5XMM J020731.9+023626

5XMM-DR15 stacked source · SRCID 3004874010100028
Position: 02h07m31.90s +02d36m26.6s (31.88291°, 2.60738°)
EP flux
3.59e-14 ± 1.7e-14 erg cm-2 s-1
CLASSX
AGN (0.938)
Detections
1

SRCID 3004874010100028
IAUNAME 5XMM J020731.9+023626
SC_RA 02h07m31.90s (31.88291°)
SC_DEC +02d36m26.6s (2.60738°)
RADEC_ERR 1.14 arcsec
LII / BII 157.5824° / -55.0615°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52478.303 (2002-07-23 07:15:46.000 UTC)
MJD_LAST 52478.847 (2002-07-23 20:20:18.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.59e-14 ± 1.7e-14 erg cm-2 s-1

Hardness ratios
HR1
0.12 ± 0.26
0.2-0.5 / 0.5-1.0 keV
HR2
0.41 ± 0.17
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.36 ± 0.40
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.6) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.0437

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
736670
Match probability
0.991
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.471 0.243
B 21.746 0.375
V — —

Photometric (TPZ) 1.2756 (conf 0.32)
Photometric (Le Phare) 2.5400 (conf 0.18)

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

Stacked power-law fit
Unabsorbed flux 1.65e-14 (+2.9e-14 / −1.0e-14) erg cm−2 s−1
NH 1.14e+20 (+7.5e+20 / −2.3e+19) cm−2
Photon index (Γ) 1.90 (+2.50 / −1.40)
DoF 138
p-value 0.036
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.