5XMM J162830.0+393120
5XMM-DR15 stacked source · SRCID 3000803020100082
Position:
16h28m30.08s +39d31m20.2s
(247.12535°, 39.52229°)
EP flux
8.30e-13
± 2.4e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
5
| SRCID | 3000803020100082 |
|---|---|
| IAUNAME | 5XMM J162830.0+393120 |
| SC_RA | 16h28m30.08s (247.12535°) |
| SC_DEC | +39d31m20.2s (39.52229°) |
| RADEC_ERR | 11.08 arcsec |
| LII / BII | 62.8932° / 43.7189° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 15 (observations covering the position) |
| MJD_FIRST | 52459.655 (2002-07-04 15:43:08.000 UTC) |
| MJD_LAST | 56533.778 (2013-08-29 18:39:43.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.30e-13 ± 2.4e-14 erg cm-2 s-1
Hardness ratios
HR1
-0.32
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.80
± 0.01
0.5-1.0 / 1.0-2.0 keV
HR3
-0.96
± 0.01
1.0-2.0 / 2.0-4.5 keV
HR4
0.34
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
41.16
± 0.37
arcsec
(ML 4796.3)
SUM_FLAG:
4
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.82
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
- 4196377
- Match probability
- 0.516
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.073 | 0.048 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.32e-13 (+2.6e-13 / −2.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.38e+20 (+1.1e+21 / −5.1e+19) cm−2 |
| Photon index (Γ) | 1.94 (+2.18 / −1.77) |
| DoF | 428 |
| p-value | 0.707 |
| 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.