5XMM J033839.1-351933
5XMM-DR15 stacked source · SRCID 3001283010100451
Position:
03h38m39.11s -35d19m33.6s
(54.66298°, -35.32600°)
EP flux
2.46e-14
± 1.3e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
4
| SRCID | 3001283010100451 |
|---|---|
| IAUNAME | 5XMM J033839.1-351933 |
| SC_RA | 03h38m39.11s (54.66298°) |
| SC_DEC | -35d19m33.6s (-35.32600°) |
| RADEC_ERR | 9.41 arcsec |
| LII / BII | 236.5049° / -53.6042° |
| N_CONTRIB | 4 (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): 2.46e-14 ± 1.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.78
± 0.21
0.2-0.5 / 0.5-1.0 keV
HR2
-0.10
± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.74
± 0.22
1.0-2.0 / 2.0-4.5 keV
HR4
0.66
± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent:
18.43
± 3.19
arcsec
(ML 7.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.42
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
- 990395
- Match probability
- 0.573
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.958 | 0.224 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.41e-15 (+8.8e-15 / −4.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.26e+20 (+1.3e+21 / −2.8e+19) cm−2 |
| Photon index (Γ) | 1.79 (+2.26 / −1.44) |
| DoF | 429 |
| p-value | 0.744 |
| 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.