5XMM J092746.6-060417

5XMM-DR15 stacked source · SRCID 3003234030100001
Position: 09h27m46.67s -06d04m17.6s (141.94444°, -6.07155°)
EP flux
1.78e-13 ± 8.3e-16 erg cm-2 s-1
CLASSX
AGN (0.334)
Detections
44

SRCID 3003234030100001
IAUNAME 5XMM J092746.6-060417
SC_RA 09h27m46.67s (141.94444°)
SC_DEC -06d04m17.6s (-6.07155°)
RADEC_ERR 0.03 arcsec
LII / BII 239.1442° / 30.6462°
N_CONTRIB 44 (detections)
N_OBS 44 (observations covering the position)
MJD_FIRST 52024.899 (2001-04-25 21:34:09.000 UTC)
MJD_LAST 59330.183 (2021-04-26 04:22:48.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.78e-13 ± 8.3e-16 erg cm-2 s-1

Hardness ratios
HR1
0.49 ± 0.00
0.2-0.5 / 0.5-1.0 keV
HR2
-0.75 ± 0.00
0.5-1.0 / 1.0-2.0 keV
HR3
-0.98 ± 0.00
1.0-2.0 / 2.0-4.5 keV
HR4
-0.53 ± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -5.9) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.914

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
2747329
Match probability
1
FilterMag (AB)Err
UVW2 11.020 0.001
UVM2 10.795 0.000
UVW1
U
B
V
Gaia DR3
Source ID
5745464991235898752
Match probability
0.966
Parallax
32.299 ± 0.360 mas
Proper motion
(-242.63, -52.65) mas/yr
Magnitudes
G=5.16, BP=5.54, RP=4.69
AllWISE
Name
J092746.61-060416.9
Match probability
0.989
BandMagErr
W1 3.751 0.501
W2 3.482 0.267
W3 3.766 0.015
W4 3.706 0.028
CLASSOPT
Class
Star
Star
0.98
AGN
0.01
Galaxy
0.01

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.

APPROX_SOURCE_VAR 20.100 (approximate flux variability amplitude)

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.