5XMM J033908.3-353120
5XMM-DR15 stacked source · SRCID 3001283010100062
Position:
03h39m08.30s -35d31m20.9s
(54.78458°, -35.52248°)
EP flux
1.95e-14
± 1.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.912)
Detections
5
| SRCID | 3001283010100062 |
|---|---|
| IAUNAME | 5XMM J033908.3-353120 |
| SC_RA | 03h39m08.30s (54.78458°) |
| SC_DEC | -35d31m20.9s (-35.52248°) |
| RADEC_ERR | 0.29 arcsec |
| LII / BII | 236.8320° / -53.5010° |
| 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): 1.95e-14 ± 1.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.16
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.08
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.47
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.1)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.251
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 | 2.76e-14 (+3.1e-14 / −2.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.54e+20 (+1.0e+21 / −6.4e+19) cm−2 |
| Photon index (Γ) | 2.04 (+2.31 / −1.85) |
| DoF | 427 |
| p-value | 0.251 |
| Inter-instrument norm. | 0.72 (0.62–0.83) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.900 (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.