5XMM J022036.1-033804
5XMM-DR15 stacked source · SRCID 3003798260103578
Position:
02h20m36.17s -03d38m04.5s
(35.15069°, -3.63457°)
EP flux
1.55e-14
± 9.4e-15
erg cm-2 s-1
CLASSX
Star
(0.903)
Detections
2
| SRCID | 3003798260103578 |
|---|---|
| IAUNAME | 5XMM J022036.1-033804 |
| SC_RA | 02h20m36.17s (35.15069°) |
| SC_DEC | -03d38m04.5s (-3.63457°) |
| RADEC_ERR | 0.87 arcsec |
| LII / BII | 169.0043° / -58.2908° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52501.025 (2002-08-15 00:36:35.000 UTC) |
| MJD_LAST | 54110.383 (2007-01-10 09:11:49.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.55e-14 ± 9.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.41
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.44
± 0.15
0.5-1.0 / 1.0-2.0 keV
HR3
-0.86
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.92
± 4.27
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.58
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
- 782167
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.394 | 0.191 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.41e-14 (+1.9e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.65e+20 (+6.3e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 2.56 (+2.84 / −2.26) |
| DoF | 56 |
| p-value | 0.408 |
| 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.