5XMM J064124.5+093735
5XMM-DR15 stacked source · SRCID 3001142020100356
Position:
06h41m24.58s +09d37m35.8s
(100.35241°, 9.62660°)
EP flux
1.57e-14
± 3.6e-15
erg cm-2 s-1
CLASSX
Star
(0.921)
Detections
1
| SRCID | 3001142020100356 |
|---|---|
| IAUNAME | 5XMM J064124.5+093735 |
| SC_RA | 06h41m24.58s (100.35241°) |
| SC_DEC | +09d37m35.8s (9.62660°) |
| RADEC_ERR | 0.71 arcsec |
| LII / BII | 203.2246° / 2.1703° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 52350.758 (2002-03-17 18:12:08.000 UTC) |
| MJD_LAST | 52351.235 (2002-03-18 05:38:16.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.57e-14 ± 3.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.08
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.88
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
0.38
± 0.47
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.47
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 | 1.59e-14 (+1.8e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.96e+21 (+2.5e+21 / −1.4e+21) cm−2 |
| Photon index (Γ) | 2.89 (+2.97 / −2.70) |
| DoF | 153 |
| p-value | 0.155 |
| Inter-instrument norm. | 1.17 (0.92–1.41) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 23.300 (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.