5XMM J160902.5+540150

5XMM-DR15 stacked source · SRCID 3005975050100033
Position: 16h09m02.52s +54d01m50.6s (242.26051°, 54.03071°)
EP flux
2.02e-13 ± 4.3e-14 erg cm-2 s-1
CLASSX
AGN (0.85)
Detections
1

SRCID 3005975050100033
IAUNAME 5XMM J160902.5+540150
SC_RA 16h09m02.52s (242.26051°)
SC_DEC +54d01m50.6s (54.03071°)
RADEC_ERR 0.83 arcsec
LII / BII 83.6908° / 45.1713°
N_CONTRIB 1 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52391.750 (2002-04-27 18:00:21.000 UTC)
MJD_LAST 52391.821 (2002-04-27 19:42:06.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.02e-13 ± 4.3e-14 erg cm-2 s-1

Hardness ratios
HR1
-0.04 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.00 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.21 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.68 ± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.736

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
4079536
Match probability
0.993
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 19.979 0.132
B — —
V — —

Spectroscopic (zsp) 0.60800
Photometric (TPZ) 0.6258 (conf 0.78)
Photometric (Le Phare) 0.6024 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 1.79e-13 (+2.2e-13 / −1.4e-13) erg cm−2 s−1
NH 5.35e+19 (+2.3e+20 / −1.8e+19) cm−2
Photon index (Γ) 1.78 (+1.98 / −1.63)
DoF 261
p-value 0.903
Inter-instrument norm. 0.97 (0.78–1.19)
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.