5XMM J160447.5+430148

5XMM-DR15 stacked source · SRCID 3002574010100032
Position: 16h04m47.58s +43d01m48.0s (241.19825°, 43.03001°)
EP flux
5.07e-14 ± 1.1e-14 erg cm-2 s-1
CLASSX
AGN (0.905)
Detections
2

SRCID 3002574010100032
IAUNAME 5XMM J160447.5+430148
SC_RA 16h04m47.58s (241.19825°)
SC_DEC +43d01m48.0s (43.03001°)
RADEC_ERR 0.87 arcsec
LII / BII 68.1669° / 48.0399°
N_CONTRIB 2 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 52314.157 (2002-02-09 03:46:38.000 UTC)
MJD_LAST 52316.191 (2002-02-11 04:35:09.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.07e-14 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
0.77 ± 0.23
0.2-0.5 / 0.5-1.0 keV
HR2
0.75 ± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.36 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
0.01 ± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.356

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
4072168
Match probability
0.991
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 22.386 0.210
B
V

Spectroscopic (zsp) 0.25700
Photometric (TPZ) 0.2259 (conf 0.52)
Photometric (Le Phare) 0.4084 (conf 0.98)

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

Stacked power-law fit
Unabsorbed flux 1.89e-14 (+2.8e-14 / −1.2e-14) erg cm−2 s−1
NH 3.19e+21 (+6.2e+21 / −8.2e+20) cm−2
Photon index (Γ) 1.62 (+2.23 / −1.18)
DoF 124
p-value 0.909
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.