5XMM J213840.4-424239
5XMM-DR15 stacked source · SRCID 3006194020100004
Position:
21h38m40.41s -42d42m39.8s
(324.66839°, -42.71107°)
EP flux
1.36e-13
± 1.4e-14
erg cm-2 s-1
CLASSX
Star
(0.999)
Detections
2
| SRCID | 3006194020100004 |
|---|---|
| IAUNAME | 5XMM J213840.4-424239 |
| SC_RA | 21h38m40.41s (324.66839°) |
| SC_DEC | -42d42m39.8s (-42.71107°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 358.1554° / -48.1804° |
| 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): 1.36e-13 ± 1.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.49
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.71
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.91
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.34
± 1.48
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.37
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
- 6379905
- Match probability
- 1
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 14.483 | 0.014 |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.23e-13 (+1.4e-13 / −1.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 9.00e+19 (+3.5e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 2.88 (+2.96 / −2.73) |
| DoF | 72 |
| p-value | 0.07 |
| 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.