5XMM J180307.2-295726
5XMM-DR15 stacked source · SRCID 3005094010100021
Position:
18h03m07.24s -29d57m26.5s
(270.78017°, -29.95735°)
EP flux
1.52e-14
± 2.3e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
2
| SRCID | 3005094010100021 |
|---|---|
| IAUNAME | 5XMM J180307.2-295726 |
| SC_RA | 18h03m07.24s (270.78017°) |
| SC_DEC | -29d57m26.5s (-29.95735°) |
| RADEC_ERR | 0.56 arcsec |
| LII / BII | 1.0442° / -3.8036° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 52344.742 (2002-03-11 17:47:50.000 UTC) |
| MJD_LAST | 53278.725 (2004-09-30 17:24:22.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.52e-14 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.42
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.90
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.86
± 0.28
1.0-2.0 / 2.0-4.5 keV
HR4
0.03
± 0.90
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.19
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
- 5146985
- Match probability
- 0.833
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 18.364 | 0.039 |
| UVW1 | 14.956 | 0.006 |
| U | 13.614 | 0.002 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.73e-15 (+1.2e-14 / −6.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.59e+19 (+2.6e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.77 (+2.94 / −2.44) |
| DoF | 45 |
| p-value | 0.427 |
| 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.