5XMM J105324.5+572818

5XMM-DR15 stacked source · SRCID 3002274010100043
Position: 10h53m24.58s +57d28m18.3s (163.35240°, 57.47176°)
EP flux
1.18e-14 ± 7.3e-16 erg cm-2 s-1
CLASSX
AGN (0.665)
Detections
16

SRCID 3002274010100043
IAUNAME 5XMM J105324.5+572818
SC_RA 10h53m24.58s (163.35240°)
SC_DEC +57d28m18.3s (57.47176°)
RADEC_ERR 0.19 arcsec
LII / BII 149.1845° / 53.2200°
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): 1.18e-14 ± 7.3e-16 erg cm-2 s-1

Hardness ratios
HR1
0.29 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.12 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41 ± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.59 ± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.6) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.691

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
2961227
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.963 0.188
U 23.023 0.177
B 22.287 0.177
V

Spectroscopic (zsp) 1.51800
Photometric (TPZ) 0.6258 (conf 0.29)
Photometric (Le Phare) 1.9600 (conf 0.16)

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

Stacked power-law fit
Unabsorbed flux 1.75e-14 (+2.0e-14 / −1.5e-14) erg cm−2 s−1
NH 3.40e+20 (+8.9e+20 / −4.8e+19) cm−2
Photon index (Γ) 1.86 (+2.10 / −1.69)
DoF 868
p-value 0.427
Inter-instrument norm. 0.78 (0.66–0.93)
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.