Adaptive Optics in High-Contrast Imaging
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David Mouillet | Dimitri Mawet | Julien H. Girard | Julien Milli | Markus Kasper | D. Mawet | J. Milli | M. Kasper | J. Girard | D. Mouillet | Julien H. V. Girard
[1] A. Labeyrie,et al. The Four-Quadrant Phase-Mask Coronagraph. I. Principle , 2000 .
[2] Frans Snik,et al. The vector-APP: a broadband apodizing phase plate that yields complementary PSFs , 2012, Other Conferences.
[3] Kjetil Dohlen,et al. Long slit spectroscopy for exoplanet characterization in SPHERE , 2008, Astronomical Telescopes + Instrumentation.
[4] Amir Give'on,et al. Broadband wavefront correction algorithm for high-contrast imaging systems , 2007, SPIE Optical Engineering + Applications.
[5] A. Boccaletti,et al. A Giant Planet Imaged in the Disk of the Young Star β Pictoris , 2010, Science.
[6] R. Vanderbei,et al. Extrasolar Planet Finding via Optimal Apodized-Pupil and Shaped-Pupil Coronagraphs , 2003 .
[7] B. Macintosh,et al. M-BAND IMAGING OF THE HR 8799 PLANETARY SYSTEM USING AN INNOVATIVE LOCI-BASED BACKGROUND SUBTRACTION TECHNIQUE , 2011, 1107.0967.
[8] J. Graham,et al. The IRCAL Polarimeter: Design, Calibration, and Data Reduction for an Adaptive Optics Imaging Polarimeter , 2008, 0804.1550.
[9] Jean-Luc Beuzit,et al. MESS: Multi-purpose Exoplanet Simulation System , 2011 .
[10] D. Mouillet,et al. A giant planet candidate near a young brown dwarf - Direct VLT/NACO observations using IR wavefront sensing , 2004 .
[11] R. Angel,et al. CORONAGRAPHIC LOW-ORDER WAVE-FRONT SENSOR: PRINCIPLE AND APPLICATION TO A PHASE-INDUCED AMPLITUDE CORONAGRAPH , 2009, 0911.1301.
[12] W. Traub,et al. A laboratory demonstration of the capability to image an Earth-like extrasolar planet , 2007, Nature.
[13] D. Mawet,et al. Annular Groove Phase Mask Coronagraph , 2005 .
[14] Gautam Vasisht,et al. Project 1640: the world's first ExAO coronagraphic hyperspectral imager for comparative planetary science , 2012, Other Conferences.
[15] Kjetil Dohlen,et al. EPICS: direct imaging of exoplanets with the E-ELT , 2010, Astronomical Telescopes + Instrumentation.
[16] Francois Roddier,et al. Adaptive Optics in Astronomy: Imaging through the atmosphere , 2004 .
[17] D. Mawet,et al. Impact of angular differential imaging on circumstellar disk images , 2012, 1207.5909.
[18] Andrew W. Serio,et al. First light of the Gemini Planet Imager , 2014, Proceedings of the National Academy of Sciences.
[19] B. Macintosh,et al. Angular Differential Imaging: A Powerful High-Contrast Imaging Technique , 2005, astro-ph/0512335.
[20] Claude Aime,et al. The Usefulness and Limits of Coronagraphy in the Presence of Pinned Speckles , 2004 .
[21] Gautam Vasisht,et al. SPECKLE SUPPRESSION WITH THE PROJECT 1640 INTEGRAL FIELD SPECTROGRAPH , 2010, 1012.4016.
[22] S. Ridgway,et al. Theoretical Limits on Extrasolar Terrestrial Planet Detection with Coronagraphs , 2006, astro-ph/0608506.
[23] Markus Janson,et al. HIGH-CONTRAST IMAGING SEARCH FOR PLANETS AND BROWN DWARFS AROUND THE MOST MASSIVE STARS IN THE SOLAR NEIGHBORHOOD , 2011, 1105.2577.
[24] B. Macintosh,et al. Images of a fourth planet orbiting HR 8799 , 2010, Nature.
[25] Gordon A. H. Walker,et al. Speckle Noise and the Detection of Faint Companions , 1999 .
[26] A. Lagrange,et al. Sparse aperture masking at the VLT. I. Faint companion detection limits for the two debris disk stars HD 92945 and HD 141569 , 2011, 1107.1426.
