5XMM J022027.5-044934
5XMM-DR15 stacked source · SRCID 3003798200100158
Position:
02h20m27.59s -04d49m34.2s
(35.11494°, -4.82616°)
EP flux
1.02e-13
± 6.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.758)
Detections
5
| SRCID | 3003798200100158 |
|---|---|
| IAUNAME | 5XMM J022027.5-044934 |
| SC_RA | 02h20m27.59s (35.11494°) |
| SC_DEC | -04d49m34.2s (-4.82616°) |
| RADEC_ERR | 0.22 arcsec |
| LII / BII | 170.4465° / -59.2191° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52500.578 (2002-08-14 13:52:48.000 UTC) |
| MJD_LAST | 57770.061 (2017-01-17 01:28:18.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.02e-13 ± 6.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.16
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.05
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.41
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.584
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
- 781340
- Match probability
- 0.99
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.398 | 0.271 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.86e-14 (+7.6e-14 / −6.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.00e+20 (+1.1e+21 / −3.5e+20) cm−2 |
| Photon index (Γ) | 2.01 (+2.19 / −1.82) |
| DoF | 411 |
| p-value | 0.791 |
| Inter-instrument norm. | 1.27 (1.14–1.41) |
| 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.