5XMM J180340.1-295122
5XMM-DR15 stacked source · SRCID 3005094010100022
Position:
18h03m40.16s -29d51m22.8s
(270.91733°, -29.85634°)
EP flux
9.88e-14
± 1.4e-14
erg cm-2 s-1
CLASSX
AGN
(0.608)
Detections
2
| SRCID | 3005094010100022 |
|---|---|
| IAUNAME | 5XMM J180340.1-295122 |
| SC_RA | 18h03m40.16s (270.91733°) |
| SC_DEC | -29d51m22.8s (-29.85634°) |
| RADEC_ERR | 0.55 arcsec |
| LII / BII | 1.1907° / -3.8580° |
| 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): 9.88e-14 ± 1.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.71
± 0.33
0.2-0.5 / 0.5-1.0 keV
HR2
0.78
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
0.17
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.15
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 3.29
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.
Optical Monitor (OM)
- OM Source ID
- 5153090
- Match probability
- 0.686
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.779 | 0.357 |
| U | 18.864 | 0.056 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.28e-14 (+8.5e-14 / −6.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.33e+20 (+2.0e+21 / −1.8e+20) cm−2 |
| Photon index (Γ) | 1.14 (+1.32 / −1.03) |
| DoF | 288 |
| p-value | 0.859 |
| Inter-instrument norm. | 1.19 (0.96–1.46) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 10.100 (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.