5XMM J163203.9+374331

5XMM-DR15 stacked source · SRCID 3003354090100005
Position: 16h32m03.98s +37d43m31.6s (248.01658°, 37.72543°)
EP flux
6.01e-14 ± 1.1e-14 erg cm-2 s-1
CLASSX
AGN (0.912)
Detections
1

SRCID 3003354090100005
IAUNAME 5XMM J163203.9+374331
SC_RA 16h32m03.98s (248.01658°)
SC_DEC +37d43m31.6s (37.72543°)
RADEC_ERR 0.57 arcsec
LII / BII 60.4723° / 42.9364°
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): 6.01e-14 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
0.06 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.13 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.62 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
0.08 ± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.4) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.222

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
4215230
Match probability
0.995
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 21.092 0.266
V

Spectroscopic (zsp) 0.93300
Photometric (TPZ) 0.8758 (conf 0.34)
Photometric (Le Phare) 0.8982 (conf 0.59)

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

Stacked power-law fit
Unabsorbed flux 3.71e-14 (+4.6e-14 / −3.0e-14) erg cm−2 s−1
NH 9.79e+19 (+4.2e+20 / −2.2e+19) cm−2
Photon index (Γ) 2.16 (+2.42 / −1.97)
DoF 259
p-value 0.787
Inter-instrument norm. 0.69 (0.58–0.84)
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.