5XMM J140620.3+221949

5XMM-DR15 stacked source · SRCID 3005176020100016
Position: 14h06m20.35s +22d19m49.2s (211.58479°, 22.33035°)
EP flux
1.95e-14 ± 3.7e-15 erg cm-2 s-1
CLASSX
AGN (0.664)
Detections
2

SRCID 3005176020100016
IAUNAME 5XMM J140620.3+221949
SC_RA 14h06m20.35s (211.58479°)
SC_DEC +22d19m49.2s (22.33035°)
RADEC_ERR 0.48 arcsec
LII / BII 21.2655° / 72.3488°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52078.071 (2001-06-18 01:41:59.000 UTC)
MJD_LAST 57413.657 (2016-01-26 15:46:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.95e-14 ± 3.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.25 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26 ± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.0316

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
3611967
Match probability
0.839
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.695 0.162
U — —
B — —
V — —
AllWISE
Name
J140620.26+221951.3
Match probability
0.994
BandMagErr
W1 16.553 0.065
W2 16.263 0.175
W3 12.244 —
W4 9.024 —
CLASSOPT
Class
Galaxy
Star
0.40
AGN
0.02
Galaxy
0.58

Photometric (TPZ) 0.6258 (conf 0.73)
Photometric (Le Phare) 0.7540 (conf 0.81)

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

Stacked power-law fit
Unabsorbed flux 2.09e-14 (+2.4e-14 / −1.8e-14) erg cm−2 s−1
NH 8.53e+19 (+3.3e+20 / −2.1e+19) cm−2
Photon index (Γ) 2.32 (+2.53 / −2.15)
DoF 1111
p-value 0.439
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.