5XMM J175752.8-334704
5XMM-DR15 stacked source · SRCID 3003294010100039
Position:
17h57m52.80s -33d47m04.3s
(269.47000°, -33.78452°)
EP flux
2.08e-14
± 4.5e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.641)
Detections
3
| SRCID | 3003294010100039 |
|---|---|
| IAUNAME | 5XMM J175752.8-334704 |
| SC_RA | 17h57m52.80s (269.47000°) |
| SC_DEC | -33d47m04.3s (-33.78452°) |
| RADEC_ERR | 0.65 arcsec |
| LII / BII | 357.1544° / -4.7189° |
| 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): 2.08e-14 ± 4.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.45
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.21
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26
± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.5
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 | 2.95e-14 (+4.0e-14 / −2.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.28e+21 (+4.1e+21 / −7.3e+19) cm−2 |
| Photon index (Γ) | 1.49 (+2.13 / −1.19) |
| DoF | 144 |
| p-value | 0.961 |
| Inter-instrument norm. | 1.11 (0.85–1.53) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 6.500 (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.