5XMM J032934.3+311744
5XMM-DR15 stacked source · SRCID 3006582010100021
Position:
03h29m34.34s +31d17m44.1s
(52.39307°, 31.29558°)
EP flux
5.09e-14
± 6.6e-15
erg cm-2 s-1
CLASSX
Star
(0.929)
Detections
1
| SRCID | 3006582010100021 |
|---|---|
| IAUNAME | 5XMM J032934.3+311744 |
| SC_RA | 03h29m34.34s (52.39307°) |
| SC_DEC | +31d17m44.1s (31.29558°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 158.4221° / -20.4671° |
| 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): 5.09e-14 ± 6.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.68
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.12
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.73
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.71
± 0.31
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.28
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
- 956964
- Match probability
- 0.994
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.550 | 0.243 |
| UVW1 | 21.531 | 0.146 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.03e-14 (+5.3e-14 / −4.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.25e+21 (+2.5e+21 / −2.0e+21) cm−2 |
| Photon index (Γ) | 2.96 (+2.99 / −2.90) |
| DoF | 547 |
| p-value | 0.06 |
| Inter-instrument norm. | 0.99 (0.90–1.11) |
| Quality flag | 6 |
| APPROX_SOURCE_VAR | 7.700 (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.