5XMM J064106.6+094727
5XMM-DR15 stacked source · SRCID 3001142010100138
Position:
06h41m06.67s +09d47m27.5s
(100.27780°, 9.79096°)
EP flux
4.70e-14
± 3.8e-15
erg cm-2 s-1
CLASSX
CV
(0.499)
Detections
1
| SRCID | 3001142010100138 |
|---|---|
| IAUNAME | 5XMM J064106.6+094727 |
| SC_RA | 06h41m06.67s (100.27780°) |
| SC_DEC | +09d47m27.5s (9.79096°) |
| RADEC_ERR | 0.35 arcsec |
| LII / BII | 203.0446° / 2.1799° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 51988.103 (2001-03-20 02:28:07.000 UTC) |
| MJD_LAST | 51988.575 (2001-03-20 13:48:05.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.70e-14 ± 3.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.78
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.04
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.77
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.66
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
CV
CLASSX outlier: 4.86
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 | 4.87e-14 (+5.2e-14 / −4.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.18e+21 (+2.4e+21 / −2.0e+21) cm−2 |
| Photon index (Γ) | 2.97 (+2.99 / −2.91) |
| DoF | 400 |
| p-value | 0.011 |
| Inter-instrument norm. | 0.99 (0.89–1.11) |
| Quality flag | 6 |
| APPROX_SOURCE_VAR | 11.500 (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.