5XMM J180241.7-295510
5XMM-DR15 stacked source · SRCID 3005094010100004
Position:
18h02m41.72s -29d55m10.4s
(270.67383°, -29.91955°)
EP flux
1.16e-13
± 1.0e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.412)
Detections
2
| SRCID | 3005094010100004 |
|---|---|
| IAUNAME | 5XMM J180241.7-295510 |
| SC_RA | 18h02m41.72s (270.67383°) |
| SC_DEC | -29d55m10.4s (-29.91955°) |
| RADEC_ERR | 0.26 arcsec |
| LII / BII | 1.0320° / -3.7048° |
| 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): 1.16e-13 ± 1.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.79
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.30
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.60
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.69
± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.54
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 | 2.56e-13 (+2.7e-13 / −2.4e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.22e+21 (+4.6e+21 / −3.8e+21) cm−2 |
| Photon index (Γ) | 2.77 (+2.91 / −2.61) |
| DoF | 869 |
| p-value | 0.37 |
| Inter-instrument norm. | 1.03 (0.95–1.11) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.300 (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.