GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang: Observations of the oldest cosmic explosion after the Big Bang

G Tagliaferri; LA Antonelli; G Chincarini; A Fernandez-Soto; D Malesani; M Della Valle; P D'Avanzo; A Grazian; V Testa; S Campana; S Covino; F Fiore; L Stella; AJ Castro-Tirado; J Gorosabel; DN Burrows; M Capalbi; G Cusumano; ML Conciatore; V D'Elia; P Filliatre; D Fugazza; N Gehrels; D Guetta; S Guziy; EV Held; K Hurley; GL Israel; M Jelinek; D Lazzati; A Lopez-Echarri; A Melandri; IF Mirabel; M Moles; A Moretti; KO Mason; J Nousek; J Osborne; LJ Pellizza; R Perna; S Piranomonte; L Piro; AD Postigo; P Romano

doi:10.1051/0004-6361:200500196

GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang: Observations of the oldest cosmic explosion after the Big Bang

G Tagliaferri
, LA Antonelli
, G Chincarini
, A Fernandez-Soto
, D Malesani
, M Della Valle
, P D'Avanzo
, A Grazian
, V Testa
, S Campana
, S Covino
, F Fiore
, L Stella
, AJ Castro-Tirado
, J Gorosabel
, DN Burrows
, M Capalbi
, G Cusumano
, ML Conciatore
, V D'Elia

P Filliatre, D Fugazza, N Gehrels, D Guetta, S Guziy, EV Held, K Hurley, GL Israel, M Jelinek, D Lazzati, A Lopez-Echarri, A Melandri, IF Mirabel, M Moles, A Moretti, KO Mason, J Nousek, J Osborne, LJ Pellizza, R Perna, S Piranomonte, L Piro, AD Postigo, P Romano

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

118 Scopus citations

Abstract

We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB 050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4 × 10⁵³ erg in the rest-frame 110-1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at t_b = 2.6 ± 1.0 d (observer frame). If we assume this is the jet break, we derive a beaming-corrected energy E_γ ∼ (4 ÷ 12) × 10⁵¹ erg. This limit shows that GRB 050904 is consistent with the Amati and Ghirlanda relations. This detection is consistent with the expected number of GRBs at z > 6 and shows that GRBs are a powerful tool to study the star formation history UD to very high redshift.

Original language	English
Pages (from-to)	L1-L5
Journal	Astronomy and Astrophysics
Volume	443
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361:200500196
State	Published - Nov 2005
Externally published	Yes

Keywords

cosmology : observations
early Universe
gamma rays : bursts
gamma rays : individual : GRB 050904

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10.1051/0004-6361:200500196

Cite this

Tagliaferri, G., Antonelli, LA., Chincarini, G., Fernandez-Soto, A., Malesani, D., Della Valle, M., D'Avanzo, P., Grazian, A., Testa, V., Campana, S., Covino, S., Fiore, F., Stella, L., Castro-Tirado, AJ., Gorosabel, J., Burrows, DN., Capalbi, M., Cusumano, G., Conciatore, ML., ... Romano, P. (2005). GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang: Observations of the oldest cosmic explosion after the Big Bang. Astronomy and Astrophysics, 443(1), L1-L5. https://doi.org/10.1051/0004-6361:200500196

@article{cd830545fb4740dc89ea921230b0df96,

title = "GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang: Observations of the oldest cosmic explosion after the Big Bang",

abstract = "We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB 050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4 × 1053 erg in the rest-frame 110-1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at tb = 2.6 ± 1.0 d (observer frame). If we assume this is the jet break, we derive a beaming-corrected energy Eγ ∼ (4 ÷ 12) × 1051 erg. This limit shows that GRB 050904 is consistent with the Amati and Ghirlanda relations. This detection is consistent with the expected number of GRBs at z > 6 and shows that GRBs are a powerful tool to study the star formation history UD to very high redshift.",

keywords = "cosmology : observations, early Universe, gamma rays : bursts, gamma rays : individual : GRB 050904",

author = "G Tagliaferri and LA Antonelli and G Chincarini and A Fernandez-Soto and D Malesani and \{Della Valle\}, M and P D'Avanzo and A Grazian and V Testa and S Campana and S Covino and F Fiore and L Stella and AJ Castro-Tirado and J Gorosabel and DN Burrows and M Capalbi and G Cusumano and ML Conciatore and V D'Elia and P Filliatre and D Fugazza and N Gehrels and D Guetta and S Guziy and EV Held and K Hurley and GL Israel and M Jelinek and D Lazzati and A Lopez-Echarri and A Melandri and IF Mirabel and M Moles and A Moretti and KO Mason and J Nousek and J Osborne and LJ Pellizza and R Perna and S Piranomonte and L Piro and AD Postigo and P Romano",

