Zobrazeno 1 - 10
of 2 517
pro vyhledávání: '"LORENZO, V."'
Comparing transit spectroscopy pipelines at the catalogue level: evidence for systematic differences
Publikováno v:
MNRAS, Volume 531, Issue 1, June 2024, Pages 35-51
The challenge of inconsistent results from different data pipelines, even when starting from identical data, is a recognized concern in exoplanetary science. As we transition into the James Webb Space Telescope (JWST) era and prepare for the ARIEL sp
Externí odkaz:
http://arxiv.org/abs/2402.15803
Autor:
Jaziri, Adam Yassin, Pluriel, William, Bocchieri, Andrea, Panek, Emilie, Teinturier, Lucas, Ivanova, Anastasiia, Rektsini, Natalia E., Drossart, Pierre, Beaulieu, Jean-Philippe, Falco, Aurélien, Leconte, Jeremy, Mugnai, Lorenzo V., Venot, Olivia
Publikováno v:
A&A, 684 (2024) A25
Observed exoplanet transit spectra are usually retrieved using 1D models to determine atmospheric composition while planetary atmospheres are 3D. With the JWST and future space telescopes such as Ariel, we will be able to obtain increasingly accurate
Externí odkaz:
http://arxiv.org/abs/2401.03809
The Ariel Space Mission aims to observe a diverse sample of exoplanet atmospheres across a wide wavelength range of 0.5 to 7.8 microns. The observations are organized into four Tiers, with Tier 1 being a reconnaissance survey. This Tier is designed t
Externí odkaz:
http://arxiv.org/abs/2309.06817
Autor:
Tiffany A. Kosch, María Torres-Sánchez, H. Christoph Liedtke, Kyle Summers, Maximina H. Yun, Andrew J. Crawford, Simon T. Maddock, Md. Sabbir Ahammed, Victor L. N. Araújo, Lorenzo V. Bertola, Gary M. Bucciarelli, Albert Carné, Céline M. Carneiro, Kin O. Chan, Ying Chen, Angelica Crottini, Jessica M. da Silva, Robert D. Denton, Carolin Dittrich, Gonçalo Espregueira Themudo, Katherine A. Farquharson, Natalie J. Forsdick, Edward Gilbert, Jing Che, Barbara A. Katzenback, Ramachandran Kotharambath, Nicholas A. Levis, Roberto Márquez, Glib Mazepa, Kevin P. Mulder, Hendrik Müller, Mary J. O’Connell, Pablo Orozco-terWengel, Gemma Palomar, Alice Petzold, David W. Pfennig, Karin S. Pfennig, Michael S. Reichert, Jacques Robert, Mark D. Scherz, Karen Siu-Ting, Anthony A. Snead, Matthias Stöck, Adam M. M. Stuckert, Jennifer L. Stynoski, Rebecca D. Tarvin, Katharina C. Wollenberg Valero, The Amphibian Genomics Consortium
Publikováno v:
BMC Genomics, Vol 25, Iss 1, Pp 1-19 (2024)
Abstract Amphibians represent a diverse group of tetrapods, marked by deep divergence times between their three systematic orders and families. Studying amphibian biology through the genomics lens increases our understanding of the features of this a
Externí odkaz:
https://doaj.org/article/0868fe54848f4903803e6af94a2fabda
RAPOC (Rosseland and Planck Opacity Converter) is a Python 3 code that calculates Rosseland and Planck mean opacities (RPMs) from wavelength-dependent opacities for a given temperature, pressure, and wavelength range. In addition to being user-friend
Externí odkaz:
http://arxiv.org/abs/2209.07535
Autor:
Lorenzo, V.
