5XMM J000241.7-295259
5XMM-DR15 stacked source · SRCID 3004175010100127
Position:
00h02m41.78s -29d52m59.1s
(0.67407°, -29.88307°)
EP flux
4.53e-15
± 2.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.918)
Detections
1
| SRCID | 3004175010100127 |
|---|---|
| IAUNAME | 5XMM J000241.7-295259 |
| SC_RA | 00h02m41.78s (0.67407°) |
| SC_DEC | -29d52m59.1s (-29.88307°) |
| RADEC_ERR | 1.07 arcsec |
| LII / BII | 15.6411° / -78.9495° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52440.823 (2002-06-15 19:44:59.000 UTC) |
| MJD_LAST | 52441.421 (2002-06-16 10:06:17.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.53e-15 ± 2.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.09
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
0.01
± 0.18
0.5-1.0 / 1.0-2.0 keV
HR3
-0.57
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.79
± 0.46
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.0382
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
- 8320
- Match probability
- 0.981
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.916 | 0.134 |
| B | — | — |
| V | 21.214 | 0.284 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.18e-15 (+7.1e-15 / −3.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 9.46e+19 (+5.9e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 1.82 (+2.22 / −1.47) |
| DoF | 81 |
| p-value | 0.819 |
| 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.