5XMM J182933.3+010825
5XMM-DR15 stacked source · SRCID 3006582020100055
Position:
18h29m33.35s +01d08m25.0s
(277.38895°, 1.14028°)
EP flux
1.78e-14
± 3.5e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
4
| SRCID | 3006582020100055 |
|---|---|
| IAUNAME | 5XMM J182933.3+010825 |
| SC_RA | 18h29m33.35s (277.38895°) |
| SC_DEC | +01d08m25.0s (1.14028°) |
| RADEC_ERR | 0.52 arcsec |
| LII / BII | 31.4498° / 5.3882° |
| 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): 1.78e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.91
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.09
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.93
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 0.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.18
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
- 5448877
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 17.317 | 0.042 |
| UVM2 | 17.029 | 0.020 |
| UVW1 | 15.251 | 0.005 |
| U | 14.227 | 0.004 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.51e-14 (+2.9e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.91e+21 (+4.6e+21 / −3.1e+21) cm−2 |
| Photon index (Γ) | 2.80 (+2.94 / −2.53) |
| DoF | 91 |
| p-value | 0.578 |
| 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.