5XMM J130520.3-101855
5XMM-DR15 stacked source · SRCID 3003214120100022
Position:
13h05m20.37s -10d18m55.0s
(196.33487°, -10.31528°)
EP flux
9.79e-15
± 3.7e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.496)
Detections
1
| SRCID | 3003214120100022 |
|---|---|
| IAUNAME | 5XMM J130520.3-101855 |
| SC_RA | 13h05m20.37s (196.33487°) |
| SC_DEC | -10d18m55.0s (-10.31528°) |
| RADEC_ERR | 1.06 arcsec |
| LII / BII | 308.5420° / 52.4050° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52277.625 (2002-01-03 14:59:24.000 UTC) |
| MJD_LAST | 52277.781 (2002-01-03 18:45:19.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.79e-15 ± 3.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.92
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.43
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.74
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.15
± 1.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 3.63
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
- 3403330
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 19.825 | 0.059 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.07e-14 (+1.3e-14 / −8.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.17e+21 (+2.0e+21 / −1.9e+20) cm−2 |
| Photon index (Γ) | 2.59 (+2.88 / −2.17) |
| DoF | 51 |
| p-value | 0.428 |
| 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.