5XMM J124932.1-412009

5XMM-DR15 stacked source · SRCID 3004634010100387
Position: 12h49m32.18s -41d20m09.5s (192.38407°, -41.33597°)
EP flux
2.35e-15 ± 1.1e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.611)
Detections
9

SRCID 3004634010100387
IAUNAME 5XMM J124932.1-412009
SC_RA 12h49m32.18s (192.38407°)
SC_DEC -41d20m09.5s (-41.33597°)
RADEC_ERR 1.62 arcsec
LII / BII 302.5482° / 21.5344°
N_CONTRIB 9 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52277.006 (2002-01-03 00:08:36.000 UTC)
MJD_LAST 58666.366 (2019-07-02 08:46:52.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.35e-15 ± 1.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.85 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.79 ± 0.21
0.5-1.0 / 1.0-2.0 keV
HR3
-0.65 ± 0.77
1.0-2.0 / 2.0-4.5 keV
HR4
0.60 ± 0.80
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 3.54

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
3306553
Match probability
0.971
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.014 0.099
U — —
B — —
V — —
Gaia DR3
Source ID
6139978529312544640
Match probability
0.989
Magnitudes
G=20.31, BP=18.80, RP=17.16
CLASSOPT
Class
Galaxy
Star
0.09
AGN
0.01
Galaxy
0.90

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 2.42e-14 (+2.9e-14 / −2.0e-14) erg cm−2 s−1
NH 2.61e+21 (+3.3e+21 / −1.8e+21) cm−2
Photon index (Γ) 2.44 (+2.73 / −2.07)
DoF 498
p-value 0.414
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.