5XMM J004430.6+644237

5XMM-DR15 stacked source · SRCID 3004014030100025
Position: 00h44m30.67s +64d42m37.0s (11.12779°, 64.71027°)
EP flux
5.35e-15 ± 9.3e-15 erg cm-2 s-1
CLASSX
Star (1)
Detections
2

SRCID 3004014030100025
IAUNAME 5XMM J004430.6+644237
SC_RA 00h44m30.67s (11.12779°)
SC_DEC +64d42m37.0s (64.71027°)
RADEC_ERR 2.36 arcsec
LII / BII 122.1919° / 1.8485°
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): 5.35e-15 ± 9.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.21 ± 0.29
0.2-0.5 / 0.5-1.0 keV
HR2
-0.97 ± 0.31
0.5-1.0 / 1.0-2.0 keV
HR3
0.99 ± 2.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.16 ± 1.72
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

Star

CLASSX outlier: 4

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
170528
Match probability
0.802
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 16.380 0.018
Gaia DR3
Source ID
524099985671684096
Match probability
0.938
Parallax
29.076 ± 0.023 mas
Proper motion
(166.33, -31.78) mas/yr
Magnitudes
G=14.75, BP=16.63, RP=13.46
Distance
34 pc
AllWISE
Name
J004430.49+644237.7
Match probability
0.993
BandMagErr
W1 10.476 0.023
W2 10.301 0.020
W3 10.171 0.059
W4 9.202 —
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.