5XMM J004336.7-203325
5XMM-DR15 stacked source · SRCID 3004234020100026
Position:
00h43m36.72s -20d33m25.3s
(10.90300°, -20.55703°)
EP flux
1.58e-14
± 3.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.932)
Detections
2
| SRCID | 3004234020100026 |
|---|---|
| IAUNAME | 5XMM J004336.7-203325 |
| SC_RA | 00h43m36.72s (10.90300°) |
| SC_DEC | -20d33m25.3s (-20.55703°) |
| RADEC_ERR | 0.54 arcsec |
| LII / BII | 107.2927° / -83.1899° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52278.767 (2002-01-04 18:23:55.000 UTC) |
| MJD_LAST | 58644.428 (2019-06-10 10:16:11.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.58e-14 ± 3.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.48
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.21
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.22
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.37
± 0.22
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: -0.545
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
- 155067
- Match probability
- 0.989
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.262 | 0.251 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.79e-14 (+2.3e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.13e+19 (+1.5e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.93 (+2.23 / −1.69) |
| DoF | 246 |
| p-value | 0.659 |
| Inter-instrument norm. | 0.56 (0.52–0.65) |
| 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.