5XMM J142847.1-624022

5XMM-DR15 stacked source · SRCID 3004935010100021
Position: 14h28m47.12s -62d40m22.6s (217.19635°, -62.67293°)
EP flux
9.90e-15 ± 2.0e-15 erg cm-2 s-1
CLASSX
Star (1)
Detections
8

SRCID 3004935010100021
IAUNAME 5XMM J142847.1-624022
SC_RA 14h28m47.12s (217.19635°)
SC_DEC -62d40m22.6s (-62.67293°)
RADEC_ERR 0.50 arcsec
LII / BII 313.8430° / -1.8817°
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): 9.90e-15 ± 2.0e-15 erg cm-2 s-1

Hardness ratios
HR1
0.13 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.51 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.80 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
0.38 ± 0.43
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.4) SUM_FLAG: 1
Long-term lightcurve

Star

CLASSX outlier: 3.48

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
3701678
Match probability
0.887
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 17.694 0.004
B — —
V — —
Gaia DR3
Source ID
5853497991626386944
Match probability
0.986
Parallax
12.681 ± 0.062 mas
Proper motion
(16.07, -51.68) mas/yr
Magnitudes
G=13.77, BP=14.93, RP=12.69
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.08e-14 (+1.3e-14 / −8.8e-15) erg cm−2 s−1
NH 2.30e+20 (+6.7e+20 / −3.5e+19) cm−2
Photon index (Γ) 2.72 (+2.91 / −2.49)
DoF 178
p-value 0.571
Inter-instrument norm. 0.87 (0.70–1.08)
Quality flag 0

APPROX_SOURCE_VAR 6.000 (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.