5XMM J124911.3-410915
5XMM-DR15 stacked source · SRCID 3004634010100203
Position:
12h49m11.36s -41d09m15.4s
(192.29732°, -41.15428°)
EP flux
6.49e-16
± 7.0e-16
erg cm-2 s-1
CLASSX
AGN
(0.817)
Detections
6
| SRCID | 3004634010100203 |
|---|---|
| IAUNAME | 5XMM J124911.3-410915 |
| SC_RA | 12h49m11.36s (192.29732°) |
| SC_DEC | -41d09m15.4s (-41.15428°) |
| RADEC_ERR | 0.60 arcsec |
| LII / BII | 302.4763° / 21.7155° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 12 (observations covering the position) |
| MJD_FIRST | 52277.006 (2002-01-03 00:08:36.000 UTC) |
| MJD_LAST | 58506.812 (2019-01-23 19:29:35.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.49e-16 ± 7.0e-16 erg cm-2 s-1
Hardness ratios
HR1
-0.02
± 0.62
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03
± 0.90
0.5-1.0 / 1.0-2.0 keV
HR3
0.02
± 0.90
1.0-2.0 / 2.0-4.5 keV
HR4
-0.08
± 0.74
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.6)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.598
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
- 3303925
- Match probability
- 0.982
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 22.250 | 0.346 |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.67e-14 (+2.2e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.59e+20 (+1.4e+21 / −2.3e+19) cm−2 |
| Photon index (Γ) | 1.36 (+1.77 / −1.12) |
| DoF | 436 |
| p-value | 0.869 |
| 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.