5XMM J172805.7-142108

5XMM-DR15 stacked source · SRCID 3004116010100045
Position: 17h28m05.70s -14d21m08.9s (262.02376°, -14.35247°)
EP flux
4.94e-14 ± 2.0e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.507)
Detections
13

SRCID 3004116010100045
IAUNAME 5XMM J172805.7-142108
SC_RA 17h28m05.70s (262.02376°)
SC_DEC -14d21m08.9s (-14.35247°)
RADEC_ERR 0.46 arcsec
LII / BII 10.2863° / 11.1657°
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): 4.94e-14 ± 2.0e-15 erg cm-2 s-1

Hardness ratios
HR1
0.16 ± 0.52
0.2-0.5 / 0.5-1.0 keV
HR2
0.76 ± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
0.69 ± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
0.38 ± 0.03
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 48.5) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.08

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
4667129
Match probability
0.509
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.523 0.212
B 19.106 0.061
V 17.845 0.052
Gaia DR3
Source ID
4137499879240706176
Match probability
0.993
Parallax
0.149 ± 0.124 mas
Proper motion
(-1.62, -4.94) mas/yr
Magnitudes
G=17.64, BP=18.46, RP=16.72
Distance
1201 pc
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 4.63e-14 (+5.7e-14 / −3.7e-14) erg cm−2 s−1
NH 1.07e+23 (+1.7e+23 / −6.4e+22) cm−2
Photon index (Γ) 1.65 (+2.36 / −1.19)
DoF 170
p-value 0.072
Quality flag 0

APPROX_SOURCE_VAR 7.300 (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

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