5XMM J044803.8-062326
5XMM-DR15 stacked source · SRCID 3001474060100055
Position:
04h48m03.82s -06d23m26.1s
(72.01593°, -6.39059°)
EP flux
7.64e-15
± 2.6e-15
erg cm-2 s-1
CLASSX
AGN
(0.867)
Detections
3
| SRCID | 3001474060100055 |
|---|---|
| IAUNAME | 5XMM J044803.8-062326 |
| SC_RA | 04h48m03.82s (72.01593°) |
| SC_DEC | -06d23m26.1s (-6.39059°) |
| RADEC_ERR | 0.81 arcsec |
| LII / BII | 204.0546° / -30.2790° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52525.021 (2002-09-08 00:30:04.000 UTC) |
| MJD_LAST | 53975.011 (2006-08-28 00:16:07.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.64e-15 ± 2.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.00
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.45
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.14
± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.82
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
- 1098362
- Match probability
- 0.919
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.138 | 0.321 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.20e-14 (+1.5e-14 / −8.8e-15) erg cm−2 s−1 |
|---|---|
| NH | 8.46e+20 (+2.5e+21 / −7.3e+19) cm−2 |
| Photon index (Γ) | 1.53 (+2.10 / −1.24) |
| DoF | 489 |
| p-value | 0.564 |
| Inter-instrument norm. | 0.71 (0.57–0.92) |
| 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.