5XMM J184505.2-030105

5XMM-DR15 stacked source · SRCID 3004654020100135
Position: 18h45m05.23s -03d01m05.5s (281.27179°, -3.01819°)
EP flux
7.98e-15 ± 1.9e-15 erg cm-2 s-1
CLASSX
Gal_XRB (0.427)
Detections
3

SRCID 3004654020100135
IAUNAME 5XMM J184505.2-030105
SC_RA 18h45m05.23s (281.27179°)
SC_DEC -03d01m05.5s (-3.01819°)
RADEC_ERR 0.64 arcsec
LII / BII 29.5221° / 0.0353°
N_CONTRIB 3 (detections)
N_OBS 11 (observations covering the position)
MJD_FIRST 52717.705 (2003-03-19 16:55:35.000 UTC)
MJD_LAST 55302.956 (2010-04-16 22:56:45.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 7.98e-15 ± 1.9e-15 erg cm-2 s-1

Hardness ratios
HR1
0.38 ± 0.60
0.2-0.5 / 0.5-1.0 keV
HR2
0.92 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.11 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.81 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 1
Long-term lightcurve

Gal_XRB

CLASSX outlier: 5.49

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
5637327
Match probability
0.989
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.121 0.278
U 21.426 0.105
B 19.402 0.037
V 17.740 0.088
Gaia DR3
Source ID
4258610539591097088
Match probability
0.992
Parallax
0.911 ± 0.083 mas
Proper motion
(1.97, -1.25) mas/yr
Magnitudes
G=17.04, BP=18.10, RP=15.98
Distance
627 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 1.50e-14 (+1.9e-14 / −1.1e-14) erg cm−2 s−1
NH 9.14e+21 (+1.3e+22 / −6.1e+21) cm−2
Photon index (Γ) 2.20 (+2.70 / −1.72)
DoF 258
p-value 0.961
Inter-instrument norm. 1.42 (1.10–1.73)
Quality flag 0

APPROX_SOURCE_VAR 13.200 (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.