5XMM J105125.2+573050

5XMM-DR15 stacked source · SRCID 3002274010100044
Position: 10h51m25.26s +57d30m50.5s (162.85527°, 57.51404°)
EP flux
2.09e-14 ± 1.4e-15 erg cm-2 s-1
CLASSX
AGN (0.892)
Detections
16

SRCID 3002274010100044
IAUNAME 5XMM J105125.2+573050
SC_RA 10h51m25.26s (162.85527°)
SC_DEC +57d30m50.5s (57.51404°)
RADEC_ERR 0.19 arcsec
LII / BII 149.4340° / 52.9948°
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): 2.09e-14 ± 1.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.20 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39 ± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.33 ± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.6) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.318

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
2949645
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 21.524 0.051
B 20.435 0.046
V

Spectroscopic (zsp) 3.40900
Photometric (TPZ) 3.4250 (conf 0.35)
Photometric (Le Phare) 3.3730 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 2.04e-14 (+2.4e-14 / −1.7e-14) erg cm−2 s−1
NH 1.16e+20 (+4.9e+20 / −2.2e+19) cm−2
Photon index (Γ) 1.66 (+1.88 / −1.46)
DoF 150
p-value 0.827
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.