5XMM J210627.1+385239
5XMM-DR15 stacked source · SRCID 3004174030100015
Position:
21h06m27.15s +38d52m39.5s
(316.61315°, 38.87763°)
EP flux
4.36e-14
± 3.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.904)
Detections
37
| SRCID | 3004174030100015 |
|---|---|
| IAUNAME | 5XMM J210627.1+385239 |
| SC_RA | 21h06m27.15s (316.61315°) |
| SC_DEC | +38d52m39.5s (38.87763°) |
| RADEC_ERR | 0.20 arcsec |
| LII / BII | 82.3570° / -5.6677° |
| N_CONTRIB | 37 (detections) |
| N_OBS | 42 (observations covering the position) |
| MJD_FIRST | 52595.976 (2002-11-17 23:26:00.000 UTC) |
| MJD_LAST | 59166.038 (2020-11-13 00:54:49.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.36e-14 ± 3.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.88
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.49
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.03
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
- 6278821
- Match probability
- 0.974
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.944 | 0.281 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.59e-14 (+1.0e-13 / −7.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.31e+20 (+7.0e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.32 (+1.52 / −1.16) |
| DoF | 130 |
| p-value | 0.711 |
| Inter-instrument norm. | 0.88 (0.69–1.11) |
| 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.