5XMM J033926.1-352918
5XMM-DR15 stacked source · SRCID 3001283010100658
Position:
03h39m26.18s -35d29m18.7s
(54.85906°, -35.48854°)
EP flux
1.80e-14
± 5.4e-15
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
5
| SRCID | 3001283010100658 |
|---|---|
| IAUNAME | 5XMM J033926.1-352918 |
| SC_RA | 03h39m26.18s (54.85906°) |
| SC_DEC | -35d29m18.7s (-35.48854°) |
| RADEC_ERR | 5.22 arcsec |
| LII / BII | 236.7728° / -53.4411° |
| 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): 1.80e-14 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.89
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.17
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.95
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.57
± 0.87
2.0-4.5 / 4.5-12.0 keV
Extent:
31.52
± 2.38
arcsec
(ML 48.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 1.98
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
- 993512
- Match probability
- 0.79
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 20.750 | 0.150 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.26e-15 (+5.6e-15 / −1.8e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.87e+20 (+2.2e+21 / −2.7e+19) cm−2 |
| Photon index (Γ) | 1.77 (+2.45 / −1.35) |
| DoF | 306 |
| p-value | 0.462 |
| 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.