ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

Searching for codes credited to 'Deleuil, M.'

Tip: Author search checks name variants (e.g., Smith, John, Smith J). Last names are still best when results are broad.

Found 3 codes.

[ascl:2412.027] mr-plotter: Mass-radius diagrams plotter
Castro-González, A.; Demangeon, O. D. S.; Lillo-Box, J.; Lovis, C.; Lavie, B.; Adibekyan, V.; Acuña, L.; Deleuil, M.; Aguichine, A.; Zapatero Osorio, M. R.; Tabernero, H. M.; Davoult, J.; Alibert, Y.; Santos, N.; Sousa, S. G.; Antoniadis-Karnavas, A.; Borsa, F.; Winn, J. N.; Allende Prieto, C.; Figueira, P.; Jenkins, J. M.; Sozzetti, A.; Damasso, M.; Silva, A. M.; Astudillo-Defru, N.; Barros, S. C. C.; Bonfils, X.; Cristiani, S.; Di Marcantonio, P.; González Hernández, J. I.; Curto, G. Lo; Martins, C. J. A. P.; Nunes, N. J.; Palle, E.; Pepe, F.; Seager, S.; Suárez Mascareño, A.
Mister plotter (mr-plotter) creates paper-quality mass-radius diagrams based on a wide range of state-of-the-art models of planetary interiors and atmospheres. It can be used to contextualize planets and infer their possible internal structures. It can also be used to search for correlations at a population level with its color-coding option based on any property collected in the NASA Exoplanet Archive, PlanetS, and Exoplanet.eu catalogs. mr-plotter can also produce article-ready two-column plots.
[ascl:2312.034] pycheops: Light curve analysis for ESA CHEOPS data
Maxted, P. F. L.; Ehrenreich, D.; Wilson, T. G.; Alibert, Y.; Cameron, A. Collier; Hoyer, S.; Sousa, S. G.; Olofsson, G.; Bekkelien, A.; Deline, A.; Delrez, L.; Bonfanti, A.; Borsato, L.; Alonso, R.; Anglada Escudé, G.; Barrado, D.; Barros, S. C. C.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Biondi, F.; Bonfils, X.; Brandeker, A.; Broeg, C.; Bárczy, T.; Cabrera, J.; Charnoz, S.; Corral Van Damme, C.; Csizmadia, Sz; Davies, M. B.; Deleuil, M.; Demangeon, O. D. S.; Demory, B. -O.; Erikson, A.; Florén, H. G.; Fortier, A.; Fossati, L.; Fridlund, M.; Futyan, D.; Gandolfi, D.; Gillon, M.; Guedel, M.; Guterman, P.; Heng, K.; Isaak, K. G.; Kiss, L.; Laskar, J.; Lecavelier des Etangs, A.; Lendl, M.; Lovis, C.; Magrin, D.; Nascimbeni, V.; Ottensamer, R.; Pagano, I.; Pallé, E.; Peter, G.; Piotto, G.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Reimers, C.; Ribas, I.; Salmon, S.; Santos, N. C.; Scandariato, G.; Simon, A. E.; Smith, A. M. S.; Steller, M.; Swayne, M. I.; Szabó, Gy M.; Ségransan, D.; Thomas, N.; Udry, S.; Van Grootel, V.; Walton, N. A.
pycheops analyzes CHEOPS light curve data. The models in the package can also be applied to other types of data. pycheops includes a "cook book" and examples; in addition, it provides a command-line tool that aids in the preparation of observing requests for CHEOPS observers.
[ascl:2006.015] ARCHI: Add-on pipeline module for background star analysis from CHEOPS data
Silva, André M.; Sousa, Sérgio G.; Santos, Nuno; Demangeon, Olivier D. S.; Silva, Pedro; Hoyer, S.; Guterman, P.; Deleuil, Magali; Ehrenreich, David
The CHaracterizing ExOPlanet Satellite (CHEOPS) mission pipeline provides photometry for the central star in its field; ARCHI takes in data from the CHEOPS mission pipeline, analyzes the background stars, and determines the photometry of these stars, thus creating the possibility of producing photometric time-series of several close-by targets at once, in addition to using different stars in the image to calibrate systematic errors.