5XMM J160324.3+425940

5XMM-DR15 stacked source · SRCID 3002574010100027
Position: 16h03m24.34s +42d59m40.9s (240.85140°, 42.99470°)
EP flux
5.89e-14 ± 2.0e-14 erg cm-2 s-1
CLASSX
AGN (0.709)
Detections
2

SRCID 3002574010100027
IAUNAME 5XMM J160324.3+425940
SC_RA 16h03m24.34s (240.85140°)
SC_DEC +42d59m40.9s (42.99470°)
RADEC_ERR 0.88 arcsec
LII / BII 68.1550° / 48.2958°
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): 5.89e-14 ± 2.0e-14 erg cm-2 s-1

Hardness ratios
HR1
0.06 ± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
-0.07 ± 0.15
0.5-1.0 / 1.0-2.0 keV
HR3
-0.14 ± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.19 ± 0.28
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.18

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
4067935
Match probability
0.986
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.487 0.080
U 20.550 0.056
B
V

Spectroscopic (zsp) 1.55600
Photometric (TPZ) 0.5758 (conf 0.36)
Photometric (Le Phare) 2.0490 (conf 0.59)

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

Stacked power-law fit
Unabsorbed flux 2.77e-14 (+3.8e-14 / −2.1e-14) erg cm−2 s−1
NH 2.11e+20 (+7.3e+20 / −3.1e+19) cm−2
Photon index (Γ) 2.38 (+2.74 / −2.00)
DoF 138
p-value 0.971
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.