[27] C. Aime,et al. Stellar coronagraphy with prolate apodized circular apertures , 2003 .
[28] Olivier Absil,et al. On the sensitivity of closure phases to faint companions in optical long baseline interferometry , 2012, 1204.3721.
[29] Glenn Schneider. A Quick Study of Science Return from Direct Imaging Exoplanet Missions: Detection and Characterization of Circumstellar Material with an AFTA or EXO-C/S CGI , 2014 .
[30] C. Marois,et al. Differential Imaging with a Multicolor Detector Assembly: A New Exoplanet Finder Concept , 2004, astro-ph/0410010.
[31] F. Roddier,et al. The Nulling Stellar Coronagraph: Laboratory Tests and Performance Evaluation , 1999 .
[32] O. Guyon. Limits of Adaptive Optics for High-Contrast Imaging , 2005, astro-ph/0505086.
[33] Julien H. Girard,et al. New constraints on the dust surrounding HR 4796A , 2014, 1407.2539.
[34] Russell B. Makidon,et al. Temporal Evolution of Coronagraphic Dynamic Range and Constraints on Companions to Vega , 2006, astro-ph/0609337.
[35] Gerard Rousset,et al. First diffraction-limited astronomical images with adaptive optics , 1990, Astronomical Telescopes and Instrumentation.
[36] R. Ragazzoni,et al. Sensitivity of a pyramidic Wave Front sensor in closed loop Adaptive Optics , 1999 .
[37] L M Mugnier,et al. High-order myopic coronagraphic phase diversity (COFFEE) for wave-front control in high-contrast imaging systems. , 2013, Optics express.
[38] Michael C. Liu,et al. The Gemini NICI planet-finding campaign: The offset ring of HR 4796 A , , 2014, 1404.6525.
[39] D. Mouillet,et al. A STELLAR CORONOGRAPH FOR THE COME-ON-PLUS ADAPTIVE OPTICS SYSTEM. II. FIRST ASTRONOMICAL RESULTS , 1997 .
[40] J. Angel,et al. First On-Sky High-Contrast Imaging with an Apodizing Phase Plate* , 2007, astro-ph/0702324.
[41] A. Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images , 1970 .
[42] C. Marois,et al. Confidence Level and Sensitivity Limits in High-Contrast Imaging , 2007, 0709.3548.
[43] Frantz Martinache,et al. The Subaru Coronagraphic Extreme AO project , 2009 .
[44] Olivier Guyon,et al. Review of small-angle coronagraphic techniques in the wake of ground-based second-generation adaptive optics systems , 2012, Other Conferences.
[45] Mamadou N'Diaye,et al. FIVE DEBRIS DISKS NEWLY REVEALED IN SCATTERED LIGHT FROM THE HUBBLE SPACE TELESCOPE NICMOS ARCHIVE , 2014, 1404.5614.
[46] Tyson Hare,et al. First closed-loop visible AO test results for the advanced adaptive secondary AO system for the Magellan Telescope: MagAO's performance and status , 2012, Other Conferences.
[47] Thierry Fusco,et al. First laboratory validation of vibration filtering with LQG control law for adaptive optics. , 2008, Optics express.
[48] Michael C. Liu,et al. EARLY RESULTS FROM VLT SPHERE: LONG-SLIT SPECTROSCOPY OF 2MASS 0122–2439 B, A YOUNG COMPANION NEAR THE DEUTERIUM BURNING LIMIT , 2015, 1504.07240.
[49] Bruno Leibundgut,et al. Scientific Requirements for Extremely Large Telescopes , 2006 .
[50] Nicholas Devaney,et al. Chromatic effects of the atmosphere on astronomical adaptive optics. , 2008, Applied optics.
[51] Dmitry Savransky,et al. POLARIMETRY WITH THE GEMINI PLANET IMAGER: METHODS, PERFORMANCE AT FIRST LIGHT, AND THE CIRCUMSTELLAR RING AROUND HR 4796A , 2014, 1407.2495.
[52] W. Traub,et al. TRANSITS OF EARTH-LIKE PLANETS , 2009, 0903.3371.
[53] P. H. Hauschildt,et al. Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458 , 2003 .
[54] Adam Amara,et al. PYNPOINT: An image processing package for finding exoplanets , 2012, 1207.6637.
