5XMM J173409.6-322945
5XMM-DR15 stacked source · SRCID 3000173020100596
Position:
17h34m09.68s -32d29m45.2s
(263.54032°, -32.49588°)
EP flux
1.06e-14
± 5.6e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.509)
Detections
4
| SRCID | 3000173020100596 |
|---|---|
| IAUNAME | 5XMM J173409.6-322945 |
| SC_RA | 17h34m09.68s (263.54032°) |
| SC_DEC | -32d29m45.2s (-32.49588°) |
| RADEC_ERR | 0.59 arcsec |
| LII / BII | 355.6762° / 0.1927° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 180 (observations covering the position) |
| MJD_FIRST | 51977.535 (2001-03-09 12:50:44.000 UTC) |
| MJD_LAST | 60398.199 (2024-03-29 04:46:13.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.06e-14 ± 5.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.79
± 0.61
0.2-0.5 / 0.5-1.0 keV
HR2
0.52
± 0.28
0.5-1.0 / 1.0-2.0 keV
HR3
-0.63
± 0.23
1.0-2.0 / 2.0-4.5 keV
HR4
0.39
± 0.38
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.
Bkg_AGN
CLASSX outlier: 4.95
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-13 (+1.8e-13 / −1.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.12e+21 (+5.3e+21 / −3.0e+21) cm−2 |
| Photon index (Γ) | 1.66 (+1.93 / −1.44) |
| DoF | 471 |
| p-value | 0.908 |
| Inter-instrument norm. | 1.16 (1.02–1.35) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 18.300 (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.