Volume 421, Issue 2 pp. 1256-1264

A complete sample of bright Swift long gamma-ray bursts: testing the spectral-energy correlations

L. Nava

Corresponding Author

L. Nava

SISSA – via Bonomea 265, I-34136 Trieste, Italy

E-mail: [email protected]Search for more papers by this author
R. Salvaterra

R. Salvaterra

INAF – IASF Milano, via E. Bassini 15, I-20133 Milano, Italy

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G. Ghirlanda

G. Ghirlanda

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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G. Ghisellini

G. Ghisellini

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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S. Campana

S. Campana

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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S. Covino

S. Covino

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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G. Cusumano

G. Cusumano

INAF – IASF Palermo, via Ugo La Malfa 153, I-90146 Palermo, Italy

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P. D’Avanzo

P. D’Avanzo

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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V. D’Elia

V. D’Elia

ASI – Science Data Centre, via Galileo Galilei, I-00044 Frascati, Italy

INAF – Osservatorio Astronomico di Roma, via di Frascati 33, 00040 Monte Porzio Catone, Italy

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D. Fugazza

D. Fugazza

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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A. Melandri

A. Melandri

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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B. Sbarufatti

B. Sbarufatti

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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S. D. Vergani

S. D. Vergani

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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G. Tagliaferri

G. Tagliaferri

INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate, Italy

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First published: 21 February 2012
Citations: 5

ABSTRACT

We use a nearly complete sample of gamma-ray bursts (GRBs) detected by the Swift satellite to study the correlations between the spectral peak energy Epeak of the prompt emission, the isotropic energetics Eiso and the isotropic luminosity Liso. This GRB sample is characterized by a high level of completeness in redshift (90 per cent). This allows us to probe in an unbiased way the issue related to the physical origin of these correlations against selection effects. We find that one burst, GRB 061021, is an outlier to the EpeakEiso correlation. Despite this case, we find strong EpeakEiso and EpeakLiso correlations for the bursts of the complete sample. Their slopes, normalizations and dispersions are consistent with those found with the whole sample of bursts with measured redshift and Epeak. This means that the biases present in the total sample commonly used to study these correlations do not affect their properties. Finally, we also find no evolution with redshift of the EpeakEiso and EpeakLiso correlations.

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