5XMM J161048.8+541841

5XMM-DR15 stacked source · SRCID 3005975230100129
Position: 16h10m48.83s +54d18m41.6s (242.70348°, 54.31155°)
EP flux
2.16e-14 ± 8.6e-15 erg cm-2 s-1
CLASSX
AGN (0.921)
Detections
5

SRCID 3005975230100129
IAUNAME 5XMM J161048.8+541841
SC_RA 16h10m48.83s (242.70348°)
SC_DEC +54d18m41.6s (54.31155°)
RADEC_ERR 1.25 arcsec
LII / BII 83.9676° / 44.8430°
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): 2.16e-14 ± 8.6e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.10 ± 0.28
0.2-0.5 / 0.5-1.0 keV
HR2
0.24 ± 0.24
0.5-1.0 / 1.0-2.0 keV
HR3
0.12 ± 0.22
1.0-2.0 / 2.0-4.5 keV
HR4
-0.20 ± 0.28
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.4) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.204

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
4081505
Match probability
0.919
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.333 0.161
U 21.007 0.094
B 20.929 0.107
V — —

Spectroscopic (zsp) 1.52600
Photometric (TPZ) 1.8255 (conf 0.73)
Photometric (Le Phare) 1.9020 (conf 0.62)

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

Stacked power-law fit
Unabsorbed flux 3.60e-14 (+5.7e-14 / −2.0e-14) erg cm−2 s−1
NH 8.86e+19 (+4.3e+20 / −1.8e+19) cm−2
Photon index (Γ) 1.77 (+2.41 / −1.35)
DoF 85
p-value 0.742
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.