. De Gaetano; N. Di Lalla; L. Di Venere; A. Domínguez; S. J. Fegan; E. C. Ferrara; H. Fleischhack; Y. Fukazawa; S. Funk; P. Fusco; G. Galanti; V. Gammaldi; F. Gargano; C. Gasbarra; D. Gasparrini; S. Germani; F. Giacchino; N. Giglietto; R. Gill; M. Giroletti; J. Granot; D. Green; I. A. Grenier; S. Guiriec; M. Gustafsson; E. Hays; J. W. Hewitt; D. Horan; X. Hou; M. Kuss; L. Latronico; A. Laviron; M. Lemoine-Goumard; J. Li; I. Liodakis; F. Longo; F. Loparco; L. Lorusso; M. N. Lovellette; P. Lubrano; S. Maldera; A. Manfreda; G. Martí-Devesa; M. N. Mazziotta; J. E. McEnery; I. Mereu; M. Meyer; P. F. Michelson; T. Mizuno; M. E. Monzani; A. Morselli; I. V. Moskalenko; M. Negro; E. Nuss; N. Omodei; E. Orlando; J. F. Ormes; D. Paneque; G. Panzarini; M. Persic; M. Pesce-Rollins; R. Pillera; F. Piron; H. Poon; T. A. Porter; G. Principe; S. Rainò; R. Rando; B. Rani; M. Razzano; S. Razzaque; A. Reimer; O. Reimer; F. Ryde; M. Sánchez-Conde; P. M. Saz Parkinson; L. Scotton; D. Serini; C. Sgrò; V. Sharma; E. J. Siskind; G. Spandre; P. Spinelli; H. Tajima; D. F. Torres; J. Valverde; T. Venters; Z. Wadiasingh; K. Wood; G. Zaharijas

Fermi-GBM Analysis of GRB 221009A

S. Lesage, P. Veres, M. S. Briggs, A. Goldstein, D. Kocevski, E. Burns, C. A. Wilson-Hodge, P. Veres, P. N. Bhat, D. Huppenkothen, C. L. Fryer, R. Hamburg, J. Racusin, E. Bissaldi, W. H. Cleveland, S. Dalessi, C. Fletcher, M. M. Giles, B. A. Hristov, C. M. HuiB. Mailyan, C. Malacaria, S. Poolakkil, O. J. Roberts, A. von Kienlin, J. Wood, M. Ajello, M. Arimoto, L. Baldini, J. Ballet, M. G. Baring, D. Bastieri, J. Becerra Gonzalez, R. Bellazzini, R. D. Blandford, R. Bonino, P. Bruel, S. Buson, R. A. Cameron, R. Caputo, P. A. Caraveo, E. Cavazzuti, G. Chiaro, N. Cibrario, S. Ciprini, P. Cristarella Orestano, M. Crnogorcevic, A. Cuoco, S. Cutini, F. D’Ammando, S. De Gaetano, N. Di Lalla, L. Di Venere, A. Domínguez, S. J. Fegan, E. C. Ferrara, H. Fleischhack, Y. Fukazawa, S. Funk, P. Fusco, G. Galanti, V. Gammaldi, F. Gargano, C. Gasbarra, D. Gasparrini, S. Germani, F. Giacchino, N. Giglietto, R. Gill, M. Giroletti, J. Granot, D. Green, I. A. Grenier, S. Guiriec, M. Gustafsson, E. Hays, J. W. Hewitt, D. Horan, X. Hou, M. Kuss, L. Latronico, A. Laviron, M. Lemoine-Goumard, J. Li, I. Liodakis, F. Longo, F. Loparco, L. Lorusso, M. N. Lovellette, P. Lubrano, S. Maldera, A. Manfreda, G. Martí-Devesa, M. N. Mazziotta, J. E. McEnery, I. Mereu, M. Meyer, P. F. Michelson, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, M. Negro, E. Nuss, N. Omodei, E. Orlando, J. F. Ormes, D. Paneque, G. Panzarini, M. Persic, M. Pesce-Rollins, R. Pillera, F. Piron, H. Poon, T. A. Porter, G. Principe, S. Rainò, R. Rando, B. Rani, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, F. Ryde, M. Sánchez-Conde, P. M. Saz Parkinson, L. Scotton, D. Serini, C. Sgrò, V. Sharma, E. J. Siskind, G. Spandre, P. Spinelli, H. Tajima, D. F. Torres, J. Valverde, T. Venters, Z. Wadiasingh, K. Wood, G. Zaharijas

