5XMM J105044.0+572920

5XMM-DR15 stacked source · SRCID 3002274010100046
Position: 10h50m44.03s +57d29m20.3s (162.68346°, 57.48898°)
EP flux
3.33e-14 ± 2.6e-15 erg cm-2 s-1
CLASSX
AGN (0.881)
Detections
7

SRCID 3002274010100046
IAUNAME 5XMM J105044.0+572920
SC_RA 10h50m44.03s (162.68346°)
SC_DEC +57d29m20.3s (57.48898°)
RADEC_ERR 0.22 arcsec
LII / BII 149.5678° / 52.9432°
N_CONTRIB 7 (detections)
N_OBS 21 (observations covering the position)
MJD_FIRST 52207.311 (2001-10-25 07:28:18.000 UTC)
MJD_LAST 52569.311 (2002-10-22 07:27:35.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.33e-14 ± 2.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.02 ± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.80 ± 0.10
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: -0.358

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
2945047
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 22.513 0.201
B 21.698 0.123
V

Spectroscopic (zsp) 0.48000
Photometric (TPZ) 0.4759 (conf 0.68)
Photometric (Le Phare) 0.3892 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 3.05e-14 (+3.5e-14 / −2.7e-14) erg cm−2 s−1
NH 9.13e+19 (+3.7e+20 / −2.0e+19) cm−2
Photon index (Γ) 1.99 (+2.14 / −1.88)
DoF 643
p-value 0.912
Inter-instrument norm. 1.15 (1.04–1.30)
Quality flag 0

APPROX_SOURCE_VAR 5.100 (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.