5XMM J105003.1+325045

5XMM-DR15 stacked source · SRCID 3005599020100025
Position: 10h50m03.15s +32d50m45.5s (162.51315°, 32.84597°)
EP flux
3.74e-14 ± 8.7e-15 erg cm-2 s-1
CLASSX
AGN (0.861)
Detections
1

SRCID 3005599020100025
IAUNAME 5XMM J105003.1+325045
SC_RA 10h50m03.15s (162.51315°)
SC_DEC +32d50m45.5s (32.84597°)
RADEC_ERR 0.60 arcsec
LII / BII 193.2154° / 63.1992°
N_CONTRIB 1 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52226.012 (2001-11-13 00:17:04.000 UTC)
MJD_LAST 52226.450 (2001-11-13 10:48:00.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.74e-14 ± 8.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.17 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.17 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.54 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43 ± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.647

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
2942186
Match probability
0.997
FilterMag (AB)Err
UVW2 20.377 0.222
UVM2 — —
UVW1 20.071 0.103
U 20.209 0.120
B — —
V 19.935 0.196

Spectroscopic (zsp) 0.83900
Photometric (TPZ) 0.8758 (conf 0.74)
Photometric (Le Phare) 0.7202 (conf 0.92)

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

Stacked power-law fit
Unabsorbed flux 2.88e-14 (+3.5e-14 / −2.4e-14) erg cm−2 s−1
NH 4.65e+19 (+1.6e+20 / −1.5e+19) cm−2
Photon index (Γ) 2.36 (+2.60 / −2.17)
DoF 1030
p-value 0.1
Inter-instrument norm. 1.51 (1.28–1.74)
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.