5XMM J033917.6-352529
5XMM-DR15 stacked source · SRCID 3001283010100158
Position:
03h39m17.65s -35d25m29.9s
(54.82352°, -35.42496°)
EP flux
1.10e-14
± 1.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.816)
Detections
5
| SRCID | 3001283010100158 |
|---|---|
| IAUNAME | 5XMM J033917.6-352529 |
| SC_RA | 03h39m17.65s (54.82352°) |
| SC_DEC | -35d25m29.9s (-35.42496°) |
| RADEC_ERR | 0.47 arcsec |
| LII / BII | 236.6670° / -53.4714° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51916.608 (2001-01-07 14:34:55.000 UTC) |
| MJD_LAST | 57752.928 (2016-12-30 22:15:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.10e-14 ± 1.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.33
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.00
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.27
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.81
± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.797
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
- 993158
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 20.221 | 0.100 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.30e-14 (+2.7e-14 / −2.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.27e+19 (+3.1e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 1.69 (+1.85 / −1.56) |
| DoF | 537 |
| p-value | 0.649 |
| Inter-instrument norm. | 0.82 (0.68–0.96) |
| 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.