Searching for dark clouds in the outer galactic plane - I. A statistical approach for identifying extended red(dened) regions in 2MASS

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Table 1:

Excerpt from the catalog of extended red objects.
FrSh	l	b	$N_{\rm cell}$	$\Delta l$	$\Delta b$	2M
(1)	(2)	(3)	(4)	(5)	(6)	(7)
	deg	deg		pix	pix
H456	111.08	1.44	5	5	4	43
H457	111.27	2.02	41	15	15	299
H458	111.18	1.38	5	3	6	49
H459	111.20	2.17	6	3	5	51
H460	111.22	-0.83	5	3	5	79
H461	111.27	-0.75	4	3	5	68
H462	111.40	1.92	5	3	3	38
H463	111.53	0.78	40	17	9	655
H464	111.47	0.99	16	9	8	122
H465	111.47	1.76	9	7	8	67
H466	111.46	1.97	4	4	3	29
H467	111.48	-0.66	5	5	2	78
H468	111.52	1.89	10	7	6	70
H469	111.59	1.77	13	12	6	80
H470	111.60	0.38	8	5	4	123
H471	111.62	2.17	4	6	2	24
H472	111.64	0.90	4	4	5	32
H473	111.71	0.00	8	6	7	84
H474	111.76	0.74	34	12	20	335
H475	111.83	0.44	20	11	8	162
H476	111.85	1.67	16	11	10	122
H477	111.82	0.35	5	4	5	46
H478	111.99	0.88	52	20	18	468
H479	111.97	1.10	4	5	3	31
H480	112.03	1.52	5	4	4	53
H481	112.05	1.71	4	3	4	29
H482	112.07	0.94	4	3	6	34
H483	112.14	1.42	4	4	2	41
H484	112.24	1.59	11	8	8	101
H485	112.32	2.84	7	5	6	51
H486	112.43	1.55	15	15	7	109

Source LaTeX | All tables | In the text

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