標(biāo)題: Titlebook: Radial-velocity Searches for Planets Around Active Stars; Rapha?lle D. Haywood Book 2016 Springer International Publishing Switzerland 201 [打印本頁] 作者: 是消毒 時間: 2025-3-21 19:13
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作者: 態(tài)度暖昧 時間: 2025-3-21 20:33
Rapha?lle D. Haywoodhnische Systeme halte, in angemessen erweiterter Gestalt als Buch verfügbar zu machen. Leider hat sich die Ver- wirklichung dieses Plans wegen der gro?en Fülle anderer Verpflichtungen immer wieder verz?gert, und auch jetzt habe ich gegenüber meinen ursprünglichen Vorstellungen, wie ein solches Buch 作者: Parameter 時間: 2025-3-22 03:46 作者: 鋼盔 時間: 2025-3-22 08:29
Rapha?lle D. Haywood Wichtiges Element sind Schalter. Mechanisches, elektrooptisches, mechanooptisches und thermisches Schalten sowie mikro-elektromechanische Schalter (MEMS) werden beschrieben. Von gro?er Bedeutung sind Filter für optische Netze. Filter auf Basis von Interferenz (Dünnschichtfilter), Fabry-Perot-Filter作者: commodity 時間: 2025-3-22 11:17 作者: medium 時間: 2025-3-22 15:04 作者: 使乳化 時間: 2025-3-22 19:24 作者: follicle 時間: 2025-3-23 00:08
https://doi.org/10.1007/978-3-319-41273-3Exoplanet (extra-solar planet) Detection; Exoplanet Characterisation; Exoplanet Mass Determination; Sun作者: LUT 時間: 2025-3-23 02:17
Rapha?lle D. HaywoodNominated as an outstanding Ph.D. thesis by the University of St. Andrews, UK.Includes clear explanations, making it easy to read and accessible to a broad audience with minimum scientific background 作者: Alcove 時間: 2025-3-23 09:33
Introduction: The Hunt for Extra-Solar Planets,ades, developments in instrumentation and observation techniques have led to revolutionary discoveries: we now know that planets revolving around other stars than our Sun exist, and better still, they appear to be very common.作者: WAIL 時間: 2025-3-23 10:47 作者: Acupressure 時間: 2025-3-23 14:40
Radial-velocity Searches for Planets Around Active Stars978-3-319-41273-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: heckle 時間: 2025-3-23 20:05 作者: 拖債 時間: 2025-3-23 22:11 作者: Heresy 時間: 2025-3-24 04:25
Rapha?lle D. Haywood ausführlich erl?utert. Zu Regeneration der Form (Re-Shaping) werden dispersionskompensierende Glasfasern und Faser-Bragg-Gitter benutzt. Die Taktrückgewinnung (Re-Timing, clock recovery) wird durch nichtlineare?Methoden der Bearbeitung des Eingangssignals oder durch entscheidungsrückgekoppelte Verf作者: 社團(tuán) 時間: 2025-3-24 09:38
Rapha?lle D. Haywood ausführlich erl?utert. Zu Regeneration der Form (Re-Shaping) werden dispersionskompensierende Glasfasern und Faser-Bragg-Gitter benutzt. Die Taktrückgewinnung (Re-Timing, clock recovery) wird durch nichtlineare?Methoden der Bearbeitung des Eingangssignals oder durch entscheidungsrückgekoppelte Verf作者: inquisitive 時間: 2025-3-24 10:57 作者: 刺耳的聲音 時間: 2025-3-24 18:01
Radial-velocity Searches for Planets Around Active Stars作者: Offset 時間: 2025-3-24 20:04 作者: SNEER 時間: 2025-3-25 00:38 作者: 匯總 時間: 2025-3-25 04:43 作者: 意外 時間: 2025-3-25 08:57
Book 2016s for distinguishing genuine planetary signals from false positives produced by stellar magnetic activity..The findings of this thesis represent a significant step towards determining the masses of potentially habitable planets orbiting Sun-like stars.?.作者: Feedback 時間: 2025-3-25 13:35
Introduction: The Hunt for Extra-Solar Planets,ades, developments in instrumentation and observation techniques have led to revolutionary discoveries: we now know that planets revolving around other stars than our Sun exist, and better still, they appear to be very common.作者: 大廳 時間: 2025-3-25 17:50
Stellar Activity as a Source of Radial-Velocity Variability, variability. This chapter provides a review of the manifestations of magnetic activity, their impact on photometric and spectroscopic observations, and the analysis techniques that have been developed in recent years to account for activity-induced RV signals. I also present the target selection cr作者: Coordinate 時間: 2025-3-25 20:53
A Toolkit to Detect Planets Around Active Stars,ntroducing Gaussian processes, which are a powerful and elegant way to model correlated noise. I will start from the very basics of Gaussian distributions, leading up?to how I incorporate them in my model to account for stellar activity signals. I then present the model that I use to fit RV observat作者: 盲信者 時間: 2025-3-26 00:21 作者: Hamper 時間: 2025-3-26 04:29
An Exploration into the Radial-Velocity Variability of the Sun,pler signature of orbiting planets. This has resulted in several false detections (see Queloz et?al. .; Bonfils et?al. .; Huélamo et?al. .; Boisse et?al. ., .; Gregory .; Haywood et?al. .; Santos et?al. .; Robertson et?al. . and many others). Understanding the RV signatures of stellar activity, in p作者: 緯度 時間: 2025-3-26 11:51
Conclusion: Next Steps and Aims for the Future,aced by the exoplanet community today, and we must overcome this barrier in order to become able to routinely detect Earth-mass planets at greater distances from their stars. Building on my thesis work, I now intend to tackle this issue in two ways. First, I plan to incorporate activity proxies into作者: expound 時間: 2025-3-26 14:52 作者: 斜坡 時間: 2025-3-26 19:13 作者: 網(wǎng)絡(luò)添麻煩 時間: 2025-3-26 23:57
Application to Observations of Planet-Hosting Stars,ose discovery challenges our theories of planet formation. All three of these systems were first discovered via the transit method, by the CoRoT and . space missions. They were followed up with HARPS, HARPS-N and HIRES in order to obtain a precise mass determination of the planets present in these systems.作者: Bph773 時間: 2025-3-27 02:05 作者: obscurity 時間: 2025-3-27 05:48 作者: septicemia 時間: 2025-3-27 12:04
Book 2016 the physical origin of stellar intrinsic variability, using unique observations of the Sun seen as a star. In particular, it establishes that the intrinsic stellar radial-velocity variations mainly arise from suppression of photospheric convection by magnetic fields.?With the advent of powerful tel作者: flaunt 時間: 2025-3-27 15:54 作者: 外表讀作 時間: 2025-3-27 18:06
