The extinction law at high redshift and its implications

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Volume 523 (November-December 2010)

A&A, 523 (2010) A85

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Table A.1

Unreddened quasars.

Name	z	α _λ,Noext

SDSS J1030	6.28	−2.05	1.00
CFHQS 1509^a	6.12	−1.29	0.71
SDSS J1602	6.07	−0.82	1.00
SDSS J1630	6.06	−1.71	0.08
SDSS J1306	5.99	−2.27	0.19
SDSS J1411	5.93	−1.66	0.88
SDSS J0836	5.80	−1.87	0.97
SDSS J0005	5.85	−1.42	1.00
SDSS J0002	5.80	−1.60	0.06
SDSS J1044^a	5.78	−1.65	0.32
SDSS J02313	5.41	−2.71	0.33
SDSS J1614	5.31	−1.22	1.00
SDSSp J1208	5.27	−2.62	0.59
SDSS J0957	5.16	−2.66	0.36
SDSS J0756^b	5.05	−1.64	0.98
SDSS J1204	5.05	−2.10	0.24
SDSS J0017^a	5.01	−1.95	0.10
SDSS J0338	5.00	−1.87	0.42
SDSS J2216	4.99	−1.49	0.45
SDSS J1605^a,^c	4.92	−1.33	1.00
SDSS J2200	4.77	−1.37	0.48
SDSS J0120^a	4.73	−1.21	1.00
SDSSp J1021	4.70	−1.01	0.86
SDSS J1603	4.39	−1.78	0.82
SDSS J0156^a	4.32	−1.22	0.91
SDSS J0239^a	4.02	−1.39	1.00

Notes.

^(a)

BAL quasars.

^(b)

For this spectrum we find a P(χ²) ~0.6 in the case of reddening by an extinction curve given by 30% SMC + 70% PISN2.

^(c)

For this spectrum we find a P(χ²) ~0.6 in the case of reddening by an extinction curve given by 70% SMC + 30% H2.

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