5XMM J163154.8+374114

5XMM-DR15 stacked source · SRCID 3003354090100011
Position: 16h31m54.86s +37d41m14.5s (247.97858°, 37.68736°)
EP flux
8.73e-14 ± 1.2e-14 erg cm-2 s-1
CLASSX
AGN (0.914)
Detections
1

SRCID 3003354090100011
IAUNAME 5XMM J163154.8+374114
SC_RA 16h31m54.86s (247.97858°)
SC_DEC +37d41m14.5s (37.68736°)
RADEC_ERR 0.76 arcsec
LII / BII 60.4176° / 42.9638°
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): 8.73e-14 ± 1.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.80 ± 0.81
0.2-0.5 / 0.5-1.0 keV
HR2
0.69 ± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
0.50 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30 ± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.523

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
4212631
Match probability
0.982
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 20.329 0.125
V 18.958 0.091

Spectroscopic (zsp) 0.18100
Photometric (TPZ) 0.2259 (conf 0.52)
Photometric (Le Phare) 0.1867 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 7.77e-14 (+9.2e-14 / −6.7e-14) erg cm−2 s−1
NH 9.19e+21 (+1.5e+22 / −6.0e+21) cm−2
Photon index (Γ) 1.24 (+1.57 / −1.07)
DoF 141
p-value 0.315
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.