5XMM J120047.2-033649

5XMM-DR15 stacked source · SRCID 3005602070100022
Position: 12h00m47.28s -03d36m49.8s (180.19702°, -3.61385°)
EP flux
2.05e-14 ± 4.6e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.991)
Detections
3

SRCID 3005602070100022
IAUNAME 5XMM J120047.2-033649
SC_RA 12h00m47.28s (180.19702°)
SC_DEC -03d36m49.8s (-3.61385°)
RADEC_ERR 0.56 arcsec
LII / BII 279.3050° / 56.9163°
N_CONTRIB 3 (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): 2.05e-14 ± 4.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.75 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.54 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.75 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22 ± 0.57
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 39.7) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.05

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
3126330
Match probability
0.642
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.796 0.201
B — —
V — —
Gaia DR3
Source ID
3600858494582093696
Match probability
0.981
Magnitudes
G=21.32, BP=19.33, RP=17.45
AllWISE
Name
J120047.23-033647.6
Match probability
0.995
BandMagErr
W1 13.664 0.026
W2 13.358 0.031
W3 12.009 0.336
W4 8.542 —
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.00
Galaxy
1.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.18e-14 (+1.5e-14 / −9.1e-15) erg cm−2 s−1
NH 3.17e+20 (+1.1e+21 / −3.9e+19) cm−2
Photon index (Γ) 2.67 (+2.90 / −2.35)
DoF 62
p-value 0.251
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.