5XMM J051543.5+010208

5XMM-DR15 stacked source · SRCID 3001062010100122
Position: 05h15m43.55s +01d02m08.1s (78.93145°, 1.03559°)
EP flux
1.22e-15 ± 2.6e-15 erg cm-2 s-1
CLASSX
Star (1)
Detections
2

SRCID 3001062010100122
IAUNAME 5XMM J051543.5+010208
SC_RA 05h15m43.55s (78.93145°)
SC_DEC +01d02m08.1s (1.03559°)
RADEC_ERR 2.74 arcsec
LII / BII 200.5282° / -20.6507°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 51985.989 (2001-03-17 23:44:34.000 UTC)
MJD_LAST 56368.652 (2013-03-17 15:39:27.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.22e-15 ± 2.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.80 ± 0.87
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01 ± 0.37
0.5-1.0 / 1.0-2.0 keV
HR3
-0.94 ± 0.33
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00 ± 26.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.8) SUM_FLAG: 0
Long-term lightcurve

Star

CLASSX outlier: 1.36

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
1427270
Match probability
0.985
FilterMag (AB)Err
UVW2 16.780 0.023
UVM2 16.416 0.005
UVW1 14.886 0.002
U
B
V
Gaia DR3
Source ID
3233707643395489024
Match probability
0.997
Parallax
1.099 ± 0.014 mas
Proper motion
(5.12, 1.98) mas/yr
Magnitudes
G=12.49, BP=12.75, RP=12.07
Distance
942 pc
AllWISE
Name
J051543.39+010209.7
Match probability
0.997
BandMagErr
W1 11.290 0.023
W2 11.301 0.022
W3 11.171 0.140
W4 8.979
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.