5XMM J163213.6+373422

5XMM-DR15 stacked source · SRCID 3003354090100018
Position: 16h32m13.66s +37d34m22.0s (248.05691°, 37.57278°)
EP flux
3.55e-14 ± 7.9e-15 erg cm-2 s-1
CLASSX
AGN (0.933)
Detections
1

SRCID 3003354090100018
IAUNAME 5XMM J163213.6+373422
SC_RA 16h32m13.66s (248.05691°)
SC_DEC +37d34m22.0s (37.57278°)
RADEC_ERR 0.76 arcsec
LII / BII 60.2673° / 42.8940°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52280.159 (2002-01-06 03:48:18.000 UTC)
MJD_LAST 52280.356 (2002-01-06 08:32:04.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.55e-14 ± 7.9e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.09 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
-0.15 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.51 ± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
0.21 ± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.513

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
4218069
Match probability
0.97
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 21.010 0.205
V 20.692 0.254

Spectroscopic (zsp) 1.47900
Photometric (TPZ) 0.7258 (conf 0.45)
Photometric (Le Phare) 2.0050 (conf 0.52)

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

Stacked power-law fit
Unabsorbed flux 2.59e-14 (+3.5e-14 / −1.8e-14) erg cm−2 s−1
NH 1.04e+20 (+7.1e+20 / −2.3e+19) cm−2
Photon index (Γ) 1.60 (+1.99 / −1.30)
DoF 114
p-value 0.827
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.