5XMM J230157.2+584517
5XMM-DR15 stacked source · SRCID 3003814010100042
Position:
23h01m57.23s +58d45m17.0s
(345.48844°, 58.75471°)
EP flux
2.46e-14
± 4.9e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.348)
Detections
12
| SRCID | 3003814010100042 |
|---|---|
| IAUNAME | 5XMM J230157.2+584517 |
| SC_RA | 23h01m57.23s (345.48844°) |
| SC_DEC | +58d45m17.0s (58.75471°) |
| RADEC_ERR | 0.52 arcsec |
| LII / BII | 109.1326° / -1.1524° |
| N_CONTRIB | 12 (detections) |
| N_OBS | 13 (observations covering the position) |
| MJD_FIRST | 52296.715 (2002-01-22 17:09:56.000 UTC) |
| MJD_LAST | 60126.222 (2023-07-01 05:19:00.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.46e-14 ± 4.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.86
± 0.22
0.2-0.5 / 0.5-1.0 keV
HR2
0.77
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.33
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.89
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
- 6520770
- Match probability
- 0.714
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.624 | 0.317 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.94e-14 (+8.2e-14 / −6.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.20e+21 (+9.1e+21 / −4.2e+21) cm−2 |
| Photon index (Γ) | 1.97 (+2.31 / −1.63) |
| DoF | 256 |
| p-value | 0.221 |
| Inter-instrument norm. | 1.85 (1.68–1.96) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 14.700 (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.