5XMM J174744.3-282304

5XMM-DR15 stacked source · SRCID 3003054010102353
Position: 17h47m44.31s -28d23m04.9s (266.93464°, -28.38468°)
EP flux
3.52e-15 ± 7.9e-16 erg cm-2 s-1
CLASSX
Star (0.999)
Detections
13

SRCID 3003054010102353
IAUNAME 5XMM J174744.3-282304
SC_RA 17h47m44.31s (266.93464°)
SC_DEC -28d23m04.9s (-28.38468°)
RADEC_ERR 0.73 arcsec
LII / BII 0.7126° / -0.1109°
N_CONTRIB 13 (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): 3.52e-15 ± 7.9e-16 erg cm-2 s-1

Hardness ratios
HR1
0.75 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.35 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.62 ± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 2
Long-term lightcurve

Star

CLASSX outlier: 3.69

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
4885669
Match probability
0.993
FilterMag (AB)Err
UVW2
UVM2 22.260 0.318
UVW1 19.694 0.024
U 18.337 0.012
B 16.383 0.006
V 15.192 0.003
Gaia DR3
Source ID
4057621562067911552
Match probability
0.964
Parallax
0.620 ± 0.039 mas
Proper motion
(0.02, -2.14) mas/yr
Magnitudes
G=15.27, BP=16.04, RP=14.38
Distance
2738 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 3.65e-15 (+5.7e-15 / −2.6e-15) erg cm−2 s−1
NH 3.34e+21 (+4.9e+21 / −1.6e+21) cm−2
Photon index (Γ) 2.30 (+2.80 / −1.45)
DoF 254
p-value 0.003
Quality flag 5

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.