5XMM J032921.9+311536
5XMM-DR15 stacked source · SRCID 3006582010100037
Position:
03h29m21.92s +31d15m36.7s
(52.34135°, 31.26019°)
EP flux
3.03e-14
± 4.9e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3006582010100037 |
|---|---|
| IAUNAME | 5XMM J032921.9+311536 |
| SC_RA | 03h29m21.92s (52.34135°) |
| SC_DEC | +31d15m36.7s (31.26019°) |
| RADEC_ERR | 0.69 arcsec |
| LII / BII | 158.4074° / -20.5220° |
| 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): 3.03e-14 ± 4.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.82
0.2-0.5 / 0.5-1.0 keV
HR2
0.81
± 0.17
0.5-1.0 / 1.0-2.0 keV
HR3
0.52
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.52
± 0.09
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: 2.07
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
- 956187
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 19.598 | 0.103 |
| UVM2 | 18.863 | 0.046 |
| UVW1 | 16.869 | 0.008 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.85e-14 (+3.7e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.83e+22 (+4.1e+22 / −1.6e+22) cm−2 |
| Photon index (Γ) | 2.27 (+2.78 / −1.50) |
| DoF | 82 |
| p-value | 0.47 |
| 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.