The baryonic Tully-Fisher relation and its implication for dark matter halos

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Volume 505 / No 2 (October II 2009)

A&A, 505 2 (2009) 577-587

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Table 1:

Properties of the data.
ID	Date	length	${b_{\rm maj}}$	${b_{\rm min}}$	PA	Noise/channel	Pixel size	Channel width
	of Obs.	of Obs.	$^{\prime\prime}$	$^{\prime\prime}$	$^\circ$	${\rm ~mJy\ beam^{-1}}$	$^{\prime\prime}$	km s^-1
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
D500-2	01-05-2002	12h	25.0	10.6	0.0	1.0	5	4.12
D500-3	03-05-2002	12h	33.0	12.3	0.0	0.6	5	4.12
D512-2	16-05-2004	12h	28.9	13.4	0.6	0.9	4	2.10
D564-8	08-05-2002	12h	36.4	12.8	0.0	0.6	5	4.12
D572-5	10-05-2004	12h	86.6	24.0	-0.2	1.2	4	2.10
D575-1^a	07-05-2004	12h	48.2	18.4	0.2	0.9	4	2.10
$\cdots$	12-05-2004	12h	$\cdots$	$\cdots$	$\cdots$	$\cdots$	$\cdots$	$\cdots$
D575-2^b	09-05-2004	12h	45.6	14.0	-3.5	0.6	4	2.10
$\cdots$	13-05-2004	10h	$\cdots$	$\cdots$	$\cdots$	$\cdots$	$\cdots$	$\cdots$
$\cdots$	17-10-2004	7h	$\cdots$	$\cdots$	$\cdots$	$\cdots$	$\cdots$	$\cdots$
D575-5	05-05-2004	12h	37.5	11.3	-0.1	1.1	4	2.10
D631-7	04-11-2004	12h	57.7	12.0	0.2	1.1	4	2.10
D640-13	10-11-2004	12h	70.8	11.5	-0.1	1.1	4	2.10
D646-7	11-05-2004	12h	133.8	20.6	0.6	1.4	4	2.10

^a The data for D575-1 are combined from two individual observations.
^b The data for D575-2 are combined from three individual observations.
Notes: (1) galaxy identifier; (2) date of observations; (3) length of observations; (4, 5) major and minor axis diameter of the robust weighted beam in arcsec; (6) position angle of the beam (in degrees), measured counter-clockwise from the north; (7) noise per channel in mJy beam^-1; (8) pixel size in arcsec; (9) channel width in km s^-1.

Source LaTeX | All tables | In the text

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