5XMM J125857.7-691133

5XMM-DR15 stacked source · SRCID 3006074010100116
Position: 12h58m57.78s -69d11m33.3s (194.74074°, -69.19258°)
EP flux
4.98e-15 ± 4.3e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.615)
Detections
5

SRCID 3006074010100116
IAUNAME 5XMM J125857.7-691133
SC_RA 12h58m57.78s (194.74074°)
SC_DEC -69d11m33.3s (-69.19258°)
RADEC_ERR 1.76 arcsec
LII / BII 303.6042° / -6.3307°
N_CONTRIB 5 (detections)
N_OBS 5 (observations covering the position)
MJD_FIRST 51931.640 (2001-01-22 15:22:00.000 UTC)
MJD_LAST 54168.861 (2007-03-09 20:39:44.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.98e-15 ± 4.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.70 ± 0.31
0.2-0.5 / 0.5-1.0 keV
HR2
0.24 ± 0.29
0.5-1.0 / 1.0-2.0 keV
HR3
-0.90 ± 0.47
1.0-2.0 / 2.0-4.5 keV
HR4
0.75 ± 1.04
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.8) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 3.73

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
3359662
Match probability
0.709
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 19.499 0.067
Gaia DR3
Source ID
5844940385184379264
Match probability
0.984
Parallax
0.580 ± 0.267 mas
Proper motion
(-1.76, -2.71) mas/yr
Magnitudes
G=19.40, BP=19.98, RP=18.64
CLASSOPT
Class
Star
Star
0.88
AGN
0.12
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.