5XMM J105357.1+573241

5XMM-DR15 stacked source · SRCID 3002274010100050
Position: 10h53m57.17s +57d32m41.5s (163.48821°, 57.54487°)
EP flux
1.37e-14 ± 1.6e-15 erg cm-2 s-1
CLASSX
AGN (0.868)
Detections
14

SRCID 3002274010100050
IAUNAME 5XMM J105357.1+573241
SC_RA 10h53m57.17s (163.48821°)
SC_DEC +57d32m41.5s (57.54487°)
RADEC_ERR 0.22 arcsec
LII / BII 149.0120° / 53.2234°
N_CONTRIB 14 (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): 1.37e-14 ± 1.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.10 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.10 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.417

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
2962720
Match probability
0.998
FilterMag (AB)Err
UVW2 21.773 0.199
UVM2 21.859 0.183
UVW1 21.604 0.072
U 21.655 0.056
B 21.634 0.090
V

Spectroscopic (zsp) 1.28200
Photometric (TPZ) 1.2756 (conf 0.78)
Photometric (Le Phare) 1.3550 (conf 0.71)

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

Stacked power-law fit
Unabsorbed flux 1.12e-14 (+1.3e-14 / −9.9e-15) erg cm−2 s−1
NH 1.11e+20 (+4.6e+20 / −2.3e+19) cm−2
Photon index (Γ) 2.41 (+2.64 / −2.24)
DoF 347
p-value 0.469
Inter-instrument norm. 1.07 (0.90–1.25)
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.