5XMM J044813.7-063440
5XMM-DR15 stacked source · SRCID 3001474060100016
Position:
04h48m13.76s -06d34m40.3s
(72.05732°, -6.57785°)
EP flux
2.65e-14
± 1.3e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
2
| SRCID | 3001474060100016 |
|---|---|
| IAUNAME | 5XMM J044813.7-063440 |
| SC_RA | 04h48m13.76s (72.05732°) |
| SC_DEC | -06d34m40.3s (-6.57785°) |
| RADEC_ERR | 3.31 arcsec |
| LII / BII | 204.2687° / -30.3297° |
| N_CONTRIB | 2 (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): 2.65e-14 ± 1.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.56
± 0.17
0.2-0.5 / 0.5-1.0 keV
HR2
0.08
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42
± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent:
13.19
± 1.71
arcsec
(ML 18.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 1.82
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
- 1100045
- Match probability
- 0.898
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.983 | 0.136 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.05e-14 (+1.5e-14 / −7.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 4.24e+20 (+1.7e+21 / −3.5e+19) cm−2 |
| Photon index (Γ) | 2.03 (+2.59 / −1.65) |
| DoF | 387 |
| p-value | 0.665 |
| 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.