5XMM J011130.3-381126

5XMM-DR15 stacked source · SRCID 3000294230100065
Position: 01h11m30.30s -38d11m26.8s (17.87625°, -38.19078°)
EP flux
2.41e-14 ± 5.8e-15 erg cm-2 s-1
CLASSX
Extended (1)
Detections
2

SRCID 3000294230100065
IAUNAME 5XMM J011130.3-381126
SC_RA 01h11m30.30s (17.87625°)
SC_DEC -38d11m26.8s (-38.19078°)
RADEC_ERR 6.57 arcsec
LII / BII 283.3542° / -78.1640°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52253.198 (2001-12-10 04:44:57.000 UTC)
MJD_LAST 54809.311 (2008-12-09 07:28:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.41e-14 ± 5.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.80 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.36 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39 ± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73 ± 0.32
2.0-4.5 / 4.5-12.0 keV
Extent: 35.50 ± 3.11 arcsec (ML 35.4) SUM_FLAG: 1
Long-term lightcurve

Extended

CLASSX outlier: 2.32

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
540952
Match probability
0.53
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.498 0.181
U 21.206 0.131
B 20.260 0.064
V 18.730 0.046
Gaia DR3
Source ID
4988793703320088192
Match probability
0.99
Magnitudes
G=20.77, BP=19.60, RP=17.94
AllWISE
Name
J011130.78-381122.4
Match probability
0.995
BandMagErr
W1 14.526 0.029
W2 14.241 0.043
W3 12.694 0.541
W4 8.652
CLASSOPT
Class
Galaxy
Star
0.03
AGN
0.00
Galaxy
0.97

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.