5XMM J223521.5+340935

5XMM-DR15 stacked source · SRCID 3002114020100046
Position: 22h35m21.52s +34d09m35.8s (338.83966°, 34.15994°)
EP flux
3.13e-14 ± 8.0e-15 erg cm-2 s-1
CLASSX
AGN (0.927)
Detections
1

SRCID 3002114020100046
IAUNAME 5XMM J223521.5+340935
SC_RA 22h35m21.52s (338.83966°)
SC_DEC +34d09m35.8s (34.15994°)
RADEC_ERR 0.70 arcsec
LII / BII 93.2569° / -20.7541°
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): 3.13e-14 ± 8.0e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.04 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.30 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00 ± 0.22
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: 0.714

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.

No multi-wavelength counterpart data available for this source.

Spectroscopic (zsp) 0.62000
Photometric (TPZ) 0.6258 (conf 0.63)
Photometric (Le Phare) 0.6216 (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 1.59e-14 (+2.0e-14 / −1.3e-14) erg cm−2 s−1
NH 4.69e+19 (+1.8e+20 / −1.6e+19) cm−2
Photon index (Γ) 2.29 (+2.53 / −2.05)
DoF 303
p-value 0.676
Inter-instrument norm. 1.59 (1.33–1.87)
Quality flag 0

APPROX_SOURCE_VAR 5.800 (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.