5XMM J044751.0-063239

5XMM-DR15 stacked source · SRCID 3001474060100041
Position: 04h47m51.01s -06d32m39.1s (71.96254°, -6.54419°)
EP flux
7.02e-15 ± 2.8e-15 erg cm-2 s-1
CLASSX
AGN (0.868)
Detections
2

SRCID 3001474060100041
IAUNAME 5XMM J044751.0-063239
SC_RA 04h47m51.01s (71.96254°)
SC_DEC -06d32m39.1s (-6.54419°)
RADEC_ERR 1.01 arcsec
LII / BII 204.1835° / -30.3974°
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): 7.02e-15 ± 2.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.06 ± 0.25
0.2-0.5 / 0.5-1.0 keV
HR2
0.57 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.73 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.26 ± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.7) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.236

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
1096530
Match probability
0.987
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.530 0.182
U
B
V

Photometric (TPZ) 0.2759 (conf 0.73)
Photometric (Le Phare) 0.4520 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 3.60e-14 (+4.6e-14 / −2.7e-14) erg cm−2 s−1
NH 9.68e+20 (+2.5e+21 / −1.2e+20) cm−2
Photon index (Γ) 1.46 (+1.91 / −1.16)
DoF 469
p-value 0.587
Inter-instrument norm. 1.49 (1.20–1.78)
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.