5XMM J124913.8-055918

5XMM-DR15 stacked source · SRCID 3006037020100019
Position: 12h49m13.83s -05d59m18.7s (192.30764°, -5.98854°)
EP flux
4.72e-14 ± 2.9e-15 erg cm-2 s-1
CLASSX
AGN (0.566)
Detections
3

SRCID 3006037020100019
IAUNAME 5XMM J124913.8-055918
SC_RA 12h49m13.83s (192.30764°)
SC_DEC -05d59m18.7s (-5.98854°)
RADEC_ERR 0.25 arcsec
LII / BII 301.9275° / 56.8789°
N_CONTRIB 3 (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): 4.72e-14 ± 2.9e-15 erg cm-2 s-1

Hardness ratios
HR1
0.37 ± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.29 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.24 ± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.58 ± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.4) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 2.48

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
3304206
Match probability
0.998
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 18.624 0.008
U — —
B — —
V — —

Spectroscopic (zsp) 2.22600
Photometric (TPZ) 2.2754 (conf 0.92)
Photometric (Le Phare) 0.0549 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 4.01e-14 (+4.5e-14 / −3.6e-14) erg cm−2 s−1
NH 9.12e+20 (+1.4e+21 / −4.6e+20) cm−2
Photon index (Γ) 1.81 (+1.99 / −1.63)
DoF 477
p-value 0.995
Inter-instrument norm. 1.04 (0.92–1.17)
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.