5XMM J001348.2-302107

5XMM-DR15 stacked source · SRCID 3004234010100023
Position: 00h13m48.28s -30d21m07.7s (3.45115°, -30.35213°)
EP flux
2.31e-14 ± 2.7e-15 erg cm-2 s-1
CLASSX
AGN (0.905)
Detections
2

SRCID 3004234010100023
IAUNAME 5XMM J001348.2-302107
SC_RA 00h13m48.28s (3.45115°)
SC_DEC -30d21m07.7s (-30.35213°)
RADEC_ERR 0.29 arcsec
LII / BII 9.3655° / -81.1470°
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): 2.31e-14 ± 2.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.09 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.11 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.41 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.209

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
20098
Match probability
0.986
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 21.188 0.172
AllWISE
Name
J001348.36-302107.7
Match probability
0.994
BandMagErr
W1 17.291 0.152
W2 16.692 0.330
W3 12.293 —
W4 8.774 —
CLASSOPT
Class
QSO
Star
0.00
AGN
0.67
Galaxy
0.33

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 2.83e-14 (+3.1e-14 / −2.6e-14) erg cm−2 s−1
NH 2.75e+19 (+7.7e+19 / −1.4e+19) cm−2
Photon index (Γ) 1.97 (+2.06 / −1.89)
DoF 433
p-value 0.332
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.