![]() We find a fraction of heavy elements of 0.13 −0.06 +0.05 and metal enrichment of the planet ( Z P/ Z star) of 4.2 −2.0 +1.6. The eccentricity of 0.325 ± 0.020 and an orbital separation of 0.0888 ± 0.0010 AU from its host star suggest that the planet is likely undergoing high-eccentricity tidal migration. It lies in the transition mass region of massive giant planets and low-mass brown dwarfs, an important addition to the population of fewer than five known objects in this mass range. This makes it one of the few known massive giant planets with an extreme density. ![]() Using radial velocity measurements with the PARAS and TRES spectrographs, we determined the planet’s mass to be 12.89 −0.57 +0.58 M J, resulting in a bulk density of 14.1 −1.6 +1.7 g cm −3. We present the discovery of a transiting massive giant planet around TOI-4603, a sub-giant F-type star from NASA’s Transiting Exoplanet Survey Satellite (TESS). Physikalisches Institut, University of Bern, GesellsschaftstraBern, SwitzerlandĬenter for Astrophysics | Harvard & Smithsonian, 60 Garden St., Cambridge, MA 02138, USA NASA Exoplanet Science Institute, Caltech/IPAC, Pasadena, CA 91125, USA Observatoire de Genève, Université de Genève, Chemin Pegasi, 51, 1290 Versoix, Switzerland Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany Prasad 1, Ashirbad Nayak 1, Monika Lendl 4 and Christoph Mordasini 6Īstronomy & Astrophysics Division, Physical Research Laboratory, Ahmedabad 380009, IndiaĮ-mail: Institute of Technology, 382355 Gandhinagar, India Boyle 5, Sanjay Baliwal 1 ,2, Allyson Bieryla 7, David W. Astronomical objects: linking to databasesĪkanksha Khandelwal 1 ,2, Rishikesh Sharma 1, Abhijit Chakraborty 1, Priyanka Chaturvedi 3, Solène Ulmer-Moll 4 ,6, David R.Including author names using non-Roman alphabets.Suggested resources for more tips on language editing in the sciences Punctuation and style concerns regarding equations, figures, tables, and footnotes The query language allows for basic unit conversions for columns that have associated units. Takes the ceiling of the passed in number Inverse Trigonometric Tangent, returns radiansĬ-like arctangent, takes two arguments and returns radians Inverse Trigonometric Cosine, returns radians Inverse Trigonometric Sine, returns radians !(RECON & ADAPTIVE) or NOT (RECON AND ADAPTIVE) N_OBJ = 2 || N_OBJ = 3 or N_OBJ = 2 OR N_OBJ = 3 The following operations and functions are supported by the query language. Here are some examples:Ĭomputes the KOI's orbital velocity in units of meters-per-second. This quantity can then be plotted against other numerical quantities, or presented in the table. In this context, KOI properties can be combined mathematically in order to yield a new numerical quantity for each KOI. The query language is also used, however, when constructing custom scatter and histogram plots in the Plotter and custom columns in the table. This behavior is appropriate in the context of filters. The query language supports a number of common mathematical functions.Īll of the above examples combine and compare planet properties in order to ultimately produce a true or false cut on each planet in the Kepler database. Note the use of the sqrt and cos functions. This is accomplished by computing the angular distane in degrees between each planet's RA and DEC coordinate and the point (285, 41) using the spherical coordinate metric. Selects all planets that lie (roughly) within one degree of the coordinate RA=19h, DEC=41°. If you would rather jump to a list of available operations and functions skip to below. Perhaps the simplest way to introduce the query language is to present some examples. The former is used in the Table and Plotter to select a subset of planets to view, the latter is used in the plotter to produce scatter plots and histograms of combinations of planet properties and in the table to construct custom columns. ![]() The query language is used in two distinct contexts: to construct filters and to combine and transform planet properties to create new quantities. Advanced users who would like to leverage the full flexibility of the Kepler Data Explorer should peruse this section of the documentation to familiarize themselves with the query language. ![]() This latter, more advanced feature, is made possible through a simple query language that is built into the table and plotter components. The Kepler Data Explorer has been designed with two goals in mind: to make access to the Kepler Database fun and straightforward, and to enable users to quickly build customizable, powerful, and useful filters and views of the dataset.
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