Radio emission from flaring stars and brown dwarfs

Open Access

Table A.1

List of the 55 radio detected flaring stars. The 7 objects with coincident TESS observations are marked with asterisks.

ID	Rate	Teff (K)	Prot (day)	T_gyro (Myr)	Spectral type	SNR₁	S₁ (mJy)	SNR₂	S₂ (mJy)	SNR₃	S₃ (mJy)	l_1RX (erg s⁻¹)	l_2RX,PL (erg s⁻¹)	l_R,I (erg s⁻¹)	l_R,P3 (erg s⁻¹)	l_XMM (erg s⁻¹)
TIC 11756053	0.538	4852 ± 133	3.89 ± 0.58	95 $_{- 66}^{+ 200}$ $^{+200}_{-66}$	K0-2IV (15)	20.6	6.3 ± 0.3	3.4	<0.9	3.3	<0.8	31.2	31.3	31.1	30.7
TIC 19559847			1.64 ± 0.25		K7 (26)	3.0	<0.7	3.5	<0.7	9.5	1.5 ± 0.2	30.0	30.1	30.2	29.6
TIC 20299889	0.090	4906 ± 133			G8V (1)	3.9	<0.6	5.5	<0.7	9.8	1.1 ± 0.2	30.7	31.3
TIC 30981628	0.262	5038 ± 124	3.41 ± 0.51	90 $_{- 62}^{+ 186}$ $^{+186}_{-62}$	G9III (11)	7.0	1.0 ± 0.2	3.6	<0.7	7.5	1.3 ± 0.3	30.9	31.6
TIC 39699561	0.445	5651 ± 125	5.69 ± 0.85	321 $_{- 149}^{+ 136}$ $^{+136}_{-149}$	G0 (9)	6.6	1.3 ± 0.3	3.9	<0.6	3.4	<0.6	30.7	30.6
TIC 45373627	0.136	5358 ± 138	0.37 ± 0.06	81 $_{- 56}^{+ 159}$ $^{+159}_{-56}$	G5V (24)	7.7	1.4 ± 0.3	8.4	1.3 ± 0.2	7.2	1.0 ± 0.2	30.6	31.2	30.7	30.1
TIC 47757785	0.170	5581 ± 124			G5 (9)	4.7	<0.6	3.7	<0.7	6.8	0.9 ± 0.2	30.8	30.9
TIC 52588257	0.139	5362 ± 138	1.51 ± 0.23	81 $_{- 56}^{+ 159}$ $^{+159}_{-56}$	G0V (14)	3.5	<0.6	14.1	3.2 ± 0.3	3.7	<0.7	30.7	30.8	30.6	30.1
TIC 53417036	0.247	5555 ± 109	1.53 ± 0.23	77 $_{- 53}^{+ 142}$ $^{+142}_{-53}$	G0 (10)	19.7	6.0 ± 0.3	4.0	<1.0	6.5	1.1 ± 0.2	30.3	30.4	30.4	29.9
TIC 54007252^*	0.298	4489 ± 124	2.48 ± 0.37	96 $_{- 67}^{+ 220}$ $^{+220}_{-67}$	G9 (17)	3.6	<0.7	9.6	1.3 ± 0.2	3.5	<0.8	30.8		30.8	30.5
TIC 56624881^*	0.317	4464 ± 36	2.64 ± 0.4	95 $_{- 66}^{+ 221}$ $^{+221}_{-66}$	K3Ve (2)	20.8	6.0 ± 0.2	12.3	2.2 ± 0.3	12.9	2.0 ± 0.2	30.6				30.3
TIC 58231482^*	0.365	4329 ± 131	1.87 ± 0.28	100 $_{- 70}^{+ 229}$ $^{+229}_{-70}$	K3Ve (2)	7.7	1.2 ± 0.3	10.6	1.3 ± 0.2	5.6	<0.7	30.6	30.5			30.2
TIC 58285785^*	0.045	3637 ± 129	1.56 ± 0.23		K7 (19)	7.9	1.1 ± 0.2	11.1	1.7 ± 0.2	18.3	3.4 ± 0.3	30.2				29.9
TIC 58288494^*	0.118	3935 ± 105	5.45 ± 0.82	144 $_{- 98}^{+ 245}$ $^{+245}_{-98}$	K7 (16)	3.5	<0.6	14.9	2.5 ± 0.2	3.3	<0.6					29.6
