5XMM J144944.7+085925
5XMM-DR15 stacked source · SRCID 3005756030100002
Position:
14h49m44.77s +08d59m25.3s
(222.43652°, 8.99037°)
EP flux
1.19e-13
± 4.8e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.676)
Detections
3
| SRCID | 3005756030100002 |
|---|---|
| IAUNAME | 5XMM J144944.7+085925 |
| SC_RA | 14h49m44.77s (222.43652°) |
| SC_DEC | +08d59m25.3s (8.99037°) |
| RADEC_ERR | 0.16 arcsec |
| LII / BII | 5.5407° / 56.6954° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52130.132 (2001-08-09 03:10:43.000 UTC) |
| MJD_LAST | 52868.447 (2003-08-17 10:44:11.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.19e-13 ± 4.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.08
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.06
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.38
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.0)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.7
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
- 3782823
- Match probability
- 0.97
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.148 | 0.244 |
| UVW1 | 21.170 | 0.138 |
| U | 21.155 | 0.114 |
| B | 20.286 | 0.071 |
| V | 19.520 | 0.082 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.09e-13 (+1.2e-13 / −1.0e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.85e+19 (+1.9e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 1.78 (+1.89 / −1.70) |
| DoF | 306 |
| p-value | 0.905 |
| 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.