Hunting star forming galaxies in the gamma-ray domain

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Table B.1.

Sample of SFGs studied in this work.

Name	d	R.A.	Dec	Revised	IRAS	Ackermann	Ṁ_∗	4FGL Name	ℱ_2 GeV	CTAO	LHAASO,
	Mpc	deg	deg	MANGROVE	RBGS	2012 sample	M_⊙ yr⁻¹		10⁻¹³ erg s⁻¹ cm⁻²		SWGO
LMC	0.049 ± 0.002	80.00	-68.75	✓	✓	✓	0.192 ± 0.022	J0519.9-6845e	240.0 ± 5.9	?	?
SMC	0.064 ± 0.001	14.50	-72.75	✓	✓	✓	0.030 ± 0.003	J0058.0-7245e	50.3 ± 2.5	?	?
NGC 6822	0.4603 ± 0.0040	296.24	-14.80	✓			0.0070 ± 0.0006	-	< 2.05	-	-
M31	0.74 ± 0.02	10.82	41.24	✓	✓	✓	0.245 ± 0.023	J0043.2+4114	3.91 ± 0.55	?	-
M33	0.853 ± 0.016	23.46	30.66	✓	✓	✓	0.251 ± 0.013	-	< 2.49	+	-
NGC 300	1.944 ± 0.040	13.72	-37.68	✓			0.138 ± 0.005	-	< 0.15	-	-
NGC 55	1.981 ± 0.020	3.79	-39.22	✓			0.186 ± 0.010	-	< 0.37	-	-
IC 342	2.24 ± 0.10	56.70	68.10	✓		✓	0.40 ± 0.03	-	< 0.89	-	-
Circinus	2.41 ± 0.26	213.29	-65.33	✓			0.68 ± 0.13	J1413.1-6519	8.3 ± 1.2	++	+
NGC 2403	3.13 ± 0.06	114.37	65.59	✓			0.355 ± 0.012	J0737.4+6535	1.79 ± 0.39	o	o
NGC 1569	3.25 ± 0.24	67.70	64.85	✓			0.70 ± 0.08	-	< 2.34	-	-
M81	3.61 ± 0.20	148.89	69.07	✓			0.42 ± 0.04	-	< 0.32	-	-
M82	3.53 ± 0.03	148.95	69.67	✓	✓	✓	$10.41 \pm 0.19$ $10.41 \pm 0.19\phantom{0}$	J0955.7+6940	17.0 ± 1.0	++	+
NGC 253	3.61 ± 0.03	11.90	-25.29	✓	✓	✓	5.19 ± 0.09	J0047.5-2517	14.0 ± 1.0	++	+
NGC 4945	4.06 ± 0.77	196.36	-49.47	✓	✓	✓	1.46 ± 0.44	J1305.4-4928	16.5 ± 0.9	++	+
M83	4.79 ± 0.09	204.25	-29.87	✓	✓	✓	3.29 ± 0.10	-	< 2.27	+	-
NGC 3621	6.70 ± 0.37	169.57	-32.81	✓			0.86 ± 0.07	-	< 1.72	-	-
M101	6.76 ± 0.11	210.80	54.35	✓			3.13 ± 0.22	-	< 0.74	-	-
NGC 6946	6.95 ± 0.38	308.71	60.15	✓		✓	3.70 ± 0.33	-	< 0.36	-	-
M106	7.54 ± 0.09	184.74	47.30	✓			1.03 ± 0.08	-	< 0.78	-	-
M51	8.34 ± 0.30	202.47	47.23	✓			2.83 ± 0.15	-	< 1.13	-	-
NGC1068	$13.4 \pm 1.8$ $13.4 \pm 1.8\phantom{0}$	40.67	-0.01		✓	✓	40 ± 10	J0242.6-0000	9.12 ± 0.68	++	o
NGC 2146	$17.2 \pm 3.2$ $17.2 \pm 3.2\phantom{0}$	94.53	78.33				$14.0 \pm 5.1$ $14.0\pm 5.1\phantom{0}$	J0618.1+7819	2.49 ± 0.38	o	-
NGC 3424	$18.8 \pm 3.7$ $18.8 \pm 3.7\phantom{0}$	162.91	32.89				0.86 ± 0.32	J1051.6+3253	1.32 ± 0.35	o	-
NGC 7059	$24.7 \pm 4.6$ $24.7 \pm 4.6\phantom{0}$	321.84	-60.01				0.67 ± 0.09	J2127.6-5959	1.30 ± 0.34	?	?
Arp 299	$46.8 \pm 3.3$ $46.8 \pm 3.3\phantom{0}$	172.07	58.52				97 ± 14	J1128.2+5831	2.00 ± 0.37	o	-
Arp 220	$80.9 \pm 5.7$ $80.9 \pm 5.7\phantom{0}$	233.70	23.53				$214 \pm 32$ $214 \pm 32\phantom{0}$	J1534.7+2331	2.99 ± 0.53	o	-

Notes. The first two columns provide the common name of the galaxy, d is the luminosity distance, R.A. and Dec are the right ascension and declination in the ICRS reference system of the center of the associated 4FGL source. The next three columns indicate whether the source meets the selection criterion described in section 2.1 (flux relative to that of NGC 253 > 1/3.5) in the Revised MANGROVE Sample (Biteau 2021), the IRAS Revised Bright Galaxy Sample (Sanders et al. 2003), and the sample proposed by Ackermann et al. (2012). Ṁ_∗ is the SFR. 4FGL Name is the name of the associated γ-ray source in 4FGL-DR4. ℱ_2 GeV is the energy flux at 2 GeV. The last two columns qualify the reliability of detection by the new γ-ray observatories, whether pointed (CTAO) or wide field (LHAASO, SWGO): “++”, “+”, “o”, “-”, “?” indicate, respectively, a high degree of reliability, a good degree of reliability, a possibility of detection, an unlikely detection, and that a detailed study is needed before concluding.

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