AN INDEPENDENT ANALYSIS OF KEPLER-4b THROUGH KEPLER-8b [PDF]
The Astrophysical Journal, 2011 We present two independent, homogeneous, global analyses of the transit light curves, radial velocities and spectroscopy of Kepler-4b through Kepler-8b, with numerous differences over the previous methods. These include: 1) improved decorrelated parameter fitting set, 2) new limb darkening coefficients, 3) time-stamps modified to BJD for consistency ...
Kipping, David M., Bakos, Gáspár Á.
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EXOPLANET CHARACTERIZATION BY PROXY: A TRANSITING 2.15R⊕PLANET NEAR THE HABITABLE ZONE OF THE LATE K DWARF KEPLER-61 [PDF]
, 2013 We present the validation and characterization of Kepler-61b: a 2.15 R_Earth planet orbiting near the inner edge of the habitable zone of a low-mass star.
Sarah Ballard +15 more
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Improved parameters of seven Kepler giant companions characterized with SOPHIE and HARPS-N [PDF]
, 2015 Radial-velocity observations of Kepler candidates obtained with the SOPHIE and HARPS-N spectrographs have permitted unveiling the nature of the five giant planets Kepler-41b, Kepler-43b, Kepler-44b, Kepler-74b, and Kepler-75b, the massive companion ...
Almenara, J. -M. +8 more
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Characterisation and impact of intratumoural stroma in melanoma and carcinoma brain metastases. [PDF]
J Pathol Clin ResAbstract Research on the tumour microenvironment in brain metastases (BM) has predominantly focused on the immune response, while the presence, morphological patterns, and potential clinical relevance of intratumoural stroma remain less intensively investigated.
Bandke D +6 more
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A 38 Million Year Old Neptune-sized Planet in the Kepler Field
The Astronomical Journal, 2022 Kepler 1627A is a G8V star previously known to host a 3.8 R _⊕ planet on a 7.2 day orbit. The star was observed by the Kepler space telescope because it is nearby ( d = 329 pc) and it resembles the Sun.
L. G. Bouma +14 more
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The Astronomical Journal, 2023 We present the latest and most precise characterization of the architecture for the ancient (≈11 Gyr) Kepler-444 system, which is composed of a K0 primary star (Kepler-444 A) hosting five transiting planets and a tight M-type spectroscopic binary (Kepler-
Zhoujian Zhang +13 more
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Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates [PDF]
, 2011 We present the discovery of the Kepler-20 planetary system, which we initially identified through the detection of five distinct periodic transit signals in the Kepler light curve of the host star 2MASSJ19104752+4220194.
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Experiencia estética y formulación científica: el caso del Harmonices Mundi de Johannes Kepler
Anuario Musical, 2013 La música como modelo explicativo del universo ha estado presente desde el mismo nacimiento de la reflexión filosófica. En el caso de Kepler, la música y la astronomía quedaban homologadas sobre la base de un único arquetipo geométrico, y por ello podían
Carlos Calderón Urreiztieta
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The atmospheres of the hot-Jupiters Kepler-5b and Kepler-6b observed during occultations with Warm-Spitzer and Kepler [PDF]
, 2011 This paper reports the detection and the measurements of occultations of the two transiting hot giant exoplanets Kepler-5b and Kepler-6b by their parent stars. The observations are obtained in the near infrared with Spitzer Space Telescope and at optical
Borucki, William J. +15 more
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Physica Scripta, 1999 LaTex, 11 pages, 2 PostScript ...
Kaulakys, B., Vilutis, G.
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