5XMM J032859.9+312151
5XMM-DR15 stacked source · SRCID 3006582010100067
Position:
03h28m59.99s +31d21m51.7s
(52.24994°, 31.36435°)
EP flux
2.60e-14
± 1.3e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
1
| SRCID | 3006582010100067 |
|---|---|
| IAUNAME | 5XMM J032859.9+312151 |
| SC_RA | 03h28m59.99s (52.24994°) |
| SC_DEC | +31d21m51.7s (31.36435°) |
| RADEC_ERR | 2.87 arcsec |
| LII / BII | 158.2738° / -20.4861° |
| 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): 2.60e-14 ± 1.3e-14 erg cm-2 s-1
Hardness ratios
HR1
1.00
± 0.18
0.2-0.5 / 0.5-1.0 keV
HR2
0.38
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.30
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50
± 0.39
2.0-4.5 / 4.5-12.0 keV
Extent:
8.06
± 1.80
arcsec
(ML 6.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 4.43
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
- 954870
- Match probability
- 0.738
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.175 | 0.178 |
| UVW1 | 18.902 | 0.029 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.67e-14 (+2.4e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.19e+21 (+5.3e+21 / −2.2e+20) cm−2 |
| Photon index (Γ) | 1.60 (+2.24 / −1.15) |
| DoF | 62 |
| p-value | 0.417 |
| 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.