5XMM J022230.8+430357
5XMM-DR15 stacked source · SRCID 3000297020100189
Position:
02h22m30.83s +43d03m57.2s
(35.62847°, 43.06588°)
EP flux
1.13e-13
± 3.4e-14
erg cm-2 s-1
CLASSX
Extended
(0.999)
Detections
1
| SRCID | 3000297020100189 |
|---|---|
| IAUNAME | 5XMM J022230.8+430357 |
| SC_RA | 02h22m30.83s (35.62847°) |
| SC_DEC | +43d03m57.2s (43.06588°) |
| RADEC_ERR | 2.93 arcsec |
| LII / BII | 140.1055° / -16.7482° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 9 (observations covering the position) |
| MJD_FIRST | 52310.692 (2002-02-05 16:35:53.000 UTC) |
| MJD_LAST | 52310.949 (2002-02-05 22:46:20.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.13e-13 ± 3.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.36
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.17
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.13
± 0.29
2.0-4.5 / 4.5-12.0 keV
Extent:
20.70
± 2.02
arcsec
(ML 48.6)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.27
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
- 795492
- Match probability
- 0.87
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 18.929 | 0.024 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.85e-14 (+2.5e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.16e+20 (+9.8e+20 / −3.1e+19) cm−2 |
| Photon index (Γ) | 2.03 (+2.45 / −1.70) |
| DoF | 87 |
| p-value | 0.753 |
| 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.