5XMM J102842.8+682817
5XMM-DR15 stacked source · SRCID 3002634030100001
Position:
10h28m42.86s +68d28m17.1s
(157.17859°, 68.47140°)
EP flux
3.55e-13
± 1.4e-14
erg cm-2 s-1
CLASSX
AGN
(0.569)
Detections
1
| SRCID | 3002634030100001 |
|---|---|
| IAUNAME | 5XMM J102842.8+682817 |
| SC_RA | 10h28m42.86s (157.17859°) |
| SC_DEC | +68d28m17.1s (68.47140°) |
| RADEC_ERR | 0.19 arcsec |
| LII / BII | 140.1196° / 43.5872° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52375.297 (2002-04-11 07:07:34.000 UTC) |
| MJD_LAST | 52375.575 (2002-04-11 13:48:06.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.55e-13 ± 1.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.41
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.23
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.63
± 0.04
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.366
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
- 2887661
- Match probability
- 0.819
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 18.964 | 0.061 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.95e-13 (+3.2e-13 / −2.8e-13) erg cm−2 s−1 |
|---|---|
| NH | 1.56e+21 (+1.9e+21 / −1.2e+21) cm−2 |
| Photon index (Γ) | 2.13 (+2.26 / −1.99) |
| DoF | 416 |
| p-value | 0.376 |
| 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.