5XMM J124922.0-055950

5XMM-DR15 stacked source · SRCID 3006037020100049
Position: 12h49m22.07s -05d59m50.3s (192.34198°, -5.99731°)
EP flux
1.66e-14 ± 2.1e-15 erg cm-2 s-1
CLASSX
AGN (0.924)
Detections
2

SRCID 3006037020100049
IAUNAME 5XMM J124922.0-055950
SC_RA 12h49m22.07s (192.34198°)
SC_DEC -05d59m50.3s (-5.99731°)
RADEC_ERR 0.41 arcsec
LII / BII 301.9902° / 56.8707°
N_CONTRIB 2 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52101.640 (2001-07-11 15:22:08.000 UTC)
MJD_LAST 53201.820 (2004-07-15 19:41:14.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.66e-14 ± 2.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.12 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.30 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.67 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.641

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
3305261
Match probability
0.998
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 23.367 0.218
U — —
B — —
V — —

Photometric (TPZ) 0.4759 (conf 0.70)
Photometric (Le Phare) 0.4908 (conf 0.96)

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

Stacked power-law fit
Unabsorbed flux 2.90e-14 (+3.3e-14 / −2.4e-14) erg cm−2 s−1
NH 4.71e+19 (+1.8e+20 / −1.6e+19) cm−2
Photon index (Γ) 1.66 (+1.78 / −1.53)
DoF 502
p-value 0.637
Inter-instrument norm. 1.11 (0.98–1.30)
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.