5XMM J105311.6+572306

5XMM-DR15 stacked source · SRCID 3002274010100099
Position: 10h53m11.66s +57d23m06.6s (163.29860°, 57.38516°)
EP flux
7.39e-15 ± 9.3e-16 erg cm-2 s-1
CLASSX
AGN (0.835)
Detections
16

SRCID 3002274010100099
IAUNAME 5XMM J105311.6+572306
SC_RA 10h53m11.66s (163.29860°)
SC_DEC +57d23m06.6s (57.38516°)
RADEC_ERR 0.26 arcsec
LII / BII 149.3234° / 53.2577°
N_CONTRIB 16 (detections)
N_OBS 21 (observations covering the position)
MJD_FIRST 51661.158 (2000-04-27 03:47:47.000 UTC)
MJD_LAST 52615.196 (2002-12-07 04:41:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 7.39e-15 ± 9.3e-16 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.1) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.606

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
2960451
Match probability
0.991
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.613 0.119
U 22.746 0.137
B 22.100 0.212
V

Spectroscopic (zsp) 1.54400
Photometric (TPZ) 1.0757 (conf 0.22)
Photometric (Le Phare) 3.0630 (conf 0.17)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Stacked power-law fit
Unabsorbed flux 6.93e-15 (+8.6e-15 / −5.5e-15) erg cm−2 s−1
NH 1.61e+20 (+7.3e+20 / −2.3e+19) cm−2
Photon index (Γ) 2.03 (+2.35 / −1.80)
DoF 280
p-value 0.286
Inter-instrument norm. 1.05 (0.78–1.33)
Quality flag 0

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.