Table 2.
Sources per FXT for which we fitted K and M dwarf spectra to the extracted MUSE spectra.
| Source | RA | Dec | offset | Type | χν2 |
|---|---|---|---|---|---|
| (degrees) | (degrees) | (arcsec) | |||
| XRT 100831 | |||||
| 22 | 90.01830 | −52.71495 | 30.3 | M4V | 1.4 |
| 43 | 90.01155 | −52.71092 | 21.3 | M3V | 2.5 |
| XRT 060207 | |||||
| 8 | 196.83675 | −40.46642 | 23.4 | M3V | 1.7 |
| 18 | 196.82833 | −40.46325 | 13.6 | M5V | 1.9 |
| 23 | 196.82550 | −40.46300 | 19.8 | M1V | 1.7 |
| 40 | 196.83250 | −40.45978 | 4.2 | M1V | 2.4 |
| 53 | 196.84175 | −40.45661 | 30.5 | M5V | 2.2 |
| XRT 070618 | |||||
| 28 | 24.26996 | −12.94903 | 22.6 | M5V | 2.0 |
Notes. The sources are indicated in Figure 1 by orange circles and their corresponding number. We list RA and Dec for each source as well as the angular offset in arcseconds. The best-fitting K or M dwarf spectral type is listed as well as the corresponding reduced χ2 of the fit. The number of the degrees of freedom was 3596 for all sources, except for sources 22 an 42 of XRT 100831, for which there were 3595 degrees of freedom.
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