[55] C. Alvarez,et al. A Search for Hot Massive Extrasolar Planets around Nearby Young Stars with the Adaptive Optics System NACO , 2005, astro-ph/0502376.
[56] D. Mawet,et al. Improved high-contrast imaging with on-axis telescopes using a multistage vortex coronagraph. , 2011, Optics letters.
[57] R. Soummer,et al. HIGH PERFORMANCE PIAA CORONAGRAPHY WITH COMPLEX AMPLITUDE FOCAL PLANE MASKS , 2010 .
[58] Frantz Martinache,et al. The Subaru coronagraphic extreme AO (SCExAO) system: wavefront control and detection of exoplanets with coherent light modulation in the focal plane , 2010, Astronomical Telescopes + Instrumentation.
[59] C. Baranec,et al. PALM-3000: EXOPLANET ADAPTIVE OPTICS FOR THE 5 m HALE TELESCOPE , 2013, 1309.1216.
[60] D. Ehrenreich,et al. High-resolution imaging of young M-type stars of the solar neighbourhood: probing for companions down to the mass of Jupiter , 2011, 1112.3008.
[61] P.-Y. Madec. Overview of deformable mirror technologies for adaptive optics and astronomy , 2012, Other Conferences.
[62] Gérard Rousset,et al. Adaptive Optics in Astronomy: Wave-front sensors , 1999 .
[63] A. Labeyrie,et al. The Four‐Quadrant Phase‐Mask Coronagraph. I. Principle , 2000 .
[64] Markus Kasper,et al. Adaptive optics for high contrast imaging , 2012, Other Conferences.
[65] P. Cochat,et al. Et al , 2008, Archives de pediatrie : organe officiel de la Societe francaise de pediatrie.
[66] O. Guyon,et al. The VAMPIRES instrument: imaging the innermost regions of protoplanetary discs with polarimetric interferometry , 2014, 1405.7426.
[67] O. Guyon. Phase-induced amplitude apodization of telescope pupils for extrasolar terrestrial planet imaging , 2003, astro-ph/0301190.
[68] T. Fusco,et al. SPHERE eXtreme AO control scheme: final performance assessment and on sky validation of the first auto-tuned LQG based operational system , 2014, Astronomical Telescopes and Instrumentation.
[69] R. Soummer,et al. DETECTION AND CHARACTERIZATION OF EXOPLANETS AND DISKS USING PROJECTIONS ON KARHUNEN–LOÈVE EIGENIMAGES , 2012, 1207.4197.
[70] T. Fusco,et al. Maximum likelihood-based method for angular differential imaging , 2008, Astronomical Telescopes + Instrumentation.
[71] H. Ford,et al. Imaging Spectroscopy for Extrasolar Planet Detection , 2002, astro-ph/0209078.
[72] Markus Janson,et al. A novel L-band imaging search for giant planets in the Tucana and β Pictoris moving groups , 2007, 0706.0095.
[73] Gerard Rousset,et al. ADONIS: a user-friendly adaptive optics system for the ESO 3.6-m telescope , 1994, Astronomical Telescopes and Instrumentation.
[74] Virendra N. Mahajan. Strehl ratio for primary aberrations in terms of their aberration variance , 1983 .
[75] R. Ragazzoni. Pupil plane wavefront sensing with an oscillating prism , 1996 .
[76] S. Rappaport,et al. NEW CONSTRAINTS ON QUANTUM GRAVITY FROM X-RAY AND GAMMA-RAY OBSERVATIONS , 2014, 1411.7262.
[77] E. Serabyn,et al. EXTREME ADAPTIVE OPTICS IMAGING WITH A CLEAR AND WELL-CORRECTED OFF-AXIS TELESCOPE SUBAPERTURE , 2007, astro-ph/0702592.
[78] J. K. Wallace,et al. Phase contrast techniques for wavefront sensing and calibration in adaptive optics , 2003, SPIE Optics + Photonics.
[79] Mamadou N'Diaye,et al. Archival Legacy Investigation of Circumstellar Environments using KLIP algorithm on HST NICMOS coronagraphic data , 2013 .
[80] Andrew Serio,et al. THE FIRST H-BAND SPECTRUM OF THE GIANT PLANET β PICTORIS b , 2014, 1407.4469.
