5XMM J170219.2-294856
5XMM-DR15 stacked source · SRCID 3000862070100031
Position:
17h02m19.29s -29d48m56.1s
(255.58036°, -29.81558°)
EP flux
1.14e-14
± 2.7e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.626)
Detections
6
| SRCID | 3000862070100031 |
|---|---|
| IAUNAME | 5XMM J170219.2-294856 |
| SC_RA | 17h02m19.29s (255.58036°) |
| SC_DEC | -29d48m56.1s (-29.81558°) |
| RADEC_ERR | 0.50 arcsec |
| LII / BII | 353.9596° / 7.3073° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 7 (observations covering the position) |
| MJD_FIRST | 51960.342 (2001-02-20 08:12:43.000 UTC) |
| MJD_LAST | 57987.250 (2017-08-22 06:00:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.14e-14 ± 2.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.73
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.46
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.82
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.31
± 0.33
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 1.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.72
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 | 1.92e-14 (+2.3e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.73e+21 (+4.8e+21 / −2.7e+21) cm−2 |
| Photon index (Γ) | 2.57 (+2.87 / −2.22) |
| DoF | 296 |
| p-value | 0.846 |
| Inter-instrument norm. | 1.17 (0.95–1.45) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 40.500 (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.