5XMM J093930.6+354716

5XMM-DR15 stacked source · SRCID 3002174010100033
Position: 09h39m30.62s +35d47m16.8s (144.87759°, 35.78799°)
EP flux
1.86e-14 ± 9.4e-15 erg cm-2 s-1
CLASSX
AGN (0.662)
Detections
2

SRCID 3002174010100033
IAUNAME 5XMM J093930.6+354716
SC_RA 09h39m30.62s (144.87759°)
SC_DEC +35d47m16.8s (35.78799°)
RADEC_ERR 1.25 arcsec
LII / BII 188.5724° / 48.5817°
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): 1.86e-14 ± 9.4e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.04 ± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
0.19 ± 0.20
0.5-1.0 / 1.0-2.0 keV
HR3
-0.36 ± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26 ± 0.48
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 0.1) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 2.12

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
2757511
Match probability
0.641
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B
V 18.006 0.064

Photometric (TPZ) 3.5000 (conf 0.35)
Photometric (Le Phare) 0.1309 (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 1.56e-14 (+2.3e-14 / −1.1e-14) erg cm−2 s−1
NH 7.76e+19 (+4.4e+20 / −2.0e+19) cm−2
Photon index (Γ) 1.83 (+2.23 / −1.48)
DoF 254
p-value 0.946
Inter-instrument norm. 1.31 (0.91–1.71)
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.