5XMM J174737.8-283041

5XMM-DR15 stacked source · SRCID 3003054010105142
Position: 17h47m37.80s -28d30m41.1s (266.90752°, -28.51142°)
EP flux
3.09e-15 ± 2.3e-15 erg cm-2 s-1
CLASSX
Extended (1)
Detections
17

SRCID 3003054010105142
IAUNAME 5XMM J174737.8-283041
SC_RA 17h47m37.80s (266.90752°)
SC_DEC -28d30m41.1s (-28.51142°)
RADEC_ERR 2.74 arcsec
LII / BII 0.5918° / -0.1561°
N_CONTRIB 17 (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): 3.09e-15 ± 2.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.65 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.14 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.83 ± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
-0.91 ± 3.44
2.0-4.5 / 4.5-12.0 keV
Extent: 10.54 ± 1.56 arcsec (ML 10.8) SUM_FLAG: 2
Long-term lightcurve

Extended

CLASSX outlier: 5.37

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
4882633
Match probability
0.538
FilterMag (AB)Err
UVW2 20.548 0.215
UVM2
UVW1
U
B
V
Gaia DR3
Source ID
4057525840140231040
Match probability
0.991
Parallax
2.644 ± 0.026 mas
Proper motion
(1.56, 5.38) mas/yr
Magnitudes
G=14.14, BP=14.70, RP=13.42
Distance
352 pc
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

No redshift estimate available for this source.

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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.