[81] Etienne Artigau,et al. A New Algorithm for Point-Spread Function Subtraction in High-Contrast Imaging: A Demonstration with Angular Differential Imaging , 2007, astro-ph/0702697.
[82] Bruce A. Macintosh,et al. The Gemini Planet Imager: from science to design to construction , 2008, Astronomical Telescopes + Instrumentation.
[83] Ben R. Oppenheimer,et al. THE LYOT PROJECT DIRECT IMAGING SURVEY OF SUBSTELLAR COMPANIONS: STATISTICAL ANALYSIS AND INFORMATION FROM NONDETECTIONS , 2010, 1006.3409.
[84] K. Ulaczyk,et al. One or more bound planets per Milky Way star from microlensing observations , 2012, Nature.
[85] Laird M. Close,et al. An Imaging Survey for Extrasolar Planets around 45 Close, Young Stars with the Simultaneous Differential Imager at the Very Large Telescope and MMT , 2007 .
[86] G. G. Stokes. "J." , 1890, The New Yale Book of Quotations.
[87] Jean-Pierre Véran,et al. Toward feasible and effective predictive wavefront control for adaptive optics , 2008, Astronomical Telescopes + Instrumentation.
[88] C. Fabron,et al. SPHERE: a planet finder instrument for the VLT , 2006, Astronomical Telescopes + Instrumentation.
[89] S. Gladysz,et al. Statistics of intensity in adaptive-optics images and their usefulness for detection and photometry of exoplanets. , 2010, Journal of the Optical Society of America. A, Optics, image science, and vision.
[90] Tyson Hare,et al. The Magellan Telescope Adaptive Secondary AO System: a visible and mid-IR AO facility , 2010, Astronomical Telescopes + Instrumentation.
[91] Jr.,et al. RECONNAISSANCE OF THE HR 8799 EXOSOLAR SYSTEM. I. NEAR-INFRARED SPECTROSCOPY , 2013, 1303.2627.
[92] F. Roddier. V The Effects of Atmospheric Turbulence in Optical Astronomy , 1981 .
[93] Armando Riccardi,et al. MAGELLAN ADAPTIVE OPTICS FIRST-LIGHT OBSERVATIONS OF THE EXOPLANET β PIC b. I. DIRECT IMAGING IN THE FAR-RED OPTICAL WITH MagAO+VisAO AND IN THE NEAR-IR WITH NICI, , 2014, 1403.0560.
[94] Horace W. Babcock,et al. THE POSSIBILITY OF COMPENSATING ASTRONOMICAL SEEING , 1953 .
[95] Dimitri Mawet,et al. Image quality and high contrast improvements on VLT/NACO , 2012, Other Conferences.
[96] J. Laskar,et al. The HARPS search for southern extra-solar planets - XXXIV. A planetary system around the nearby M dwarf GJ 163, with a super-Earth possibly in the habitable zone , 2013, 1306.0904.
[97] A. Pocheau,et al. Front propagation in a turbulent medium , 1992 .
[98] Kjetil Dohlen,et al. SPHERE non-common path aberrations measurement and pre-compensation with optimized phase diversity processes: experimental results , 2011 .
[99] Roberto Ragazzoni,et al. An update of the on-sky performance of the layer-oriented wavefront sensor for MAD , 2010, Astronomical Telescopes + Instrumentation.
[100] C. Marois,et al. A NEW ALGORITHM FOR POINT SPREAD FUNCTION SUBTRACTION IN HIGH-CONTRAST IMAGING: A DEMONSTRATION WITH ANGULAR DIFFERENTIAL IMAGING , 2007 .
[101] David Ehrenreich,et al. Instrumentation for the detection and characterization of exoplanets , 2014, Nature.
[102] F Roddier,et al. Curvature sensing and compensation: a new concept in adaptive optics. , 1988, Applied optics.
[103] R. Vanderbei,et al. Optimal pupil apodizations of arbitrary apertures for high-contrast imaging. , 2011, Optics express.
[104] C. A. Haniff,et al. Closure phase in high-resolution optical imaging , 1986, Nature.
[105] Armando Riccardi,et al. First light AO (FLAO) system for LBT: final integration, acceptance test in Europe, and preliminary on-sky commissioning results , 2010, Astronomical Telescopes + Instrumentation.
[106] Cambridge,et al. Lucky imaging: High angular resolution imaging in the visible from the ground , 2005, astro-ph/0507299.