5XMM J013951.2-675550
5XMM-DR15 stacked source · SRCID 3003214040100023
Position:
01h39m51.25s -67d55m50.2s
(24.96354°, -67.93060°)
EP flux
2.12e-14
± 5.6e-15
erg cm-2 s-1
CLASSX
AGN
(0.924)
Detections
2
| SRCID | 3003214040100023 |
|---|---|
| IAUNAME | 5XMM J013951.2-675550 |
| SC_RA | 01h39m51.25s (24.96354°) |
| SC_DEC | -67d55m50.2s (-67.93060°) |
| RADEC_ERR | 0.73 arcsec |
| LII / BII | 296.0965° / -48.5500° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52032.413 (2001-05-03 09:54:03.000 UTC) |
| MJD_LAST | 52625.252 (2002-12-17 06:03:10.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.12e-14 ± 5.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.11
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.17
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.45
± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.508
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
- 675735
- Match probability
- 0.941
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 22.002 | 0.464 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.54e-14 (+1.9e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.13e+21 (+2.4e+21 / −1.5e+20) cm−2 |
| Photon index (Γ) | 2.03 (+2.53 / −1.63) |
| DoF | 95 |
| p-value | 0.765 |
| 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.