5XMM J160500.3+431028

5XMM-DR15 stacked source · SRCID 3002574010100021
Position: 16h05m00.32s +43d10m28.1s (241.25134°, 43.17448°)
EP flux
3.89e-14 ± 1.2e-14 erg cm-2 s-1
CLASSX
AGN (0.927)
Detections
8

SRCID 3002574010100021
IAUNAME 5XMM J160500.3+431028
SC_RA 16h05m00.32s (241.25134°)
SC_DEC +43d10m28.1s (43.17448°)
RADEC_ERR 0.70 arcsec
LII / BII 68.3754° / 47.9860°
N_CONTRIB 8 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 52314.157 (2002-02-09 03:46:38.000 UTC)
MJD_LAST 53794.175 (2006-02-28 04:11:43.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.89e-14 ± 1.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.21 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.04 ± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.53 ± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.3) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.625

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
4073066
Match probability
0.988
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.664 0.191
U
B
V

Spectroscopic (zsp) 0.37700
Photometric (TPZ) 0.3259 (conf 0.74)
Photometric (Le Phare) 0.3760 (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 3.80e-14 (+4.9e-14 / −2.9e-14) erg cm−2 s−1
NH 5.22e+19 (+2.5e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.89 (+2.14 / −1.70)
DoF 271
p-value 0.973
Inter-instrument norm. 1.15 (0.92–1.38)
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.