Origin and z-distribution of Galactic diffuse [C II] emission

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Volume 572 (December 2014)

A&A, 572 (2014) A45

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Table 2

Summary of the spaxel analysis of spectral line profiles.

Item	Total	H i^† Detections with			[C ii] Detections		¹²CO Detections		¹³CO
	H i	[C ii]	¹²CO	[C ii] and CO	Total	with CO	¹²CO	with [C ii]

3σ detection limit K km s^-16	7.0	7.0	7.0	7.0	0.5	0.5	3.0	3.0	0.5

All data (354 LOS)
Total No. of spaxels	23 229	6484	4421	2705	6484	2705	4421	2705	3653
Intensity (K km s^-1)	3336	1501	1117	794	10 317	5811	61 549	43 236	8159

Spaxels with R_G< 8.5 kpc
Total No. of spaxels	15 278	5711	4197	2609	5711	2609	4197	2609	3448
at b = 0.0°	5198	2356	2096	1388	2356	1388	2096	1388	1792
at b = ±0.5°	5363	1948	1340	826	1948	826	1340	826	1078
at b = ±1.0°	4717	1407	761	395	1407	395	761	395	578
Intensity (K km s^-1)
Total	2524	1377	1059	765	9132	5501	58 790	41 979	7807
at b = 0.0°	985	637	548	422	4272	3006	31 913	23 170	4361
at b = ±0.5°	883	465	338	239	2966	1692	18 082	13 273	2443
at b = ±1.0°	656	275	173	103	1894	803	8795	5536	1004
Spaxels without distance ambiguity
(used for z-distribution)
Total No. of spaxels	11 738	4484	3380	2162	4484	2162	3380	2162	2854
Intensity (K km s^-1)	1918	1098	868	644	7425	4629	49 369	35 773	6722

Notes.

^(†)

All H i intensities are in units of 10³ K km s^-1.

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