5XMM J080433.2-280523
5XMM-DR15 stacked source · SRCID 3005757010100034
Position:
08h04m33.28s -28d05m23.1s
(121.13866°, -28.08976°)
EP flux
4.67e-15
± 2.3e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3005757010100034 |
|---|---|
| IAUNAME | 5XMM J080433.2-280523 |
| SC_RA | 08h04m33.28s (121.13866°) |
| SC_DEC | -28d05m23.1s (-28.08976°) |
| RADEC_ERR | 0.94 arcsec |
| LII / BII | 245.9907° / 1.8086° |
| 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): 4.67e-15 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.64
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.67
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.82
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
0.57
± 0.44
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.45
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
- 2468622
- Match probability
- 0.984
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 15.712 | 0.012 |
| UVM2 | 15.356 | 0.007 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.30e-15 (+1.2e-14 / −5.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.07e+20 (+1.1e+21 / −3.0e+19) cm−2 |
| Photon index (Γ) | 2.02 (+2.52 / −1.64) |
| DoF | 497 |
| p-value | 0.597 |
| Inter-instrument norm. | 1.05 (0.74–1.50) |
| 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.