5XMM J104023.4+090629

5XMM-DR15 stacked source · SRCID 3003854040100008
Position: 10h40m23.49s +09d06m29.1s (160.09787°, 9.10809°)
EP flux
1.78e-14 ± 4.9e-15 erg cm-2 s-1
CLASSX
AGN (0.834)
Detections
2

SRCID 3003854040100008
IAUNAME 5XMM J104023.4+090629
SC_RA 10h40m23.49s (160.09787°)
SC_DEC +09d06m29.1s (9.10809°)
RADEC_ERR 0.89 arcsec
LII / BII 236.9173° / 54.2096°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52238.172 (2001-11-25 04:08:12.000 UTC)
MJD_LAST 53350.123 (2004-12-11 02:57:37.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.78e-14 ± 4.9e-15 erg cm-2 s-1

Hardness ratios
HR1
0.21 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
-0.16 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.74 ± 0.33
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.3) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.06

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
2920637
Match probability
0.999
FilterMag (AB)Err
UVW2 — —
UVM2 19.667 0.056
UVW1 19.116 0.079
U — —
B — —
V — —

Photometric (TPZ) 1.3756 (conf 0.57)
Photometric (Le Phare) 1.5200 (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 2.56e-14 (+3.5e-14 / −1.9e-14) erg cm−2 s−1
NH 1.10e+20 (+5.8e+20 / −1.9e+19) cm−2
Photon index (Γ) 2.34 (+2.71 / −1.97)
DoF 40
p-value 0.93
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.