GRB 130427A: A nearby ordinary monster

A. Maselli; A. Melandri; L. Nava; C. G. Mundell; N. Kawai; S. Campana; S. Covino; J. R. Cummings; G. Cusumano; P. A. Evans; G. Ghirlanda; G. Ghisellini; C. Guidorzi; S. Kobayashi; P. Kuin; V. La Parola; V. Mangano; S. Oates; T. Sakamoto; M. Serino; F. Virgili; B. B. Zhang; S. Barthelmy; A. Beardmore; M. G. Bernardini; D. Bersier; D. Burrows; G. Calderone; M. Capalbi; J. Chiang; P. D'Avanzo; V. D'Elia; M. De Pasquale; D. Fugazza; N. Gehrels; A. Gomboc; R. Harrison; H. Hanayama; J. Japelj; J. Kennea; D. Kopac; C. Kouveliotou; D. Kuroda; A. Levan; D. Malesani; F. Marshall; J. Nousek; P. O'Brien; J. P. Osborne; C. Pagani; K. L. Page; M. Page; M. Perri; T. Pritchard; P. Romano; Y. Saito; B. Sbarufatti; R. Salvaterra; I. Steele; N. Tanvir; G. Vianello; B. Wiegand; K. Wiersema; Y. Yatsu; T. Yoshii; G. Tagliaferri

doi:10.1126/science.1242279

GRB 130427A: A nearby ordinary monster

A. Maselli, A. Melandri, L. Nava, C. G. Mundell, N. Kawai, S. Campana, S. Covino, J. R. Cummings, G. Cusumano, P. A. Evans, G. Ghirlanda, G. Ghisellini, C. Guidorzi, S. Kobayashi, P. Kuin, V. La Parola, V. Mangano, S. Oates, T. Sakamoto, M. SerinoF. Virgili, B. B. Zhang, S. Barthelmy, A. Beardmore, M. G. Bernardini, D. Bersier, D. Burrows, G. Calderone, M. Capalbi, J. Chiang, P. D'Avanzo, V. D'Elia, M. De Pasquale, D. Fugazza, N. Gehrels, A. Gomboc, R. Harrison, H. Hanayama, J. Japelj, J. Kennea, D. Kopac, C. Kouveliotou, D. Kuroda, A. Levan, D. Malesani, F. Marshall, J. Nousek, P. O'Brien, J. P. Osborne, C. Pagani, K. L. Page, M. Page, M. Perri, T. Pritchard, P. Romano, Y. Saito, B. Sbarufatti, R. Salvaterra, I. Steele, N. Tanvir, G. Vianello, B. Wiegand, K. Wiersema, Y. Yatsu, T. Yoshii, G. Tagliaferri

Astronomy & Astrophysics

Research output: Contribution to journal › Article › peer-review

113 Scopus citations

Abstract

Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ∼ 3 × 10⁵³ ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.

Original language	English (US)
Pages (from-to)	48-51
Number of pages	4
Journal	Science
Volume	343
Issue number	6166
DOIs	https://doi.org/10.1126/science.1242279
State	Published - 2014

All Science Journal Classification (ASJC) codes

General

Access to Document

10.1126/science.1242279

Cite this

Maselli, A., Melandri, A., Nava, L., Mundell, C. G., Kawai, N., Campana, S., Covino, S., Cummings, J. R., Cusumano, G., Evans, P. A., Ghirlanda, G., Ghisellini, G., Guidorzi, C., Kobayashi, S., Kuin, P., La Parola, V., Mangano, V., Oates, S., Sakamoto, T., ... Tagliaferri, G. (2014). GRB 130427A: A nearby ordinary monster. Science, 343(6166), 48-51. https://doi.org/10.1126/science.1242279

@article{b35c8d22aded4012bdd89339fe8bd969,

title = "GRB 130427A: A nearby ordinary monster",

abstract = "Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ∼ 3 × 1053 ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.",

author = "A. Maselli and A. Melandri and L. Nava and Mundell, {C. G.} and N. Kawai and S. Campana and S. Covino and Cummings, {J. R.} and G. Cusumano and Evans, {P. A.} and G. Ghirlanda and G. Ghisellini and C. Guidorzi and S. Kobayashi and P. Kuin and {La Parola}, V. and V. Mangano and S. Oates and T. Sakamoto and M. Serino and F. Virgili and Zhang, {B. B.} and S. Barthelmy and A. Beardmore and Bernardini, {M. G.} and D. Bersier and D. Burrows and G. Calderone and M. Capalbi and J. Chiang and P. D'Avanzo and V. D'Elia and {De Pasquale}, M. and D. Fugazza and N. Gehrels and A. Gomboc and R. Harrison and H. Hanayama and J. Japelj and J. Kennea and D. Kopac and C. Kouveliotou and D. Kuroda and A. Levan and D. Malesani and F. Marshall and J. Nousek and P. O'Brien and Osborne, {J. P.} and C. Pagani and Page, {K. L.} and M. Page and M. Perri and T. Pritchard and P. Romano and Y. Saito and B. Sbarufatti and R. Salvaterra and I. Steele and N. Tanvir and G. Vianello and B. Wiegand and K. Wiersema and Y. Yatsu and T. Yoshii and G. Tagliaferri",

