5XMM J064050.7+095553
5XMM-DR15 stacked source · SRCID 3001142010100221
Position:
06h40m50.76s +09d55m53.3s
(100.21151°, 9.93147°)
EP flux
3.03e-14
± 4.5e-15
erg cm-2 s-1
CLASSX
Star
(0.873)
Detections
1
| SRCID | 3001142010100221 |
|---|---|
| IAUNAME | 5XMM J064050.7+095553 |
| SC_RA | 06h40m50.76s (100.21151°) |
| SC_DEC | +09d55m53.3s (9.93147°) |
| RADEC_ERR | 0.49 arcsec |
| LII / BII | 202.8897° / 2.1860° |
| 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): 3.03e-14 ± 4.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.58
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.13
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.62
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.25
± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.57
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 | 2.28e-14 (+2.5e-14 / −2.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.77e+21 (+2.1e+21 / −1.4e+21) cm−2 |
| Photon index (Γ) | 2.89 (+2.97 / −2.73) |
| DoF | 239 |
| p-value | 0.319 |
| Inter-instrument norm. | 0.77 (0.64–0.93) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 8.700 (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.