5XMM J120128.9-032742

5XMM-DR15 stacked source · SRCID 3005602070100051
Position: 12h01m28.95s -03d27m42.2s (180.37064°, -3.46173°)
EP flux
1.83e-14 ± 5.6e-15 erg cm-2 s-1
CLASSX
AGN (0.925)
Detections
4

SRCID 3005602070100051
IAUNAME 5XMM J120128.9-032742
SC_RA 12h01m28.95s (180.37064°)
SC_DEC -03d27m42.2s (-3.46173°)
RADEC_ERR 0.77 arcsec
LII / BII 279.5030° / 57.1201°
N_CONTRIB 4 (detections)
N_OBS 5 (observations covering the position)
MJD_FIRST 52254.813 (2001-12-11 19:30:15.000 UTC)
MJD_LAST 58487.542 (2019-01-04 13:00:41.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.83e-14 ± 5.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.15 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.26 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.61 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.19 ± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.625

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
3128247
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.681 0.160
U — —
B — —
V — —
AllWISE
Name
J120128.97-032741.4
Match probability
0.995
BandMagErr
W1 16.746 0.103
W2 16.360 0.281
W3 12.176 —
W4 8.744 —
CLASSOPT
Class
QSO
Star
0.06
AGN
0.58
Galaxy
0.36

Photometric (TPZ) 0.6758 (conf 0.35)
Photometric (Le Phare) 0.8821 (conf 0.69)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Stacked power-law fit
Unabsorbed flux 1.21e-14 (+1.7e-14 / −8.5e-15) erg cm−2 s−1
NH 1.70e+20 (+1.1e+21 / −2.3e+19) cm−2
Photon index (Γ) 1.82 (+2.26 / −1.48)
DoF 46
p-value 0.321
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.