5XMM J220450.5-015624
5XMM-DR15 stacked source · SRCID 3001244030100094
Position:
22h04m50.55s -01d56m24.6s
(331.21064°, -1.94017°)
EP flux
1.31e-15
± 8.7e-16
erg cm-2 s-1
CLASSX
Star
(1)
Detections
2
| SRCID | 3001244030100094 |
|---|---|
| IAUNAME | 5XMM J220450.5-015624 |
| SC_RA | 22h04m50.55s (331.21064°) |
| SC_DEC | -01d56m24.6s (-1.94017°) |
| RADEC_ERR | 1.16 arcsec |
| LII / BII | 57.9805° / -42.8502° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52053.362 (2001-05-24 08:40:51.000 UTC) |
| MJD_LAST | 57333.559 (2015-11-07 13:25:36.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.31e-15 ± 8.7e-16 erg cm-2 s-1
Hardness ratios
HR1
0.80
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
-0.40
± 0.15
0.5-1.0 / 1.0-2.0 keV
HR3
-0.55
± 0.28
1.0-2.0 / 2.0-4.5 keV
HR4
-0.78
± 1.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.6)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 0.803
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
- 6430337
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 17.510 | 0.028 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.01e-15 (+9.3e-15 / −4.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.24e+21 (+3.9e+21 / −5.2e+20) cm−2 |
| Photon index (Γ) | 2.18 (+2.77 / −1.47) |
| DoF | 472 |
| p-value | 0.568 |
| 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.