These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
2. Detection of Earth-like planets around nearby stars using a petal-shaped occulter. Cash W Nature; 2006 Jul; 442(7098):51-3. PubMed ID: 16823446 [TBL] [Abstract][Full Text] [Related]
3. An image of an exoplanet separated by two diffraction beamwidths from a star. Serabyn E; Mawet D; Burruss R Nature; 2010 Apr; 464(7291):1018-20. PubMed ID: 20393557 [TBL] [Abstract][Full Text] [Related]
4. High-order adaptive optics requirements for direct detection of extrasolar planets: Application to the SPHERE instrument. Fusco T; Rousset G; Sauvage JF; Petit C; Beuzit JL; Dohlen K; Mouillet D; Charton J; Nicolle M; Kasper M; Baudoz P; Puget P Opt Express; 2006 Aug; 14(17):7515-34. PubMed ID: 19529118 [TBL] [Abstract][Full Text] [Related]
5. Possibilities for the detection of microbial life on extrasolar planets. Knacke RF Astrobiology; 2003; 3(3):531-41. PubMed ID: 14678662 [TBL] [Abstract][Full Text] [Related]
6. Suppression of coupling between optical aberration and tilt-to-length noise in a space-based gravitational wave telescope. Lin H; Li J; Huang Y; Yu M; Luo J; Wang Z; Wu Y Opt Express; 2023 Jan; 31(3):4367-4378. PubMed ID: 36785407 [TBL] [Abstract][Full Text] [Related]
7. Rolled edges and phasing of segmented telescopes. Yaitskova N; Troy M Appl Opt; 2011 Feb; 50(4):542-53. PubMed ID: 21283246 [TBL] [Abstract][Full Text] [Related]
8. Durham extremely large telescope adaptive optics simulation platform. Basden A; Butterley T; Myers R; Wilson R Appl Opt; 2007 Mar; 46(7):1089-98. PubMed ID: 17304307 [TBL] [Abstract][Full Text] [Related]
9. Wave aberration corrections in PSF ellipticity measurements of astronomical telescopes using a multi-objective optimization. Xu T; Luo J; He X; Li C; Zhang X Appl Opt; 2024 Jan; 63(3):743-756. PubMed ID: 38294387 [TBL] [Abstract][Full Text] [Related]
10. Analysis of stellar interferometers as wave-front sensors. Hénault F Appl Opt; 2005 Aug; 44(22):4733-44. PubMed ID: 16075886 [TBL] [Abstract][Full Text] [Related]
11. Active Alignment of Large-Aperture Space Telescopes for Optimal Ellipticity Performance. Bai X; Gu X; Xu B; Jiang F; Lu Z; Xu S; Ju G Sensors (Basel); 2023 May; 23(10):. PubMed ID: 37430618 [TBL] [Abstract][Full Text] [Related]
12. Development of a prototype active optics system for future space telescopes. Devaney N; Kenny F; Goncharov AV; Goy M; Reinlein C Appl Opt; 2018 Aug; 57(22):E101-E106. PubMed ID: 30117927 [TBL] [Abstract][Full Text] [Related]
13. Analytical study of diffraction effects in extremely large segmented telescopes. Yaitskova N; Dohlen K; Dierickx P J Opt Soc Am A Opt Image Sci Vis; 2003 Aug; 20(8):1563-75. PubMed ID: 12938912 [TBL] [Abstract][Full Text] [Related]
14. Evaluation of least-squares phase-diversity technique for space telescope wave-front sensing. Lee DJ; Roggemann MC; Welsh BM; Crosby ER Appl Opt; 1997 Dec; 36(35):9186-97. PubMed ID: 18264477 [TBL] [Abstract][Full Text] [Related]
15. Analytic diffraction analysis of a 32-m telescope with hexagonal segments for high-contrast imaging. Sabatke E; Burge J; Sabatke D Appl Opt; 2005 Mar; 44(8):1360-5. PubMed ID: 15796232 [TBL] [Abstract][Full Text] [Related]
16. Direct imaging of nonsolar planets with infrared telescopes using apodized coronagraphs. Watson SM; Mills JP; Gaiser SL; Diner DJ Appl Opt; 1991 Aug; 30(22):3253-62. PubMed ID: 20706384 [TBL] [Abstract][Full Text] [Related]
17. DM/LCWFC based adaptive optics system for large aperture telescopes imaging from visible to infrared waveband. Sun F; Cao Z; Wang Y; Zhang C; Zhang X; Liu Y; Mu Q; Xuan L Opt Express; 2016 Nov; 24(24):27494-27508. PubMed ID: 27906321 [TBL] [Abstract][Full Text] [Related]
18. Designs for a large-aperture telescope to map the CMB 10× faster. Niemack MD Appl Opt; 2016 Mar; 55(7):1688-96. PubMed ID: 26974631 [TBL] [Abstract][Full Text] [Related]