5XMM J064100.5+094503
5XMM-DR15 stacked source · SRCID 3001142010100144
Position:
06h41m00.50s +09d45m03.9s
(100.25207°, 9.75108°)
EP flux
3.82e-14
± 5.5e-15
erg cm-2 s-1
CLASSX
Star
(0.84)
Detections
2
| SRCID | 3001142010100144 |
|---|---|
| IAUNAME | 5XMM J064100.5+094503 |
| SC_RA | 06h41m00.50s (100.25207°) |
| SC_DEC | +09d45m03.9s (9.75108°) |
| RADEC_ERR | 0.36 arcsec |
| LII / BII | 203.0686° / 2.1391° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 51988.103 (2001-03-20 02:28:07.000 UTC) |
| MJD_LAST | 52351.235 (2002-03-18 05:38:16.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.82e-14 ± 5.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.63
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.27
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.50
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.46
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.65
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 | 6.22e-14 (+6.7e-14 / −5.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.36e+21 (+2.6e+21 / −2.1e+21) cm−2 |
| Photon index (Γ) | 2.90 (+2.97 / −2.77) |
| DoF | 379 |
| p-value | 0.006 |
| Inter-instrument norm. | 0.53 (0.51–0.57) |
| Quality flag | 5 |
| APPROX_SOURCE_VAR | 10.900 (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.