5XMM J011523.1-731638

5XMM-DR15 stacked source · SRCID 3001145010104042
Position: 01h15m23.10s -73d16m38.8s (18.84625°, -73.27745°)
EP flux
1.45e-14 ± 3.4e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.767)
Detections
17

SRCID 3001145010104042
IAUNAME 5XMM J011523.1-731638
SC_RA 01h15m23.10s (18.84625°)
SC_DEC -73d16m38.8s (-73.27745°)
RADEC_ERR 1.97 arcsec
LII / BII 300.5513° / -43.7399°
N_CONTRIB 17 (detections)
N_OBS 182 (observations covering the position)
MJD_FIRST 52060.097 (2001-05-31 02:20:10.000 UTC)
MJD_LAST 59708.768 (2022-05-09 18:26:09.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.45e-14 ± 3.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.13 ± 5.63
0.2-0.5 / 0.5-1.0 keV
HR2
0.95 ± 0.32
0.5-1.0 / 1.0-2.0 keV
HR3
0.59 ± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.05 ± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 0.1) SUM_FLAG: 2
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 3.43

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
565735
Match probability
0.501
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 20.238 0.082
B
V
Gaia DR3
Source ID
4687165400041945856
Match probability
0.956
Parallax
-0.738 ± 0.527 mas
Proper motion
(2.45, -1.07) mas/yr
Magnitudes
G=20.10, BP=20.17, RP=20.01
CLASSOPT
Class
QSO
Star
0.00
AGN
1.00
Galaxy
0.00

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.