5XMM J104856.7-583245
5XMM-DR15 stacked source · SRCID 3005454010100010
Position:
10h48m56.73s -58d32m45.2s
(162.23638°, -58.54590°)
EP flux
1.17e-14
± 6.3e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3005454010100010 |
|---|---|
| IAUNAME | 5XMM J104856.7-583245 |
| SC_RA | 10h48m56.73s (162.23638°) |
| SC_DEC | -58d32m45.2s (-58.54590°) |
| RADEC_ERR | 1.00 arcsec |
| LII / BII | 287.5161° / 0.6108° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52496.374 (2002-08-10 08:58:30.000 UTC) |
| MJD_LAST | 52496.646 (2002-08-10 15:30:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.17e-14 ± 6.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.81
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.65
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-1.00
± 0.47
1.0-2.0 / 2.0-4.5 keV
HR4
—
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.15
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
- 2939216
- Match probability
- 0.758
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 15.019 | 0.020 |
| UVM2 | 14.872 | 0.014 |
| UVW1 | 13.362 | 0.007 |
| U | 12.395 | 0.002 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.24e-14 (+2.8e-14 / −1.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.47e+20 (+1.3e+21 / −4.6e+19) cm−2 |
| Photon index (Γ) | 2.70 (+2.92 / −2.37) |
| DoF | 63 |
| p-value | 0.062 |
| 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.