TIC 58467533	0.263	5857 ± 113	1.53 ± 0.23	66 $_{- 45}^{+ 70}$ $^{+70}_{-45}$	G5IVe (8)	13.5	2.5 ± 0.3	4.9	<0.6	4.0	<0.7	30.9				30.5
TIC 58606910	0.068	4071 ± 122	1.93 ± 0.29	111 $_{- 78}^{+ 240}$ $^{+240}_{-78}$	K0 (18)	5.9	<0.7	4.7	<0.6	7.5	1.2 ± 0.3	30.8
TIC 61259674	0.160	10593 ± 73	3.21 ± 0.48		B9IVn (13)	8.1	1.8 ± 0.3	12.1	1.6 ± 0.2	5.0	<0.6	31.0				30.8
TIC 68416596					M0IVe (25)	16.7	3.4 ± 0.2	5.4	<0.8	8.6	2.3 ± 0.4
TIC 86339506	0.426	4519 ± 80	3.29 ± 0.49	96 $_{- 67}^{+ 219}$ $^{+219}_{-67}$	G5 (9)	19.7	4.6 ± 0.2	8.1	1.4 ± 0.3	20.4	9.0 ± 0.2	31.4	31.6
TIC 114085232	0.039	4672 ± 150	0.34 ± 0.05	95 $_{- 66}^{+ 211}$ $^{+211}_{-66}$	~	3.4	<0.8	6.6	1.1 ± 0.3	3.8	<0.6	30.1
TIC 120837437	0.206	5372 ± 132	1.09 ± 0.16	81 $_{- 56}^{+ 157}$ $^{+157}_{-56}$	~	7.1	0.9 ± 0.2	6.8	1.0 ± 0.3	6.2	0.8 ± 0.2	31.1	31.1	30.7	30.3
TIC 127572976	0.084	5343 ± 123			G6III (11)	6.1	0.8 ± 0.2	11.9	2.2 ± 0.2	4.5	<0.7	31.8	32.4	31.8	31.5
TIC 132764448	0.058	4612 ± 123	0.42 ± 0.06	95 $_{- 66}^{+ 214}$ $^{+214}_{-66}$	~	3.2	<0.8	3.1	<0.9	7.1	1.9 ± 0.4			29.8	29.2	29.3
TIC 135443051	0.045	5714 ± 80			G0V+G5V (7)	11.0	2.1 ± 0.2	6.2	0.7 ± 0.1	11.2	1.6 ± 0.2	30.5	30.7
TIC 141146667		3051 ± 157	0.16 ± 0.02		~	8.4	1.8 ± 0.3	6.1	1.1 ± 0.2	6.9	1.0 ± 0.2
TIC 148841573	0.288	4495 ± 146	6.33 ± 0.95	117 $_{- 78}^{+ 204}$ $^{+204}_{-78}$	K7e (28)	12.1	2.3 ± 0.3	4.2	<0.8	15.7	2.5 ± 0.2	30.8	31.0
TIC 150002985	0.046	3066 ± 122			M1Ve (2)	13.3	2.9 ± 0.3	3.2	<0.5	10.0	1.7 ± 0.3					29.5
TIC 150173452	0.069				M0.6 (20)	3.3	<0.7	3.5	<0.6	18.3	4.3 ± 0.2	30.3	30.6			29.7
TIC 152346470	0.540	5844 ± 134	1.96 ± 0.29	68 $_{- 47}^{+ 70}$ $^{+70}_{-47}$	G5V (11)	3.8	<0.6	8.8	1.8 ± 0.3	4.0	<0.7	30.8	30.7	30.8	30.4
TIC 186777643	0.063	5796 ± 132	3.25 ± 0.49	106 $_{- 72}^{+ 114}$ $^{+114}_{-72}$	G1V (11)	15.6	2.9 ± 0.3	7.6	1.4 ± 0.3	4.7	<0.7	30.9	30.9	31.0	30.6
TIC 195165333^*	0.355	5230 ± 130	7.29 ± 1.09	371 $_{- 187}^{+ 194}$ $^{+194}_{-187}$	G9III (11)	2.8	<0.6	4.0	<0.9	14.8	2.8 ± 0.3	31.3		31.0	30.5	30.4
