5XMM J041958.7+560126

5XMM-DR15 stacked source · SRCID 3000011010100062
Position: 04h19m58.79s +56d01m26.4s (64.99497°, 56.02399°)
EP flux
4.05e-15 ± 2.0e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.381)
Detections
4

SRCID 3000011010100062
IAUNAME 5XMM J041958.7+560126
SC_RA 04h19m58.79s (64.99497°)
SC_DEC +56d01m26.4s (56.02399°)
RADEC_ERR 2.44 arcsec
LII / BII 149.1868° / 4.1779°
N_CONTRIB 4 (detections)
N_OBS 4 (observations covering the position)
MJD_FIRST 52140.300 (2001-08-19 07:11:46.000 UTC)
MJD_LAST 55980.039 (2012-02-23 00:55:53.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.05e-15 ± 2.0e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.35 ± 0.75
0.2-0.5 / 0.5-1.0 keV
HR2
0.65 ± 0.64
0.5-1.0 / 1.0-2.0 keV
HR3
0.23 ± 0.51
1.0-2.0 / 2.0-4.5 keV
HR4
0.07 ± 0.35
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 2.4) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 4.71

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
1050481
Match probability
0.777
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B
V 21.131 0.173
Gaia DR3
Source ID
276650701946825472
Match probability
0.994
Parallax
0.017 ± 1.556 mas
Proper motion
(-0.20, 1.64) mas/yr
Magnitudes
G=20.81, BP=21.72, RP=19.64
AllWISE
Name
J041958.99+560130.5
Match probability
0.996
BandMagErr
W1 16.235 0.076
W2 17.083
W3 12.233
W4 9.015
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.