5XMM J161059.5+542153

5XMM-DR15 stacked source · SRCID 3005975180100043
Position: 16h10m59.59s +54d21m53.6s (242.74830°, 54.36489°)
EP flux
5.49e-14 ± 1.6e-14 erg cm-2 s-1
CLASSX
AGN (0.912)
Detections
6

SRCID 3005975180100043
IAUNAME 5XMM J161059.5+542153
SC_RA 16h10m59.59s (242.74830°)
SC_DEC +54d21m53.6s (54.36489°)
RADEC_ERR 0.61 arcsec
LII / BII 84.0294° / 44.8029°
N_CONTRIB 6 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52413.797 (2002-05-19 19:07:35.000 UTC)
MJD_LAST 52575.391 (2002-10-28 09:22:54.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.49e-14 ± 1.6e-14 erg cm-2 s-1

Hardness ratios
HR1
0.33 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
-0.05 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.15 ± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.478

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
4082181
Match probability
0.992
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.534 0.061
U 20.684 0.065
B 20.762 0.101
V — —

Spectroscopic (zsp) 1.09500
Photometric (TPZ) 1.0757 (conf 0.44)
Photometric (Le Phare) 1.3650 (conf 0.65)

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

Stacked power-law fit
Unabsorbed flux 3.75e-14 (+5.1e-14 / −2.9e-14) erg cm−2 s−1
NH 6.46e+20 (+1.5e+21 / −5.0e+19) cm−2
Photon index (Γ) 2.42 (+2.86 / −1.90)
DoF 576
p-value 0.019
Inter-instrument norm. 1.42 (1.06–1.75)
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.