5XMM J163325.5+565916
5XMM-DR15 stacked source · SRCID 3004954010100052
Position:
16h33m25.54s +56d59m16.7s
(248.35641°, 56.98798°)
EP flux
8.12e-15
± 3.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.901)
Detections
6
| SRCID | 3004954010100052 |
|---|---|
| IAUNAME | 5XMM J163325.5+565916 |
| SC_RA | 16h33m25.54s (248.35641°) |
| SC_DEC | +56d59m16.7s (56.98798°) |
| RADEC_ERR | 0.76 arcsec |
| LII / BII | 86.3787° / 41.0736° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 52208.338 (2001-10-26 08:07:10.000 UTC) |
| MJD_LAST | 53674.442 (2005-10-31 10:36:41.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.12e-15 ± 3.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.38
± 0.29
0.2-0.5 / 0.5-1.0 keV
HR2
0.40
± 0.15
0.5-1.0 / 1.0-2.0 keV
HR3
0.23
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.39
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.677
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
- 4234355
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 23.385 | 0.225 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.26e-14 (+1.7e-14 / −9.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.21e+20 (+1.4e+21 / −5.5e+19) cm−2 |
| Photon index (Γ) | 2.41 (+2.80 / −2.02) |
| DoF | 395 |
| p-value | 0.529 |
| Inter-instrument norm. | 1.15 (0.83–1.54) |
| 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.