5XMM J094013.1+355930

5XMM-DR15 stacked source · SRCID 3002174010100016
Position: 09h40m13.11s +35d59m30.4s (145.05464°, 35.99178°)
EP flux
1.45e-14 ± 4.7e-15 erg cm-2 s-1
CLASSX
AGN (0.93)
Detections
2

SRCID 3002174010100016
IAUNAME 5XMM J094013.1+355930
SC_RA 09h40m13.11s (145.05464°)
SC_DEC +35d59m30.4s (35.99178°)
RADEC_ERR 0.74 arcsec
LII / BII 188.2705° / 48.7311°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52209.321 (2001-10-27 07:42:42.000 UTC)
MJD_LAST 58796.982 (2019-11-09 23:33:27.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.45e-14 ± 4.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.28 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.26 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.52 ± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.116

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
2759004
Match probability
0.985
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.809 0.168
U
B
V

Spectroscopic (zsp) 1.94400
Photometric (TPZ) 1.9754 (conf 0.84)
Photometric (Le Phare) 1.6570 (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 1.68e-14 (+2.2e-14 / −1.3e-14) erg cm−2 s−1
NH 1.74e+20 (+8.0e+20 / −2.9e+19) cm−2
Photon index (Γ) 2.43 (+2.79 / −2.08)
DoF 78
p-value 0.942
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.