5XMM J004144.5-092825

5XMM-DR15 stacked source · SRCID 3006514010100054
Position: 00h41m44.54s -09d28m25.1s (10.43560°, -9.47363°)
EP flux
3.12e-14 ± 5.0e-15 erg cm-2 s-1
CLASSX
AGN (0.938)
Detections
3

SRCID 3006514010100054
IAUNAME 5XMM J004144.5-092825
SC_RA 00h41m44.54s (10.43560°)
SC_DEC -09d28m25.1s (-9.47363°)
RADEC_ERR 0.63 arcsec
LII / BII 115.0899° / -72.1976°
N_CONTRIB 3 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 52281.557 (2002-01-07 13:21:35.000 UTC)
MJD_LAST 56462.381 (2013-06-19 09:08:46.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.12e-14 ± 5.0e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.51 ± 0.39
0.2-0.5 / 0.5-1.0 keV
HR2
0.96 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.07 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.329

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
121935
Match probability
0.992
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.891 0.173
B — —
V — —
AllWISE
Name
J004144.67-092826.4
Match probability
0.995
BandMagErr
W1 16.989 0.121
W2 15.980 0.198
W3 12.527 0.509
W4 8.906 —
CLASSOPT
Class
QSO
Star
0.00
AGN
1.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.59e-14 (+2.1e-14 / −1.0e-14) erg cm−2 s−1
NH 9.18e+21 (+1.6e+22 / −3.9e+21) cm−2
Photon index (Γ) 2.08 (+2.74 / −1.39)
DoF 417
p-value 0.482
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.