5XMM J230014.0+584857
5XMM-DR15 stacked source · SRCID 3003814010100190
Position:
23h00m14.03s +58d48m57.1s
(345.05846°, 58.81586°)
EP flux
3.44e-14
± 1.4e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
12
| SRCID | 3003814010100190 |
|---|---|
| IAUNAME | 5XMM J230014.0+584857 |
| SC_RA | 23h00m14.03s (345.05846°) |
| SC_DEC | +58d48m57.1s (58.81586°) |
| RADEC_ERR | 3.90 arcsec |
| LII / BII | 108.9547° / -1.0049° |
| 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): 3.44e-14 ± 1.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.95
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.64
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.79
± 0.24
1.0-2.0 / 2.0-4.5 keV
HR4
0.47
± 0.62
2.0-4.5 / 4.5-12.0 keV
Extent:
25.16
± 2.28
arcsec
(ML 33.3)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.53
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
- 6515388
- Match probability
- 0.656
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 20.030 | 0.085 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 20.311 | 0.131 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.55e-14 (+1.8e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.64e+21 (+2.2e+21 / −1.0e+21) cm−2 |
| Photon index (Γ) | 2.85 (+2.96 / −2.65) |
| DoF | 130 |
| p-value | 0.087 |
| 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.