The neutral gas extent of galaxies as derived from weak intervening Ca ii absorbers

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Volume 528 (April 2011)

A&A, 528 (2011) A12

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Table 3

Supplementary information for selected absorbers in our sample.

QSO	z_abs	log N(H i)^a	Absorber type	Galaxy type	d	L/L_⊙	Ref.
		(N in [cm^-2])			[kpc]

J121509+330955	0.00396	20.34	DLA	Early Type	7.9	0.44	a
J215501-092224	0.08091	17.98	LLS	Spiral	34.0	0.50	b
J044117-431343	0.10114	20.00	sub-DLA	Disk	6.8	1.00	c, d, e
J095456+174331	0.23782	21.32	DLA	Dwarf LSB	≤ 3.9	0.02	f
J113007-144927	0.31273	21.71	DLA	Group (tidal debris)	17 − 241	...	f,d,g,h
J123200-022404	0.39498	20.75	DLA	Irr. LSB	6.6	0.17	i
J045608-215909	0.47439	19.50	sub-DLA	...	...	...	j

Notes.

^(a)

From H i Ly α absorption.

References. (a) Miller et al. (1999); (b) Jenkins et al. (2003); (c) Petitjean et al. (1996); (d) Chen & Lanzetta (2003); (e) Chen et al. (2005); (f) Rao et al. (2003); (g) Lane et al. (1998); (h) Kacprzak, Murphy & Churchill (2010b); (i) Le Brun et al. (1997); (j) Turnshek & Rao (2002).

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