Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Dietrich, Jeremy"'
The minimum orbital separation of planets in long-stable planetary systems is often modeled as a step function, parameterized with a single value $\Delta_{min}$ (measured in mutual Hill radius of the two neighboring planets). Systems with smaller sep
Externí odkaz:
http://arxiv.org/abs/2312.02349
Autor:
Dietrich, Jeremy, Apai, Dániel, Schlecker, Martin, Hardegree-Ullman, Kevin K., Rackham, Benjamin V., Kurtovic, Nicolas, Molaverdikhani, Karan, Gabor, Paul, Henning, Thomas, Chen, Wen-Ping, Mancini, Luigi, Bixel, Alex, Gibbs, Aidan, Boyle, Richard P., Brown-Sevilla, Samantha, Burn, Remo, Delage, Timmy N., Flores-Rivera, Lizxandra, Franceschi, Riccardo, Pichierri, Gabriele, Savvidou, Sofia, Syed, Jonas, Bruni, Ivan, Ip, Wing-Huen, Ngeow, Chow-Choong, Tsai, An-Li, Lin, Chia-Lung, Hou, Wei-Jie, Hsiao, Hsiang-Yao, Lin, Chi-Sheng, Lin, Hung-Chin, Basant, Ritvik
Earth-sized exoplanets that transit nearby, late spectral type red dwarfs will be prime targets for atmospheric characterization in the coming decade. Such systems, however, are difficult to find via wide-field transit surveys like Kepler or TESS. Co
Externí odkaz:
http://arxiv.org/abs/2302.04138
e Eridani, the fifth-closest Sun-like star, hosts at least three planets and could possibly harbor more. However, the veracity of the planet candidates in the system and its full planetary architecture remain unknown. Here we analyze the planetary ar
Externí odkaz:
http://arxiv.org/abs/2205.06250
Planetary architectures remain unexplored for the vast majority of exoplanetary systems, even among the closest ones, with potentially hundreds of planets still ``hidden" from our knowledge. DYNAMITE is a powerful software package that can predict th
Externí odkaz:
http://arxiv.org/abs/2112.05337
Herbig Ae/Be stars represent the early outcomes of star formation and the initial stages of planet formation at intermediate stellar masses. Understanding both of these processes requires detailed characterization of their disk structures and compani
Externí odkaz:
http://arxiv.org/abs/2011.07082
Autor:
Dietrich, Jeremy, Apai, Dániel
tau Ceti is the closest single Sun-like star to the solar system and hosts a multi-planet system with four confirmed planets. The possible presence of additional planets, especially potentially habitable worlds, remains of great interest. We analyze
Externí odkaz:
http://arxiv.org/abs/2010.14675
Autor:
P., Andrés F. Ramos, Ashby, M. L. N., Smith, Howard A., Martínez-Galarza, Juan R., Beverage, Aliza G., Dietrich, Jeremy, Higuera-G., Mario-A., Weiner, Aaron S.
Emission from active galactic nuclei (AGNs) is known to play an important role in the evolution of many galaxies including luminous and ultraluminous systems (U/LIRGs), as well as merging systems. However, the extent, duration, and exact effects of i
Externí odkaz:
http://arxiv.org/abs/2009.05614
Autor:
Dietrich, Jeremy, Apai, Daniel
Multi-planet systems produce a wealth of information for exoplanet science, but our understanding of planetary architectures is incomplete. Probing these systems further will provide insight into orbital architectures and formation pathways. Here we
Externí odkaz:
http://arxiv.org/abs/2007.06745
Autor:
Gibbs, Aidan, Bixel, Alex, Rackham, Benjamin, Apai, Daniel, Schlecker, Martin, Espinoza, Nestor, Mancini, Luigi, Chen, Wen-Ping, Henning, Thomas, Gabor, Paul, Boyle, Richard, Chavez, Jose Perez, Mousseau, Allie, Dietrich, Jeremy, Socia, Quentin Jay, Ip, Wing, Ngeow, Chow-Choong, Tsai, Anli, Bhandare, Asmita, Marian, Victor, Baehr, Hans, Brown, Samantha, Haberle, Maximilian, Keppler, Miriam, Molaverdikhani, Karan, Sarkis, Paula
Small planets are common around late-M dwarfs and can be detected through highly precise photometry by the transit method. Planets orbiting nearby stars are particularly important as they are often the best-suited for future follow-up studies. We pre
Externí odkaz:
http://arxiv.org/abs/2002.10017
Autor:
Lopez-Morales, Mercedes, Ben-Ami, Sagi, Gonzalez-Abad, Gonzalo, Garcia-Mejia, Juliana, Dietrich, Jeremy, Szentgyorgyi, Andrew
We present the result of calculations to optimize the search for molecular oxygen (O2) in Earth analogs transiting around nearby, low-mass stars using ground-based, high-resolution, Doppler shift techniques. We investigate a series of parameters, nam
Externí odkaz:
http://arxiv.org/abs/1905.05862