5XMM J125501.7+271851
5XMM-DR15 stacked source · SRCID 3005894070102127
Position:
12h55m01.78s +27d18m51.7s
(193.75742°, 27.31437°)
EP flux
1.07e-14
± 6.5e-15
erg cm-2 s-1
CLASSX
Star
(0.956)
Detections
1
| SRCID | 3005894070102127 |
|---|---|
| IAUNAME | 5XMM J125501.7+271851 |
| SC_RA | 12h55m01.78s (193.75742°) |
| SC_DEC | +27d18m51.7s (27.31437°) |
| RADEC_ERR | 1.20 arcsec |
| LII / BII | 46.2578° / 89.1801° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 60 (observations covering the position) |
| MJD_FIRST | 52800.064 (2003-06-10 01:31:43.000 UTC) |
| MJD_LAST | 52800.323 (2003-06-10 07:44:41.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.07e-14 ± 6.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.38
± 0.23
0.2-0.5 / 0.5-1.0 keV
HR2
0.05
± 0.20
0.5-1.0 / 1.0-2.0 keV
HR3
-0.97
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49
± 2.30
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.93
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
- 3325476
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 19.614 | 0.148 |
| UVW1 | 17.353 | 0.028 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.00e-14 (+2.8e-14 / −1.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.24e+20 (+2.1e+21 / −4.4e+19) cm−2 |
| Photon index (Γ) | 2.20 (+2.73 / −1.74) |
| DoF | 52 |
| p-value | 0.594 |
| 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.