5XMM J213924.0-423521
5XMM-DR15 stacked source · SRCID 3006194020100001
Position:
21h39m24.04s -42d35m21.3s
(324.85015°, -42.58926°)
EP flux
8.90e-13
± 2.8e-14
erg cm-2 s-1
CLASSX
AGN
(0.645)
Detections
2
| SRCID | 3006194020100001 |
|---|---|
| IAUNAME | 5XMM J213924.0-423521 |
| SC_RA | 21h39m24.04s (324.85015°) |
| SC_DEC | -42d35m21.3s (-42.58926°) |
| RADEC_ERR | 0.14 arcsec |
| LII / BII | 358.3171° / -48.3258° |
| 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): 8.90e-13 ± 2.8e-14 erg cm-2 s-1
Hardness ratios
HR1
-0.12
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
-0.25
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.11
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.00e-13 (+5.2e-13 / −4.8e-13) erg cm−2 s−1 |
|---|---|
| NH | 1.82e+19 (+3.4e+19 / −1.2e+19) cm−2 |
| Photon index (Γ) | 2.52 (+2.56 / −2.47) |
| DoF | 819 |
| p-value | 0.099 |
| Inter-instrument norm. | 0.92 (0.87–0.97) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.300 (approximate flux variability amplitude) |
|---|
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.