Minimal algebraic surfaces of general type $X$ such that $K^2_X=2\chi(\mathcal{O}_X)-6$ are called Horikawa surfaces. In this note the group of automorphisms of Horikawa surfaces is studied. The main result states that given an admissible pair $(K^2,
Externí odkaz:
http://arxiv.org/abs/2201.04890
Autor:
Mugnai, Lorenzo V., Al-Refaie, Ahmed, Bocchieri, Andrea, Changeat, Quentin, Pascale, Enzo, Tinetti, Giovanna
The ARIEL Space Telescope will provide a large and diverse sample of exoplanet spectra, performing spectroscopic observations of about 1000 exoplanets in the wavelength range $0.5 \to 7.8 \; \mu m$. In this paper, we investigate the information conte
Externí odkaz:
http://arxiv.org/abs/2110.00503
Autor:
Mugnai, Lorenzo V., Modirrousta-Galian, Darius, Edwards, Billy, Changeat, Quentin, Bouwman, Jeroen, Morello, Giuseppe, Al-Refaie, Ahmed, Baeyens, Robin, Bieger, Michelle Fabienne, Blain, Doriann, Gressier, Amélie, Guilluy, Gloria, Jaziri, Yassin, Kiefer, Flavien, Morvan, Mario, Pluriel, William, Poveda, Mathilde, Skaf, Nour, Whiteford, Niall, Wright, Sam, Yip, Kai Hou, Zingales, Tiziano, Charnay, Benjamin, Drossart, Pierre, Leconte, Jérémy, Venot, Olivia, Waldmann, Ingo, Beaulieu, Jean-Philippe
We present a study on the spatially scanned spectroscopic observations of the transit of GJ 1132 b, a warm ($\sim$500 K) Super-Earth (1.13 R$_\oplus$) that was obtained with the G141 grism (1.125 - 1.650 $\mu$m) of the Wide Field Camera 3 (WFC3) onbo
Externí odkaz:
http://arxiv.org/abs/2104.01873
Autor:
Charnay, Benjamin, Mendonça, Joao M., Kreidberg, Laura, Cowan, Nicolas B., Taylor, Jake, Bell, Taylor J., Demangeon, Olivier, Edwards, Billy, Haswell, Carole A., Morello, Giuseppe, Mugnai, Lorenzo V., Pascale, Enzo, Tinetti, Giovanna, Tremblin, Pascal, Zellem, Robert T.
The ESA-Ariel mission will include a tier dedicated to exoplanet phase curves corresponding to ~10% of the science time. We present here the current observing strategy for studying exoplanet phase curves with Ariel. We define science questions, requi
Externí odkaz:
http://arxiv.org/abs/2102.06523
Autor:
Kokori, Anastasia, Tsiaras, Angelos, Edwards, Billy, Rocchetto, Marco, Tinetti, Giovanna, Wünsche, Anaël, Paschalis, Nikolaos, Agnihotri, Vikrant Kumar, Bachschmidt, Matthieu, Bretton, Marc, Caines, Hamish, Caló, Mauro, Casali, Roland, Crow, Martin, Dawes, Simon, Deldem, Marc, Deligeorgopoulos, Dimitrios, Dymock, Roger, Evans, Phil, Falco, Carmelo, Ferratfiat, Stephane, Fowler, Martin, Futcher, Stephen, Guerra, Pere, Hurter, Francois, Jones, Adrian, Kang, Wonseok, Kim, Taewoo, Lee, Richard, Lopresti, Claudio, Marino, Antonio, Mallonn, Matthias, Mortari, Fabio, Morvan, Mario, Mugnai, Lorenzo V., Nastasi, Alessandro, Perroud, Valère, Pereira, Cédric, Phillips, Mark, Pintr, Pavel, Raetz, Manfred, Regembal, Francois, Savage, John, Sedita, Danilo, Sioulas, Nick, Strikis, Iakovos, Thurston, Geoffrey, Tomacelli, Andrea, Tomatis, Alberto
The Ariel mission will observe spectroscopically around 1000 exoplanets to further characterise their atmospheres. For the mission to be as efficient as possible, a good knowledge of the planets' ephemerides is needed before its launch in 2028. While
Externí odkaz:
http://arxiv.org/abs/2012.07478