5XMM J163300.2+570042

5XMM-DR15 stacked source · SRCID 3004954010100098
Position: 16h33m00.25s +57d00m42.9s (248.25105°, 57.01193°)
EP flux
4.98e-15 ± 3.6e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.638)
Detections
6

SRCID 3004954010100098
IAUNAME 5XMM J163300.2+570042
SC_RA 16h33m00.25s (248.25105°)
SC_DEC +57d00m42.9s (57.01193°)
RADEC_ERR 1.84 arcsec
LII / BII 86.4273° / 41.1238°
N_CONTRIB 6 (detections)
N_OBS 6 (observations covering the position)
MJD_FIRST 52208.338 (2001-10-26 08:07:10.000 UTC)
MJD_LAST 53674.442 (2005-10-31 10:36:41.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.98e-15 ± 3.6e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.54 ± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
0.15 ± 0.35
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40 ± 0.47
1.0-2.0 / 2.0-4.5 keV
HR4
-0.00 ± 0.68
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.8) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.66

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
4230919
Match probability
0.889
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 18.525 0.009
U — —
B — —
V — —
AllWISE
Name
J163300.55+570047.7
Match probability
0.72
BandMagErr
W1 13.608 0.031
W2 13.227 0.031
W3 8.957 0.024
W4 7.151 0.077
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.00
Galaxy
1.00

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.