5XMM J044726.9-063327

5XMM-DR15 stacked source · SRCID 3001474060100012
Position: 04h47m26.94s -06d33m27.1s (71.86225°, -6.55754°)
EP flux
4.91e-14 ± 8.7e-15 erg cm-2 s-1
CLASSX
AGN (0.909)
Detections
2

SRCID 3001474060100012
IAUNAME 5XMM J044726.9-063327
SC_RA 04h47m26.94s (71.86225°)
SC_DEC -06d33m27.1s (-6.55754°)
RADEC_ERR 0.44 arcsec
LII / BII 204.1435° / -30.4919°
N_CONTRIB 2 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52525.021 (2002-09-08 00:30:04.000 UTC)
MJD_LAST 53975.011 (2006-08-28 00:16:07.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.91e-14 ± 8.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.44 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.17 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.32 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.177

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
1093619
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.283 0.279
U
B
V

Photometric (TPZ) 1.1257 (conf 0.67)
Photometric (Le Phare) 1.0400 (conf 0.21)

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

Stacked power-law fit
Unabsorbed flux 6.80e-14 (+8.1e-14 / −5.7e-14) erg cm−2 s−1
NH 9.52e+20 (+1.7e+21 / −2.0e+20) cm−2
Photon index (Γ) 1.96 (+2.31 / −1.64)
DoF 474
p-value 0.016
Inter-instrument norm. 0.51 (0.50–0.54)
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.