The Epeak – Eiso relation revisited with Fermi GRBs - Resolving a long-standing debate?

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Volume 557 (September 2013)

A&A, 557 (2013) A100

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Table A.1

43 GRBs with a redshift.

GRB Name	z ^*	α	α	β ^†	β	E _po ^**	E _po	Fluence, S_γ	Fluence
			error		error	(keV)	error	(10^-7 erg cm^-2)	error

GRB 080804972	2.20^a	–0.52	0.09	–1.90	0.08	218^ba	25	91.3	1.1
GRB 080810549	3.35^b	–1.16	0.03	–2.30		834^ba	125	108.2	0.5
GRB 080905705	2.37^c	–0.85	0.23	–2.28	0.62	179^ba	60	29.1	0.4
GRB 080916009	4.35^d	–1.08	0.01	–2.15	0.07	662^ba	45	602.7	0.7
GRB 080916406	0.69^e	–0.90	0.10	–2.30		109^bb	9	78.1	0.8

GRB 081008832	1.97^f	–1.01	0.12	–2.09	0.21	166^ba	36	103.2	1.5
GRB 081121858	2.51^g	–0.43	0.13	–2.09	0.09	161^ba	17	152.7	2.2
GRB 081221681	2.26^h	–0.90	0.02	–3.86	0.49	87^ba	1	300.4	0.9
GRB 081222204	2.77ⁱ	–0.86	0.05	–2.31	0.12	142^ba	10	118.9	1.0
GRB 090102122	1.55^j	–0.94	0.02	–2.30		417^ba	18	279.1	0.6

GRB 090323002	3.57^k	–1.29	0.01	–2.45	0.18	639^ba	41	1180.9	1.7
GRB 090328401	0.74 ^l	–1.13	0.01	–2.65	0.26	1458^ba	74	420.2	0.7
GRB 090424592	0.54^m	–1.04	0.02	–2.76	0.13	154^ba	4	463.2	0.4
GRB 090516353	4.11ⁿ	–1.52	0.05	–2.30	0.27	142^ba	26	172.2	0.6
GRB 090618353	0.54^o	–1.26	0.06	–2.50	0.33	156^bc	11	2684.5	4.3

GRB 090902462	1.82^p	–1.00	0.00	–2.30		1044^ba	17	2217.9	3.2
GRB 090926181	2.11^q	–0.85	0.01	–2.39	0.04	336^ba	6	1465.7	3.4
GRB 090926914	1.24^r	0.13	0.12	–3.25	0.34	82^ba	3	107.9	1.5
GRB 091003191	0.90^s	–1.07	0.02	–2.22	0.11	366^ba	27	233.2	0.8
GRB 091020900	1.71^t	–1.26	0.06	–2.30		246^ba	36	83.5	1.5

GRB 091127976	0.49^u	–1.26	0.07	–2.22	0.02	35^ba	2	207.3	0.4
GRB 091208410	1.06^v	–1.44	0.07	–2.32	0.47	124^bd	20	61.9	1.9
GRB 100414097	1.37^w	–0.62	0.01	–3.53	0.48	664^ba	16	884.7	1.9
GRB 100615083	1.40^x	–1.24	0.08	–2.27	0.12	86^be	8	87.2	0.8
GRB 100728095	1.57^y	–0.75	0.01	–3.04	0.57	344^bf	9	1278.8	5.8

GRB 100728439	2.11^z	–0.80	0.20	–2.20	0.20	104^bg	14	33.4	0.6
GRB 100814160	1.44^aa	–0.64	0.14	–2.02	0.12	106^bh	14	149.4	0.9
GRB 100906576	1.73^ab	–1.34	0.08	–1.98	0.07	106^bi	18	232.9	0.6
GRB 101213451	0.41^ac	–1.10	0.07	–2.35	0.72	310^bj	49	74.0	1.0
GRB 101219686	0.55^ad	0.33	0.36	–2.12	0.12	70^bk	8	39.9	0.5

GRB 110731465	2.83^ae	–0.80	0.03	–2.98	0.30	304^bl	13	228.9	0.6
GRB 111228657	0.71^af	–1.90	0.10	–2.70	0.30	34^bm	3	181.4	0.6
GRB 120119170	1.73^ag	–0.98	0.03	–2.36	0.09	189^bn	8	386.7	1.4
GRB 120326056	1.80^ah	–0.98	0.14	–2.53	0.15	46^bo	4	32.6	0.5
GRB 120711115	1.41^ai	–0.94	0.01	–2.40	0.04	973^bp	35	1942.8	2.3

