5XMM J004217.7-093949

5XMM-DR15 stacked source · SRCID 3006514020100036
Position: 00h42m17.78s -09d39m49.5s (10.57409°, -9.66376°)
EP flux
2.20e-13 ± 1.6e-14 erg cm-2 s-1
CLASSX
AGN (0.812)
Detections
1

SRCID 3006514020100036
IAUNAME 5XMM J004217.7-093949
SC_RA 00h42m17.78s (10.57409°)
SC_DEC -09d39m49.5s (-9.66376°)
RADEC_ERR 0.34 arcsec
LII / BII 115.4606° / -72.4028°
N_CONTRIB 1 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 52281.739 (2002-01-07 17:43:45.000 UTC)
MJD_LAST 52281.884 (2002-01-07 21:12:30.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.20e-13 ± 1.6e-14 erg cm-2 s-1

Hardness ratios
HR1
0.24 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.01 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.45 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.34 ± 0.09
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.3) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.818

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
130154
Match probability
0.995
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 19.959 0.181

Spectroscopic (zsp) 0.58000
Photometric (TPZ) 0.6258 (conf 0.61)
Photometric (Le Phare) 1.9160 (conf 0.93)

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

Stacked power-law fit
Unabsorbed flux 1.49e-13 (+1.7e-13 / −1.3e-13) erg cm−2 s−1
NH 5.78e+19 (+2.3e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.88 (+2.03 / −1.76)
DoF 227
p-value 0.805
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.