Scaling relations at the central regions of nearby galaxies

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Table A.1.

Properties of the sample of galaxies.

Galaxy	Morphological Type	Distance (Mpc)	Inclination (deg)	log M* (Msun)	Nuclear Activity	r (pc)	FOV size (pc)
NGC 134	SAB(s)bc	18.3^a	90	9.92	L	20.41	266 × 395
NGC 157	SAB(rs)bc	12.9^b	61.8	10.99	T	10.63	175 × 275
NGC 247	SAB(s)d	3.34^c	76.4	9.28	HII/T/S	3.89	47 × 72
NGC 253	SAB(s)c	3.05^c	90	10.76	T	3.40	41 × 63
NGC 300	SA(s)d	2.17^a	48.5	9.19	–	2.52	34 × 49
NGC 613	SB(rs)bc	21.4^d	35.7	11.08	L	25.94	311 × 394
NGC 720	E5	30.7^e	90	11.02	HII/T/L/S	95.26	432 × 707
NGC 908	SA(s)c	18.5^a	64.7	10.74	HII	25.11	287 × 377
NGC 936	SB0	19.9^f	50.4	10.926¹	L	29.91	251 × 410
NGC 1068	(R)SA(rs)b	10.1^d	34.7	10.861¹	S	17.63	135 × 235
NGC 1097	SB(s)b	15.4^a	54.8	10.87	L/S	17.17	202 × 317
NGC 1187	SB(r)c	21.4^a	44.1	10.38	HII	29.05	311 × 451
NGC 1232	SAB(rs)c	14.5^d	32.7	10.38	–	58.35	928 × 422
NGC 1291	(R)SB0/a(s)	8.6^g	29.3	10.75	L	10.42	100 × 167
NGC 1300	SB(rs)bc	14.5^d	61.8	10.3²	L	14.06	218 × 323
NGC 1313	SB(s)d	3.7^g	34.8	9.35	HII	4.84	55 × 75
NGC 1316	SAB0	20.8^h	67.8	11.84³	L/S	37.31	313 × 439
NGC 1365	SB(s)b	13.6^a	62.6	11.02	S	18.46	181 × 254
NGC 1380	SA0	20.6ⁱ	90	10.93	L	49.94	295 × 444
NGC 1395	E2	24.3^f	47.4	11.02	HII/T/L/S	49.48	359 × 501
NGC 1398	(R’)SB(r)ab	28.6^a	47.5	11.14	L	24.96	416 × 610
NGC 1399	E1	21.1ⁱ	34.2	11.11	HII/T/S	48.08	286 × 455
NGC 1404	E1	19^e	44.7	10.99⁴	HII/T/S	32.24	258 × 428
NGC 1407	E0	25.1^j	30.3	11.21	–	43.81	341 × 578
NGC 1433	(R’)SB(r)ab	8.32^c	67.4	10.04	L/S	10.49	119 × 169
NGC 1549	E0-1	16.3^e	42.3	10.91	–	25.29	237 × 332
NGC 1553	SA0	9.51^e	56.6	11.09	L/S	13.83	104 × 166
NGC 1559	SB(s)cd	11.6^a	59.9	10.43	HII	11.81	163 × 236
NGC 1566	SAB(s)bc	18^k	49.1	9.98	S	30.54	275 × 358
NGC 1574	SA0	20.1^f	76.6	10.84	L/S	38.98	283 × 419
NGC 1672	SB(s)b	11.4^l	28.9	10.65	S	11.05	133 × 232
NGC 1792	SA(rs)bc	10.8^a	63.1	10.39	HII	13.09	152 × 220
NGC 1808	(R)SAB(s)a	9.51^a	82.7	10.68	T	10.14	122 × 191
NGC 2442	SAB(s)bc	20.1^m	50.3	10.8	L	29.23	287 × 390
NGC 2835	SB(rs)c	8.75ⁿ	56.2	9.97	HII/T/L/S	7.64	121 × 163
NGC 2997	SAB(rs)c	13.1^d	53.7	10.31	L	16.51	187 × 273
NGC 3115	S0	9.68^o	90	10.73	T/L/S	15.49	106 × 209
NGC 3585	E6	13.1^e	90	10.98	T	18.42	197 × 289
NGC 3621	SA(s)d	6.4^a	67.6	10.12	L/S	6.21	92 × 140
NGC 3923	E4-5	16^e	90	11.06	–	27.93	240 × 345
NGC 4030	SA(s)bc	29.9ⁿ	47	11.01	HII/L	37.69	435 × 623
NGC 4594	SA(s)a	21.7^p	59.4	11.1	L	37.87	316 × 500
NGC 4697	E6	12.4ⁿ	90	10.9³	L/S	13.23	150 × 246
NGC 4699	SAB(rs)b	19.5^a	42.1	11.2	L/S	30.25	279 × 425
NGC 4753	I0	24.1ⁿ	78.2	10.98	L/S	26.87	310 × 508
NGC 5068	SAB(rs)cd	6.7^g	27.3	9.56	HII	4.22	94 × 133
NGC 5102	SA0	4^o	90	9.48	HII/T/L/S	4.07	59 × 86
NGC 5128	S0	3.53^q	45.3	10.67	L/S	22.25	488 × 770
NGC 5236	SAB(s)c	4.79^r	15.3	10.64	HII/L	5.11	63 × 101
NGC 5247	SA(s)bc	22.2^g	38.5	10.55	HII/T/L/S	20.45	344 × 457
NGC 5643	SAB(rs)c	16.9^g	29.6	–	S	16.39	254 × 348
NGC 6744	SAB(r)bc	7.66^a	53.5	10.69	L	6.31	117 × 150
NGC 7090	SBc	6.22^a	90	9.81	HII	6.63	90 × 122
NGC 7213	SA(s)a	22^g	39.1	11	L	37.33	251 × 363
NGC 7424	SAB(rs)cd	11.5^g	59	9.24	HII	10.59	176 × 237
NGC 7793	SA(s)d	3.73^a	63.5	9.48	HII	3.80	58 × 80
IC 1459	E3-4	28.7ⁿ	74	11.5³	L	54.27	404 × 633

Notes. The galaxies morphological types were taken from de Vaucouleurs et al. (1991). The distances of the galaxies were taken from: (a) Tully et al. (2016), (b) Erwin & Debattista (2017), (c) Tully et al. (2009), (d) Nasonova et al. (2011), (e) Springob et al. (2014), (f) Blakeslee et al. (2001), (g) Tully & Fisher (1988), (h) Cantiello et al. (2013), (i) Blakeslee et al. (2010), (j) Cantiello et al. (2005), (k) Sabbi et al. (2018), (l) Bottinelli et al. (1986), (m) Riess et al. (2016), (n) Tully et al. (2013), (o) Tonry et al. (2001), (p) Sorce et al. (2014), (q) Theureau et al. (2007), and (r) Pierce (1994). The total stellar mass were mainly taken from Biteau (2021), and the others were taken from (1) Sheth et al. (2010), (2) Davis et al. (2019), (3) Greene et al. (2020), and (4) Harris et al. (2020). The nuclear activity was taken from Paper I (Menezes et al. 2022), L states for Low Ionization Nuclear Emission-Line Regions (LINERs), HII states for HII regions, T for transition objects, and S for Seyferts. The radius (r), for which the nuclear spectra were obtained, is also shown in pc, together with the x and y axis of the FoVs of each data cube. The galaxies inclinations were taken from Hyperleda (Makarov et al. 2014).

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