5XMM J182319.8-134009
5XMM-DR15 stacked source · SRCID 3004014020100007
Position:
18h23m19.80s -13d40m09.8s
(275.83251°, -13.66938°)
EP flux
2.58e-13
± 1.8e-14
erg cm-2 s-1
CLASSX
Gal_XRB
(0.965)
Detections
2
| SRCID | 3004014020100007 |
|---|---|
| IAUNAME | 5XMM J182319.8-134009 |
| SC_RA | 18h23m19.80s (275.83251°) |
| SC_DEC | -13d40m09.8s (-13.66938°) |
| RADEC_ERR | 0.46 arcsec |
| LII / BII | 17.5932° / -0.1125° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52356.582 (2002-03-23 13:58:12.000 UTC) |
| MJD_LAST | 52358.101 (2002-03-25 02:25:12.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.58e-13 ± 1.8e-14 erg cm-2 s-1
Hardness ratios
HR1
0.04
± 0.88
0.2-0.5 / 0.5-1.0 keV
HR2
0.97
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
0.67
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.11
± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 8.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 5.09
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 | 2.06e-13 (+2.3e-13 / −1.9e-13) erg cm−2 s−1 |
|---|---|
| NH | 3.10e+22 (+3.9e+22 / −2.5e+22) cm−2 |
| Photon index (Γ) | 1.25 (+1.50 / −1.06) |
| DoF | 350 |
| p-value | 0.892 |
| Inter-instrument norm. | 1.24 (1.09–1.41) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 6.600 (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.