5XMM J161147.7+541132

5XMM-DR15 stacked source · SRCID 3005975230100032
Position: 16h11m47.71s +54d11m32.9s (242.94880°, 54.19248°)
EP flux
4.26e-14 ± 9.8e-15 erg cm-2 s-1
CLASSX
AGN (0.917)
Detections
5

SRCID 3005975230100032
IAUNAME 5XMM J161147.7+541132
SC_RA 16h11m47.71s (242.94880°)
SC_DEC +54d11m32.9s (54.19248°)
RADEC_ERR 0.49 arcsec
LII / BII 83.7501° / 44.7387°
N_CONTRIB 5 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52529.479 (2002-09-12 11:30:08.000 UTC)
MJD_LAST 52575.391 (2002-10-28 09:22:54.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.26e-14 ± 9.8e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.11 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.49 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.83 ± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.657

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
4087235
Match probability
0.997
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.861 0.073
U 20.733 0.067
B 20.398 0.058
V — —

Spectroscopic (zsp) 0.33200
Photometric (TPZ) 0.2759 (conf 0.74)
Photometric (Le Phare) 0.2148 (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 4.67e-14 (+6.5e-14 / −3.5e-14) erg cm−2 s−1
NH 5.59e+19 (+2.1e+20 / −1.7e+19) cm−2
Photon index (Γ) 2.52 (+2.78 / −2.25)
DoF 712
p-value 0.023
Inter-instrument norm. 1.48 (1.17–1.80)
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.