פיסיקה

نتاج البحث: نشر في مجلة › مقالة من مؤنمر › مراجعة النظراء

ملخص

At 13:16:59.99 UT on October 9th, 2022, the Fermi Gamma-ray Burst Monitor (GBM) triggered on gamma-ray burst (GRB) 221009A. This GRB has the highest fluence value GBM has ever detected. The light curve consists of two distinct emission episodes, a single isolated peak with a thermal spectra followed by a longer, extremely bright, multi-pulsed event with a non-thermal spectra. The two main peaks of the second event, from t₀+218 to t₀+276 seconds and t₀+508 to t₀+513 s, had such high photon rates they caused pulse-pile up effects in the GBM detectors. Afterglow emission is detectable in the GBM energy range out to t₀+1467 seconds when the field of view was occulted by Earth. Here we present the key parts of our spectrotemporal analysis for the triggering pulse, prompt emission, and afterglow and the pulse pile-up corrected energetics for the this historically bright event.

اللغة الأصلية	الإنجليزيّة
رقم المقال	882
دورية	Proceedings of Science
مستوى الصوت	444
حالة النشر	نُشِر - 27 سبتمبر 2024
الحدث	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, اليابان المدة: ٢٦ يوليو ٢٠٢٣ → ٣ أغسطس ٢٠٢٣

ملاحظة ببليوغرافية

Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.

الملفات والروابط الأخرى

Link to publication in Scopus

قم بذكر هذا

Lesage, S., Veres, P., Briggs, M. S., Goldstein, A., Kocevski, D., Burns, E., Wilson-Hodge, C. A., Veres, P., Bhat, P. N., Huppenkothen, D., Fryer, C. L., Hamburg, R., Racusin, J., Bissaldi, E., Cleveland, W. H., Dalessi, S., Fletcher, C., Giles, M. M., Hristov, B. A., ... Zaharijas, G. (2024). Fermi-GBM Analysis of GRB 221009A. Proceedings of Science, 444, المقال 882.

@article{5d578a5d90ad459d8ee9db792716b9d2,

title = "Fermi-GBM Analysis of GRB 221009A",

abstract = "At 13:16:59.99 UT on October 9th, 2022, the Fermi Gamma-ray Burst Monitor (GBM) triggered on gamma-ray burst (GRB) 221009A. This GRB has the highest fluence value GBM has ever detected. The light curve consists of two distinct emission episodes, a single isolated peak with a thermal spectra followed by a longer, extremely bright, multi-pulsed event with a non-thermal spectra. The two main peaks of the second event, from t0+218 to t0+276 seconds and t0+508 to t0+513 s, had such high photon rates they caused pulse-pile up effects in the GBM detectors. Afterglow emission is detectable in the GBM energy range out to t0+1467 seconds when the field of view was occulted by Earth. Here we present the key parts of our spectrotemporal analysis for the triggering pulse, prompt emission, and afterglow and the pulse pile-up corrected energetics for the this historically bright event.",

