5XMM J130519.0-102324
5XMM-DR15 stacked source · SRCID 3003214120100002
Position:
13h05m19.02s -10d23m24.7s
(196.32925°, -10.39018°)
EP flux
1.47e-13
± 6.0e-15
erg cm-2 s-1
CLASSX
Star
(0.489)
Detections
1
| SRCID | 3003214120100002 |
|---|---|
| IAUNAME | 5XMM J130519.0-102324 |
| SC_RA | 13h05m19.02s (196.32925°) |
| SC_DEC | -10d23m24.7s (-10.39018°) |
| RADEC_ERR | 0.25 arcsec |
| LII / BII | 308.5222° / 52.3309° |
| 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): 1.47e-13 ± 6.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.33
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
-0.45
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.79
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.35
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
- 3403165
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 16.744 | 0.009 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.10e-13 (+1.2e-13 / −1.0e-13) erg cm−2 s−1 |
|---|---|
| NH | 3.61e+20 (+6.5e+20 / −6.7e+19) cm−2 |
| Photon index (Γ) | 2.89 (+2.97 / −2.74) |
| DoF | 158 |
| p-value | 0.307 |
| 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.