5XMM J144029.6-604619
5XMM-DR15 stacked source · SRCID 3004534040100020
Position:
14h40m29.67s -60d46m19.2s
(220.12363°, -60.77201°)
EP flux
6.16e-15
± 1.9e-15
erg cm-2 s-1
CLASSX
Star
(0.99)
Detections
22
| SRCID | 3004534040100020 |
|---|---|
| IAUNAME | 5XMM J144029.6-604619 |
| SC_RA | 14h40m29.67s (220.12363°) |
| SC_DEC | -60d46m19.2s (-60.77201°) |
| RADEC_ERR | 0.49 arcsec |
| LII / BII | 315.8581° / -0.6669° |
| N_CONTRIB | 22 (detections) |
| N_OBS | 22 (observations covering the position) |
| MJD_FIRST | 52702.577 (2003-03-04 13:50:36.000 UTC) |
| MJD_LAST | 59056.896 (2020-07-26 21:30:44.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.16e-15 ± 1.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.79
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.16
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.70
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.12
± 0.56
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.82
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 | 6.55e-14 (+7.4e-14 / −5.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.88e+21 (+3.4e+21 / −2.4e+21) cm−2 |
| Photon index (Γ) | 2.85 (+2.96 / −2.66) |
| DoF | 241 |
| p-value | 0.816 |
| Inter-instrument norm. | 0.88 (0.73–1.05) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.100 (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.