5XMM J004419.9+644737

5XMM-DR15 stacked source · SRCID 3004014030100037
Position: 00h44m19.92s +64d47m37.2s (11.08301°, 64.79366°)
EP flux
9.00e-15 ± 7.6e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.496)
Detections
2

SRCID 3004014030100037
IAUNAME 5XMM J004419.9+644737
SC_RA 00h44m19.92s (11.08301°)
SC_DEC +64d47m37.2s (64.79366°)
RADEC_ERR 2.25 arcsec
LII / BII 122.1750° / 1.9324°
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): 9.00e-15 ± 7.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.27 ± 0.54
0.2-0.5 / 0.5-1.0 keV
HR2
0.36 ± 0.35
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29 ± 0.27
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44 ± 0.63
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 5.04

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
167810
Match probability
0.83
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 18.086 0.062
Gaia DR3
Source ID
524476121725136256
Match probability
0.989
Parallax
0.155 ± 0.089 mas
Proper motion
(-2.31, -0.30) mas/yr
Magnitudes
G=17.50, BP=18.45, RP=16.50
Distance
1087 pc
AllWISE
Name
J004419.98+644737.4
Match probability
0.993
BandMagErr
W1 13.980 0.024
W2 14.125 0.033
W3 12.527 —
W4 9.051 —
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.