5XMM J180410.0-241515
5XMM-DR15 stacked source · SRCID 3000882010100594
Position:
18h04m10.03s -24d15m15.2s
(271.04180°, -24.25421°)
EP flux
9.12e-15
± 3.5e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.281)
Detections
4
| SRCID | 3000882010100594 |
|---|---|
| IAUNAME | 5XMM J180410.0-241515 |
| SC_RA | 18h04m10.03s (271.04180°) |
| SC_DEC | -24d15m15.2s (-24.25421°) |
| RADEC_ERR | 0.74 arcsec |
| LII / BII | 6.1345° / -1.2109° |
| 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): 9.12e-15 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.57
± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
0.53
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.30
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.65
± 0.30
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.
Bkg_AGN
CLASSX outlier: 5.46
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 | 2.69e-14 (+3.4e-14 / −2.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.60e+20 (+2.0e+21 / −4.6e+19) cm−2 |
| Photon index (Γ) | 1.67 (+2.17 / −1.41) |
| DoF | 316 |
| p-value | 0.317 |
| Inter-instrument norm. | 1.66 (1.35–1.89) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 12.100 (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.