5XMM J032930.4+311903
5XMM-DR15 stacked source · SRCID 3006582010100042
Position:
03h29m30.45s +31d19m03.5s
(52.37689°, 31.31765°)
EP flux
1.26e-14
± 5.1e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3006582010100042 |
|---|---|
| IAUNAME | 5XMM J032930.4+311903 |
| SC_RA | 03h29m30.45s (52.37689°) |
| SC_DEC | +31d19m03.5s (31.31765°) |
| RADEC_ERR | 0.94 arcsec |
| LII / BII | 158.3961° / -20.4579° |
| 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): 1.26e-14 ± 5.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.90
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.20
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.83
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
0.61
± 0.19
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: 1.96
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
- 956736
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.379 | 0.092 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 9.81e-15 (+1.3e-14 / −7.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.10e+21 (+2.1e+21 / −2.4e+20) cm−2 |
| Photon index (Γ) | 2.37 (+2.80 / −1.83) |
| DoF | 160 |
| p-value | 0.393 |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.100 (approximate flux variability amplitude) |
|---|
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.