5XMM J004154.6-092127

5XMM-DR15 stacked source · SRCID 3006514010100163
Position: 00h41m54.66s -09d21m27.4s (10.47775°, -9.35762°)
EP flux
4.13e-14 ± 3.9e-15 erg cm-2 s-1
CLASSX
Extended (1)
Detections
3

SRCID 3006514010100163
IAUNAME 5XMM J004154.6-092127
SC_RA 00h41m54.66s (10.47775°)
SC_DEC -09d21m27.4s (-9.35762°)
RADEC_ERR 4.49 arcsec
LII / BII 115.2705° / -72.0875°
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): 4.13e-14 ± 3.9e-15 erg cm-2 s-1

Hardness ratios
HR1
1.00 ± 0.26
0.2-0.5 / 0.5-1.0 keV
HR2
0.96 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.58 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00 ± 0.02
2.0-4.5 / 4.5-12.0 keV
Extent: 29.90 ± 1.94 arcsec (ML 55.5) SUM_FLAG: 4
Long-term lightcurve

Extended

CLASSX outlier: 2.01

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
123994
Match probability
0.865
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.246 0.104
B 20.491 0.070
V 19.385 0.058
AllWISE
Name
J004154.65-092131.9
Match probability
0.996
BandMagErr
W1 16.116 0.062
W2 16.575 0.311
W3 12.477 —
W4 8.855 —
CLASSOPT
Class
Star
Star
0.94
AGN
0.00
Galaxy
0.06

No redshift estimate available for this source.

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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.