5XMM J143944.2-605540
5XMM-DR15 stacked source · SRCID 3004534110100008
Position:
14h39m44.28s -60d55m40.5s
(219.93451°, -60.92792°)
EP flux
4.20e-14
± 3.5e-15
erg cm-2 s-1
CLASSX
Star
(0.975)
Detections
16
| SRCID | 3004534110100008 |
|---|---|
| IAUNAME | 5XMM J143944.2-605540 |
| SC_RA | 14h39m44.28s (219.93451°) |
| SC_DEC | -60d55m40.5s (-60.92792°) |
| RADEC_ERR | 0.23 arcsec |
| LII / BII | 315.7106° / -0.7719° |
| N_CONTRIB | 16 (detections) |
| N_OBS | 22 (observations covering the position) |
| MJD_FIRST | 53033.595 (2004-01-29 14:16:27.000 UTC) |
| MJD_LAST | 59056.896 (2020-07-26 21:30:44.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.20e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.92
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.62
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.23
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.48
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.89
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 | 1.13e-13 (+1.3e-13 / −1.0e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.33e+21 (+5.6e+21 / −3.3e+21) cm−2 |
| Photon index (Γ) | 1.84 (+2.07 / −1.61) |
| DoF | 232 |
| p-value | 0.942 |
| Inter-instrument norm. | 0.68 (0.58–0.78) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.500 (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.