5XMM J052204.8-362835
5XMM-DR15 stacked source · SRCID 3006576020100050
Position:
05h22m04.81s -36d28m35.0s
(80.52004°, -36.47639°)
EP flux
1.10e-14
± 3.6e-15
erg cm-2 s-1
CLASSX
AGN
(0.931)
Detections
2
| SRCID | 3006576020100050 |
|---|---|
| IAUNAME | 5XMM J052204.8-362835 |
| SC_RA | 05h22m04.81s (80.52004°) |
| SC_DEC | -36d28m35.0s (-36.47639°) |
| RADEC_ERR | 0.71 arcsec |
| LII / BII | 240.5865° / -32.8941° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52556.992 (2002-10-09 23:49:05.000 UTC) |
| MJD_LAST | 53596.399 (2005-08-14 09:34:51.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.10e-14 ± 3.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.38
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.04
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.03
± 0.25
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.
AGN
CLASSX outlier: -0.306
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
- 1545175
- Match probability
- 0.973
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.459 | 0.217 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.13e-14 (+4.0e-14 / −2.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.06e+20 (+5.0e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.32 (+1.57 / −1.13) |
| DoF | 441 |
| p-value | 0.892 |
| Inter-instrument norm. | 1.03 (0.78–1.36) |
| 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.