5XMM J044813.8-062032

5XMM-DR15 stacked source · SRCID 3001474060100061
Position: 04h48m13.84s -06d20m32.3s (72.05765°, -6.34229°)
EP flux
9.21e-15 ± 3.7e-15 erg cm-2 s-1
CLASSX
AGN (0.943)
Detections
3

SRCID 3001474060100061
IAUNAME 5XMM J044813.8-062032
SC_RA 04h48m13.84s (72.05765°)
SC_DEC -06d20m32.3s (-6.34229°)
RADEC_ERR 0.90 arcsec
LII / BII 204.0275° / -30.2198°
N_CONTRIB 3 (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): 9.21e-15 ± 3.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.71 ± 0.18
0.2-0.5 / 0.5-1.0 keV
HR2
0.28 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.22 ± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.61 ± 0.30
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.414

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
1100034
Match probability
0.985
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.545 0.348
U
B
V

Photometric (TPZ) 2.0754 (conf 0.56)
Photometric (Le Phare) 1.5350 (conf 0.40)

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

Stacked power-law fit
Unabsorbed flux 2.20e-14 (+2.7e-14 / −1.7e-14) erg cm−2 s−1
NH 6.06e+20 (+1.6e+21 / −5.2e+19) cm−2
Photon index (Γ) 1.29 (+1.66 / −1.10)
DoF 429
p-value 0.228
Inter-instrument norm. 0.86 (0.66–1.13)
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.