5XMM J153257.3+324858

5XMM-DR15 stacked source · SRCID 3003914010100012
Position: 15h32m57.31s +32d48m58.3s (233.23880°, 32.81619°)
EP flux
3.62e-14 ± 7.0e-15 erg cm-2 s-1
CLASSX
AGN (0.71)
Detections
3

SRCID 3003914010100012
IAUNAME 5XMM J153257.3+324858
SC_RA 15h32m57.31s (233.23880°)
SC_DEC +32d48m58.3s (32.81619°)
RADEC_ERR 0.56 arcsec
LII / BII 52.2072° / 54.7749°
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): 3.62e-14 ± 7.0e-15 erg cm-2 s-1

Hardness ratios
HR1
0.36 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.05 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.43 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.68 ± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 3.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.62

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
3937399
Match probability
0.921
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.951 0.151
U 21.602 0.107
B 21.616 0.175
V — —

Photometric (TPZ) 1.5256 (conf 0.46)
Photometric (Le Phare) 1.5880 (conf 0.36)

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

Stacked power-law fit
Unabsorbed flux 5.45e-14 (+6.8e-14 / −4.4e-14) erg cm−2 s−1
NH 1.81e+20 (+7.1e+20 / −2.6e+19) cm−2
Photon index (Γ) 1.69 (+1.97 / −1.49)
DoF 594
p-value 0.147
Inter-instrument norm. 1.11 (0.89–1.34)
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.