5XMM J140434.1-335737

5XMM-DR15 stacked source · SRCID 3005894030100055
Position: 14h04m34.15s -33d57m37.4s (211.14229°, -33.96040°)
EP flux
1.15e-14 ± 1.8e-15 erg cm-2 s-1
CLASSX
Extragal_XRB (0.396)
Detections
3

SRCID 3005894030100055
IAUNAME 5XMM J140434.1-335737
SC_RA 14h04m34.15s (211.14229°)
SC_DEC -33d57m37.4s (-33.96040°)
RADEC_ERR 0.91 arcsec
LII / BII 319.8343° / 26.4997°
N_CONTRIB 3 (detections)
N_OBS 6 (observations covering the position)
MJD_FIRST 52319.337 (2002-02-14 08:05:21.000 UTC)
MJD_LAST 57771.720 (2017-01-18 17:16:38.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.15e-14 ± 1.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.85 ± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.26 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.35 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.84 ± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 39.7) SUM_FLAG: 1
Long-term lightcurve

Extragal_XRB

CLASSX outlier: 4.58

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
3605810
Match probability
0.822
FilterMag (AB)Err
UVW2 — —
UVM2 20.548 0.089
UVW1 17.782 0.012
U 16.493 0.015
B — —
V — —
Gaia DR3
Source ID
6122512615305459456
Match probability
0.993
Magnitudes
G=18.07, BP=15.63, RP=14.19
AllWISE
Name
J140434.31-335738.5
Match probability
0.996
BandMagErr
W1 10.474 0.022
W2 10.507 0.021
W3 9.983 0.043
W4 8.620 0.416
CLASSOPT
Class
Star
Star
0.56
AGN
0.01
Galaxy
0.43

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.14e-14 (+1.3e-14 / −1.1e-14) erg cm−2 s−1
NH 2.06e+21 (+2.4e+21 / −1.7e+21) cm−2
Photon index (Γ) 2.84 (+2.96 / −2.63)
DoF 321
p-value 0.231
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.