author = "S. Lesage and P. Veres and Briggs, {M. S.} and A. Goldstein and D. Kocevski and E. Burns and Wilson-Hodge, {C. A.} and P. Veres and Bhat, {P. N.} and D. Huppenkothen and Fryer, {C. L.} and R. Hamburg and J. Racusin and E. Bissaldi and Cleveland, {W. H.} and S. Dalessi and C. Fletcher and Giles, {M. M.} and Hristov, {B. A.} and Hui, {C. M.} and B. Mailyan and C. Malacaria and S. Poolakkil and Roberts, {O. J.} and {von Kienlin}, A. and J. Wood and M. Ajello and M. Arimoto and L. Baldini and J. Ballet and Baring, {M. G.} and D. Bastieri and {Becerra Gonzalez}, J. and R. Bellazzini and Blandford, {R. D.} and R. Bonino and P. Bruel and S. Buson and Cameron, {R. A.} and R. Caputo and Caraveo, {P. A.} and E. Cavazzuti and G. Chiaro and N. Cibrario and S. Ciprini and {Cristarella Orestano}, P. and M. Crnogorcevic and A. Cuoco and S. Cutini and F. D{\textquoteright}Ammando and {De Gaetano}, S. and {Di Lalla}, N. and {Di Venere}, L. and A. Dom{\'i}nguez and Fegan, {S. J.} and Ferrara, {E. C.} and H. Fleischhack and Y. Fukazawa and S. Funk and P. Fusco and G. Galanti and V. Gammaldi and F. Gargano and C. Gasbarra and D. Gasparrini and S. Germani and F. Giacchino and N. Giglietto and R. Gill and M. Giroletti and J. Granot and D. Green and Grenier, {I. A.} and S. Guiriec and M. Gustafsson and E. Hays and Hewitt, {J. W.} and D. Horan and X. Hou and M. Kuss and L. Latronico and A. Laviron and M. Lemoine-Goumard and J. Li and I. Liodakis and F. Longo and F. Loparco and L. Lorusso and Lovellette, {M. N.} and P. Lubrano and S. Maldera and A. Manfreda and G. Mart{\'i}-Devesa and Mazziotta, {M. N.} and McEnery, {J. E.} and I. Mereu and M. Meyer and Michelson, {P. F.} and T. Mizuno and Monzani, {M. E.} and A. Morselli and Moskalenko, {I. V.} and M. Negro and E. Nuss and N. Omodei and E. Orlando and Ormes, {J. F.} and D. Paneque and G. Panzarini and M. Persic and M. Pesce-Rollins and R. Pillera and F. Piron and H. Poon and Porter, {T. A.} and G. Principe and S. Rain{\`o} and R. Rando and B. Rani and M. Razzano and S. Razzaque and A. Reimer and O. Reimer and F. Ryde and M. S{\'a}nchez-Conde and {Saz Parkinson}, {P. M.} and L. Scotton and D. Serini and C. Sgr{\`o} and V. Sharma and Siskind, {E. J.} and G. Spandre and P. Spinelli and H. Tajima and Torres, {D. F.} and J. Valverde and T. Venters and Z. Wadiasingh and K. Wood and G. Zaharijas",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

