5XMM J175824.0-335257
5XMM-DR15 stacked source · SRCID 3003294010100023
Position:
17h58m24.09s -33d52m57.9s
(269.60039°, -33.88276°)
EP flux
1.57e-14
± 2.3e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.443)
Detections
3
| SRCID | 3003294010100023 |
|---|---|
| IAUNAME | 5XMM J175824.0-335257 |
| SC_RA | 17h58m24.09s (269.60039°) |
| SC_DEC | -33d52m57.9s (-33.88276°) |
| RADEC_ERR | 0.42 arcsec |
| LII / BII | 357.1225° / -4.8616° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 51976.222 (2001-03-08 05:19:45.000 UTC) |
| MJD_LAST | 54541.581 (2008-03-16 13:55:58.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.57e-14 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.88
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
0.66
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.18
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.6)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.17
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 | 3.08e-14 (+3.5e-14 / −2.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.39e+21 (+5.7e+21 / −3.2e+21) cm−2 |
| Photon index (Γ) | 1.82 (+2.06 / −1.58) |
| DoF | 582 |
| p-value | 0.926 |
| Inter-instrument norm. | 1.09 (0.92–1.30) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 7.800 (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.