5XMM J160940.4+542508
5XMM-DR15 stacked source · SRCID 3005975010100140
Position:
16h09m40.43s +54d25m08.6s
(242.41846°, 54.41904°)
EP flux
3.25e-13
± 1.2e-13
erg cm-2 s-1
CLASSX
Extended
(0.999)
Detections
2
| SRCID | 3005975010100140 |
|---|---|
| IAUNAME | 5XMM J160940.4+542508 |
| SC_RA | 16h09m40.43s (242.41846°) |
| SC_DEC | +54d25m08.6s (54.41904°) |
| RADEC_ERR | 7.45 arcsec |
| LII / BII | 84.1800° / 44.9715° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 12 (observations covering the position) |
| MJD_FIRST | 52377.816 (2002-04-13 19:35:29.000 UTC) |
| MJD_LAST | 52413.985 (2002-05-19 23:38:07.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.25e-13 ± 1.2e-13 erg cm-2 s-1
Hardness ratios
HR1
-0.15
± 0.17
0.2-0.5 / 0.5-1.0 keV
HR2
0.33
± 0.15
0.5-1.0 / 1.0-2.0 keV
HR3
-0.87
± 0.23
1.0-2.0 / 2.0-4.5 keV
HR4
0.95
± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent:
13.45
± 3.31
arcsec
(ML 4.8)
SUM_FLAG:
3
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 4.03
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
- 4080207
- Match probability
- 0.758
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.593 | 0.157 |
| B | 20.416 | 0.095 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.00e-14 (+1.4e-13 / −4.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.06e+20 (+1.5e+21 / −2.3e+19) cm−2 |
| Photon index (Γ) | 1.66 (+2.26 / −1.24) |
| DoF | 210 |
| p-value | 0.559 |
| 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.