5XMM J144929.3+090444
5XMM-DR15 stacked source · SRCID 3005756030100059
Position:
14h49m29.33s +09d04m44.4s
(222.37221°, 9.07899°)
EP flux
4.25e-15
± 1.2e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.674)
Detections
3
| SRCID | 3005756030100059 |
|---|---|
| IAUNAME | 5XMM J144929.3+090444 |
| SC_RA | 14h49m29.33s (222.37221°) |
| SC_DEC | +09d04m44.4s (9.07899°) |
| RADEC_ERR | 0.78 arcsec |
| LII / BII | 5.6006° / 56.7993° |
| 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): 4.25e-15 ± 1.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.44
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.48
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.21
± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.90
± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.46
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
- 3782309
- Match probability
- 0.98
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 19.350 | 0.094 |
| UVW1 | 18.101 | 0.034 |
| U | 17.494 | 0.019 |
| B | 16.252 | 0.009 |
| V | 15.696 | 0.008 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.61e-15 (+9.6e-15 / −4.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.42e+20 (+7.5e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.85 (+2.30 / −1.43) |
| DoF | 76 |
| p-value | 0.824 |
| 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.