The dust extinction curves of gamma-ray burst host galaxies

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Table 1

continued.

GRB	z	N_H,Gal	A_V,Gal	Epoch	UV/optical/NIR bandpasses	Rest-frame band	Best-fit model
		(10²¹ cm^-2)	(mag)	(ks)		coverage (Å)

080319C	1.95^a	0.22	0.08	0.5	R¹v b u	1310–2260	pow/SMC
080411	1.03^b	0.58	0.10	8	KHJ z′ i′ r′ g′	1900–11420	bknp/MW
080413B	1.10^c	0.31	0.11	0.65	v b u w1 m2 w2	760–2790	bknp/MW
080430	0.767^d	0.10	0.04	10	I^2,3R^3–5v b u w1 m2 w2	910–5010	bknp/SMC
080603B	2.69^e	0.12	0.04	6.5	(KHJ)⁶R^7,8b u	1050–6330	pow/SMC
080710	0.845^f	0.41	0.23	10	(KHJz′i′r′)⁹v g′⁹b u w1 m2 w2	870–12560	pow/SMC
080721	2.591^g	0.69	0.31	6	R¹⁰v b u	1070–2100	bknp/MW
080804	2.204^h	0.16	0.05	1.5	KHJz′i′r′v g′b u	1200–7230	bknp/MW
080810	3.35ⁱ	0.33	0.09	5	I¹¹R^11,12v g¹¹b	900–2030	pow/SMC
080916A	0.689^j	0.18	0.06	6	v b u w1 m2 w2	950–3470	bknp/SMC
080928	1.692^k	0.56	0.21	40	b u w1 m2 w2	590–1810	pow/SMC
081008	1.968^l	0.71	0.29	1	v b u w1	760–1970	pow/LMC
081121	2.512^m	0.40	0.16	10	KHJz′i′r′v g′b u	1100–6600	bknp/SMC
081203A	2.05ⁿ	0.17	0.06	10	I^13,14R^13–16v g^15„16b u w1	740–2900	bknp/MW
081222	2.77^o	0.22	0.06	0.7	KHJz′i′r′v g′b u w1	600–6150	bknp/MW
090102	1.546^p	0.41	0.15	1	KHJz′i′r′v g′b	1530–9100	bknp/MW
090424	0.544^q	0.19	0.08	1	(IR)¹⁷v b u w1 m2 w2	1040–5730	bknp/MW
090618	0.54^r	0.58	0.27	2	v b u w1 m2 w2	1040–3800	bknp/SMC
090927	1.37^s	0.29	0.10	9	v b u w1 m2 w2	680–2470	pow/MW
091018	0.971^t	0.28	0.09	30	KHJz′i′r′v g′b u w1 m2 w2	810–11760	bknp/SMC
091020	1.71^u	0.14	0.05	6	v b u w1 m2 w2	590–2160	pow/LMC
091029	2.752^v	0.11	0.05	1	KHJz′i′r′v g′b u w1	600–6180	bknp/LMC
091127	0.490^w	0.28	0.12	3.7	HJz′i′r′w1 m2	1340–11950	bknp/LMC
091208B	1.063^x	0.49	0.16	6	v b u w1 m2 w2	780–2840	pow/LMC

References.

^(a)

Wiersema et al. (2008);

^(b)

Thoene et al. (2008a);

^(c)

Vreeswijk et al. (2008b);

^(d)

Cucchiara & Fox (2008a);

^(e)

Cucchiara & Fox (2008b);

^(f)

Perley et al. (2008b);

^(g)

Jakobsson et al. (2008b);

^(h)

Thoene et al. (2008c);

⁽ⁱ⁾

Prochaska et al. (2008);

^(j)

Fynbo et al. (2008);

^(k)

Vreeswijk et al. (2008c);

^(l)

Cucchiara et al. (2008a);

^(m)

Berger & Rauch (2008);

⁽ⁿ⁾

Kuin et al. (2009);

^(o)

Cucchiara et al. (2008b);

^(p)

de Ugarte Postigo et al. (2009a);

^(q)

Chornock et al. (2009b);

^(r)

Cenko et al. (2009);

^(s)

Levan et al. (2009);

^(t)

de Ugarte Postigo et al. (2009b);

^(u)

Xu et al. (2009);

^(v)

Chornock et al. (2009a);

^(w)

Cucchiara et al. (2009);

^(x)

Wiersema et al. (2009);

⁽¹⁾

Li et al. (2008a);

⁽²⁾

Thoene et al. (2008b);

⁽³⁾

Terra et al. (2008);

⁽⁴⁾

Andreev et al. (2008);

⁽⁵⁾

Oksanen & Hentunen (2008);

⁽⁶⁾

Miller et al. (2008);

⁽⁷⁾

Klotz et al. (2008a);

⁽⁸⁾

Klotz et al. (2008b);

⁽⁹⁾

Krühler et al. (2009);

⁽¹⁰⁾

Starling et al. (2009);

⁽¹¹⁾

Yoshida et al. (2008);

⁽¹²⁾

Okuma et al. (2008);

⁽¹³⁾

Rumyantsev et al. (2008);

⁽¹⁴⁾

Isogai & Kawai (2008);

⁽¹⁵⁾

Volkov (2008);

⁽¹⁶⁾

Mori et al. (2008);

⁽¹⁷⁾

Kann et al. (2010).

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