PHANGS–MUSE: The H II region luminosity function of local star-forming galaxies

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Volume 658 (February 2022)

A&A, 658 (2022) A188

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Table 1.

Main properties of the galaxies in the PHANGS–MUSE sample.

Galaxy	RA	Dec	Morph⁽¹⁾	Distance⁽²⁾	i⁽³⁾	PA⁽³⁾	Log M_(∗)⁽⁴⁾	SFR⁽⁴⁾	Δ_SFMS⁽⁴⁾	R₂₅⁽¹⁾	FWHM_PSF⁽⁵⁾	pc/″	r_max
	(°)	(°)		(Mpc)	(°)	(°)	(M_⊙)	(M_⊙ yr⁻¹)		(″)	(″)
IC 5332	353.61453	−36.10108	SABc	9.01	26.9	74.4	9.67	0.41	0.01	182	0.87	43.6	0.68
NGC 0628	24.173855	15.783643	Sc	9.84	8.9	20.7	10.34	1.75	0.18	297	0.92	47.6	0.51
NGC 1087	41.60492	−0.498717	Sc	15.85	42.9	359.1	9.93	1.31	0.33	89	0.92	76.5	1.37
NGC 1300	49.920815	−19.411114	Sbc	18.99	31.8	278.0	10.62	1.17	−0.18	178	0.89	91.6	0.96
NGC 1365	53.40152	−36.140404	Sb	19.57	55.4	201.1	10.99	16.90	0.72	361	1.15	94.4	0.73
NGC 1385	54.369015	−24.501162	Sc	17.22	44.0	181.3	9.98	2.09	0.50	102	0.67	83.1	1.21
NGC 1433	55.506195	−47.221943	SBa	18.63	28.6	199.7	10.87	1.13	−0.36	186	0.91	89.9	1.05
NGC 1512	60.975574	−43.348724	Sa	18.83	42.5	261.9	10.71	1.28	−0.21	253	1.25	90.8	0.62
NGC 1566	65.00159	−54.93801	SABb	17.69	29.5	214.7	10.78	4.54	0.29	217	0.8	85.3	0.73
NGC 1672	71.42704	−59.247257	Sb	19.4	42.6	134.3	10.73	7.60	0.56	185	0.96	93.5	1.00
NGC 2835	139.47044	−22.35468	Sc	12.22	41.3	1.0	10.00	1.24	0.26	192	1.15	59.0	0.69
NGC 3351	160.99065	11.70367	Sb	9.96	45.1	193.2	10.36	1.32	0.05	217	1.05	48.2	0.76
NGC 3627	170.06252	12.9915	Sb	11.32	57.3	173.1	10.83	3.84	0.19	308	1.05	54.7	0.66
NGC 4254	184.7068	14.416412	Sc	13.1	34.4	68.1	10.42	3.07	0.37	151	0.89	63.3	1.28
NGC 4303	185.47888	4.473744	Sbc	16.99	23.5	312.4	10.52	5.33	0.54	207	0.78	82.0	0.66
NGC 4321	185.72887	15.822304	SABb	15.21	38.5	156.2	10.75	3.56	0.21	183	1.16	73.4	0.97
NGC 4535	188.5846	8.197973	Sc	15.77	44.7	179.7	10.53	2.16	0.14	244	0.56	76.1	0.56
NGC 5068	199.72807	−21.038744	Sc	5.2	35.7	342.4	9.40	0.28	0.02	224	1.04	25.2	0.89
NGC 7496	347.44702	−43.42785	Sb	18.72	35.9	193.7	10.00	2.26	0.53	100	0.89	90.3	1.06

Notes. The table reports the galaxy name (Col. 1), galaxy center sky coordinates (Cols. 2–3), Hubble morphological type (Col. 4), distance (Col. 5), inclination (Col. 6), position angle (Col. 7), total stellar mass (Col. 8), total SFR (Col. 9), offset from the star formation main sequence (Col. 10), R₂₅B-band isophotal radius (Col. 11), angular resolution of the copt data (Col. 12), the parsec per arcsecond scaling factor (Col. 13), and the maximum deprojected galactocentric radius in units of R₂₅ (Col. 14).

References.⁽¹⁾HyperLEDA, Makarov et al. (2014), ⁽²⁾Anand et al. (2021), ⁽³⁾Lang et al. (2020), ⁽⁴⁾Leroy et al. (2021), ⁽⁵⁾Emsellem et al. (2021)

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