5XMM J061529.8+710141
5XMM-DR15 stacked source · SRCID 3000922030100006
Position:
06h15m29.80s +71d01m41.0s
(93.87416°, 71.02806°)
EP flux
2.43e-14
± 2.8e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.593)
Detections
16
| SRCID | 3000922030100006 |
|---|---|
| IAUNAME | 5XMM J061529.8+710141 |
| SC_RA | 06h15m29.80s (93.87416°) |
| SC_DEC | +71d01m41.0s (71.02806°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 143.3029° / 22.7073° |
| N_CONTRIB | 16 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51836.038 (2000-10-19 00:54:32.000 UTC) |
| MJD_LAST | 57132.768 (2015-04-20 18:26:21.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.43e-14 ± 2.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.64
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.22
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.17
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 9.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.39
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 | 4.95e-14 (+5.4e-14 / −4.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.00e+20 (+3.5e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.28 (+1.37 / −1.19) |
| DoF | 635 |
| p-value | 0.187 |
| Inter-instrument norm. | 1.24 (1.11–1.37) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 44.400 (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.