5XMM J143856.6-604054
5XMM-DR15 stacked source · SRCID 3004534040100011
Position:
14h38m56.61s -60d40m54.6s
(219.73588°, -60.68183°)
EP flux
2.74e-14
± 3.5e-15
erg cm-2 s-1
CLASSX
Star
(0.999)
Detections
22
| SRCID | 3004534040100011 |
|---|---|
| IAUNAME | 5XMM J143856.6-604054 |
| SC_RA | 14h38m56.61s (219.73588°) |
| SC_DEC | -60d40m54.6s (-60.68183°) |
| RADEC_ERR | 0.28 arcsec |
| LII / BII | 315.7213° / -0.5077° |
| 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): 2.74e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.92
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.20
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.82
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.17
± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.18
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 | 7.13e-14 (+8.0e-14 / −6.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.40e+21 (+4.9e+21 / −3.9e+21) cm−2 |
| Photon index (Γ) | 2.88 (+2.97 / −2.71) |
| DoF | 230 |
| p-value | 0.744 |
| Inter-instrument norm. | 1.09 (0.93–1.31) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 8.300 (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.