5XMM J033919.9-351542
5XMM-DR15 stacked source · SRCID 3005514010100316
Position:
03h39m19.93s -35d15m42.4s
(54.83304°, -35.26178°)
EP flux
5.73e-14
± 1.1e-14
erg cm-2 s-1
CLASSX
AGN
(0.942)
Detections
2
| SRCID | 3005514010100316 |
|---|---|
| IAUNAME | 5XMM J033919.9-351542 |
| SC_RA | 03h39m19.93s (54.83304°) |
| SC_DEC | -35d15m42.4s (-35.26178°) |
| RADEC_ERR | 0.78 arcsec |
| LII / BII | 236.3927° / -53.4666° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51916.608 (2001-01-07 14:34:55.000 UTC) |
| MJD_LAST | 54645.253 (2008-06-28 06:03:36.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.73e-14 ± 1.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.57
± 0.32
0.2-0.5 / 0.5-1.0 keV
HR2
0.67
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.10
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.18
± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.1)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.269
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 | 4.48e-14 (+5.3e-14 / −3.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.89e+21 (+3.5e+21 / −6.3e+20) cm−2 |
| Photon index (Γ) | 1.34 (+1.68 / −1.11) |
| DoF | 229 |
| p-value | 0.952 |
| Inter-instrument norm. | 0.94 (0.73–1.18) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 42.300 (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.