5XMM J142832.7-624013

5XMM-DR15 stacked source · SRCID 3004935010100022
Position: 14h28m32.71s -62d40m13.8s (217.13628°, -62.67049°)
EP flux
1.52e-14 ± 2.8e-15 erg cm-2 s-1
CLASSX
Gal_XRB (0.887)
Detections
8

SRCID 3004935010100022
IAUNAME 5XMM J142832.7-624013
SC_RA 14h28m32.71s (217.13628°)
SC_DEC -62d40m13.8s (-62.67049°)
RADEC_ERR 0.41 arcsec
LII / BII 313.8182° / -1.8693°
N_CONTRIB 8 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 52133.167 (2001-08-12 04:00:28.000 UTC)
MJD_LAST 58189.108 (2018-03-12 02:36:13.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.52e-14 ± 2.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.58 ± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
0.82 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.46 ± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 12.0) SUM_FLAG: 1
Long-term lightcurve

Gal_XRB

CLASSX outlier: 3.83

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
3700524
Match probability
0.968
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 19.100 0.015
B — —
V — —
Gaia DR3
Source ID
5853509777005620480
Match probability
0.975
Magnitudes
G=20.00, BP=19.98, RP=18.73
CLASSOPT
Class
Star
Star
0.84
AGN
0.00
Galaxy
0.16

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 2.60e-14 (+3.1e-14 / −2.2e-14) erg cm−2 s−1
NH 4.61e+21 (+6.5e+21 / −3.2e+21) cm−2
Photon index (Γ) 2.01 (+2.41 / −1.66)
DoF 165
p-value 0.756
Inter-instrument norm. 1.08 (0.87–1.37)
Quality flag 0

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.