5XMM J033840.8-353305
5XMM-DR15 stacked source · SRCID 3001283010100138
Position:
03h38m40.80s -35d33m05.4s
(54.66998°, -35.55151°)
EP flux
1.31e-14
± 1.6e-15
erg cm-2 s-1
CLASSX
AGN
(0.949)
Detections
5
| SRCID | 3001283010100138 |
|---|---|
| IAUNAME | 5XMM J033840.8-353305 |
| SC_RA | 03h38m40.80s (54.66998°) |
| SC_DEC | -35d33m05.4s (-35.55151°) |
| RADEC_ERR | 0.43 arcsec |
| LII / BII | 236.8846° / -53.5935° |
| 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): 1.31e-14 ± 1.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.30
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.35
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.24
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.237
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.62e-14 (+1.9e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.65e+20 (+1.6e+21 / −1.7e+20) cm−2 |
| Photon index (Γ) | 1.63 (+1.85 / −1.42) |
| DoF | 644 |
| p-value | 1 |
| Inter-instrument norm. | 1.08 (0.93–1.25) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 10.300 (approximate flux variability amplitude) |
|---|
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.