5XMM J230452.2+121944
5XMM-DR15 stacked source · SRCID 3002554100100030
Position:
23h04m52.21s +12d19m44.0s
(346.21755°, 12.32890°)
EP flux
7.02e-15
± 1.6e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.545)
Detections
3
| SRCID | 3002554100100030 |
|---|---|
| IAUNAME | 5XMM J230452.2+121944 |
| SC_RA | 23h04m52.21s (346.21755°) |
| SC_DEC | +12d19m44.0s (12.32890°) |
| RADEC_ERR | 0.53 arcsec |
| LII / BII | 86.2546° / -42.8269° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52079.650 (2001-06-19 15:36:24.000 UTC) |
| MJD_LAST | 58269.479 (2018-05-31 11:29:14.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.02e-15 ± 1.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.66
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.14
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.75
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.31
± 0.31
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 2.33
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
- 6526313
- Match probability
- 0.987
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 20.094 | 0.075 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.52e-14 (+5.5e-14 / −3.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.70e+21 (+2.5e+21 / −6.5e+20) cm−2 |
| Photon index (Γ) | 2.24 (+2.63 / −1.83) |
| DoF | 232 |
| p-value | 0.814 |
| Inter-instrument norm. | 1.53 (1.27–1.78) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.800 (approximate flux variability amplitude) |
|---|
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.