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An astronomer researching exoplanets.[ref]
Professional profile of Didier Queloz (phy.cam.ac.uk). Independent professional identity
Portrait of Didier Queloz
. Astrofisch66 (own work). CC BY-SA 4.0, via Wikimedia Commons. Source.An astronomer studying the Milky Way centre.[ref]
Reinhard Genzel by University of California, Berkeley. Independent professional identity
Portrait of Reinhard Genzel
. MPE (Commons uploader HHgarching). CC BY-SA 3.0, via Wikimedia Commons. Source.An astronomer studying the Milky Way centre.[ref]
Andrea Ghez by University of California, Los Angeles. Independent professional identity
Portrait of Andrea M. Ghez
. International Gemini Observatory/NOIRLab/NSF/AURA; still from Feeling gravity’s pull, a video by Julie Winokur. CC BY 4.0, via Wikimedia Commons. Source.An astronomer studying the Milky Way centre.[ref]
Rainer Schödel: curriculum vitae by Rainer Schödel. Independent professional identity
An astronomer researching exoplanets.[ref]
Professional profile of Aleksander Wolszczan (science.psu.edu). Independent professional identity
Portrait of Aleksander Wolszczan
. Ludek. CC BY-SA 3.0, via Wikimedia Commons. Source.An astronomer researching radio astronomy.[ref]
Professional profile of Dale Frail (public.nrao.edu). Independent professional identity
Portrait of Dale Frail
. Dale Frail. CC BY 3.0, via Wikimedia Commons. Source.An astronomer who designed astronomical spectrographs, including ELODIE.[ref]
In Memoriam of André Baranne, founder of the group by Gérard Lemaitre and Marc Ferrari. Independent professional identity
An astronomer.[ref]
Plus de 3000 visiteurs pour la Nuit Coupoles Ouvertes 2015. Photograph caption identifies Farrokh Vakili as astronome
Portrait of Frank Watson Dyson
. Bain News Service; George Grantham Bain Collection, Library of Congress, ggbain.30244. Public domain / no known copyright restrictions (PD-Bain). Source and usage information on the linked Wikimedia file page. Source.Portrait of Arthur Eddington
. George Grantham Bain Collection, Library of Congress, ggbain.38064. Public domain in United States; Commons file notes territorial limits. Source and usage information on the linked Wikimedia file page. Source.For a linear time-invariant system, a sinusoidal wanted signal at and an unwanted sinusoidal component at acquire their separate frequency response factors. The ratio of their output amplitudes, divided by their input amplitude ratio, is . An amplitude attenuation factor of corresponds to a factor in squared-amplitude power ratios under a common impedance convention. The unwanted component's own absolute attenuation is , which need not equal its attenuation relative to the wanted signal.
Light Waves and Their Uses by Albert Abraham Michelson Lecture V: Light Waves as Standards of Length by
Codex 0 2026-10-18
Cited experimental account: Figures 70–77.
Chapter IV; inspected §§70–75.
Chapter III, pp. 119–155; inspected §§61–64.
In 1947, Willis Eugene Lamb Jr. and Robert Curtis Retherford dissociated hydrogen in a tungsten oven, crossed its atomic jet with electrons for collisional excitation, and detected surviving atoms by electron ejection from metal. An electrometer and galvanometer read the current. They interrupted fixed-frequency microwaves while sweeping the static magnetic field; a flip coil calibrated the field. Their Zeeman splitting comparison placed about above ; the plotted displacement was explicitly not a best fit.[ref]
Fine Structure of the Hydrogen Atom by a Microwave Method by Willis Eugene Lamb Jr. and Robert Curtis Retherford. Fine Structure of the Hydrogen Atom by a Microwave Method, pp. 241–243, Figs. 1–2; inspected APS full text
The 1955 lecture's apparatus cross-section identifies movable slits, an electron bombarder, a radiofrequency transmission line with beam slots, a d.c. quenching electrode, metal target, electron collector, and magnet poles. A transition followed by rapid spontaneous emission leaves a ground-state atom unable to eject detector electrons. The scan holds radiofrequency and amplitude fixed. Natural linewidth and unresolved hyperfine structure broaden resonances, whose analysis yields zero-field separations.[ref]
Fine Structure of the Hydrogen Atom by Willis Eugene Lamb Jr.. Fine Structure of the Hydrogen Atom, delivered December 12, 1955; Columbia-hosted Nobel Lectures scan, printed pp. 288–290, Figs. 2–7
Static electric field quenching supplied a control. The 1947 report identifies natural linewidth, hyperfine structure, excessive microwave intensity, and field inhomogeneity as width contributions, and flags imperfect magnetic calibration. It does not specify an absolute microwave-frequency calibration procedure.[ref]
Fine Structure of the Hydrogen Atom by a Microwave Method by Willis Eugene Lamb Jr. and Robert Curtis Retherford. pp. 242–243, Fig. 1 caption and discussion of proposed refinements
Metastable beam preparation and electron-current readout
. Original functional schematic of the Lamb-Retherford measurement principle, based on the apparatus descriptions above. The level sketch isolates the zero-field and pair; the historical field scans also addressed other Zeeman branches. Geometry and energy gaps are not to scale. Details.The surname is Robert Curtis Retherford's: “Retherford” and “Rutherford” name different people. The historical Lamb-Retherford experiment should retain the former spelling.[ref]
Retherford, Robert Curtis by Istituto della Enciclopedia Italiana. Retherford, Robert Curtis, professional biography and account of the 1947 experiment
Pinned article: Introduction to the OurBigBook Project
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Intro to OurBigBook
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