5XMM J175756.9-335409
5XMM-DR15 stacked source · SRCID 3003294010100078
Position:
17h57m56.91s -33d54m09.6s
(269.48714°, -33.90268°)
EP flux
1.72e-14
± 5.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.732)
Detections
3
| SRCID | 3003294010100078 |
|---|---|
| IAUNAME | 5XMM J175756.9-335409 |
| SC_RA | 17h57m56.91s (269.48714°) |
| SC_DEC | -33d54m09.6s (-33.90268°) |
| RADEC_ERR | 0.99 arcsec |
| LII / BII | 357.0585° / -4.7898° |
| 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): 1.72e-14 ± 5.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 1.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.71
± 0.42
0.5-1.0 / 1.0-2.0 keV
HR3
0.44
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
0.23
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.6)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.27
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 | 2.25e-14 (+3.1e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.03e+21 (+1.9e+22 / −2.8e+21) cm−2 |
| Photon index (Γ) | 1.55 (+2.22 / −1.15) |
| DoF | 166 |
| p-value | 0.955 |
| Inter-instrument norm. | 1.56 (1.14–1.86) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.800 (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.