language = "אנגלית",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Lesage, S, Veres, P, Briggs, MS, Goldstein, A, Kocevski, D, Burns, E, Wilson-Hodge, CA, Veres, P, Bhat, PN, Huppenkothen, D, Fryer, CL, Hamburg, R, Racusin, J, Bissaldi, E, Cleveland, WH, Dalessi, S, Fletcher, C, Giles, MM, Hristov, BA, Hui, CM, Mailyan, B, Malacaria, C, Poolakkil, S, Roberts, OJ, von Kienlin, A, Wood, J, Ajello, M, Arimoto, M, Baldini, L, Ballet, J, Baring, MG, Bastieri, D, Becerra Gonzalez, J, Bellazzini, R, Blandford, RD, Bonino, R, Bruel, P, Buson, S, Cameron, RA, Caputo, R, Caraveo, PA, Cavazzuti, E, Chiaro, G, Cibrario, N, Ciprini, S, Cristarella Orestano, P, Crnogorcevic, M, Cuoco, A, Cutini, S, D’Ammando, F, De Gaetano, S, Di Lalla, N, Di Venere, L, Domínguez, A, Fegan, SJ, Ferrara, EC, Fleischhack, H, Fukazawa, Y, Funk, S, Fusco, P, Galanti, G, Gammaldi, V, Gargano, F, Gasbarra, C, Gasparrini, D, Germani, S, Giacchino, F, Giglietto, N, Gill, R, Giroletti, M, Granot, J, Green, D, Grenier, IA, Guiriec, S, Gustafsson, M, Hays, E, Hewitt, JW, Horan, D, Hou, X, Kuss, M, Latronico, L, Laviron, A, Lemoine-Goumard, M, Li, J, Liodakis, I, Longo, F, Loparco, F, Lorusso, L, Lovellette, MN, Lubrano, P, Maldera, S, Manfreda, A, Martí-Devesa, G, Mazziotta, MN, McEnery, JE, Mereu, I, Meyer, M, Michelson, PF, Mizuno, T, Monzani, ME, Morselli, A, Moskalenko, IV, Negro, M, Nuss, E, Omodei, N, Orlando, E, Ormes, JF, Paneque, D, Panzarini, G, Persic, M, Pesce-Rollins, M, Pillera, R, Piron, F, Poon, H, Porter, TA, Principe, G, Rainò, S, Rando, R, Rani, B, Razzano, M, Razzaque, S, Reimer, A, Reimer, O, Ryde, F, Sánchez-Conde, M, Saz Parkinson, PM, Scotton, L, Serini, D, Sgrò, C, Sharma, V, Siskind, EJ, Spandre, G, Spinelli, P, Tajima, H, Torres, DF, Valverde, J, Venters, T, Wadiasingh, Z, Wood, K & Zaharijas, G 2024, 'Fermi-GBM Analysis of GRB 221009A', Proceedings of Science, المجلد 444, 882.

TY - JOUR

T1 - Fermi-GBM Analysis of GRB 221009A

AU - Lesage, S.

AU - Veres, P.

AU - Briggs, M. S.

AU - Goldstein, A.

AU - Kocevski, D.

AU - Burns, E.

AU - Wilson-Hodge, C. A.

AU - Veres, P.

AU - Bhat, P. N.

AU - Huppenkothen, D.

AU - Fryer, C. L.

AU - Hamburg, R.

AU - Racusin, J.

AU - Bissaldi, E.

AU - Cleveland, W. H.

AU - Dalessi, S.

AU - Fletcher, C.

AU - Giles, M. M.

AU - Hristov, B. A.

AU - Hui, C. M.

AU - Mailyan, B.

AU - Malacaria, C.

AU - Poolakkil, S.

AU - Roberts, O. J.

AU - von Kienlin, A.

AU - Wood, J.

AU - Ajello, M.

AU - Arimoto, M.

AU - Baldini, L.

AU - Ballet, J.

AU - Baring, M. G.

AU - Bastieri, D.

AU - Becerra Gonzalez, J.

AU - Bellazzini, R.

AU - Blandford, R. D.

AU - Bonino, R.

AU - Bruel, P.

AU - Buson, S.

AU - Cameron, R. A.

AU - Caputo, R.

AU - Caraveo, P. A.

AU - Cavazzuti, E.

AU - Chiaro, G.

AU - Cibrario, N.

AU - Ciprini, S.

AU - Cristarella Orestano, P.

AU - Crnogorcevic, M.

AU - Cuoco, A.

AU - Cutini, S.

AU - D’Ammando, F.

AU - De Gaetano, S.

AU - Di Lalla, N.

AU - Di Venere, L.

AU - Domínguez, A.

AU - Fegan, S. J.

AU - Ferrara, E. C.

AU - Fleischhack, H.

AU - Fukazawa, Y.

AU - Funk, S.

AU - Fusco, P.

AU - Galanti, G.

AU - Gammaldi, V.

AU - Gargano, F.

AU - Gasbarra, C.

AU - Gasparrini, D.

AU - Germani, S.

AU - Giacchino, F.

AU - Giglietto, N.

AU - Gill, R.

AU - Giroletti, M.

AU - Granot, J.

AU - Green, D.

AU - Grenier, I. A.

AU - Guiriec, S.

