5XMM J051541.3+010440

5XMM-DR15 stacked source · SRCID 3001062010100001
Position: 05h15m41.38s +01d04m40.7s (78.92243°, 1.07797°)
EP flux
1.05e-12 ± 9.8e-15 erg cm-2 s-1
CLASSX
AGN (0.629)
Detections
2

SRCID 3001062010100001
IAUNAME 5XMM J051541.3+010440
SC_RA 05h15m41.38s (78.92243°)
SC_DEC +01d04m40.7s (1.07797°)
RADEC_ERR 0.05 arcsec
LII / BII 200.4841° / -20.6375°
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): 1.05e-12 ± 9.8e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.79 ± 0.00
0.2-0.5 / 0.5-1.0 keV
HR2
-0.47 ± 0.01
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44 ± 0.04
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -5.6) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 2.35

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
1426706
Match probability
1
FilterMag (AB)Err
UVW2 16.326 0.018
UVM2 16.490 0.005
UVW1 16.398 0.003
U — —
B — —
V — —
Gaia DR3
Source ID
3233813338246568448
Match probability
0.996
Parallax
1.524 ± 0.037 mas
Proper motion
(5.42, -5.82) mas/yr
Magnitudes
G=15.73, BP=16.11, RP=15.14
AllWISE
Name
J051541.41+010440.3
Match probability
0.997
BandMagErr
W1 13.255 0.025
W2 12.986 0.026
W3 11.653 0.253
W4 8.862 —
CLASSOPT
Class
QSO
Star
0.16
AGN
0.82
Galaxy
0.02

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.

APPROX_SOURCE_VAR 14.400 (approximate flux variability amplitude)

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.

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