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Ennio Poretti (Istituto Nazionale di Astrofisica (INAF))04/05/2020, 09:30
The status of the programs on the exoplanets at TNG will be reviewed, with a particular emphasis on the current difficult situation.
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Rosario Cosentino (Istituto Nazionale di Astrofisica (INAF))04/05/2020, 09:55
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Dr Riccardo Claudi04/05/2020, 10:15
In questo contributo sono riportate le statistiche delle notti di osservazione dall'inizio del long program GAPS2.0. In particolare, vengono mostrate le statistiche relative al run AOT40 (appena finito) e quelle relative al run AOT41 (appena cominciato).
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Matteo Brogi04/05/2020, 10:35
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Alessandro Sozzetti04/05/2020, 10:55
Breve discussione di analisi dei programmi GAPS1 ancora pendenti.
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Matteo Pinamonti (Istituto Nazionale di Astrofisica (INAF))04/05/2020, 11:05
Updates/results from GAPS1-HADES
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Antonio Maggio (Istituto Nazionale di Astrofisica (INAF))04/05/2020, 11:20
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Dr Serena Benatti (Istituto Nazionale di Astrofisica (INAF))04/05/2020, 14:30
Sommario delle osservazioni, del campione stellare e delle attivita' del programma Young Objects, inclusa la definizione delle criticita' rilevate.
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Mr Mario Damasso (INAF-OATo)04/05/2020, 14:50
I will present the results for V830 Tau after the third observing season with HARPS-N came to an end. The talk will be structured following the emerging structure of the draft in preparation, highlighting the concept and the main points to be addressed in the publication.
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Luca Malavolta (Università degli Studi di Padova)04/05/2020, 15:10
I'll give a brief summary of the status of the analysis of the Young Object target YO14
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Dr Riccardo Claudi04/05/2020, 15:30
YO36 è una stella giovane attorno nella curva di luce K2 della quale sono stati osservati i transiti di quattro oggetti diversi. La stella è molto attiva e le misure di Velocità Radiale ottenute fin'ora non sembrano mostrare segnali kepleriani.
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Ilaria Carleo04/05/2020, 15:50
Here we present a validation study for the TESS object of interest TOI-942. We performed a follow-up of this object with HARPS-N, collecting about 30 spectra. The HARPS-N spectra allow us to characterise the star and confirm the presence of the planet.
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ALL04/05/2020, 16:10
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Aldo Stefano Bonomo (Istituto Nazionale di Astrofisica (INAF)), Valerio Nascimbeni (INAF-OAPD)05/05/2020, 09:30
A general introduction about the current state of the VIS/NIR observations and analysis, and the future prospects
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Daniela Sicilia (Università di Padova)05/05/2020, 09:45
Update on the VIS analysis with SLOPpy
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Gaetano Scandariato (Istituto Nazionale di Astrofisica (INAF))05/05/2020, 10:05
Reflected light from 51 Peg b
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Monica Rainer (Istituto Nazionale di Astrofisica (INAF))05/05/2020, 10:25
Atmospheric RML effect of KELT-20b
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Francesco Borsa (Istituto Nazionale di Astrofisica (INAF))05/05/2020, 10:45
H-alpha absorption on WASP-33b
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Paolo Giacobbe (Istituto Nazionale di Astrofisica (INAF))05/05/2020, 11:05
By performing high-resolution transmission spectroscopy with GIANO-B over the whole near-infrared, we measured the signature of seven molecular species via cross correlation with model spectra.
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Gloria Guilluy (Istituto Nazionale di Astrofisica (INAF))05/05/2020, 11:25
Here we report preliminary results of the atmospheric studies we performed on the three warm giant planets, Wasp-69b, Wasp-107b and Wasp-80b. By using the PCA technique, and the cross-correlation method, we succeeded in detecting 7 molecules in these exo-atmospheres. Given the low temperature of the investigated exoplanets, some of these molecules are un-expected by equilibrium theories, we...
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Matteo Brogi (University of Warwick)05/05/2020, 14:30
Near-infrared high-resolution spectroscopy relies on cross correlation with model spectra to extract information about the chemical and physical conditions of exoplanet atmospheres. In this talk I will review recent efforts to identify the most reliable molecular line lists applicable to simulate the high temperatures of extrasolar planets. Furthermore, I will explain how GIANO could be used...
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Darius Modirrousta Galian (Istituto Nazionale di Astrofisica (INAF))05/05/2020, 14:50
In the talk we will discuss the effects of X-ray and ultraviolet radiation on atmospheric erosion around young stars. Specifically, we focus on the bimodal distribution of exoplanet radii (i.e. “The Fulton Gap”; Fulton et al. 2017). In Modirrousta-Galian et al. (2020,b) this distribution is theoretically analysed in order to make several predictions that can be astronomically tested. For...
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Daniele Locci05/05/2020, 15:10
The knowledge of planetary mass and radius of young planets is crucial in the understanding if their atmospheres can survive at the intense XUV stellar irradiation
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Alessandro Sozzetti05/05/2020, 15:30
I will summarize the status of the special objects program
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Matteo Pinamonti05/05/2020, 15:50
I will provide an update on M108
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Domenico Barbato05/05/2020, 16:05
I will provide an update on M109 and M112
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Laura Affer05/05/2020, 16:35
I will provide an update on the old GAPS1 M dwarfs followed as special objects
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Alessandro Sozzetti (Istituto Nazionale di Astrofisica (INAF))06/05/2020, 09:30
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Alessandro Sozzetti (Istituto Nazionale di Astrofisica (INAF))06/05/2020, 09:50
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Giampaolo Piotto06/05/2020, 10:10
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ALL06/05/2020, 10:30
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Martina Baratella (Università degli studi di Padova)06/05/2020, 14:30
The detailed characterisation of stars is important in many astrophysical fields. In particular, knowing with great precision the atmospheric parameters and chemical composition of planet hosting stars allows to fully characterise exoplanets and address a number of aspects, e.g. the planet-metallicity relation.
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In our work, we performed a precise determination of the atmospheric parameters... -
Jesus Maldonado Prado (Istituto Nazionale di Astrofisica (INAF))06/05/2020, 14:50
Methods to derive in a consistent way stellar abundances of low-mass stars from optical spectra are still missing. In this contribution we present a first attempt to fill this gap. Our methodology is based on the use of principal componen analysis and sparse Bayesian’s fitting methods. A set of M dwarfs in binary systems orbiting around an FGK primary was observed and is used to training our...
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Serena Benatti (Istituto Nazionale di Astrofisica (INAF))06/05/2020, 15:10
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Dr Riccardo Claudi06/05/2020, 15:30
In questo contributo è presentato lo stato dello studio dell'attività delle stelle ospite di pianeti transitanti. Sono trattati sistemi osservati duranti GAPS1.0 e confrontati con altri sistemi transitanti e stelle di campo.
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Giancluca Cracchiolo06/05/2020, 15:50
In my study, I analyze the impact of stellar spots on ARIEL observations and their effects on the extraction of the planetary signal from primary transit observations. I develop a method to determine the size and temperature of the spots by using the out-of-transit observations and I define a procedure to reliably extract the planetary spectrum in the presence of spots.
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ALL06/05/2020, 16:10
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Dr Matteo Pinamonti
I will provide an update on M112
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Alessandro Sozzetti
Discuteremo dello stato del programma e delle prospettive di evoluzione
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