5XMM J223554.3+335316
5XMM-DR15 stacked source · SRCID 3002114020100027
Position:
22h35m54.39s +33d53m16.1s
(338.97662°, 33.88779°)
EP flux
1.11e-14
± 2.1e-15
erg cm-2 s-1
CLASSX
Star
(0.921)
Detections
1
| SRCID | 3002114020100027 |
|---|---|
| IAUNAME | 5XMM J223554.3+335316 |
| SC_RA | 22h35m54.39s (338.97662°) |
| SC_DEC | +33d53m16.1s (33.88779°) |
| RADEC_ERR | 0.58 arcsec |
| LII / BII | 93.2048° / -21.0449° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52250.890 (2001-12-07 21:22:09.000 UTC) |
| MJD_LAST | 52251.416 (2001-12-08 09:59:17.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.11e-14 ± 2.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.55
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.51
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.84
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.58
± 0.64
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.3
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
- 6472788
- Match probability
- 0.982
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.498 | 0.205 |
| B | 19.556 | 0.056 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.08e-14 (+1.3e-14 / −8.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 8.08e+19 (+3.8e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 2.71 (+2.90 / −2.45) |
| DoF | 584 |
| p-value | 0.296 |
| 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.