5XMM J035921.4+102510
5XMM-DR15 stacked source · SRCID 3006460010100004
Position:
03h59m21.41s +10d25m10.5s
(59.83920°, 10.41959°)
EP flux
1.70e-13
± 2.1e-14
erg cm-2 s-1
CLASSX
AGN
(0.919)
Detections
2
| SRCID | 3006460010100004 |
|---|---|
| IAUNAME | 5XMM J035921.4+102510 |
| SC_RA | 03h59m21.41s (59.83920°) |
| SC_DEC | +10d25m10.5s (10.41959°) |
| RADEC_ERR | 0.48 arcsec |
| LII / BII | 179.9338° / -30.9788° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52524.468 (2002-09-07 11:13:52.000 UTC) |
| MJD_LAST | 52675.929 (2003-02-05 22:17:16.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.70e-13 ± 2.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.54
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.32
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.23
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.19
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.9)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.305
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
- 1022259
- Match probability
- 0.986
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.531 | 0.293 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.59e-13 (+1.8e-13 / −1.4e-13) erg cm−2 s−1 |
|---|---|
| NH | 1.37e+21 (+1.8e+21 / −9.2e+20) cm−2 |
| Photon index (Γ) | 1.65 (+1.82 / −1.47) |
| DoF | 745 |
| p-value | 0.506 |
| Inter-instrument norm. | 0.76 (0.65–0.88) |
| 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.