year = "2014",

doi = "10.1126/science.1242279",

language = "English (US)",

volume = "343",

pages = "48--51",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "6166",

}

Maselli, A, Melandri, A, Nava, L, Mundell, CG, Kawai, N, Campana, S, Covino, S, Cummings, JR, Cusumano, G, Evans, PA, Ghirlanda, G, Ghisellini, G, Guidorzi, C, Kobayashi, S, Kuin, P, La Parola, V, Mangano, V, Oates, S, Sakamoto, T, Serino, M, Virgili, F, Zhang, BB, Barthelmy, S, Beardmore, A, Bernardini, MG, Bersier, D, Burrows, D, Calderone, G, Capalbi, M, Chiang, J, D'Avanzo, P, D'Elia, V, De Pasquale, M, Fugazza, D, Gehrels, N, Gomboc, A, Harrison, R, Hanayama, H, Japelj, J, Kennea, J, Kopac, D, Kouveliotou, C, Kuroda, D, Levan, A, Malesani, D, Marshall, F, Nousek, J, O'Brien, P, Osborne, JP, Pagani, C, Page, KL, Page, M, Perri, M, Pritchard, T, Romano, P, Saito, Y, Sbarufatti, B, Salvaterra, R, Steele, I, Tanvir, N, Vianello, G, Wiegand, B, Wiersema, K, Yatsu, Y, Yoshii, T & Tagliaferri, G 2014, 'GRB 130427A: A nearby ordinary monster', Science, vol. 343, no. 6166, pp. 48-51. https://doi.org/10.1126/science.1242279

TY - JOUR

T1 - GRB 130427A

T2 - A nearby ordinary monster

AU - Maselli, A.

AU - Melandri, A.

AU - Nava, L.

AU - Mundell, C. G.

AU - Kawai, N.

AU - Campana, S.

AU - Covino, S.

AU - Cummings, J. R.

AU - Cusumano, G.

AU - Evans, P. A.

AU - Ghirlanda, G.

AU - Ghisellini, G.

AU - Guidorzi, C.

AU - Kobayashi, S.

AU - Kuin, P.

AU - La Parola, V.

AU - Mangano, V.

AU - Oates, S.

AU - Sakamoto, T.

AU - Serino, M.

AU - Virgili, F.

AU - Zhang, B. B.

AU - Barthelmy, S.

AU - Beardmore, A.

AU - Bernardini, M. G.

AU - Bersier, D.

AU - Burrows, D.

AU - Calderone, G.

AU - Capalbi, M.

AU - Chiang, J.

AU - D'Avanzo, P.

AU - D'Elia, V.

AU - De Pasquale, M.

AU - Fugazza, D.

AU - Gehrels, N.

AU - Gomboc, A.

AU - Harrison, R.

AU - Hanayama, H.

AU - Japelj, J.

AU - Kennea, J.

AU - Kopac, D.

AU - Kouveliotou, C.

AU - Kuroda, D.

AU - Levan, A.

AU - Malesani, D.

AU - Marshall, F.

AU - Nousek, J.

AU - O'Brien, P.

AU - Osborne, J. P.

AU - Pagani, C.

AU - Page, K. L.

AU - Page, M.

AU - Perri, M.

AU - Pritchard, T.

AU - Romano, P.

AU - Saito, Y.

AU - Sbarufatti, B.

AU - Salvaterra, R.

AU - Steele, I.

AU - Tanvir, N.

AU - Vianello, G.

AU - Wiegand, B.

AU - Wiersema, K.

AU - Yatsu, Y.

AU - Yoshii, T.

AU - Tagliaferri, G.

PY - 2014

Y1 - 2014

N2 - Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ∼ 3 × 1053 ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.

AB - Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ∼ 3 × 1053 ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.

UR - http://www.scopus.com/inward/record.url?scp=84896711884&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84896711884&partnerID=8YFLogxK

U2 - 10.1126/science.1242279

DO - 10.1126/science.1242279

M3 - Article

C2 - 24263134

AN - SCOPUS:84896711884

SN - 0036-8075

VL - 343

SP - 48

EP - 51

JO - Science

JF - Science

IS - 6166

ER -

GRB 130427A: A nearby ordinary monster

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this