5XMM J035857.4+101939
5XMM-DR15 stacked source · SRCID 3006460010100003
Position:
03h58m57.47s +10d19m39.5s
(59.73948°, 10.32765°)
EP flux
1.89e-13
± 2.0e-14
erg cm-2 s-1
CLASSX
AGN
(0.929)
Detections
2
| SRCID | 3006460010100003 |
|---|---|
| IAUNAME | 5XMM J035857.4+101939 |
| SC_RA | 03h58m57.47s (59.73948°) |
| SC_DEC | +10d19m39.5s (10.32765°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 179.9406° / -31.1131° |
| 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): 1.89e-13 ± 2.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.49
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.18
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.33
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.769
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
- 1021247
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.646 | 0.076 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.41e-13 (+2.7e-13 / −2.2e-13) erg cm−2 s−1 |
|---|---|
| NH | 7.77e+20 (+1.2e+21 / −3.9e+20) cm−2 |
| Photon index (Γ) | 1.66 (+1.83 / −1.49) |
| DoF | 973 |
| p-value | 0.545 |
| Inter-instrument norm. | 0.92 (0.83–1.04) |
| 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.