5XMM J152659.4+355836
5XMM-DR15 stacked source · SRCID 3008134110100003
Position:
15h26m59.44s +35d58m36.4s
(231.74767°, 35.97677°)
EP flux
4.50e-14
± 5.0e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.97)
Detections
1
| SRCID | 3008134110100003 |
|---|---|
| IAUNAME | 5XMM J152659.4+355836 |
| SC_RA | 15h26m59.44s (231.74767°) |
| SC_DEC | +35d58m36.4s (35.97677°) |
| RADEC_ERR | 0.54 arcsec |
| LII / BII | 57.8110° / 55.9425° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52327.711 (2002-02-22 17:04:07.000 UTC) |
| MJD_LAST | 52327.936 (2002-02-22 22:27:53.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.50e-14 ± 5.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.48
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.53
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.48
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.24
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 26.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.39
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
- 3927922
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 17.946 | 0.089 |
| UVM2 | — | — |
| UVW1 | 17.885 | 0.035 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.39e-14 (+2.7e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.46e+20 (+1.1e+21 / −3.7e+20) cm−2 |
| Photon index (Γ) | 2.76 (+2.93 / −2.50) |
| DoF | 267 |
| p-value | 0.087 |
| Inter-instrument norm. | 1.53 (1.34–1.74) |
| 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.