year = "2005",

month = nov,

doi = "10.1051/0004-6361:200500196",

language = "אנגלית",

volume = "443",

pages = "L1--L5",

journal = "Astronomy and Astrophysics",

issn = "1432-0746",

publisher = "EDP Sciences",

number = "1",

}

Tagliaferri, G, Antonelli, LA, Chincarini, G, Fernandez-Soto, A, Malesani, D, Della Valle, M, D'Avanzo, P, Grazian, A, Testa, V, Campana, S, Covino, S, Fiore, F, Stella, L, Castro-Tirado, AJ, Gorosabel, J, Burrows, DN, Capalbi, M, Cusumano, G, Conciatore, ML, D'Elia, V, Filliatre, P, Fugazza, D, Gehrels, N, Guetta, D, Guziy, S, Held, EV, Hurley, K, Israel, GL, Jelinek, M, Lazzati, D, Lopez-Echarri, A, Melandri, A, Mirabel, IF, Moles, M, Moretti, A, Mason, KO, Nousek, J, Osborne, J, Pellizza, LJ, Perna, R, Piranomonte, S, Piro, L, Postigo, AD & Romano, P 2005, 'GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang: Observations of the oldest cosmic explosion after the Big Bang', Astronomy and Astrophysics, vol. 443, no. 1, pp. L1-L5. https://doi.org/10.1051/0004-6361:200500196

TY - JOUR

T1 - GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang

T2 - Observations of the oldest cosmic explosion after the Big Bang

AU - Tagliaferri, G

AU - Antonelli, LA

AU - Chincarini, G

AU - Fernandez-Soto, A

AU - Malesani, D

AU - Della Valle, M

AU - D'Avanzo, P

AU - Grazian, A

AU - Testa, V

AU - Campana, S

AU - Covino, S

AU - Fiore, F

AU - Stella, L

AU - Castro-Tirado, AJ

AU - Gorosabel, J

AU - Burrows, DN

AU - Capalbi, M

AU - Cusumano, G

AU - Conciatore, ML

AU - D'Elia, V

AU - Filliatre, P

AU - Fugazza, D

AU - Gehrels, N

AU - Guetta, D

AU - Guziy, S

AU - Held, EV

AU - Hurley, K

AU - Israel, GL

AU - Jelinek, M

AU - Lazzati, D

AU - Lopez-Echarri, A

AU - Melandri, A

AU - Mirabel, IF

AU - Moles, M

AU - Moretti, A

AU - Mason, KO

AU - Nousek, J

AU - Osborne, J

AU - Pellizza, LJ

AU - Perna, R

AU - Piranomonte, S

AU - Piro, L

AU - Postigo, AD

AU - Romano, P

PY - 2005/11

Y1 - 2005/11

N2 - We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB 050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4 × 1053 erg in the rest-frame 110-1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at tb = 2.6 ± 1.0 d (observer frame). If we assume this is the jet break, we derive a beaming-corrected energy Eγ ∼ (4 ÷ 12) × 1051 erg. This limit shows that GRB 050904 is consistent with the Amati and Ghirlanda relations. This detection is consistent with the expected number of GRBs at z > 6 and shows that GRBs are a powerful tool to study the star formation history UD to very high redshift.

AB - We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB 050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4 × 1053 erg in the rest-frame 110-1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at tb = 2.6 ± 1.0 d (observer frame). If we assume this is the jet break, we derive a beaming-corrected energy Eγ ∼ (4 ÷ 12) × 1051 erg. This limit shows that GRB 050904 is consistent with the Amati and Ghirlanda relations. This detection is consistent with the expected number of GRBs at z > 6 and shows that GRBs are a powerful tool to study the star formation history UD to very high redshift.

KW - cosmology : observations

KW - early Universe

KW - gamma rays : bursts

KW - gamma rays : individual : GRB 050904

UR - https://www.scopus.com/pages/publications/27844496714

U2 - 10.1051/0004-6361:200500196

DO - 10.1051/0004-6361:200500196

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

SN - 1432-0746

VL - 443

SP - L1-L5

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

GRB050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang: Observations of the oldest cosmic explosion after the Big Bang

Abstract

Keywords

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