2019MNRAS.488.3262C


Query : 2019MNRAS.488.3262C

2019MNRAS.488.3262C - Mon. Not. R. Astron. Soc., 488, 3262-3267 (2019/September-3)

Planetary system detection by estimating the covariance of coronagraphic lucky images.

CAGIGAS M.A., CAGIGAL M.P., VALLE P.J., CANALES V.F., FUENTES A. and LOPEZ R.

Abstract (from CDS):

In this paper, we review two different methods to increase image contrast and propose the combination of both to detect faint companions surrounding a host star. Coronagraphy allows us to block light coming from the host star so that the residual star light can be reduced by several orders of magnitude. On the other hand, estimating the Covariance of Lucky Images (COELI) is a proven method to detect faint companions from ground-based telescope images. The dynamic range of the detection camera limits this technique. Hence, the application of COELI to coronagraphic images may increase the magnitude range of the detectable companions. COELI only requires the existence of a reference, which can be obtained using an existing stellar companion or using a coronagraphic mask designed to create a faint image of the host star. We provide an analysis of the combination of the techniques by processing coronagraphic images obtained by the William Herschel Telescope.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: statistical - techniques: image processing - telescopes

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 * bet Tri SB* 02 09 32.62712 +34 59 14.2694 3.26 3.14 3.00 2.86 2.78 A5III 230 0
2 HD 77407 PM* 09 03 27.0837288552 +37 50 27.493558584   7.63 7.04     G0V 110 0
3 HD 112196 PM* 12 54 40.0155713280 +22 06 28.557915876   7.54 7.00 7.950   F8V 71 0
4 HD 179070 Er* 19 09 26.8349590368 +38 42 50.455534860   8.767 8.25 8.00   F6IV 200 1
5 * del Equ SB* 21 14 28.8153077 +10 00 25.125878 4.98 4.99 4.49 4.06 3.78 F7(V)+G0(V) 331 0

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