5XMM J170159.2-295024
5XMM-DR15 stacked source · SRCID 3000862070100028
Position:
17h01m59.21s -29d50m24.6s
(255.49670°, -29.84016°)
EP flux
1.08e-14
± 2.5e-15
erg cm-2 s-1
CLASSX
Star
(0.933)
Detections
6
| SRCID | 3000862070100028 |
|---|---|
| IAUNAME | 5XMM J170159.2-295024 |
| SC_RA | 17h01m59.21s (255.49670°) |
| SC_DEC | -29d50m24.6s (-29.84016°) |
| RADEC_ERR | 0.48 arcsec |
| LII / BII | 353.8957° / 7.3503° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 7 (observations covering the position) |
| MJD_FIRST | 51960.342 (2001-02-20 08:12:43.000 UTC) |
| MJD_LAST | 57987.250 (2017-08-22 06:00:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.08e-14 ± 2.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.93
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.11
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.63
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.24
± 0.25
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: 3.55
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 | 2.08e-14 (+2.5e-14 / −1.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.39e+21 (+3.1e+21 / −1.5e+21) cm−2 |
| Photon index (Γ) | 2.44 (+2.76 / −2.06) |
| DoF | 778 |
| p-value | 0.433 |
| Inter-instrument norm. | 1.73 (1.49–1.90) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 10.300 (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.