5XMM J124900.9-060058

5XMM-DR15 stacked source · SRCID 3006037020100054
Position: 12h49m00.99s -06d00m58.3s (192.25413°, -6.01620°)
EP flux
1.75e-14 ± 2.1e-15 erg cm-2 s-1
CLASSX
AGN (0.92)
Detections
3

SRCID 3006037020100054
IAUNAME 5XMM J124900.9-060058
SC_RA 12h49m00.99s (192.25413°)
SC_DEC -06d00m58.3s (-6.01620°)
RADEC_ERR 0.45 arcsec
LII / BII 301.8310° / 56.8504°
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): 1.75e-14 ± 2.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.11 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.04 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.23 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.65 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.672

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
3302589
Match probability
0.998
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.657 0.049
U — —
B — —
V — —

Photometric (TPZ) 1.7755 (conf 0.46)
Photometric (Le Phare) 1.6400 (conf 0.57)

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

Stacked power-law fit
Unabsorbed flux 1.29e-14 (+1.6e-14 / −1.1e-14) erg cm−2 s−1
NH 1.82e+20 (+7.1e+20 / −2.3e+19) cm−2
Photon index (Γ) 2.16 (+2.49 / −1.92)
DoF 476
p-value 0.851
Inter-instrument norm. 0.79 (0.65–0.98)
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.