5XMM J032918.8+312326
5XMM-DR15 stacked source · SRCID 3006582010100022
Position:
03h29m18.81s +31d23m26.2s
(52.32838°, 31.39061°)
EP flux
8.91e-14
± 1.0e-14
erg cm-2 s-1
CLASSX
Star
(0.898)
Detections
1
| SRCID | 3006582010100022 |
|---|---|
| IAUNAME | 5XMM J032918.8+312326 |
| SC_RA | 03h29m18.81s (52.32838°) |
| SC_DEC | +31d23m26.2s (31.39061°) |
| RADEC_ERR | 0.38 arcsec |
| LII / BII | 158.3139° / -20.4248° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52332.927 (2002-02-27 22:15:11.000 UTC) |
| MJD_LAST | 52333.532 (2002-02-28 12:46:29.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.91e-14 ± 1.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.75
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.16
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.48
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.78
± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.1)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.36
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
- 956003
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.655 | 0.077 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.91e-14 (+6.3e-14 / −5.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.26e+21 (+3.5e+21 / −3.0e+21) cm−2 |
| Photon index (Γ) | 2.91 (+2.98 / −2.79) |
| DoF | 569 |
| p-value | 0.816 |
| Inter-instrument norm. | 1.29 (1.17–1.43) |
| 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.