5XMM J230124.1+590252
5XMM-DR15 stacked source · SRCID 3003814010100085
Position:
23h01m24.18s +59d02m52.0s
(345.35073°, 59.04779°)
EP flux
4.40e-13
± 3.1e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
12
| SRCID | 3003814010100085 |
|---|---|
| IAUNAME | 5XMM J230124.1+590252 |
| SC_RA | 23h01m24.18s (345.35073°) |
| SC_DEC | +59d02m52.0s (59.04779°) |
| RADEC_ERR | 2.03 arcsec |
| LII / BII | 109.1879° / -0.8560° |
| N_CONTRIB | 12 (detections) |
| N_OBS | 13 (observations covering the position) |
| MJD_FIRST | 52436.379 (2002-06-11 09:06:08.000 UTC) |
| MJD_LAST | 60126.222 (2023-07-01 05:19:00.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.40e-13 ± 3.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.93
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.02
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.98
± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
0.36
± 0.48
2.0-4.5 / 4.5-12.0 keV
Extent:
58.26
± 1.61
arcsec
(ML 499.9)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.83
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
- 6518801
- Match probability
- 0.946
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 20.382 | 0.124 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.12e-14 (+3.4e-14 / −9.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.77e+20 (+1.3e+21 / −2.8e+19) cm−2 |
| Photon index (Γ) | 2.39 (+2.79 / −1.83) |
| DoF | 85 |
| p-value | 0.83 |
| 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.