5XMM J182117.6-142913
5XMM-DR15 stacked source · SRCID 3000421020100200
Position:
18h21m17.66s -14d29m13.7s
(275.32359°, -14.48715°)
EP flux
3.79e-14
± 1.8e-14
erg cm-2 s-1
CLASSX
Gal_XRB
(0.604)
Detections
2
| SRCID | 3000421020100200 |
|---|---|
| IAUNAME | 5XMM J182117.6-142913 |
| SC_RA | 18h21m17.66s (275.32359°) |
| SC_DEC | -14d29m13.7s (-14.48715°) |
| RADEC_ERR | 0.88 arcsec |
| LII / BII | 16.6394° / -0.0608° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 51976.925 (2001-03-08 22:11:33.000 UTC) |
| MJD_LAST | 54373.420 (2007-09-30 10:04:49.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.79e-14 ± 1.8e-14 erg cm-2 s-1
Hardness ratios
HR1
-0.76
± 0.69
0.2-0.5 / 0.5-1.0 keV
HR2
0.97
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.45
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.34
± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 5.13
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 | 1.53e-13 (+1.8e-13 / −1.2e-13) erg cm−2 s−1 |
|---|---|
| NH | 2.37e+21 (+4.8e+21 / −7.4e+20) cm−2 |
| Photon index (Γ) | 1.31 (+1.74 / −1.08) |
| DoF | 182 |
| p-value | 0.776 |
| Inter-instrument norm. | 1.31 (1.01–1.64) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.600 (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.