5XMM J153302.0+324328

5XMM-DR15 stacked source · SRCID 3003914010100035
Position: 15h33m02.05s +32d43m28.0s (233.25854°, 32.72446°)
EP flux
1.27e-14 ± 3.3e-15 erg cm-2 s-1
CLASSX
AGN (0.913)
Detections
3

SRCID 3003914010100035
IAUNAME 5XMM J153302.0+324328
SC_RA 15h33m02.05s (233.25854°)
SC_DEC +32d43m28.0s (32.72446°)
RADEC_ERR 0.75 arcsec
LII / BII 52.0491° / 54.7557°
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): 1.27e-14 ± 3.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.33 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.17 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.62 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.80 ± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.569

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
3937614
Match probability
0.986
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.939 0.148
U 22.230 0.199
B 21.945 0.256
V — —

Spectroscopic (zsp) 0.80200
Photometric (TPZ) 0.7258 (conf 0.61)
Photometric (Le Phare) 0.7952 (conf 0.98)

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

Stacked power-law fit
Unabsorbed flux 2.55e-14 (+3.4e-14 / −1.9e-14) erg cm−2 s−1
NH 2.61e+20 (+9.2e+20 / −3.6e+19) cm−2
Photon index (Γ) 2.25 (+2.65 / −1.93)
DoF 630
p-value 0.388
Inter-instrument norm. 0.91 (0.71–1.16)
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.