Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs: II. Star formation rates and metallicities at z < 1

被引：0

作者：

Japelj, J. ^{[1
,2
]}

Vergani, S.D. ^{[3
,4
,5
]}

Salvaterra, R. ^{[6
]}

D'Avanzo, P. ^{[4
]}

Mannucci, F. ^{[7
]}

Fernandez-Soto, A. ^{[8
,9
]}

Boissier, S. ^{[10
]}

Hunt, L.K. ^{[7
]}

Atek, H. ^{[11
,12
]}

Rodríguez-Muñoz, L. ^{[13
,14
]}

Scodeggio, M. ^{[6
]}

Cristiani, S. ^{[1
]}

Le Floc'h, E. ^{[15
]}

Flores, H. ^{[3
]}

Gallego, J. ^{[13
]}

Ghirlanda, G. ^{[4
]}

Gomboc, A. ^{[2
,16
]}

Hammer, F. ^{[3
]}

Perley, D.A. ^{[17
]}

Pescalli, A. ^{[4
]}

Petitjean, P. ^{[5
]}

Puech, M. ^{[3
]}

Rafelski, M. ^{[18
]}

Tagliaferri, G. ^{[4
]}

机构：

[1] INAF, Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, Trieste,34131, Italy

[2] Faculty of Mathematics and Physics, University of Ljubljana, Jadranska ulica 19, Ljubljana,1000, Slovenia

[3] GEPI, Observatoire de Paris Meudon, 5 place Jules Jannsen, Meudon,92195, France

[4] INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, Merate,23807, Italy

[5] Institut d'Astrophysique de Paris, Université Paris 6, CNRS, UMR7095, 98bis boulevard Arago, Paris,75014, France

[6] INAF, IASF Milano, via E. Bassini 15, Milano,20133, Italy

[7] INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze,50125, Italy

[8] Instituto de Física de Cantabria (CSIC-UC), Santander,39005, Spain

[9] Unidad Asociada Observatori Astronómic, IFCA, Universitat de Valéncia, Valencia, Spain

[10] Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, Marseille,13388, France

[11] Laboratoire d'Astrophysique, École Polytechnique Fédérale de Lausanne, Observatoire de Sauverny, Versoix,1290, Switzerland

[12] Department of Astronomy, Yale University, 260 Whitney Avenue, New Haven,CT,06511, United States

[13] Departamento de Astrofísica y Ciencias de la Atmósfera, Universidad Complutense de Madrid, Madrid,28040, Spain

[14] Dipartimento di Fisica e Astronomia 'G. Galilei', Università di Padova, Vicolo dell'Osservatorio 3, Padova,35122, Italy

[15] Laboratoire AIM, IRFU, Service d'Astrophysique, CEA/DSM, CNRS, Université Paris Diderot, CEA-Saclay, Bât. 709, Gif-sur-Yvette Cedex,91191, France

[16] Faculty of Sciences, University of Nova Gorica, Vipavska cesta 11c, Ajdovščina,5270, Slovenia

[17] Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, Copenhagen,2100, Denmark

[18] NASA, Postdoctoral Program, Goddard Space Flight Center, Greenbelt,MD,20771, United States

来源：

Astronomy and Astrophysics | 2016年 / 590卷

关键词：

Dust extinctions - Galaxies: star formation - Gamma ray burst: generals - Gamma ray bursts - Star formation rates - Star formations - Star forming galaxy - Starburst galaxies;

D O I：

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中图分类号：

学科分类号：

摘要：

Aims. Long gamma-ray bursts (LGRBs) are associated with the deaths of massive stars and might therefore be a potentially powerful tool for tracing cosmic star formation. However, especially at low redshifts (z ∗. The distributions of the obtained properties and their interrelations (e.g. mass-metallicity and SFR-M∗ relations) are compared to samples of field star-forming galaxies. Results. We find that LGRB hosts at z © 2016 ESO.

引用

共 6 条

[1] Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs II. Star formation rates and metallicities at z < 1
Japelj, J.
Vergani, S. D.
Salvaterra, R.
D'Avanzo, P.
Mannucci, F.
Fernandez-Soto, A.
Boissier, S.
Hunt, L. K.
Atek, H.
Rodriguez-Munoz, L.
Scodeggio, M.
Cristiani, S.
Le Floc'h, E.
Flores, H.
Gallego, J.
Ghirlanda, G.
Gomboc, A.
Hammer, F.
Perley, D. A.
Pescalli, A.
Petitjean, P.
Puech, M.
Rafelski, M.
Tagliaferri, G.
ASTRONOMY & ASTROPHYSICS, 2016, 590
[2] Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs
Palmerio, J. T.
Vergani, S. D.
Salvaterra, R.
Sanders, R. L.
Japelj, J.
Vidal-Garcia, A.
D'Avanzo, P.
Corre, D.
Perley, D. A.
Shapley, A. E.
Boissier, S.
Greiner, J.
Le Floc'h, E.
Wiseman, P.
ASTRONOMY & ASTROPHYSICS, 2019, 623
[3] Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of LGRBs I. Stellar mass at z < 1
Vergani, S. D.
Salvaterra, R.
Japelj, J.
Le Floc'h, E.
D'Avanzo, P.
Fernandez-Soto, A.
Kruehler, T.
Melandri, A.
Boissier, S.
Covino, S.
Puech, M.
Greiner, J.
Hunt, L. K.
Perley, D.
Petitjean, P.
Vinci, T.
Hammer, F.
Levan, A.
Mannucci, F.
Campana, S.
Flores, H.
Gomboc, A.
Tagliaferri, G.
ASTRONOMY & ASTROPHYSICS, 2015, 581
[4] THE HOST GALAXIES OF SHORT-DURATION GAMMA-RAY BURSTS: LUMINOSITIES, METALLICITIES, AND STAR FORMATION RATES
Berger, E.
ASTROPHYSICAL JOURNAL, 2009, 690 (01): : 231 - 237
[5] Low radio-derived star formation rates in z < 0.5 gamma-ray burst host galaxies
Stanway, Elizabeth R.
Davies, Luke J. M.
Levan, Andrew J.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 409 (01) : L74 - L78
[6] Constraints on the z ∼ 5 Star-forming Galaxy Luminosity Function From Hubble Space Telescope Imaging of an Unbiased and Complete Sample of Long Gamma-Ray Burst Host Galaxies
Sears, Huei
Chornock, Ryan
Strader, Jay
Perley, Daniel A.
Blanchard, Peter K.
Margutti, Raffaella
Tanvir, Nial R.
ASTROPHYSICAL JOURNAL, 2024, 966 (01):

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