5XMM J121855.8+472025

5XMM-DR15 stacked source · SRCID 3005914010100026
Position: 12h18m55.82s +47d20m25.7s (184.73259°, 47.34047°)
EP flux
1.31e-14 ± 1.6e-15 erg cm-2 s-1
CLASSX
Extragal_XRB (0.683)
Detections
6

SRCID 3005914010100026
IAUNAME 5XMM J121855.8+472025
SC_RA 12h18m55.82s (184.73259°)
SC_DEC +47d20m25.7s (47.34047°)
RADEC_ERR 0.33 arcsec
LII / BII 138.2974° / 68.8062°
N_CONTRIB 6 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 51886.934 (2000-12-08 22:25:31.000 UTC)
MJD_LAST 54057.366 (2006-11-18 08:47:36.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.31e-14 ± 1.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.54 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.01 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.51 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.9) SUM_FLAG: 0
Long-term lightcurve

Extragal_XRB

CLASSX outlier: 2.48

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
3191445
Match probability
0.996
FilterMag (AB)Err
UVW2 17.687 0.036
UVM2 — —
UVW1 — —
U — —
B 16.471 0.013
V — —
Gaia DR3
Source ID
1545203755632934784
Match probability
0.988
Magnitudes
G=21.68
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.00
Galaxy
1.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 8.72e-14 (+9.9e-14 / −7.8e-14) erg cm−2 s−1
NH 2.55e+21 (+3.2e+21 / −1.9e+21) cm−2
Photon index (Γ) 2.18 (+2.40 / −1.94)
DoF 598
p-value 0.929
Inter-instrument norm. 0.87 (0.75–1.05)
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.