5XMM J080446.9-280750
5XMM-DR15 stacked source · SRCID 3005757010100005
Position:
08h04m46.97s -28d07m50.5s
(121.19571°, -28.13070°)
EP flux
2.46e-14
± 1.4e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3005757010100005 |
|---|---|
| IAUNAME | 5XMM J080446.9-280750 |
| SC_RA | 08h04m46.97s (121.19571°) |
| SC_DEC | -28d07m50.5s (-28.13070°) |
| RADEC_ERR | 0.38 arcsec |
| LII / BII | 246.0522° / 1.8293° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52382.860 (2002-04-18 20:38:05.000 UTC) |
| MJD_LAST | 52383.245 (2002-04-19 05:52:30.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.46e-14 ± 1.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.70
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.56
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.99
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00
± 0.59
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2
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
- 2468997
- Match probability
- 0.99
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 16.587 | 0.020 |
| UVM2 | 16.689 | 0.014 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.29e-14 (+3.5e-14 / −3.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.72e+21 (+1.9e+21 / −1.5e+21) cm−2 |
| Photon index (Γ) | 2.94 (+2.98 / −2.84) |
| DoF | 932 |
| p-value | 0 |
| Quality flag | 5 |
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.