5XMM J094010.0+355447

5XMM-DR15 stacked source · SRCID 3002174010100006
Position: 09h40m10.01s +35d54m47.9s (145.04173°, 35.91330°)
EP flux
2.27e-14 ± 3.6e-15 erg cm-2 s-1
CLASSX
AGN (0.905)
Detections
2

SRCID 3002174010100006
IAUNAME 5XMM J094010.0+355447
SC_RA 09h40m10.01s (145.04173°)
SC_DEC +35d54m47.9s (35.91330°)
RADEC_ERR 0.50 arcsec
LII / BII 188.3890° / 48.7185°
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): 2.27e-14 ± 3.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.12 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.64 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.58 ± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.6) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.646

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
2758927
Match probability
0.998
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.337 0.258
U 22.087 0.127
B
V 20.366 0.104
AllWISE
Name
J094009.99+355447.9
Match probability
0.995
BandMagErr
W1 15.967 0.056
W2 15.680 0.132
W3 11.915
W4 8.780
CLASSOPT
Class
Galaxy
Star
0.43
AGN
0.12
Galaxy
0.45

Photometric (TPZ) 0.3259 (conf 0.73)
Photometric (Le Phare) 0.3564 (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 3.40e-14 (+4.1e-14 / −2.8e-14) erg cm−2 s−1
NH 6.76e+19 (+3.1e+20 / −1.7e+19) cm−2
Photon index (Γ) 2.10 (+2.36 / −1.89)
DoF 141
p-value 0.267
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.