mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
Loading...
Searching...
No Matches
Bibliography
[1]

M. Born and E. Wolf. Principles of Optics. October 1999.

[2]

Matthew Brand. Fast low-rank modifications of the thin singular value decomposition. Linear Algebra and its Applications, 415(1):20–30, 2006.

[3]

James R. Bunch and Christopher P. Nielsen. Updating the singular value decomposition. Numerische Mathematik, 31:111–129, 1978.

[4]

K. L. Cahoy, M. S. Marley, and J. J. Fortney. Exoplanet Albedo Spectra and Colors as a Function of Planet Phase, Separation, and Metallicity. ApJ, 724:189–214, November 2010.

[5]

C. Cavarroc, A. Boccaletti, P. Baudoz, T. Fusco, and D. Rouan. Fundamental limitations on Earth-like planet detection with extremely large telescopes. A&A, 447:397–403, February 2006.

[6]

N. B. Cowan and T. E. Strait. Determining Reflectance Spectra of Surfaces and Clouds on Exoplanets. ApJL, 765:L17, March 2013.

[7]

D. C. Fabrycky, J. J. Lissauer, D. Ragozzine, J. F. Rowe, J. H. Steffen, E. Agol, T. Barclay, N. Batalha, W. Borucki, D. R. Ciardi, E. B. Ford, T. N. Gautier, J. C. Geary, M. J. Holman, J. M. Jenkins, J. Li, R. C. Morehead, R. L. Morris, A. Shporer, J. C. Smith, M. Still, and J. Van Cleve. Architecture of Kepler’s Multi-transiting Systems. II. New Investigations with Twice as Many Candidates. ApJ, 790:146, August 2014.

[8]

D. J. E. Floyd, J. Thomas-Osip, and G. Prieto. Seeing, Wind, and Outer Scale Effects on Image Quality at the Magellan Telescopes. PASP, 122:731–742, June 2010.

[9]

J. J. Fortney, M. S. Marley, and J. W. Barnes. Planetary Radii across Five Orders of Magnitude in Mass and Stellar Insolation: Application to Transits. ApJ, 659:1661–1672, April 2007.

[10]

J. J. Fortney, I. Baraffe, and B. Militzer. Giant Planet Interior Structure and Thermal Evolution, pages 397–418. December 2010.

[11]

I. S. Gradshteyn, I. M. Ryzhik, A. Jeffrey, and D. Zwillinger. Table of Integrals, Series, and Products. 2007.

[12]

Ming Gu and Stanley C. Eisenstat. Downdating the Singular Value Decomposition. SIAM Journal on Matrix Analysis and Applications, 16(3):793–810, 1995.

[13]

O. Guyon, P. M. Hinz, E. Cady, R. Belikov, and F. Martinache. High Performance Lyot and PIAA Coronagraphy for Arbitrarily Shaped Telescope Apertures. ApJ, 780:171, January 2014.

[14]

O. Guyon. Limits of Adaptive Optics for High-Contrast Imaging. ApJ, 629:592–614, August 2005.

[15]

J. W. Hardy. Adaptive Optics for Astronomical Telescopes. July 1998.

[16]

Erik M. Johansson and Donald T. Gavel. Simulation of stellar speckle imaging. Proc. SPIE, 2200:372–383, June 1994.

[17]

J. J. Lissauer, D. Ragozzine, D. C. Fabrycky, J. H. Steffen, E. B. Ford, J. M. Jenkins, A. Shporer, M. J. Holman, J. F. Rowe, E. V. Quintana, N. M. Batalha, W. J. Borucki, S. T. Bryson, D. A. Caldwell, J. A. Carter, D. Ciardi, E. W. Dunham, J. J. Fortney, T. N. Gautier, III, S. B. Howell, D. G. Koch, D. W. Latham, G. W. Marcy, R. C. Morehead, and D. Sasselov. Architecture and Dynamics of Kepler’s Candidate Multiple Transiting Planet Systems. ApJS, 197:8, November 2011.

[18]

Joseph D. Long and Jared R. Males. Unlocking starlight subtraction in full data rate exoplanet imaging by efficiently updating Karhunen-Loève eigenimages. The Astronomical Journal, 161(4):166, 2021.

[19]

V. N. Mahajan. Uniform versus Gaussian beams: a comparison of the effects of diffraction, obscuration, and aberrations. Journal of the Optical Society of America A, 3:470–485, April 1986.

[20]

Jared R. Males and Olivier Guyon. Ground-based adaptive optics coronagraphic performance under closed-loop predictive control. Journal of Astronomical Telescopes, Instruments, and Systems, 4:019001, January 2018.

