5XMM J000311.5-295810
5XMM-DR15 stacked source · SRCID 3004175010100043
Position:
00h03m11.53s -29d58m10.8s
(0.79805°, -29.96967°)
EP flux
1.58e-14
± 2.8e-15
erg cm-2 s-1
CLASSX
Star
(0.677)
Detections
1
| SRCID | 3004175010100043 |
|---|---|
| IAUNAME | 5XMM J000311.5-295810 |
| SC_RA | 00h03m11.53s (0.79805°) |
| SC_DEC | -29d58m10.8s (-29.96967°) |
| RADEC_ERR | 0.54 arcsec |
| LII / BII | 15.0823° / -79.0370° |
| 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): 1.58e-14 ± 2.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.27
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.48
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.66
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26
± 0.36
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.
Star
CLASSX outlier: 3.94
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
- 9423
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.093 | 0.157 |
| B | — | — |
| V | 18.647 | 0.059 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.18e-14 (+1.3e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.52e+20 (+1.2e+21 / −5.4e+20) cm−2 |
| Photon index (Γ) | 2.85 (+2.96 / −2.65) |
| DoF | 235 |
| p-value | 0.842 |
| Inter-instrument norm. | 0.69 (0.57–0.82) |
| 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.