5XMM J032902.8+311602
5XMM-DR15 stacked source · SRCID 3006582010100018
Position:
03h29m02.86s +31d16m02.7s
(52.26190°, 31.26741°)
EP flux
3.60e-14
± 3.1e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.502)
Detections
1
| SRCID | 3006582010100018 |
|---|---|
| IAUNAME | 5XMM J032902.8+311602 |
| SC_RA | 03h29m02.86s (52.26190°) |
| SC_DEC | +31d16m02.7s (31.26741°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 158.3449° / -20.5573° |
| 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): 3.60e-14 ± 3.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.32
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.69
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.89
± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 5.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 4.81
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
- 955059
- Match probability
- 0.904
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.867 | 0.065 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.82e-14 (+3.0e-14 / −2.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.25e+21 (+1.5e+21 / −9.8e+20) cm−2 |
| Photon index (Γ) | 2.90 (+2.97 / −2.77) |
| DoF | 273 |
| p-value | 0.015 |
| 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.