5XMM J001543.7-391529

5XMM-DR15 stacked source · SRCID 3002874010100280
Position: 00h15m43.72s -39d15m29.0s (3.93216°, -39.25807°)
EP flux
1.46e-15 ± 4.7e-16 erg cm-2 s-1
CLASSX
Bkg_AGN (0.663)
Detections
10

SRCID 3002874010100280
IAUNAME 5XMM J001543.7-391529
SC_RA 00h15m43.72s (3.93216°)
SC_DEC -39d15m29.0s (-39.25807°)
RADEC_ERR 0.94 arcsec
LII / BII 332.1993° / -75.7722°
N_CONTRIB 10 (detections)
N_OBS 10 (observations covering the position)
MJD_FIRST 52227.605 (2001-11-14 14:31:49.000 UTC)
MJD_LAST 59561.812 (2021-12-13 19:29:06.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.46e-15 ± 4.7e-16 erg cm-2 s-1

Hardness ratios
HR1
0.84 ± 0.36
0.2-0.5 / 0.5-1.0 keV
HR2
0.50 ± 0.20
0.5-1.0 / 1.0-2.0 keV
HR3
-0.07 ± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.74 ± 0.22
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.6) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 3.1

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
24894
Match probability
0.974
FilterMag (AB)Err
UVW2 19.765 0.056
UVM2 19.501 0.030
UVW1 19.038 0.016
U 19.501 0.059
B 19.722 0.098
V 19.680 0.080
Gaia DR3
Source ID
4997969952486225920
Match probability
0.983
Magnitudes
G=20.65, BP=19.95, RP=20.03
CLASSOPT
Class
QSO
Star
0.00
AGN
0.90
Galaxy
0.10

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.