5XMM J105028.8+330045

5XMM-DR15 stacked source · SRCID 3005599020100006
Position: 10h50m28.88s +33d00m45.9s (162.62034°, 33.01275°)
EP flux
1.71e-13 ± 1.7e-14 erg cm-2 s-1
CLASSX
AGN (0.931)
Detections
1

SRCID 3005599020100006
IAUNAME 5XMM J105028.8+330045
SC_RA 10h50m28.88s (162.62034°)
SC_DEC +33d00m45.9s (33.01275°)
RADEC_ERR 0.35 arcsec
LII / BII 192.8306° / 63.2759°
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): 1.71e-13 ± 1.7e-14 erg cm-2 s-1

Hardness ratios
HR1
0.06 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.13 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.3) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.335

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
2943740
Match probability
0.998
FilterMag (AB)Err
UVW2 19.961 0.119
UVM2 — —
UVW1 19.037 0.034
U 19.197 0.037
B — —
V 18.963 0.064

Spectroscopic (zsp) 1.22700
Photometric (TPZ) 1.2257 (conf 0.84)
Photometric (Le Phare) 1.2420 (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 1.02e-13 (+1.1e-13 / −9.3e-14) erg cm−2 s−1
NH 1.70e+20 (+4.4e+20 / −2.9e+19) cm−2
Photon index (Γ) 2.30 (+2.49 / −2.17)
DoF 1679
p-value 0.248
Inter-instrument norm. 1.03 (0.91–1.12)
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.