5XMM J165041.4+045817

5XMM-DR15 stacked source · SRCID 3003214080100004
Position: 16h50m41.41s +04d58m17.8s (252.67256°, 4.97160°)
EP flux
5.13e-14 ± 3.7e-15 erg cm-2 s-1
CLASSX
AGN (0.784)
Detections
4

SRCID 3003214080100004
IAUNAME 5XMM J165041.4+045817
SC_RA 16h50m41.41s (252.67256°)
SC_DEC +04d58m17.8s (4.97160°)
RADEC_ERR 0.22 arcsec
LII / BII 22.9676° / 29.0347°
N_CONTRIB 4 (detections)
N_OBS 4 (observations covering the position)
MJD_FIRST 51968.999 (2001-02-28 23:58:30.000 UTC)
MJD_LAST 53994.514 (2006-09-16 12:20:46.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.13e-14 ± 3.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.33 ± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31 ± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.46 ± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.4) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.191

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
4358083
Match probability
0.991
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.370 0.175
U 22.402 0.126
B
V
AllWISE
Name
J165041.47+045817.2
Match probability
0.995
BandMagErr
W1 16.759 0.092
W2 15.994 0.171
W3 12.245
W4 8.662
CLASSOPT
Class
QSO
Star
0.00
AGN
0.99
Galaxy
0.01

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 4.97e-14 (+5.9e-14 / −4.2e-14) erg cm−2 s−1
NH 8.82e+19 (+4.4e+20 / −2.1e+19) cm−2
Photon index (Γ) 1.62 (+1.81 / −1.46)
DoF 125
p-value 0.712
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.