5XMM J174747.9-281607
5XMM-DR15 stacked source · SRCID 3003054010102544
Position:
17h47m47.96s -28d16m07.4s
(266.94981°, -28.26872°)
EP flux
3.34e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
Gal_XRB
(0.748)
Detections
15
| SRCID | 3003054010102544 |
|---|---|
| IAUNAME | 5XMM J174747.9-281607 |
| SC_RA | 17h47m47.96s (266.94981°) |
| SC_DEC | -28d16m07.4s (-28.26872°) |
| RADEC_ERR | 0.59 arcsec |
| LII / BII | 0.8188° / -0.0624° |
| N_CONTRIB | 15 (detections) |
| N_OBS | 308 (observations covering the position) |
| MJD_FIRST | 51802.795 (2000-09-15 19:04:46.000 UTC) |
| MJD_LAST | 59127.048 (2020-10-05 01:09:24.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.34e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.07
± 3.93
0.2-0.5 / 0.5-1.0 keV
HR2
0.73
± 1.19
0.5-1.0 / 1.0-2.0 keV
HR3
0.95
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
0.51
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.1)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 4.25
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 | 3.29e-14 (+3.9e-14 / −2.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.27e+23 (+1.9e+23 / −8.8e+22) cm−2 |
| Photon index (Γ) | 1.34 (+1.85 / −1.08) |
| DoF | 334 |
| p-value | 0.85 |
| Inter-instrument norm. | 1.27 (0.97–1.57) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 11.600 (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.