Millimetre observations of gamma-ray bursts at IRAM

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Standard

Millimetre observations of gamma-ray bursts at IRAM. / Castro-Tirado, A. J.; Bremer, M.; Winters, J. M.; Tello, J. C.; Pandey, S. B.; Ugarte Postigo, Antonio de; Gorosabel, J.; Guziy, S.; Jelinek, M.; Sánchez-Ramírez, R.; Pérez-Ramírez, D.; Castro Cerón, J. M.

I: E A S Publications Series, Bind 61, 01.03.2013, s. 279-281.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Castro-Tirado, AJ, Bremer, M, Winters, JM, Tello, JC, Pandey, SB, Ugarte Postigo, AD, Gorosabel, J, Guziy, S, Jelinek, M, Sánchez-Ramírez, R, Pérez-Ramírez, D & Castro Cerón, JM 2013, 'Millimetre observations of gamma-ray bursts at IRAM', E A S Publications Series, bind 61, s. 279-281. https://doi.org/10.1051/eas/1361045

APA

Castro-Tirado, A. J., Bremer, M., Winters, J. M., Tello, J. C., Pandey, S. B., Ugarte Postigo, A. D., Gorosabel, J., Guziy, S., Jelinek, M., Sánchez-Ramírez, R., Pérez-Ramírez, D., & Castro Cerón, J. M. (2013). Millimetre observations of gamma-ray bursts at IRAM. E A S Publications Series, 61, 279-281. https://doi.org/10.1051/eas/1361045

Vancouver

Castro-Tirado AJ, Bremer M, Winters JM, Tello JC, Pandey SB, Ugarte Postigo AD o.a. Millimetre observations of gamma-ray bursts at IRAM. E A S Publications Series. 2013 mar. 1;61:279-281. https://doi.org/10.1051/eas/1361045

Author

Castro-Tirado, A. J. ; Bremer, M. ; Winters, J. M. ; Tello, J. C. ; Pandey, S. B. ; Ugarte Postigo, Antonio de ; Gorosabel, J. ; Guziy, S. ; Jelinek, M. ; Sánchez-Ramírez, R. ; Pérez-Ramírez, D. ; Castro Cerón, J. M. / Millimetre observations of gamma-ray bursts at IRAM. I: E A S Publications Series. 2013 ; Bind 61. s. 279-281.

Bibtex

@article{adcb02d515ac4e339a750f681a4cc0e5,
title = "Millimetre observations of gamma-ray bursts at IRAM",
abstract = "Since 1997, and following our detection of the first mm afterglow, we have followed-up 70 GRBs, mainly with the IRAM{\AA} Plateau de Bure Interferometer, what can be considered as the IRAM Legacy GRB Sample. 66 events were observed at 3 mm, with 19 of them being detected (with another 3 having marginal detections). 32 GRBs were followed up at 1 mm, with 6 of them being detected. Redshifts for the GRB afterglows lie in the range z = 0.03-8.3, with measured flux densities (at 3 mm) varying between 0.25 and 60 mJy (but usually <1.5 mJy) with first observations taking place around 1-2 days after the GRB. Forward shock emission expleains the observations with the exception of one particular case (GRB 090423 at z = 8.2) for which reverse shock emission is required.",
author = "Castro-Tirado, {A. J.} and M. Bremer and Winters, {J. M.} and Tello, {J. C.} and Pandey, {S. B.} and {Ugarte Postigo}, {Antonio de} and J. Gorosabel and S. Guziy and M. Jelinek and R. S{\'a}nchez-Ram{\'i}rez and D. P{\'e}rez-Ram{\'i}rez and {Castro Cer{\'o}n}, {J. M.}",
year = "2013",
month = mar,
day = "1",
doi = "10.1051/eas/1361045",
language = "English",
volume = "61",
pages = "279--281",
journal = "E A S Publications Series",
issn = "1633-4760",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - Millimetre observations of gamma-ray bursts at IRAM

AU - Castro-Tirado, A. J.

AU - Bremer, M.

AU - Winters, J. M.

AU - Tello, J. C.

AU - Pandey, S. B.

AU - Ugarte Postigo, Antonio de

AU - Gorosabel, J.

AU - Guziy, S.

AU - Jelinek, M.

AU - Sánchez-Ramírez, R.

AU - Pérez-Ramírez, D.

AU - Castro Cerón, J. M.

PY - 2013/3/1

Y1 - 2013/3/1

N2 - Since 1997, and following our detection of the first mm afterglow, we have followed-up 70 GRBs, mainly with the IRAMÅ Plateau de Bure Interferometer, what can be considered as the IRAM Legacy GRB Sample. 66 events were observed at 3 mm, with 19 of them being detected (with another 3 having marginal detections). 32 GRBs were followed up at 1 mm, with 6 of them being detected. Redshifts for the GRB afterglows lie in the range z = 0.03-8.3, with measured flux densities (at 3 mm) varying between 0.25 and 60 mJy (but usually <1.5 mJy) with first observations taking place around 1-2 days after the GRB. Forward shock emission expleains the observations with the exception of one particular case (GRB 090423 at z = 8.2) for which reverse shock emission is required.

AB - Since 1997, and following our detection of the first mm afterglow, we have followed-up 70 GRBs, mainly with the IRAMÅ Plateau de Bure Interferometer, what can be considered as the IRAM Legacy GRB Sample. 66 events were observed at 3 mm, with 19 of them being detected (with another 3 having marginal detections). 32 GRBs were followed up at 1 mm, with 6 of them being detected. Redshifts for the GRB afterglows lie in the range z = 0.03-8.3, with measured flux densities (at 3 mm) varying between 0.25 and 60 mJy (but usually <1.5 mJy) with first observations taking place around 1-2 days after the GRB. Forward shock emission expleains the observations with the exception of one particular case (GRB 090423 at z = 8.2) for which reverse shock emission is required.

U2 - 10.1051/eas/1361045

DO - 10.1051/eas/1361045

M3 - Journal article

AN - SCOPUS:84887104879

VL - 61

SP - 279

EP - 281

JO - E A S Publications Series

JF - E A S Publications Series

SN - 1633-4760

ER -

ID: 120898765