Understanding the two-dimensional ionization structure in luminous infrared galaxies - A near-IR integral field spectroscopy perspective

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Volume 578 (June 2015)

A&A, 578 (2015) A48

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Table 4

H₂ 2.12 μm/Brγ line ratio for all LIRGS. Statistical results from SINFONI/IFS measurements.

Object	Median		Mode		Mean		σ		P₅		P₉₅		N_spaxel
	Obs	Corr	Obs	Corr	Obs	Corr	Obs	Corr	Obs	Corr	Obs.	Corr

NGC 2369	1.08	1.21	1.18	1.32	1.19	1.33	0.59	0.66	0.55	0.60	2.30	2.57	1583
NGC 3110	0.80	0.84	0.80	0.80	0.85	0.89	0.33	0.34	0.43	0.46	1.46	1.53	2719
NGC 3256	1.00	1.04	1.09	1.28	1.20	1.24	0.82	0.84	0.33	0.34	2.90	2.96	5553
ESO320-G030	0.74	0.76	0.69	0.69	0.99	1.02	0.84	0.86	0.35	0.36	2.46	2.53	4011
IRASF 12115-4656	0.69	0.73	0.74	0.74	0.73	0.77	0.25	0.26	0.39	0.41	1.20	1.25	3526
NGC 5135 (all)	1.31	1.37	1.88	1.88	1.45	1.52	0.84	0.87	0.48	0.50	2.89	3.01	1610
NGC 5135 ([SiVI])^a	1.46	1.53	1.99	1.98	1.54	1.61	0.76	0.79	0.55	0.58	2.82	2.91	898
NGC 5135 (no [SiVI])^b	1.09	1.14	0.68	0.80	1.34	1.40	0.92	0.95	0.44	0.46	2.93	3.06	712
IRASF 17138-1017	0.65	0.68	0.58	0.93	0.76	0.79	0.45	0.47	0.22	0.23	1.61	1.68	2327
IC 4687	0.540	0.56	0.61	0.61	0.57	0.59	0.29	0.31	0.17	0.18	1.13	1.17	4212
NGC 7130 (all)	1.05	1.10	1.11	1.11	1.42	1.47	1.24	1.28	0.26	0.27	4.20	4.33	1857
NGC 7130 ([SiVI])^a	1.79	1.88	1.23	1.22	2.31	2.42	1.42	1.44	0.95	1.06	5.15	5.31	498
NGC 7130 (no [SiVI])^b	0.76	0.79	0.61	1.11	1.09	1.12	0.98	1.01	0.23	0.24	3.12	3.21	1359
IC 5179	0.71	0.73	0.84	0.84	0.78	0.80	0.37	0.38	0.32	0.33	1.46	1.49	4490

LIRGs	0.77	0.80	0.79	0.67	0.97	1.01	0.73	0.75	0.29	0.30	2.30	2.38	31888

Notes. Columns indicate statistical results for the distribution of the observed ratios (obs) and of the extinction corrected values (corr). Last column (N_spaxels )gives the number of spaxels for each galaxy.

^(a)

Statistics using only the spaxels where [SiVI]1.96 μm emission line has been detected.

^(b)

Statistics using all the spaxels within the field-of-view with no [SiVI]1.96 μm emission line detected.

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