5XMM J020737.3+023701

5XMM-DR15 stacked source · SRCID 3004874010100007
Position: 02h07m37.31s +02d37m01.0s (31.90546°, 2.61695°)
EP flux
9.37e-14 ± 2.2e-14 erg cm-2 s-1
CLASSX
AGN (0.934)
Detections
1

SRCID 3004874010100007
IAUNAME 5XMM J020737.3+023701
SC_RA 02h07m37.31s (31.90546°)
SC_DEC +02d37m01.0s (2.61695°)
RADEC_ERR 0.75 arcsec
LII / BII 157.6078° / -55.0418°
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): 9.37e-14 ± 2.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.23 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.23 ± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.52 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.13 ± 0.22
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: 0.286

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
737048
Match probability
0.976
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 20.809 0.050
B 20.506 0.128
V — —

Spectroscopic (zsp) 1.78800
Photometric (TPZ) 1.7755 (conf 0.82)
Photometric (Le Phare) 1.7630 (conf 0.91)

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

Stacked power-law fit
Unabsorbed flux 6.51e-14 (+8.1e-14 / −5.3e-14) erg cm−2 s−1
NH 1.44e+20 (+6.0e+20 / −2.2e+19) cm−2
Photon index (Γ) 1.59 (+1.83 / −1.39)
DoF 565
p-value 0.627
Inter-instrument norm. 0.70 (0.57–0.86)
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.