AU - Gustafsson, M.

AU - Hays, E.

AU - Hewitt, J. W.

AU - Horan, D.

AU - Hou, X.

AU - Kuss, M.

AU - Latronico, L.

AU - Laviron, A.

AU - Lemoine-Goumard, M.

AU - Li, J.

AU - Liodakis, I.

AU - Longo, F.

AU - Loparco, F.

AU - Lorusso, L.

AU - Lovellette, M. N.

AU - Lubrano, P.

AU - Maldera, S.

AU - Manfreda, A.

AU - Martí-Devesa, G.

AU - Mazziotta, M. N.

AU - McEnery, J. E.

AU - Mereu, I.

AU - Meyer, M.

AU - Michelson, P. F.

AU - Mizuno, T.

AU - Monzani, M. E.

AU - Morselli, A.

AU - Moskalenko, I. V.

AU - Negro, M.

AU - Nuss, E.

AU - Omodei, N.

AU - Orlando, E.

AU - Ormes, J. F.

AU - Paneque, D.

AU - Panzarini, G.

AU - Persic, M.

AU - Pesce-Rollins, M.

AU - Pillera, R.

AU - Piron, F.

AU - Poon, H.

AU - Porter, T. A.

AU - Principe, G.

AU - Rainò, S.

AU - Rando, R.

AU - Rani, B.

AU - Razzano, M.

AU - Razzaque, S.

AU - Reimer, A.

AU - Reimer, O.

AU - Ryde, F.

AU - Sánchez-Conde, M.

AU - Saz Parkinson, P. M.

AU - Scotton, L.

AU - Serini, D.

AU - Sgrò, C.

AU - Sharma, V.

AU - Siskind, E. J.

AU - Spandre, G.

AU - Spinelli, P.

AU - Tajima, H.

AU - Torres, D. F.

AU - Valverde, J.

AU - Venters, T.

AU - Wadiasingh, Z.

AU - Wood, K.

AU - Zaharijas, G.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - At 13:16:59.99 UT on October 9th, 2022, the Fermi Gamma-ray Burst Monitor (GBM) triggered on gamma-ray burst (GRB) 221009A. This GRB has the highest fluence value GBM has ever detected. The light curve consists of two distinct emission episodes, a single isolated peak with a thermal spectra followed by a longer, extremely bright, multi-pulsed event with a non-thermal spectra. The two main peaks of the second event, from t0+218 to t0+276 seconds and t0+508 to t0+513 s, had such high photon rates they caused pulse-pile up effects in the GBM detectors. Afterglow emission is detectable in the GBM energy range out to t0+1467 seconds when the field of view was occulted by Earth. Here we present the key parts of our spectrotemporal analysis for the triggering pulse, prompt emission, and afterglow and the pulse pile-up corrected energetics for the this historically bright event.

AB - At 13:16:59.99 UT on October 9th, 2022, the Fermi Gamma-ray Burst Monitor (GBM) triggered on gamma-ray burst (GRB) 221009A. This GRB has the highest fluence value GBM has ever detected. The light curve consists of two distinct emission episodes, a single isolated peak with a thermal spectra followed by a longer, extremely bright, multi-pulsed event with a non-thermal spectra. The two main peaks of the second event, from t0+218 to t0+276 seconds and t0+508 to t0+513 s, had such high photon rates they caused pulse-pile up effects in the GBM detectors. Afterglow emission is detectable in the GBM energy range out to t0+1467 seconds when the field of view was occulted by Earth. Here we present the key parts of our spectrotemporal analysis for the triggering pulse, prompt emission, and afterglow and the pulse pile-up corrected energetics for the this historically bright event.

UR - http://www.scopus.com/inward/record.url?scp=85185597755&partnerID=8YFLogxK

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.conferencearticle???

AN - SCOPUS:85185597755

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 882

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Fermi-GBM Analysis of GRB 221009A

ملخص

ملاحظة ببليوغرافية

الملفات والروابط الأخرى

بصمة

قم بذكر هذا