5XMM J021952.2-042448
5XMM-DR15 stacked source · SRCID 3003798230100495
Position:
02h19m52.27s -04d24m48.1s
(34.96781°, -4.41336°)
EP flux
8.29e-14
± 1.2e-14
erg cm-2 s-1
CLASSX
AGN
(0.92)
Detections
4
| SRCID | 3003798230100495 |
|---|---|
| IAUNAME | 5XMM J021952.2-042448 |
| SC_RA | 02h19m52.27s (34.96781°) |
| SC_DEC | -04d24m48.1s (-4.41336°) |
| RADEC_ERR | 0.32 arcsec |
| LII / BII | 169.7042° / -59.0030° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52665.809 (2003-01-26 19:24:42.000 UTC) |
| MJD_LAST | 57756.119 (2017-01-03 02:51:26.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.29e-14 ± 1.2e-14 erg cm-2 s-1
Hardness ratios
HR1
0.37
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.25
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.24
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.32
± 0.14
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: -0.00704
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 | 1.86e-13 (+2.1e-13 / −1.7e-13) erg cm−2 s−1 |
|---|---|
| NH | 9.57e+19 (+3.1e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 1.44 (+1.54 / −1.35) |
| DoF | 384 |
| p-value | 0.949 |
| Inter-instrument norm. | 0.96 (0.85–1.08) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 14.100 (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.