5XMM J153611.6+553245

5XMM-DR15 stacked source · SRCID 3002854030100003
Position: 15h36m11.63s +55d32m45.7s (234.04846°, 55.54602°)
EP flux
4.38e-13 ± 6.8e-14 erg cm-2 s-1
CLASSX
AGN (0.921)
Detections
1

SRCID 3002854030100003
IAUNAME 5XMM J153611.6+553245
SC_RA 15h36m11.63s (234.04846°)
SC_DEC +55d32m45.7s (55.54602°)
RADEC_ERR 0.54 arcsec
LII / BII 88.3154° / 49.0170°
N_CONTRIB 1 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52411.836 (2002-05-17 20:04:25.000 UTC)
MJD_LAST 52411.948 (2002-05-17 22:44:37.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.38e-13 ± 6.8e-14 erg cm-2 s-1

Hardness ratios
HR1
0.03 ± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
0.02 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.35 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.09 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.9) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 2.18

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) 0.66700
Photometric (TPZ) 0.7258 (conf 0.66)
Photometric (Le Phare) 2.2200 (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 2.23e-13 (+2.6e-13 / −1.9e-13) erg cm−2 s−1
NH 8.97e+19 (+3.7e+20 / −2.0e+19) cm−2
Photon index (Γ) 1.79 (+1.95 / −1.67)
DoF 719
p-value 0.761
Inter-instrument norm. 1.51 (1.34–1.71)
Quality flag 0

APPROX_SOURCE_VAR 81.700 (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.