5XMM J161021.5+543103

5XMM-DR15 stacked source · SRCID 3005975010100157
Position: 16h10m21.57s +54d31m03.3s (242.58989°, 54.51757°)
EP flux
6.97e-14 ± 4.0e-14 erg cm-2 s-1
CLASSX
AGN (0.852)
Detections
2

SRCID 3005975010100157
IAUNAME 5XMM J161021.5+543103
SC_RA 16h10m21.57s (242.58989°)
SC_DEC +54d31m03.3s (54.51757°)
RADEC_ERR 1.03 arcsec
LII / BII 84.2727° / 44.8477°
N_CONTRIB 2 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52377.816 (2002-04-13 19:35:29.000 UTC)
MJD_LAST 52413.985 (2002-05-19 23:38:07.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.97e-14 ± 4.0e-14 erg cm-2 s-1

Hardness ratios
HR1
0.10 ± 0.17
0.2-0.5 / 0.5-1.0 keV
HR2
0.08 ± 0.18
0.5-1.0 / 1.0-2.0 keV
HR3
-0.27 ± 0.26
1.0-2.0 / 2.0-4.5 keV
HR4
-0.13 ± 0.50
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: 1.25

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
4080882
Match probability
0.985
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.830 0.097
U 20.396 0.093
B 20.293 0.079
V — —

Spectroscopic (zsp) 1.94700
Photometric (TPZ) 2.0254 (conf 0.93)
Photometric (Le Phare) 2.0680 (conf 0.93)

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

Stacked power-law fit
Unabsorbed flux 4.16e-14 (+6.8e-14 / −2.5e-14) erg cm−2 s−1
NH 1.61e+20 (+9.4e+20 / −2.8e+19) cm−2
Photon index (Γ) 1.92 (+2.50 / −1.47)
DoF 262
p-value 0.601
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.