5XMM J174737.6-282229

5XMM-DR15 stacked source · SRCID 3003054010101211
Position: 17h47m37.64s -28d22m29.4s (266.90685°, -28.37484°)
EP flux
3.07e-15 ± 4.7e-16 erg cm-2 s-1
CLASSX
Star (0.995)
Detections
15

SRCID 3003054010101211
IAUNAME 5XMM J174737.6-282229
SC_RA 17h47m37.64s (266.90685°)
SC_DEC -28d22m29.4s (-28.37484°)
RADEC_ERR 0.47 arcsec
LII / BII 0.7084° / -0.0849°
N_CONTRIB 15 (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): 3.07e-15 ± 4.7e-16 erg cm-2 s-1

Hardness ratios
HR1
0.75 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.00 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.83 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.92 ± 0.46
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 2
Long-term lightcurve

Star

CLASSX outlier: 3.74

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
4882732
Match probability
0.938
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 21.824 0.126
B 19.657 0.067
V 18.201 0.038
Gaia DR3
Source ID
4057530680563226496
Match probability
0.992
Parallax
1.076 ± 0.164 mas
Proper motion
(-1.20, -9.04) mas/yr
Magnitudes
G=17.75, BP=18.79, RP=16.77
Distance
647 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 4.47e-15 (+5.8e-15 / −3.6e-15) erg cm−2 s−1
NH 1.81e+21 (+2.6e+21 / −7.1e+20) cm−2
Photon index (Γ) 2.54 (+2.87 / −1.98)
DoF 354
p-value 0.239
Inter-instrument norm. 1.05 (0.80–1.35)
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.