5XMM J174811.5-283429
5XMM-DR15 stacked source · SRCID 3003054010101076
Position:
17h48m11.50s -28d34m29.8s
(267.04793°, -28.57495°)
EP flux
1.81e-13
± 1.3e-14
erg cm-2 s-1
CLASSX
Star
(0.518)
Detections
8
| SRCID | 3003054010101076 |
|---|---|
| IAUNAME | 5XMM J174811.5-283429 |
| SC_RA | 17h48m11.50s (267.04793°) |
| SC_DEC | -28d34m29.8s (-28.57495°) |
| RADEC_ERR | 0.32 arcsec |
| LII / BII | 0.6012° / -0.2945° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 308 (observations covering the position) |
| MJD_FIRST | 51802.795 (2000-09-15 19:04:46.000 UTC) |
| MJD_LAST | 59120.587 (2020-09-28 14:05:30.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.81e-13 ± 1.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.17
± 1.86
0.2-0.5 / 0.5-1.0 keV
HR2
0.87
± 0.32
0.5-1.0 / 1.0-2.0 keV
HR3
0.89
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
0.45
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 4.6)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 5.45
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.
Optical Monitor (OM)
- OM Source ID
- 4895691
- Match probability
- 0.849
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 18.554 | 0.046 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 9.44e-14 (+1.1e-13 / −7.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.18e+23 (+3.2e+23 / −1.6e+23) cm−2 |
| Photon index (Γ) | 1.27 (+1.69 / −1.07) |
| DoF | 311 |
| p-value | 0.108 |
| Inter-instrument norm. | 1.37 (1.08–1.72) |
| Quality flag | 0 |
No variability data available for this source.
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.