5XMM J180336.6-241725
5XMM-DR15 stacked source · SRCID 3000882010100230
Position:
18h03m36.65s -24d17m25.6s
(270.90269°, -24.29043°)
EP flux
8.24e-14
± 6.6e-15
erg cm-2 s-1
CLASSX
Gal_XRB
(0.871)
Detections
4
| SRCID | 3000882010100230 |
|---|---|
| IAUNAME | 5XMM J180336.6-241725 |
| SC_RA | 18h03m36.65s (270.90269°) |
| SC_DEC | -24d17m25.6s (-24.29043°) |
| RADEC_ERR | 0.33 arcsec |
| LII / BII | 6.0407° / -1.1182° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 51976.478 (2001-03-08 11:29:01.000 UTC) |
| MJD_LAST | 56721.578 (2014-03-05 13:52:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.24e-14 ± 6.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.90
± 0.59
0.2-0.5 / 0.5-1.0 keV
HR2
0.97
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
0.32
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 4.9
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.41e-13 (+1.6e-13 / −1.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 2.10e+22 (+2.5e+22 / −1.7e+22) cm−2 |
| Photon index (Γ) | 2.35 (+2.65 / −2.06) |
| DoF | 438 |
| p-value | 0.275 |
| Inter-instrument norm. | 0.98 (0.86–1.12) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.400 (approximate flux variability amplitude) |
|---|
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.