5XMM J140606.0+222018

5XMM-DR15 stacked source · SRCID 3005176020100039
Position: 14h06m06.06s +22d20m18.5s (211.52525°, 22.33847°)
EP flux
1.26e-14 ± 3.8e-15 erg cm-2 s-1
CLASSX
AGN (0.912)
Detections
2

SRCID 3005176020100039
IAUNAME 5XMM J140606.0+222018
SC_RA 14h06m06.06s (211.52525°)
SC_DEC +22d20m18.5s (22.33847°)
RADEC_ERR 0.61 arcsec
LII / BII 21.2298° / 72.4034°
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): 1.26e-14 ± 3.8e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.01 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.14 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.85 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.32 ± 0.66
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.1) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.498

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
3611282
Match probability
0.975
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.015 0.150
U — —
B — —
V — —
AllWISE
Name
J140606.11+222019.8
Match probability
0.995
BandMagErr
W1 16.261 0.055
W2 16.252 0.157
W3 12.629 0.430
W4 8.983 —
CLASSOPT
Class
Star
Star
0.95
AGN
0.00
Galaxy
0.05

Photometric (TPZ) 0.7258 (conf 0.69)
Photometric (Le Phare) 0.6699 (conf 0.95)

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

Stacked power-law fit
Unabsorbed flux 1.85e-14 (+2.9e-14 / −1.1e-14) erg cm−2 s−1
NH 1.09e+20 (+5.4e+20 / −2.4e+19) cm−2
Photon index (Γ) 1.55 (+1.96 / −1.21)
DoF 680
p-value 0.208
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.