5XMM J124638.0+022317
5XMM-DR15 stacked source · SRCID 3005176010100097
Position:
12h46m38.04s +02d23m17.5s
(191.65850°, 2.38820°)
EP flux
9.93e-16
± 5.8e-16
erg cm-2 s-1
CLASSX
AGN
(0.808)
Detections
7
| SRCID | 3005176010100097 |
|---|---|
| IAUNAME | 5XMM J124638.0+022317 |
| SC_RA | 12h46m38.04s (191.65850°) |
| SC_DEC | +02d23m17.5s (2.38820°) |
| RADEC_ERR | 0.94 arcsec |
| LII / BII | 300.0666° / 65.2332° |
| N_CONTRIB | 7 (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): 9.93e-16 ± 5.8e-16 erg cm-2 s-1
Hardness ratios
HR1
-0.22
± 0.48
0.2-0.5 / 0.5-1.0 keV
HR2
0.74
± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67
± 0.23
1.0-2.0 / 2.0-4.5 keV
HR4
0.16
± 0.58
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.5)
SUM_FLAG:
3
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.719
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
- 3284104
- Match probability
- 0.684
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 20.472 | 0.214 |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.95e-14 (+5.3e-14 / −4.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.00e+19 (+2.3e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 2.79 (+2.91 / −2.69) |
| DoF | 1849 |
| p-value | 0 |
| Quality flag | 5 |
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.