5XMM J004329.3-202839
5XMM-DR15 stacked source · SRCID 3004234020100005
Position:
00h43m29.38s -20d28m39.0s
(10.87242°, -20.47751°)
EP flux
1.97e-13
± 1.9e-14
erg cm-2 s-1
CLASSX
AGN
(0.814)
Detections
2
| SRCID | 3004234020100005 |
|---|---|
| IAUNAME | 5XMM J004329.3-202839 |
| SC_RA | 00h43m29.38s (10.87242°) |
| SC_DEC | -20d28m39.0s (-20.47751°) |
| RADEC_ERR | 0.30 arcsec |
| LII / BII | 107.2318° / -83.1057° |
| 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): 1.97e-13 ± 1.9e-14 erg cm-2 s-1
Hardness ratios
HR1
0.02
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.02
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.25
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.14
± 0.09
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.6)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.867
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
- 152668
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.013 | 0.063 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.00e-13 (+2.1e-13 / −1.9e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.39e+19 (+1.4e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 2.35 (+2.44 / −2.26) |
| DoF | 517 |
| p-value | 0.946 |
| Inter-instrument norm. | 1.01 (0.93–1.10) |
| 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.