5XMM J230043.1+584321
5XMM-DR15 stacked source · SRCID 3003814010100091
Position:
23h00m43.16s +58d43m21.7s
(345.17983°, 58.72269°)
EP flux
9.79e-15
± 2.4e-15
erg cm-2 s-1
CLASSX
Star
(0.992)
Detections
11
| SRCID | 3003814010100091 |
|---|---|
| IAUNAME | 5XMM J230043.1+584321 |
| SC_RA | 23h00m43.16s (345.17983°) |
| SC_DEC | +58d43m21.7s (58.72269°) |
| RADEC_ERR | 0.69 arcsec |
| LII / BII | 108.9734° / -1.1157° |
| N_CONTRIB | 11 (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): 9.79e-15 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.86
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.37
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.79
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.87
± 0.62
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.72
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
- 6516608
- Match probability
- 0.932
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 17.051 | 0.008 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.27e-14 (+2.6e-14 / −2.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.64e+21 (+2.2e+21 / −8.7e+20) cm−2 |
| Photon index (Γ) | 2.81 (+2.95 / −2.51) |
| DoF | 147 |
| p-value | 0.086 |
| 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.