5XMM J174817.0-281545
5XMM-DR15 stacked source · SRCID 3003054010100262
Position:
17h48m17.04s -28d15m45.3s
(267.07098°, -28.26259°)
EP flux
9.73e-14
± 6.2e-15
erg cm-2 s-1
CLASSX
Gal_XRB
(0.5)
Detections
13
| SRCID | 3003054010100262 |
|---|---|
| IAUNAME | 5XMM J174817.0-281545 |
| SC_RA | 17h48m17.04s (267.07098°) |
| SC_DEC | -28d15m45.3s (-28.26259°) |
| RADEC_ERR | 0.17 arcsec |
| LII / BII | 0.8792° / -0.1506° |
| N_CONTRIB | 13 (detections) |
| N_OBS | 308 (observations covering the position) |
| MJD_FIRST | 51810.719 (2000-09-23 17:14:57.000 UTC) |
| MJD_LAST | 59127.048 (2020-10-05 01:09:24.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.73e-14 ± 6.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.56
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.92
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
0.07
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 5.58
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 | 1.05e-13 (+1.1e-13 / −9.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.52e+22 (+1.7e+22 / −1.4e+22) cm−2 |
| Photon index (Γ) | 2.45 (+2.61 / −2.31) |
| DoF | 648 |
| p-value | 0.986 |
| Inter-instrument norm. | 1.01 (0.93–1.10) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 7.000 (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.