GRB 120716712	2.49^aj	–1.00	0.08	–2.08	0.07	114^bq	12	146.9	0.5
GRB 120811649	2.67^ak	–0.71	0.20	–2.30		54^br	3	34.5	2.1
GRB 120907017	0.97^al	–0.75	0.25	–2.30		154^bs	33	8.1	0.4
GRB 120909070	3.93^am	–1.30	0.10	–2.30		370^bt	140	98.5	1.5
GRB 121128212	2.20^an	–0.80	0.12	–2.41	0.10	62^bu	5	104.0	4.0

GRB 121211574	1.02^ao	–0.30	0.34	–2.30		96 ^bv	13	4.8	0.5
GRB 130420313	1.30^aq	–1.00	0.13	–2.30		56 ^bw	3	115.9	2.4
GRB 130427324	0.34^ar	–0.79	0.00	–3.06	0.02	830 ^bx	5	24 620.0	12.4

Notes. . The references for the redshift and spectral parameters are given below. The 9 GRBs in italic have been localized by LAT, IPN or INTEGRAL, they are at the bright end of the GRB luminosity function. four GRBs are outliers to the Amati relation, they are indicated in bold. The errors are given for a confidence level of 90%.

^(†)

When β is unconstrained, we use β = −2.3

Reference. – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – – –

^(*)

References for the redshift:

^(a)

Cucchiara et al. (2008c); Thoene et al. (2008)

^(b)

Burenin et al. (2008); de Ugarte Postigo et al. (2008); Prochaska et al. (2008)

^(c)

Vreeswijk et al. (2008)

^(d)

Greiner et al. (2009)

^(e)

Fynbo et al. (2008)

^(f)

D’Avanzo et al. (2008); Cucchiara et al. (2008a)

^(g)

Berger & Rauch (2008)

^(h)

Salvaterra et al. (2012)

⁽ⁱ⁾

Cucchiara et al. (2008b); Graham et al. (2008)

^(j)

Cucchiara & Fox (2009); de Ugarte Postigo et al. (2009b)

^(k)

Chornock et al. (2009)

^(l)

Cenko et al. (2009a)

^(m)

Chornock et al. (2009); Wiersema et al. (2009a)

⁽ⁿ⁾

de Ugarte Postigo et al. (2009a); Rossi et al. (2009)

^(o)

Cenko et al. (2009b); Fatkhullin et al. (2009)

^(p)

Cucchiara et al. (2009c)

^(q)

Malesani et al. (2009)

^(r)

Fynbo et al. (2009)

^(s)

Cucchiara et al. (2009b)

^(t)

Xu et al. (2009)

^(u)

Cucchiara et al. (2009a); Thoene et al. (2009)

^(v)

Perley et al. (2009); Wiersema et al. (2009b)

^(w)

Cucchiara & Fox (2010)

^(x)

Kruehler et al. (2013b)

^(y)

Kruehler et al. (2013a)

^(z)

Flores et al. (2010)

^(aa)

O Meara et al. (2010)

^(ab)

Tanvir et al. (2010)

^(ac)

Chornock & Berger (2011)

^(ad)

de Ugarte Postigo et al. (2011); Sparre et al. (2011)

^(ae)

Tanvir et al. (2011)

^(af)

Cucchiara & Levan (2011); Dittmann et al. (2011); Palazzi et al. (2011); Schulze et al. (2011); Xu et al. (2011)

^(ag)

Cucchiara & Prochaska (2012); Milisavljevic et al. (2012); Pancoast et al. (2012)

^(ah)

Tello et al. (2012)

^(ai)

Tanvir et al. (2012b)

^(aj)

D’Elia et al. (2012); Greiner et al. (2012)

^(ak)

Fynbo et al. (2012); Thoene et al. (2012)

^(al)

Sanchez-Ramirez et al. (2012)

^(am)

Hartoog et al. (2012)

^(an)

Tanvir et al. (2012a)

^(ao)

Perley et al. (2012)

^(ap)

Cucchiara & Fumagalli (2013)

^(aq)

de Ugarte Postigo et al. (2013)

^(ar)

Flores et al. (2010); Garnavich (2013); Levan et al. (2013); Xu et al. (2013).

^(**)

References for the peak energy:

^(ba)

Goldstein et al. (2012)

^(bb)

Bissaldi et al. (2008)

^(bc)

McBreen (2009a)

^(bd)

McBreen (2009b)

^(be)

Foley & Briggs (2010)

^(bf)

^(bg)

^(bh)

^(bi)

^(bj)

^(bk)

^(bl)

^(bm)

Briggs & Younes (2011)

^(bn)

Gruber (2012)

^(bo)

Collazzi (2012)

^(bp)

Gruber & Pelassa (2012)

^(bq)

Gruber & Goldstein (2012)

^(br)

Xiong & Meegan (2012)

^(bs)

Younes & Barthelmy (2012)

^(bt)

^(bu)

^(bv)

^(bw)

^(bx)

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