5XMM J213829.7-423957
5XMM-DR15 stacked source · SRCID 3006194020100005
Position:
21h38m29.76s -42d39m57.7s
(324.62398°, -42.66603°)
EP flux
1.96e-13
± 2.3e-14
erg cm-2 s-1
CLASSX
AGN
(0.928)
Detections
2
| SRCID | 3006194020100005 |
|---|---|
| IAUNAME | 5XMM J213829.7-423957 |
| SC_RA | 21h38m29.76s (324.62398°) |
| SC_DEC | -42d39m57.7s (-42.66603°) |
| RADEC_ERR | 0.38 arcsec |
| LII / BII | 358.2275° / -48.1525° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52030.786 (2001-05-01 18:51:27.000 UTC) |
| MJD_LAST | 54772.178 (2008-11-02 04:16:20.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.96e-13 ± 2.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.00
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.01
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.65
± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.778
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
- 6379830
- Match probability
- 1
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 19.322 | 0.172 |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.70e-13 (+1.9e-13 / −1.5e-13) erg cm−2 s−1 |
|---|---|
| NH | 7.89e+19 (+2.9e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 2.17 (+2.32 / −2.05) |
| DoF | 280 |
| p-value | 0.977 |
| Inter-instrument norm. | 1.15 (1.00–1.33) |
| 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.