5XMM J172802.3-141917

5XMM-DR15 stacked source · SRCID 3004116010100063
Position: 17h28m02.34s -14d19m17.7s (262.00976°, -14.32158°)
EP flux
2.97e-15 ± 4.0e-16 erg cm-2 s-1
CLASSX
Star (0.998)
Detections
13

SRCID 3004116010100063
IAUNAME 5XMM J172802.3-141917
SC_RA 17h28m02.34s (262.00976°)
SC_DEC -14d19m17.7s (-14.32158°)
RADEC_ERR 0.42 arcsec
LII / BII 10.3056° / 11.1936°
N_CONTRIB 13 (detections)
N_OBS 13 (observations covering the position)
MJD_FIRST 51966.410 (2001-02-26 09:50:20.000 UTC)
MJD_LAST 58751.667 (2019-09-25 16:00:27.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.97e-15 ± 4.0e-16 erg cm-2 s-1

Hardness ratios
HR1
0.93 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.79 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.75 ± 0.35
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.6) SUM_FLAG: 0
Long-term lightcurve

Star

CLASSX outlier: 2.33

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
4666464
Match probability
0.994
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 18.752 0.006
U 17.506 0.003
B 16.005 0.002
V 15.024 0.002
Gaia DR3
Source ID
4137500536388486400
Match probability
0.989
Parallax
0.388 ± 0.028 mas
Proper motion
(-7.37, -1.11) mas/yr
Magnitudes
G=14.72, BP=15.36, RP=13.94
Distance
1602 pc
AllWISE
Name
J172802.35-141917.3
Match probability
0.995
BandMagErr
W1 12.142 0.033
W2 12.170 0.033
W3 12.258 0.526
W4 8.512 —
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.08e-14 (+1.4e-14 / −7.7e-15) erg cm−2 s−1
NH 1.27e+21 (+2.8e+21 / −1.6e+20) cm−2
Photon index (Γ) 1.71 (+2.37 / −1.33)
DoF 306
p-value 0.923
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

The per-observation light curve is shown in the X-ray properties section above.