5XMM J062536.2-535107
5XMM-DR15 stacked source · SRCID 3030021100100042
Position:
06h25m36.27s -53d51m07.3s
(96.40114°, -53.85203°)
EP flux
5.98e-14
± 1.2e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.744)
Detections
3
| SRCID | 3030021100100042 |
|---|---|
| IAUNAME | 5XMM J062536.2-535107 |
| SC_RA | 06h25m36.27s (96.40114°) |
| SC_DEC | -53d51m07.3s (-53.85203°) |
| RADEC_ERR | 0.61 arcsec |
| LII / BII | 262.5199° / -25.2935° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 53662.417 (2005-10-19 10:00:46.000 UTC) |
| MJD_LAST | 56457.831 (2013-06-14 19:56:28.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.98e-14 ± 1.2e-14 erg cm-2 s-1
Hardness ratios
HR1
0.42
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.01
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
0.08
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 4.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.02
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 | 3.70e-14 (+4.5e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.65e+20 (+6.8e+20 / −2.8e+19) cm−2 |
| Photon index (Γ) | 1.95 (+2.19 / −1.76) |
| DoF | 212 |
| p-value | 0.929 |
| Inter-instrument norm. | 1.19 (0.95–1.45) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.600 (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.