TIC 238778709	0.148	5391 ± 124	11.82 ± 1.77	1120 $_{- 285}^{+ 296}$ $^{+296}_{-285}$	F8 (9)	6.9	2.0 ± 0.5	4.1	<0.6	3.1	<0.6	31.1	31.2
TIC 241351537	0.297	4955 ± 145			G8III+sdO (3)	14.9	3.6 ± 0.3	13.6	2.7 ± 0.3	5.9	<0.8	32.5	32.8
TIC 248024514	0.052	4970 ± 123	11.32 ± 1.7	975 $_{- 364}^{+ 328}$ $^{+328}_{-364}$	G5 (21)	9.0	1.2 ± 0.2	3.4	<0.6	3.8	<0.7
TIC 252873509	0.122	6539 ± 128	7.31 ± 1.1		F5 (9)	23.0	8.3 ± 0.2	24.6	10.1 ± 0.2	22.4	5.4 ± 0.2	31.7	32.0
TIC 268397995	0.128	3923 ± 63	2.72 ± 0.41	117 $_{- 82}^{+ 248}$ $^{+248}_{-82}$	M0-1 (15)	3.5	<0.8	3.9	<0.6	10.6	1.8 ± 0.2					30.1
TIC 282780307	0.165	4693 ± 127	6.33 ± 0.95	110 $_{- 74}^{+ 168}$ $^{+168}_{-74}$	~	3.3	<0.7	9.2	1.2 ± 0.2	3.5	<0.6		31.4
TIC 285643624	0.355	4629 ± 127	11.06 ± 1.66	828 $_{- 387}^{+ 403}$ $^{+403}_{-387}$	K5 (9)	18.1	3.7 ± 0.2	3.3	<0.6	5.0	<0.7	31.3	31.3
TIC 306301020	0.245	5494 ± 117	1.78 ± 0.27	78 $_{- 54}^{+ 146}$ $^{+146}_{-54}$	G2V (27)	3.2	<0.7	3.4	<0.6	8.6	1.6 ± 0.3	30.4	30.7
TIC 309965134	0.177	5107 ± 123			G5 (21)	2.9	<0.6	8.3	1.3 ± 0.3	5.2	<0.6	30.9	31.1
TIC 332487879	0.134	5192 ± 96			G5IV (4)	3.1	<0.7	16.9	3.9 ± 0.3	17.9	4.4 ± 0.3	31.5	31.6
TIC 353053003			0.37 ± 0.06		M4.5V (23)	8.5	1.2 ± 0.2	9.8	2.0 ± 0.3	8.4	1.6 ± 0.3	29.3	29.4
TIC 357345626	0.215	4960 ± 124			G8III+B9.5e (22)	3.9	<0.6	3.8	<0.6	7.7	1.6 ± 0.3	30.9
TIC 364130065	0.335	5344 ± 131			K (21)	3.0	<0.6	17.3	3.6 ± 0.3	5.6	<0.7	30.9	31.3
TIC 366680372	0.172	4192 ± 124	2.18 ± 0.33	106 $_{- 74}^{+ 236}$ $^{+236}_{-74}$	~	10.2	1.3 ± 0.2	3.4	<0.7	12.8	2.5 ± 0.3	30.8
TIC 389188453	0.140	5409 ± 122			G0V (21)	3.3	<0.7	3.7	<0.6	8.5	1.2 ± 0.3	30.7	30.9
TIC 399151944	0.351	4141 ± 125	2.07 ± 0.31	108 $_{- 75}^{+ 238}$ $^{+238}_{-75}$	K4IVe (25)	19.3	4.0 ± 0.3	3.4	<0.8	3.3	<0.8	30.6	31.0	30.4	29.9
TIC 399181042	0.150	5618 ± 124			G5 (9)	14.0	2.7 ± 0.2	3.2	<0.6	6.4	0.8 ± 0.2	31.3	31.4	31.2	30.7
TIC 415030187	0.017	4583 ± 124			K0+IIICH-1 (6)	3.0	<0.7	4.8	<0.7	19.5	5.7 ± 0.3	31.6	31.7
TIC 432909199^*	0.252	6318 ± 451	0.95 ± 0.14		G0 (29)	3.6	<0.6	7.2	1.1 ± 0.2	3.9	<0.8	30.9	31.0	30.7	30.4
TIC 436588012	0.206	6061 ± 509			G5 (18)	3.6	<0.7	8.4	1.8 ± 0.3	3.8	<1.7	30.9	31.3	31.1	30.6
