5XMM J023143.1-442552
5XMM-DR15 stacked source · SRCID 3004234030100014
Position:
02h31m43.11s -44d25m52.7s
(37.92964°, -44.43131°)
EP flux
1.40e-13
± 1.2e-14
erg cm-2 s-1
CLASSX
AGN
(0.769)
Detections
2
| SRCID | 3004234030100014 |
|---|---|
| IAUNAME | 5XMM J023143.1-442552 |
| SC_RA | 02h31m43.11s (37.92964°) |
| SC_DEC | -44d25m52.7s (-44.43131°) |
| RADEC_ERR | 0.26 arcsec |
| LII / BII | 260.2493° / -63.4919° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 52466.430 (2002-07-11 10:18:36.000 UTC) |
| MJD_LAST | 59215.542 (2021-01-01 13:00:24.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.40e-13 ± 1.2e-14 erg cm-2 s-1
Hardness ratios
HR1
0.12
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.00
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.24
± 0.09
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.444
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
- 837396
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.605 | 0.132 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.03e-13 (+1.1e-13 / −9.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.79e+19 (+2.8e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.87 (+1.97 / −1.79) |
| DoF | 544 |
| p-value | 0.823 |
| Inter-instrument norm. | 0.94 (0.85–1.04) |
| 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.