1999
DOI: 10.1364/ao.38.007128
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Deep nulling of visible laser light

Abstract: Nulling interferometry, a proposed technique for dimming a star relative to its surroundings by destructively interfering the light collected by two individual telescopes [Bracewell, Nature 274, 780-781 (1978); Shao and Colavita, Ann. Rev. Astron. Astrophys. 30, 457-498 (1992)], has the potential to permit the direct detection of nearby extrasolar planets. However, because of the extremely high degree of symmetry required for useful levels of starlight nulling, the technique remains in its infancy. We present … Show more

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Cited by 43 publications
(29 citation statements)
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“…To our knowledge, the best nulls in a tabletop setup reported in the literature were achieved by astronomers for the cancellation of star light to detect light from planets nearby. [27][28][29] Besides a special geometrical design, these nulls were achieved by actively controlling the optical path length difference, x OPD , using a piezotransducer attached to a mirror of one interferometer arm. When all optical elements are perfect, the nulling depth, D, as function of the optical pathway difference, x OPD , is Here, N 0 is the number of incident photons, N, the number of photons at the dark exit (D), λ, the wavelength of the incident …”
Section: Practical Implementationmentioning
confidence: 99%
See 1 more Smart Citation
“…To our knowledge, the best nulls in a tabletop setup reported in the literature were achieved by astronomers for the cancellation of star light to detect light from planets nearby. [27][28][29] Besides a special geometrical design, these nulls were achieved by actively controlling the optical path length difference, x OPD , using a piezotransducer attached to a mirror of one interferometer arm. When all optical elements are perfect, the nulling depth, D, as function of the optical pathway difference, x OPD , is Here, N 0 is the number of incident photons, N, the number of photons at the dark exit (D), λ, the wavelength of the incident …”
Section: Practical Implementationmentioning
confidence: 99%
“…This ensures that only the core of the output point-spread function is detected, thus largely eliminating the effect of wave front irregularities. 28 …”
Section: Practical Implementationmentioning
confidence: 99%
“…[13][14][15] The advantage of this interferometer is that the residual light at the dark exit is diminished by a large factor of about 10 5 or better with respect to the incident light, thus allowing immediate measurements of disturbances in the optical pathway of less than 0.6 nm. As a consequence, particles or proteins that diffuse in an aqueous solution through the microscopic focus in deep-nulling microscopy cause photon-burst fluctuations at the otherwise completely dark exit of the interferometer.…”
Section: Introductionmentioning
confidence: 99%
“…These include fine path-length control, intensity balance and polarization matching between the incoming beams, the requirement of a broadband achromatic π phase shifter (Labèque et al 2004) and fine control of the wavefront errors. As a consequence, the experimental demonstration of a deep broadband nulling has been actively pursued during the last years, first in the visible range (Serabyn et al 1999;Wallace et al 2000;Haguenauer & Serabyn 2006) then at 10 µm Gappinger et al 2005), in order to validate critical technologies. Among the different mentioned instrumental issues, the control of the wavefront corrugations is of major importance since the null is greatly degraded either by low-order errors (i.e.…”
Section: Introductionmentioning
confidence: 99%