5XMM J124326.8+112631
5XMM-DR15 stacked source · SRCID 3002154020100042
Position:
12h43m26.81s +11d26m31.3s
(190.86169°, 11.44203°)
EP flux
6.51e-15
± 2.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.568)
Detections
3
| SRCID | 3002154020100042 |
|---|---|
| IAUNAME | 5XMM J124326.8+112631 |
| SC_RA | 12h43m26.81s (190.86169°) |
| SC_DEC | +11d26m31.3s (11.44203°) |
| RADEC_ERR | 0.44 arcsec |
| LII / BII | 295.7221° / 74.2018° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 51911.682 (2001-01-02 16:22:30.000 UTC) |
| MJD_LAST | 58643.477 (2019-06-09 11:26:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.51e-15 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.30
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.39
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41
± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
0.14
± 0.31
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.96
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 | 2.59e-14 (+2.8e-14 / −2.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.54e+21 (+1.9e+21 / −1.1e+21) cm−2 |
| Photon index (Γ) | 2.67 (+2.88 / −2.45) |
| DoF | 344 |
| p-value | 0.916 |
| Inter-instrument norm. | 1.03 (0.90–1.16) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 6.600 (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.