5XMM J222732.5+610820

5XMM-DR15 stacked source · SRCID 3001266010100087
Position: 22h27m32.54s +61d08m20.6s (336.88560°, 61.13906°)
EP flux
4.30e-15 ± 3.8e-15 erg cm-2 s-1
CLASSX
Star (1)
Detections
4

SRCID 3001266010100087
IAUNAME 5XMM J222732.5+610820
SC_RA 22h27m32.54s (336.88560°)
SC_DEC +61d08m20.6s (61.13906°)
RADEC_ERR 1.88 arcsec
LII / BII 106.4378° / 2.9630°
N_CONTRIB 4 (detections)
N_OBS 4 (observations covering the position)
MJD_FIRST 52440.400 (2002-06-15 09:35:37.000 UTC)
MJD_LAST 58528.764 (2019-02-14 18:20:22.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.30e-15 ± 3.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.64 ± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
-0.23 ± 0.25
0.5-1.0 / 1.0-2.0 keV
HR3
-0.95 ± 0.42
1.0-2.0 / 2.0-4.5 keV
HR4
0.85 ± 1.06
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.0) SUM_FLAG: 2
Long-term lightcurve

Star

CLASSX outlier: 2.24

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
6466209
Match probability
0.967
FilterMag (AB)Err
UVW2
UVM2
UVW1 18.319 0.009
U
B
V
Gaia DR3
Source ID
2201415350484026240
Match probability
0.981
Parallax
1.208 ± 0.013 mas
Proper motion
(4.74, -2.74) mas/yr
Magnitudes
G=11.72, BP=12.75, RP=10.72
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.