5XMM J180350.7-300337
5XMM-DR15 stacked source · SRCID 3005094010100038
Position:
18h03m50.72s -30d03m37.1s
(270.96135°, -30.06032°)
EP flux
1.62e-14
± 5.2e-15
erg cm-2 s-1
CLASSX
Star
(0.868)
Detections
2
| SRCID | 3005094010100038 |
|---|---|
| IAUNAME | 5XMM J180350.7-300337 |
| SC_RA | 18h03m50.72s (270.96135°) |
| SC_DEC | -30d03m37.1s (-30.06032°) |
| RADEC_ERR | 0.82 arcsec |
| LII / BII | 1.0309° / -3.9908° |
| 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): 1.62e-14 ± 5.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.76
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.24
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.42
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.84
± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.13
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.
Optical Monitor (OM)
- OM Source ID
- 5155466
- Match probability
- 0.823
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.056 | 0.056 |
| U | 17.711 | 0.019 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.27e-14 (+3.4e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.50e+20 (+2.5e+21 / −3.7e+19) cm−2 |
| Photon index (Γ) | 2.00 (+2.55 / −1.52) |
| DoF | 47 |
| p-value | 0.669 |
| Quality flag | 0 |
No variability data available for this source.
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.