5XMM J182922.7+011033
5XMM-DR15 stacked source · SRCID 3006582020100015
Position:
18h29m22.71s +01d10m33.9s
(277.34462°, 1.17609°)
EP flux
5.82e-14
± 6.5e-15
erg cm-2 s-1
CLASSX
Star
(0.631)
Detections
4
| SRCID | 3006582020100015 |
|---|---|
| IAUNAME | 5XMM J182922.7+011033 |
| SC_RA | 18h29m22.71s (277.34462°) |
| SC_DEC | +01d10m33.9s (1.17609°) |
| RADEC_ERR | 0.29 arcsec |
| LII / BII | 31.4615° / 5.4440° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 52741.650 (2003-04-12 15:36:24.000 UTC) |
| MJD_LAST | 52909.341 (2003-09-27 08:10:31.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.82e-14 ± 6.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.94
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.36
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.61
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73
± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.37
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.41e-13 (+1.5e-13 / −1.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 5.22e+21 (+5.8e+21 / −4.6e+21) cm−2 |
| Photon index (Γ) | 2.89 (+2.97 / −2.74) |
| DoF | 334 |
| p-value | 0 |
| Inter-instrument norm. | 1.96 (1.91–1.99) |
| Quality flag | 5 |
| APPROX_SOURCE_VAR | 13.500 (approximate flux variability amplitude) |
|---|
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.