5XMM J174743.9-282046

5XMM-DR15 stacked source · SRCID 3003054010102089
Position: 17h47m43.90s -28d20m46.5s (266.93293°, -28.34626°)
EP flux
9.09e-15 ± 1.5e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.338)
Detections
16

SRCID 3003054010102089
IAUNAME 5XMM J174743.9-282046
SC_RA 17h47m43.90s (266.93293°)
SC_DEC -28d20m46.5s (-28.34626°)
RADEC_ERR 0.61 arcsec
LII / BII 0.7447° / -0.0898°
N_CONTRIB 16 (detections)
N_OBS 308 (observations covering the position)
MJD_FIRST 51802.795 (2000-09-15 19:04:46.000 UTC)
MJD_LAST 59127.048 (2020-10-05 01:09:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 9.09e-15 ± 1.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.80 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.57 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.14 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.33 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 2
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 5.46

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
4885507
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 22.736 0.267
B 20.639 0.104
V 19.365 0.050
Gaia DR3
Source ID
4057624620084729216
Match probability
0.989
Parallax
0.739 ± 0.239 mas
Proper motion
(-0.19, -1.88) mas/yr
Magnitudes
G=18.36, BP=19.46, RP=17.23
Distance
523 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 1.07e-14 (+1.3e-14 / −8.6e-15) erg cm−2 s−1
NH 6.21e+21 (+8.0e+21 / −4.6e+21) cm−2
Photon index (Γ) 2.21 (+2.64 / −1.86)
DoF 397
p-value 0.987
Inter-instrument norm. 0.97 (0.76–1.22)
Quality flag 0

APPROX_SOURCE_VAR 14.500 (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.