5XMM J105306.0+573424

5XMM-DR15 stacked source · SRCID 3002274010100063
Position: 10h53m06.02s +57d34m24.7s (163.27507°, 57.57354°)
EP flux
1.04e-14 ± 9.5e-16 erg cm-2 s-1
CLASSX
AGN (0.747)
Detections
17

SRCID 3002274010100063
IAUNAME 5XMM J105306.0+573424
SC_RA 10h53m06.02s (163.27507°)
SC_DEC +57d34m24.7s (57.57354°)
RADEC_ERR 0.21 arcsec
LII / BII 149.1073° / 53.1203°
N_CONTRIB 17 (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): 1.04e-14 ± 9.5e-16 erg cm-2 s-1

Hardness ratios
HR1
-0.02 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.01 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.53 ± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.29 ± 0.12
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: 1.57

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
2960091
Match probability
0.998
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.634 0.262
U 21.829 0.043
B 20.728 0.030
V 20.419 0.156

Spectroscopic (zsp) 2.94400
Photometric (TPZ) 2.8252 (conf 0.78)
Photometric (Le Phare) 2.7490 (conf 0.98)

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

Stacked power-law fit
Unabsorbed flux 1.18e-14 (+1.3e-14 / −1.0e-14) erg cm−2 s−1
NH 7.04e+19 (+3.1e+20 / −1.9e+19) cm−2
Photon index (Γ) 1.94 (+2.10 / −1.81)
DoF 375
p-value 0.904
Inter-instrument norm. 0.84 (0.71–0.99)
Quality flag 0

APPROX_SOURCE_VAR 7.600 (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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