5XMM J150655.0+012944

5XMM-DR15 stacked source · SRCID 3002154010100042
Position: 15h06m55.07s +01d29m44.0s (226.72947°, 1.49555°)
EP flux
1.49e-14 ± 2.3e-15 erg cm-2 s-1
CLASSX
AGN (0.899)
Detections
5

SRCID 3002154010100042
IAUNAME 5XMM J150655.0+012944
SC_RA 15h06m55.07s (226.72947°)
SC_DEC +01d29m44.0s (1.49555°)
RADEC_ERR 0.42 arcsec
LII / BII 0.4083° / 48.6432°
N_CONTRIB 5 (detections)
N_OBS 5 (observations covering the position)
MJD_FIRST 51934.595 (2001-01-25 14:16:08.000 UTC)
MJD_LAST 56679.394 (2014-01-22 09:26:40.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.49e-14 ± 2.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.36 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.15 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.36 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.23 ± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.49

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
3853919
Match probability
0.996
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 21.406 0.160
B
V

Photometric (TPZ) 0.3259 (conf 0.50)
Photometric (Le Phare) 2.0350 (conf 0.15)

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

Stacked power-law fit
Unabsorbed flux 1.47e-14 (+1.7e-14 / −1.2e-14) erg cm−2 s−1
NH 6.03e+20 (+1.4e+21 / −7.8e+19) cm−2
Photon index (Γ) 1.87 (+2.20 / −1.65)
DoF 295
p-value 0.512
Inter-instrument norm. 1.30 (1.09–1.54)
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.