5XMM J153301.1+324707

5XMM-DR15 stacked source · SRCID 3003914010100006
Position: 15h33m01.13s +32d47m07.2s (233.25470°, 32.78533°)
EP flux
1.20e-13 ± 1.5e-14 erg cm-2 s-1
CLASSX
AGN (0.891)
Detections
3

SRCID 3003914010100006
IAUNAME 5XMM J153301.1+324707
SC_RA 15h33m01.13s (233.25470°)
SC_DEC +32d47m07.2s (32.78533°)
RADEC_ERR 0.41 arcsec
LII / BII 52.1544° / 54.7607°
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): 1.20e-13 ± 1.5e-14 erg cm-2 s-1

Hardness ratios
HR1
0.35 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.25 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.20 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.17 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.0) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.0998

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
3937570
Match probability
0.942
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.590 0.113
U 21.194 0.086
B 20.714 0.087
V — —

Spectroscopic (zsp) 0.99100
Photometric (TPZ) 1.0257 (conf 0.58)
Photometric (Le Phare) 1.1050 (conf 0.92)

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

Stacked power-law fit
Unabsorbed flux 1.38e-13 (+1.6e-13 / −1.2e-13) erg cm−2 s−1
NH 4.92e+19 (+1.9e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.53 (+1.66 / −1.43)
DoF 846
p-value 0.81
Inter-instrument norm. 0.74 (0.64–0.85)
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.