2001A&A...374.1161A


Query : 2001A&A...374.1161A

2001A&A...374.1161A - Astronomy and Astrophysics, volume 3741161-1168 (2001/8-2)

The achromatic phase knife coronagraph.

ABE L., VAKILI F. and BOCCALETTI A.

Abstract (from CDS):

We present the concept of a nulling coronagraph which theoretically attains the brightness ratio of 108 suitable to directly detect exo-Earths in the vicinity of their parent stars. The concept is derived from the classical Foucault's optics test and Zernike's self-destructive phase contrast principle. We propose an achromatic set-up which should dramatically improve its wide band efficiency. The whole system is simulated against a numerical model which validates a formal analytical approach. The coronagraph is then compared to other concepts and its advantages and shortcomings are outlined, suggesting future laboratory developments and tests on the sky.

Abstract Copyright: ∼

Journal keyword(s): techniques: interferometric - stars: binaries: close - stars: planetary systems

Simbad objects: 1

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Number of rows : 1
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 * 51 Peg b Pl 22 57 27.9804852576 +20 46 07.797040104           ~ 744 1

Query : 2001A&A...374.1161A

Basic data :
* 51 Peg b -- Extra-solar Planet
Other object types:
otypes_help
Pl? (), * (*,HD), Pl (1995Natur)
ICRS coord. (ep=J2000) :
22 57 27.9804852576 +20 46 07.797040104 (Optical) [ 0.0535 0.0543 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
22 55 00.3824419857 +20 30 01.119685421 [ 0.0535 0.0543 90 ]
Gal coord. (ep=J2000) :
090.0626441289023 -34.7272597942784 [ 0.0535 0.0543 90 ]
Proper motions mas/yr :
207.328 61.164 [0.088 0.075 90] A 2020yCat.1350....0G
Parallaxes (mas):
64.4048 [0.0771] A 2020yCat.1350....0G
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

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Identifiers (3) :
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* 51 Peg b HD 217014b NAME Dimidium

References (744 between 1850 and 2026) (Total 744)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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HD 217014b

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