5XMM J163417.5+571313
5XMM-DR15 stacked source · SRCID 3004954010100018
Position:
16h34m17.56s +57d13m13.7s
(248.57317°, 57.22047°)
EP flux
2.30e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.913)
Detections
6
| SRCID | 3004954010100018 |
|---|---|
| IAUNAME | 5XMM J163417.5+571313 |
| SC_RA | 16h34m17.56s (248.57317°) |
| SC_DEC | +57d13m13.7s (57.22047°) |
| RADEC_ERR | 0.47 arcsec |
| LII / BII | 86.6423° / 40.9053° |
| 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): 2.30e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.17
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.10
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.32
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.666
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
- 4239714
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.830 | 0.086 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.09e-14 (+2.5e-14 / −1.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.19e+20 (+5.0e+20 / −2.6e+19) cm−2 |
| Photon index (Γ) | 2.27 (+2.53 / −2.01) |
| DoF | 206 |
| p-value | 0.927 |
| 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.