5XMM J034118.1-011110

5XMM-DR15 stacked source · SRCID 3000294040100003
Position: 03h41m18.14s -01d11m10.4s (55.32559°, -1.18622°)
EP flux
1.05e-13 ± 2.2e-14 erg cm-2 s-1
CLASSX
AGN (0.881)
Detections
2

SRCID 3000294040100003
IAUNAME 5XMM J034118.1-011110
SC_RA 03h41m18.14s (55.32559°)
SC_DEC -01d11m10.4s (-1.18622°)
RADEC_ERR 0.54 arcsec
LII / BII 187.7155° / -41.7455°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52302.856 (2002-01-28 20:33:21.000 UTC)
MJD_LAST 53026.876 (2004-01-22 21:00:55.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.05e-13 ± 2.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.38 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.23 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.11 ± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.312

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
999022
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.270 0.170
U
B
V

Spectroscopic (zsp) 0.27700
Photometric (TPZ) 0.3259 (conf 0.76)
Photometric (Le Phare) 0.2488 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 8.80e-14 (+1.1e-13 / −6.9e-14) erg cm−2 s−1
NH 2.24e+20 (+9.1e+20 / −3.0e+19) cm−2
Photon index (Γ) 1.40 (+1.69 / −1.21)
DoF 121
p-value 0.908
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.