5XMM J161014.1+545858

5XMM-DR15 stacked source · SRCID 3005975020100167
Position: 16h10m14.11s +54d58m58.9s (242.55879°, 54.98303°)
EP flux
5.97e-14 ± 5.7e-14 erg cm-2 s-1
CLASSX
AGN (0.909)
Detections
1

SRCID 3005975020100167
IAUNAME 5XMM J161014.1+545858
SC_RA 16h10m14.11s (242.55879°)
SC_DEC +54d58m58.9s (54.98303°)
RADEC_ERR 1.38 arcsec
LII / BII 84.9075° / 44.7293°
N_CONTRIB 1 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52379.840 (2002-04-15 20:10:07.000 UTC)
MJD_LAST 52380.022 (2002-04-16 00:32:19.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.97e-14 ± 5.7e-14 erg cm-2 s-1

Hardness ratios
HR1
-0.01 ± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.20
0.5-1.0 / 1.0-2.0 keV
HR3
-0.18 ± 0.29
1.0-2.0 / 2.0-4.5 keV
HR4
-0.32 ± 0.59
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.14

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
4080737
Match probability
0.895
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.564 0.191
U 21.137 0.152
B 21.299 0.260
V — —

Spectroscopic (zsp) 1.77400
Photometric (TPZ) 1.8255 (conf 0.83)
Photometric (Le Phare) 1.6770 (conf 0.91)

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

Stacked power-law fit
Unabsorbed flux 2.91e-14 (+5.4e-14 / −1.6e-14) erg cm−2 s−1
NH 9.71e+19 (+4.2e+20 / −2.1e+19) cm−2
Photon index (Γ) 2.23 (+2.71 / −1.67)
DoF 237
p-value 0.897
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.