5XMM J124643.6+022738
5XMM-DR15 stacked source · SRCID 3005176010100033
Position:
12h46m43.61s +02d27m38.1s
(191.68172°, 2.46059°)
EP flux
5.31e-14
± 1.0e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
8
| SRCID | 3005176010100033 |
|---|---|
| IAUNAME | 5XMM J124643.6+022738 |
| SC_RA | 12h46m43.61s (191.68172°) |
| SC_DEC | +02d27m38.1s (2.46059°) |
| RADEC_ERR | 1.81 arcsec |
| LII / BII | 300.1144° / 65.3066° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52077.875 (2001-06-17 20:59:59.000 UTC) |
| MJD_LAST | 57038.758 (2015-01-16 18:11:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.31e-14 ± 1.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.23
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.23
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.27
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.59
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
17.28
± 0.96
arcsec
(ML 125.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 1.53
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
- 3284556
- Match probability
- 0.778
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.403 | 0.281 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.66e-14 (+2.2e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.55e+20 (+8.2e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.67 (+2.01 / −1.38) |
| DoF | 331 |
| p-value | 0.933 |
| 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.