5XMM J105129.8+573737

5XMM-DR15 stacked source · SRCID 3002274010100048
Position: 10h51m29.82s +57d37m37.7s (162.87427°, 57.62715°)
EP flux
2.57e-14 ± 2.7e-15 erg cm-2 s-1
CLASSX
AGN (0.826)
Detections
14

SRCID 3002274010100048
IAUNAME 5XMM J105129.8+573737
SC_RA 10h51m29.82s (162.87427°)
SC_DEC +57d37m37.7s (57.62715°)
RADEC_ERR 0.20 arcsec
LII / BII 149.2839° / 52.9261°
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): 2.57e-14 ± 2.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.21 ± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.13 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.22 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.35 ± 0.11
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: -0.405

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
2950202
Match probability
0.97
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.012 0.162
U 22.929 0.279
B 22.585 0.345
V

Spectroscopic (zsp) 1.21900
Photometric (TPZ) 1.2756 (conf 0.83)
Photometric (Le Phare) 1.1980 (conf 0.48)

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

Stacked power-law fit
Unabsorbed flux 2.44e-14 (+2.7e-14 / −2.2e-14) erg cm−2 s−1
NH 6.97e+19 (+2.7e+20 / −1.9e+19) cm−2
Photon index (Γ) 2.18 (+2.32 / −2.07)
DoF 488
p-value 0.307
Inter-instrument norm. 1.05 (0.93–1.19)
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.