5XMM J001432.9-302801

5XMM-DR15 stacked source · SRCID 3004234010100078
Position: 00h14m32.92s -30d28m01.9s (3.63717°, -30.46719°)
EP flux
2.50e-15 ± 9.3e-16 erg cm-2 s-1
CLASSX
Bkg_AGN (0.492)
Detections
2

SRCID 3004234010100078
IAUNAME 5XMM J001432.9-302801
SC_RA 00h14m32.92s (3.63717°)
SC_DEC -30d28m01.9s (-30.46719°)
RADEC_ERR 0.99 arcsec
LII / BII 8.3048° / -81.2596°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52059.831 (2001-05-30 19:57:00.000 UTC)
MJD_LAST 57011.090 (2014-12-20 02:09:28.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.50e-15 ± 9.3e-16 erg cm-2 s-1

Hardness ratios
HR1
0.50 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.64 ± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.96 ± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
0.73 ± 1.57
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 0.2) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 3.42

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
21680
Match probability
0.883
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 20.990 0.245
AllWISE
Name
J001432.77-302801.7
Match probability
0.994
BandMagErr
W1 15.528 0.042
W2 15.416 0.099
W3 12.651 —
W4 9.216 —
CLASSOPT
Class
Galaxy
Star
0.30
AGN
0.05
Galaxy
0.65

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 3.62e-15 (+4.5e-15 / −3.0e-15) erg cm−2 s−1
NH 1.03e+20 (+4.2e+20 / −2.3e+19) cm−2
Photon index (Γ) 2.62 (+2.85 / −2.33)
DoF 195
p-value 0.439
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.