5XMM J171648.4-624924
5XMM-DR15 stacked source · SRCID 3005977010100002
Position:
17h16m48.44s -62d49m24.1s
(259.20183°, -62.82335°)
EP flux
5.51e-15
± 1.5e-15
erg cm-2 s-1
CLASSX
Star
(0.61)
Detections
1
| SRCID | 3005977010100002 |
|---|---|
| IAUNAME | 5XMM J171648.4-624924 |
| SC_RA | 17h16m48.44s (259.20183°) |
| SC_DEC | -62d49m24.1s (-62.82335°) |
| RADEC_ERR | 0.87 arcsec |
| LII / BII | 328.4773° / -14.0360° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 51970.154 (2001-03-02 03:42:27.000 UTC) |
| MJD_LAST | 51970.689 (2001-03-02 16:31:49.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.51e-15 ± 1.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.31
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.17
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.63
± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.1
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 | 9.54e-15 (+1.1e-14 / −8.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 3.46e+21 (+4.4e+21 / −2.6e+21) cm−2 |
| Photon index (Γ) | 2.62 (+2.87 / −2.32) |
| DoF | 582 |
| p-value | 0 |
| Inter-instrument norm. | 1.95 (1.88–1.99) |
| Quality flag | 5 |
| APPROX_SOURCE_VAR | 34.700 (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.