5XMM J053933.4-694825
5XMM-DR15 stacked source · SRCID 3002394040101650
Position:
05h39m33.48s -69d48m25.1s
(84.88950°, -69.80698°)
EP flux
1.30e-14
± 3.5e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.526)
Detections
4
| SRCID | 3002394040101650 |
|---|---|
| IAUNAME | 5XMM J053933.4-694825 |
| SC_RA | 05h39m33.48s (84.88950°) |
| SC_DEC | -69d48m25.1s (-69.80698°) |
| RADEC_ERR | 2.27 arcsec |
| LII / BII | 280.2783° / -31.5160° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 336 (observations covering the position) |
| MJD_FIRST | 51838.662 (2000-10-21 15:53:07.000 UTC) |
| MJD_LAST | 56971.170 (2014-11-10 04:05:09.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.30e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.86
± 0.37
0.2-0.5 / 0.5-1.0 keV
HR2
0.63
± 0.18
0.5-1.0 / 1.0-2.0 keV
HR3
-0.24
± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
-0.52
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 2.7)
SUM_FLAG:
3
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.82
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 2028553
- Match probability
- 0.577
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.263 | 0.160 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.15e-13 (+1.3e-13 / −1.0e-13) erg cm−2 s−1 |
|---|---|
| NH | 9.16e+21 (+1.1e+22 / −7.6e+21) cm−2 |
| Photon index (Γ) | 2.55 (+2.82 / −2.22) |
| DoF | 275 |
| p-value | 0.939 |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.