5XMM J004324.6+645328

5XMM-DR15 stacked source · SRCID 3004014030100039
Position: 00h43m24.68s +64d53m28.5s (10.85284°, 64.89125°)
EP flux
7.58e-15 ± 8.3e-15 erg cm-2 s-1
CLASSX
Star (0.338)
Detections
2

SRCID 3004014030100039
IAUNAME 5XMM J004324.6+645328
SC_RA 00h43m24.68s (10.85284°)
SC_DEC +64d53m28.5s (64.89125°)
RADEC_ERR 1.76 arcsec
LII / BII 122.0800° / 2.0328°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52507.006 (2002-08-21 00:09:06.000 UTC)
MJD_LAST 54867.037 (2009-02-05 00:53:44.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 7.58e-15 ± 8.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.98 ± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
-0.78 ± 0.27
0.5-1.0 / 1.0-2.0 keV
HR3
0.69 ± 0.31
1.0-2.0 / 2.0-4.5 keV
HR4
-0.80 ± 0.71
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.1) SUM_FLAG: 0
Long-term lightcurve

Star

CLASSX outlier: 5.63

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
151307
Match probability
0.565
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.376 0.173
U — —
B — —
V 17.049 0.025
Gaia DR3
Source ID
524480451052252544
Match probability
0.986
Parallax
0.301 ± 0.050 mas
Proper motion
(-2.49, -0.07) mas/yr
Magnitudes
G=16.56, BP=17.41, RP=15.53
AllWISE
Name
J004324.85+645331.2
Match probability
0.993
BandMagErr
W1 13.155 0.025
W2 13.211 0.028
W3 12.510 —
W4 9.070 —
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.