5XMM J124925.9-412542

5XMM-DR15 stacked source · SRCID 3004634010100024
Position: 12h49m25.99s -41d25m42.7s (192.35830°, -41.42853°)
EP flux
6.61e-14 ± 2.3e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.706)
Detections
9

SRCID 3004634010100024
IAUNAME 5XMM J124925.9-412542
SC_RA 12h49m25.99s (192.35830°)
SC_DEC -41d25m42.7s (-41.42853°)
RADEC_ERR 0.11 arcsec
LII / BII 302.5282° / 21.4417°
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): 6.61e-14 ± 2.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.34 ± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.09 ± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44 ± 0.04
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.9) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 1.88

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
3305795
Match probability
0.992
FilterMag (AB)Err
UVW2 21.539 0.142
UVM2 20.965 0.123
UVW1 20.591 0.056
U — —
B — —
V — —
Gaia DR3
Source ID
6139977532878284928
Match probability
0.99
Parallax
-0.738 ± 0.639 mas
Proper motion
(-0.08, -1.36) mas/yr
Magnitudes
G=20.33, BP=20.40, RP=19.40
CLASSOPT
Class
QSO
Star
0.00
AGN
0.86
Galaxy
0.13

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 7.20e-14 (+7.6e-14 / −6.9e-14) erg cm−2 s−1
NH 6.75e+20 (+8.5e+20 / −4.9e+20) cm−2
Photon index (Γ) 1.99 (+2.07 / −1.90)
DoF 1276
p-value 0.992
Inter-instrument norm. 1.07 (1.01–1.13)
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.