The population of tidal disruption events discovered with eROSITA

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Volume 697 (May 2025)

A&A, 697 (2025) A159

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Table D.1.

SED modeling results for 28 sources from eROSITA TDE sample.

Name	Mass	mfrac	^{0, 0}u−r
	×10¹⁰M_⊙		[mag]
J0240-59	$6 . 88_{- 3.76}^{+ 3.8}$ $6.88^{+3.8}_{-3.76}$	0.62	$1 . 68_{- 0.25}^{+ 0.33}$ $1.68^{+0.33}_{-0.25}$
J0340-38	$5 . 09_{- 1.97}^{+ 5.59}$ $5.09^{+5.59}_{-1.97}$	0.66	$1 . 63_{- 0.27}^{+ 0.22}$ $1.63^{+0.22}_{-0.27}$
J0341-45	$6 . 52_{- 3.47}^{+ 3.64}$ $6.52^{+3.64}_{-3.47}$	0.67	$1 . 31_{- 0.18}^{+ 0.32}$ $1.31^{+0.32}_{-0.18}$
J0615-44	$5 . 84_{- 3.32}^{+ 6.56}$ $5.84^{+6.56}_{-3.32}$	0.62	$2 . 13_{- 0.14}^{+ 0.10}$ $2.13^{+0.10}_{-0.14}$
J0707-84	$3 . 18_{- 1.11}^{+ 9.79}$ $3.18^{+9.79}_{-1.11}$	0.61	$2 . 08_{- 0.79}^{+ 0.10}$ $2.08^{+0.10}_{-0.79}$
J1102-05	$3 . 01_{- 1.63}^{+ 2.05}$ $3.01^{+2.05}_{-1.63}$	0.64	$1 . 58_{- 0.33}^{+ 0.42}$ $1.58^{+0.42}_{-0.33}$
J1305+01	$3 . 0_{- 1.36}^{+ 1.76}$ $3.0^{+1.76}_{-1.36}$	0.61	$1 . 9_{- 0.37}^{+ 0.29}$ $1.9^{+0.29}_{-0.37}$
J1730-85	$22 . 5_{- 8.48}^{+ 14.93}$ $22.5^{+14.93}_{-8.48}$	0.63	$1 . 95_{- 0.25}^{+ 0.31}$ $1.95^{+0.31}_{-0.25}$
J0114-59	$13 . 43_{- 1.74}^{+ 1.91}$ $13.43^{+1.91}_{-1.74}$	0.61	$2 . 31_{- 0.05}^{+ 0.05}$ $2.31^{+0.05}_{-0.05}$
J0141-44	$0 . 88_{- 0.16}^{+ 0.17}$ $0.88^{+0.17}_{-0.16}$	0.6	$2 . 1_{- 0.06}^{+ 0.06}$ $2.1^{+0.06}_{-0.06}$
J0318-20	$1 . 77_{- 0.97}^{+ 2.14}$ $1.77^{+2.14}_{-0.97}$	0.61	$1 . 63_{- 0.48}^{+ 0.31}$ $1.63^{+0.31}_{-0.48}$
J0439-65	$16 . 35_{- 2.53}^{+ 4.0}$ $16.35^{+4.0}_{-2.53}$	0.64	$2 . 21_{- 0.06}^{+ 0.06}$ $2.21^{+0.06}_{-0.06}$
J0608-43	$2 . 17_{- 0.32}^{+ 0.49}$ $2.17^{+0.49}_{-0.32}$	0.64	$1 . 78_{- 0.11}^{+ 0.11}$ $1.78^{+0.11}_{-0.11}$
J0634-71	$1 . 72_{- 0.3}^{+ 0.39}$ $1.72^{+0.39}_{-0.3}$	0.62	$1 . 98_{- 0.06}^{+ 0.06}$ $1.98^{+0.06}_{-0.06}$
J0644-60	$2 . 12_{- 0.33}^{+ 0.44}$ $2.12^{+0.44}_{-0.33}$	0.61	$2 . 0_{- 0.06}^{+ 0.06}$ $2.0^{+0.06}_{-0.06}$
J0744+29	$0 . 19_{- 0.03}^{+ 0.05}$ $0.19^{+0.05}_{-0.03}$	0.62	$2 . 07_{- 0.08}^{+ 0.08}$ $2.07^{+0.08}_{-0.08}$
J0820+19	$2 . 26_{- 0.41}^{+ 0.51}$ $2.26^{+0.51}_{-0.41}$	0.61	$2 . 07_{- 0.08}^{+ 0.08}$ $2.07^{+0.08}_{-0.08}$
J0823+04	$2 . 29_{- 0.42}^{+ 0.57}$ $2.29^{+0.57}_{-0.42}$	0.62	$2 . 25_{- 0.08}^{+ 0.08}$ $2.25^{+0.08}_{-0.08}$
J0916+06	$1 . 02_{- 0.17}^{+ 0.19}$ $1.02^{+0.19}_{-0.17}$	0.57	$2 . 11_{- 0.05}^{+ 0.05}$ $2.11^{+0.05}_{-0.05}$
J1401+08	$10 . 65_{- 4.37}^{+ 7.37}$ $10.65^{+7.37}_{-4.37}$	0.63	$1 . 82_{- 0.28}^{+ 0.26}$ $1.82^{+0.26}_{-0.28}$
J1436-17	$10 . 92_{- 4.0}^{+ 10.67}$ $10.92^{+10.67}_{-4.0}$	0.61	$2 . 14_{- 0.18}^{+ 0.16}$ $2.14^{+0.16}_{-0.18}$
J1456-28	$17 . 55_{- 3.81}^{+ 4.86}$ $17.55^{+4.86}_{-3.81}$	0.61	$2 . 12_{- 0.06}^{+ 0.06}$ $2.12^{+0.06}_{-0.06}$
J1459-26	$0 . 88_{- 0.16}^{+ 0.18}$ $0.88^{+0.18}_{-0.16}$	0.6	$2 . 11_{- 0.06}^{+ 0.06}$ $2.11^{+0.06}_{-0.06}$
J1534-09	$2 . 31_{- 0.29}^{+ 0.32}$ $2.31^{+0.32}_{-0.29}$	0.61	$2 . 15_{- 0.07}^{+ 0.07}$ $2.15^{+0.07}_{-0.07}$
J1901-55	$4 . 51_{- 0.94}^{+ 1.2}$ $4.51^{+1.2}_{-0.94}$	0.61	$2 . 07_{- 0.08}^{+ 0.08}$ $2.07^{+0.08}_{-0.08}$
J1921-50	$9 . 1_{- 1.72}^{+ 2.26}$ $9.1^{+2.26}_{-1.72}$	0.62	$2 . 15_{- 0.07}^{+ 0.07}$ $2.15^{+0.07}_{-0.07}$
J2108-56	$7 . 85_{- 1.56}^{+ 1.84}$ $7.85^{+1.84}_{-1.56}$	0.6	$1 . 97_{- 0.10}^{+ 0.10}$ $1.97^{+0.10}_{-0.10}$
J2344-35	$2 . 41_{- 0.33}^{+ 0.47}$ $2.41^{+0.47}_{-0.33}$	0.65	$2 . 07_{- 0.08}^{+ 0.08}$ $2.07^{+0.08}_{-0.08}$

Notes. The mass column lists host stellar masses. The surviving mass, used in this work, was obtained by multiplying the total mass by the coefficient mfrac. The ^{0, 0}u−r represents the rest frame colors.

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