[21]

G. W. Marcy, H. Isaacson, A. W. Howard, J. F. Rowe, J. M. Jenkins, S. T. Bryson, D. W. Latham, S. B. Howell, T. N. Gautier, III, N. M. Batalha, L. Rogers, D. Ciardi, D. A. Fischer, R. L. Gilliland, H. Kjeldsen, J. Christensen-Dalsgaard, D. Huber, W. J. Chaplin, S. Basu, L. A. Buchhave, S. N. Quinn, W. J. Borucki, D. G. Koch, R. Hunter, D. A. Caldwell, J. Van Cleve, R. Kolbl, L. M. Weiss, E. Petigura, S. Seager, T. Morton, J. A. Johnson, S. Ballard, C. Burke, W. D. Cochran, M. Endl, P. MacQueen, M. E. Everett, J. J. Lissauer, E. B. Ford, G. Torres, F. Fressin, T. M. Brown, J. H. Steffen, D. Charbonneau, G. S. Basri, D. D. Sasselov, J. Winn, R. Sanchis-Ojeda, J. Christiansen, E. Adams, C. Henze, A. Dupree, D. C. Fabrycky, J. J. Fortney, J. Tarter, M. J. Holman, P. Tenenbaum, A. Shporer, P. W. Lucas, W. F. Welsh, J. A. Orosz, T. R. Bedding, T. L. Campante, G. R. Davies, Y. Elsworth, R. Handberg, S. Hekker, C. Karoff, S. D. Kawaler, M. N. Lund, M. Lundkvist, T. S. Metcalfe, A. Miglio, V. Silva Aguirre, D. Stello, T. R. White, A. Boss, E. Devore, A. Gould, A. Prsa, E. Agol, T. Barclay, J. Coughlin, E. Brugamyer, F. Mullally, E. V. Quintana, M. Still, S. E. Thompson, D. Morrison, J. D. Twicken, J.-M. Désert, J. Carter, J. R. Crepp, G. Hébrard, A. Santerne, C. Moutou, C. Sobeck, D. Hudgins, M. R. Haas, P. Robertson, J. Lillo-Box, and D. Barrado. Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets. ApJS, 210:20, February 2014.

[22]

A. F. J. Moffat. A Theoretical Investigation of Focal Stellar Images in the Photographic Emulsion and Application to Photographic Photometry. aap , 3:455, Dec 1969.

[23]

P. J. Mohr, D. B. Newell, and B. N. Taylor. CODATA recommended values of the fundamental physical constants: 2014*. Reviews of Modern Physics, 88(3):035009, July 2016.

[24]

R. J. Noll. Zernike polynomials and atmospheric turbulence. Journal of the Optical Society of America (1917-1983), 66:207–211, March 1976.

[25]

Alan V. Oppenheim and Ronald W. Schafer. Discrete-Time Signal Processing. Prentice Hall Press, USA, 3rd edition, 2009.

[26]

L. A. Poyneer and J.-P. Véran. Optimal modal Fourier-transform wavefront control. Journal of the Optical Society of America A, 22:1515–1526, August 2005.

[27]

R. Racine, G. A. H. Walker, D. Nadeau, R. Doyon, and C. Marois. Speckle Noise and the Detection of Faint Companions. PASP, 111:587–594, May 1999.

[28]

F. Roddier. The effects of atmospheric turbulence in optical astronomy. Progress in optics. Volume 19. Amsterdam, North-Holland Publishing Co., 1981, p. 281-376., 19:281–376, 1981.

[29]

L. A. Rogers. Most 1.6 Earth-radius Planets are Not Rocky. ApJ, 801:41, March 2015.

[30]

J.-F. Sauvage, L. M. Mugnier, G. Rousset, and T. Fusco. Analytical expression of long-exposure adaptive-optics-corrected coronagraphic image First application to exoplanet detection. Journal of the Optical Society of America A, 27(27), November 2010.

[31]

P. K. Seidelmann, B. A. Archinal, M. F. A’Hearn, A. Conrad, G. J. Consolmagno, D. Hestroffer, J. L. Hilton, G. A. Krasinsky, G. Neumann, J. Oberst, P. Stooke, E. F. Tedesco, D. J. Tholen, P. C. Thomas, and I. P. Williams. Report of the IAU/IAG Working Group on cartographic coordinates and rotational elements: 2006. Celestial Mechanics and Dynamical Astronomy, 98:155–180, July 2007.

[32]

R. Soummer, L. Pueyo, A. Sivaramakrishnan, and R. J. Vanderbei. Fast computation of Lyot-style coronagraph propagation. Optics Express, 15(24):15935, January 2007.

[33]

Daniel P. Thorngren, Mark S. Marley, and Jonathan J. Fortney. An empirical mass textendash radius relation for cool giant planets. Research Notes of the AAS, 3(9):128, sep 2019.

[34]

A. Tokovinin. From Differential Image Motion to Seeing. PASP, 114:1156–1166, October 2002.

[35]

M. C. Turnbull, W. A. Traub, K. W. Jucks, N. J. Woolf, M. R. Meyer, N. Gorlova, M. F. Skrutskie, and J. C. Wilson. Spectrum of a Habitable World: Earthshine in the Near-Infrared. ApJ, 644:551–559, June 2006.