5XMM J223537.8+340143

5XMM-DR15 stacked source · SRCID 3002114020100039
Position: 22h35m37.82s +34d01m43.0s (338.90760°, 34.02861°)
EP flux
3.92e-14 ± 6.2e-15 erg cm-2 s-1
CLASSX
AGN (0.94)
Detections
1

SRCID 3002114020100039
IAUNAME 5XMM J223537.8+340143
SC_RA 22h35m37.82s (338.90760°)
SC_DEC +34d01m43.0s (34.02861°)
RADEC_ERR 0.67 arcsec
LII / BII 93.2330° / -20.8952°
N_CONTRIB 1 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52250.890 (2001-12-07 21:22:09.000 UTC)
MJD_LAST 52251.416 (2001-12-08 09:59:17.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.92e-14 ± 6.2e-15 erg cm-2 s-1

Hardness ratios
HR1
0.92 ± 0.22
0.2-0.5 / 0.5-1.0 keV
HR2
0.70 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.03 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.10 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.3) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.321

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
6472123
Match probability
0.663
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.779 0.159
U 20.679 0.079
B 19.107 0.047
V

Photometric (TPZ) 0.2259 (conf 0.49)
Photometric (Le Phare) 0.2785 (conf 0.94)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Stacked power-law fit
Unabsorbed flux 2.94e-14 (+3.4e-14 / −2.5e-14) erg cm−2 s−1
NH 4.00e+21 (+6.1e+21 / −2.6e+21) cm−2
Photon index (Γ) 1.12 (+1.31 / −1.03)
DoF 127
p-value 0.255
Quality flag 0

APPROX_SOURCE_VAR 12.200 (approximate flux variability amplitude)

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.