5XMM J164959.3+045323
5XMM-DR15 stacked source · SRCID 3003214080100006
Position:
16h49m59.36s +04d53m23.0s
(252.49731°, 4.88971°)
EP flux
9.62e-13
± 7.6e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.765)
Detections
1
| SRCID | 3003214080100006 |
|---|---|
| IAUNAME | 5XMM J164959.3+045323 |
| SC_RA | 16h49m59.36s (252.49731°) |
| SC_DEC | +04d53m23.0s (4.88971°) |
| RADEC_ERR | 0.34 arcsec |
| LII / BII | 22.7902° / 29.1493° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 51968.999 (2001-02-28 23:58:30.000 UTC) |
| MJD_LAST | 51969.040 (2001-03-01 00:57:41.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.62e-13 ± 7.6e-14 erg cm-2 s-1
Hardness ratios
HR1
0.35
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
0.24
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.02
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
- 4352549
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 19.490 | 0.084 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.39e-13 (+9.3e-13 / −7.6e-13) erg cm−2 s−1 |
|---|---|
| NH | 1.10e+20 (+4.7e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 1.58 (+1.72 / −1.45) |
| DoF | 462 |
| p-value | 0.935 |
| 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.