2007MNRAS.379L..55L


Query : 2007MNRAS.379L..55L

2007MNRAS.379L..55L - Mon. Not. R. Astron. Soc., 379, L55-L59 (2007/July-3)

Variation of the Amati relation with cosmological redshift: a selection effect or an evolution effect ?

LI L.-X.

Abstract (from CDS):

Because of the limit in the number of gamma-ray bursts (GRBs) with available redshifts and spectra, all current investigations on the correlation among GRB variables use burst samples with redshifts that span a very large range. Evolution and selection effects have thus been ignored, which might have an important influence on the results. In this Letter, we divide the 48 long-duration GRBs studied by Amati into four groups with redshift from low to high, each group containing 12 GRBs. Then we fit each group with the Amati relation logEiso= a + blogEpeak, and check whether the parameters a and b evolve with the GRB redshift. We find that a and b vary with the mean redshift of the GRBs in each group systematically and significantly. Monte Carlo simulations show that there is only a ∼4 per cent chance that the variation is caused by the selection effect arising from the fluence limit. Hence our results may indicate that GRBs evolve strongly with cosmological redshift.

Abstract Copyright: 2007 The Author. Journal compilation © 2007 RAS

Journal keyword(s): cosmology: theory - gamma-rays: bursts - gamma-rays: observations

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GRB 061007 gB 03 05 19.510 -50 30 02.50 14.28 14.40 12.95     ~ 315 1
2 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
3 GRB 060115 gB 03 36 08.400 +17 20 43.00           ~ 179 0
4 GRB 060124 gB 05 08 25.900 +69 44 26.98   18.91 17.35     ~ 280 0
5 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
6 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 330 0
7 GRB 060418 gB 15 45 42.600 -03 38 20.00 15.73 16.19 14.98     ~ 389 0
8 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
9 GRB 060927A gB 21 58 11.930 +05 21 50.32           ~ 215 0
10 GRB 060707 gB 23 48 19.000 -17 54 17.00     19.79     ~ 170 0

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