5XMM J160724.8+544033

5XMM-DR15 stacked source · SRCID 3005975030100421
Position: 16h07m24.87s +54d40m33.1s (241.85363°, 54.67586°)
EP flux
6.40e-14 ± 1.1e-13 erg cm-2 s-1
CLASSX
AGN (0.892)
Detections
1

SRCID 3005975030100421
IAUNAME 5XMM J160724.8+544033
SC_RA 16h07m24.87s (241.85363°)
SC_DEC +54d40m33.1s (54.67586°)
RADEC_ERR 1.96 arcsec
LII / BII 84.6646° / 45.2087°
N_CONTRIB 1 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52376.072 (2002-04-12 01:43:35.000 UTC)
MJD_LAST 52376.084 (2002-04-12 02:00:27.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.40e-14 ± 1.1e-13 erg cm-2 s-1

Hardness ratios
HR1
-0.31 ± 0.21
0.2-0.5 / 0.5-1.0 keV
HR2
-0.16 ± 0.37
0.5-1.0 / 1.0-2.0 keV
HR3
-1.00 ± 1.38
1.0-2.0 / 2.0-4.5 keV
HR4
1.00 ± 0.90
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.933

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
4076981
Match probability
0.957
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.077 0.147
U 21.054 0.147
B 20.562 0.148
V — —

Spectroscopic (zsp) 0.38700
Photometric (TPZ) 0.3259 (conf 0.73)
Photometric (Le Phare) 0.3883 (conf 0.95)

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

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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.