TIC 442932272		2950 ± 52	0.4 ± 0.06		M4.5 (12)	4.4	<0.9	5.9	<1.0	12.5	4.6 ± 0.5	29.1	29.0	28.9	28.2
TIC 444062991	0.243	5227 ± 110	0.66 ± 0.1	84 $_{- 58}^{+ 170}$ $^{+170}_{-58}$	G0 (5)	4.1	<0.6	3.9	<1.0	8.2	1.0 ± 0.2	31.1	31.6
TIC 444656050	0.398	5570 ± 152	0.78 ± 0.12	77 $_{- 53}^{+ 142}$ $^{+142}_{-53}$	G3IV(e) (11)	11.9	2.3 ± 0.2	3.7	<1.0	5.2	<0.7	30.8	31.3	30.7	30.3
TIC 456942208	0.481	5859 ± 104	0.73 ± 0.11	73 $_{- 50}^{+ 121}$ $^{+121}_{-50}$	G8 (18)	3.4	<0.9	8.0	1.2 ± 0.2	3.8	<0.8	30.4	31.2

Notes. Column 1 - TESS Input catalogue number of the star. Column 2 - flare rate ( flares per day above 10³⁴ erg ). Column 3 - rotation period. Column 4 - gyrochronological age estimate. Column 5 - effective temperature. Column 6 - spectral type (1) Joy & Wilson (1949).(2) Herbig (1977).(3) Dworetsky et al. (1982).(4) Houk (1982).(5) Roeser & Bastian (1988).(6) Keenan & McNeil ( 1989).(7) Strassmeier & Fekel ( 1990).(8) Patterer et al. (1993).(9) Cannon & Pickering ( 1993).( 10) Nesterov et al. (1995 ).( 11) Torres et al. (2006).(12) Riaz et al. (2006).(13) Royer et al. (2007).(14) White etal. (2007).( 15) Strassmeier (2009).( 16) Riviere -Marichalar et al. (2012).( 17) Biazzo et al. (2012).( 18) Nguyen et al. (2012).( 19) Xiao et al. (2012).(20) Herczeg & Hillenbrand (2014).(21) Bourgés et al. (2014), (22) Harmanec et al. (2015).(23) Alonso-Floriano et al. (2015).(24) Myers et al. (2015).(25) Pecaut & Mamajek (2016).(26) Kraus et al. (2017).(27) Frasca et al. (2018).(28) Bowler et al. (2019).(29) Liu et al. (2021 ). Columns 7.9.11 - signal-to-noise ratio of the epoch 1-3 VLASS maps. Columns 8.10.12 - flux density at 3 GHz in the VLASS 1-3 epoch observations. Upper limits for the non-detections are given at 5σ rms noise levels. Columns 13-17 - log X-ray luminosities from the first (Voges et al. 1999. 2000) and second (Boiler et al. 2016) ROSAT, and the SRG/eROSITA (Merloni et al. 2024) all-sky surveys, and the XMM-Newton serendipitous survey (Rosen et al. 2016).

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