5XMM J153222.9+324025

5XMM-DR15 stacked source · SRCID 3003914010100014
Position: 15h32m22.94s +32d40m25.8s (233.09560°, 32.67384°)
EP flux
3.13e-14 ± 5.6e-15 erg cm-2 s-1
CLASSX
AGN (0.891)
Detections
3

SRCID 3003914010100014
IAUNAME 5XMM J153222.9+324025
SC_RA 15h32m22.94s (233.09560°)
SC_DEC +32d40m25.8s (32.67384°)
RADEC_ERR 0.56 arcsec
LII / BII 51.9542° / 54.8912°
N_CONTRIB 3 (detections)
N_OBS 4 (observations covering the position)
MJD_FIRST 52485.506 (2002-07-30 12:08:00.000 UTC)
MJD_LAST 53369.317 (2004-12-30 07:36:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.13e-14 ± 5.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.17 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.36 ± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.6) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.241

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
3934876
Match probability
0.985
FilterMag (AB)Err
UVW2 — —
UVM2 21.886 0.287
UVW1 21.158 0.083
U 21.141 0.082
B 21.302 0.138
V — —

Spectroscopic (zsp) 1.49000
Photometric (TPZ) 1.4756 (conf 0.82)
Photometric (Le Phare) 1.4720 (conf 0.49)

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

Stacked power-law fit
Unabsorbed flux 4.31e-14 (+5.7e-14 / −3.2e-14) erg cm−2 s−1
NH 1.18e+20 (+5.8e+20 / −2.2e+19) cm−2
Photon index (Γ) 1.68 (+1.98 / −1.47)
DoF 881
p-value 0.613
Inter-instrument norm. 1.27 (1.03–1.56)
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.