5XMM J001544.8-392249
5XMM-DR15 stacked source · SRCID 3002874020100104
Position:
00h15m44.87s -39d22m49.8s
(3.93694°, -39.38051°)
EP flux
2.70e-14
± 3.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.739)
Detections
9
| SRCID | 3002874020100104 |
|---|---|
| IAUNAME | 5XMM J001544.8-392249 |
| SC_RA | 00h15m44.87s (3.93694°) |
| SC_DEC | -39d22m49.8s (-39.38051°) |
| RADEC_ERR | 0.40 arcsec |
| LII / BII | 331.9089° / -75.6728° |
| N_CONTRIB | 9 (detections) |
| N_OBS | 10 (observations covering the position) |
| MJD_FIRST | 52227.605 (2001-11-14 14:31:49.000 UTC) |
| MJD_LAST | 59561.812 (2021-12-13 19:29:06.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.70e-14 ± 3.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.02
± 0.30
0.2-0.5 / 0.5-1.0 keV
HR2
0.85
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
0.28
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.06
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.6)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.25
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
- 24953
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.221 | 0.075 |
| U | — | — |
| B | — | — |
| V | 18.281 | 0.067 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.48e-14 (+3.9e-14 / −3.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.41e+19 (+3.7e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 1.13 (+1.25 / −1.04) |
| DoF | 708 |
| p-value | 0.122 |
| Inter-instrument norm. | 0.56 (0.52–0.63) |
| 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.