Table 4.
TDEs discovered in the XMM-Newton slew survey.
| Name | Hard | Poss. | References |
|---|---|---|---|
| component? | AGN?a | ||
| NGC3599 | yes | yes | (1) |
| 2MASX 0740 | yes | no | (2) |
| XMMSL1 1446+68 | yes | no | (3) |
| XMMSL2 1404-25 | yes | no | (4) |
| XMMSL1 1201+30 | yes | no | (5) |
| XMMSL1 0619-65 | yes | yes | (6) |
| SDSS J1323+4827 | yes | no | (1) |
| NGC 5092 | yes | yes | (7) |
| GSN 069b | no | yes | (8) |
| XMMSL2 2030+04 | yes | yes | (9) |
| MCG+07 | yes | no | (9) |
| 2MASX 0249b | no | no | (1) |
Notes. (1) Esquej et al. (2008); (2) Saxton et al. (2017); (3) Saxton et al. (2019); (4) This paper; (5) Saxton et al. (2012); (6) Saxton et al. (2014); (7) Li et al. (2020); (8) Miniutti et al. (2013); (9) Li et al. in prep.
A power law component is ubiquitous in GSN 069 but has very low luminosity so that the corona, if present, is extremely weak. Chakraborty et al. (2021) did find a low-luminosity power-law component in 2MASX J0249 in an observation taken 16 years after discovery. However, the thermal component was still strongly dominant and so we consider this source to have not created a prominent corona to date.
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