Exomoons to Galactic Structure

Exomoons to Galactic Structure: High Precision Studies with the Microlensing and Transit Methods (Repost)

Exomoons to Galactic Structure: High Precision Studies with the Microlensing and Transit Methods By Supachai Awiphan
English | PDF,EPUB | 2018 | 206 Pages | ISBN : 3319909568 | 19.09 MB

This book presents three major studies covering exomoon and exoplanet detection and characterisation. Firstly, it reports the observations and analysis of the atmosphere of the hot Neptune GJ3470b, one of the lowest-mass planets with a measured atmosphere, using transmission spectroscopy techniques. The result provided improved measurements of Rayleigh scattering in the atmosphere and the first limits on additional planetary companions in the system.
Exomoons to Galactic Structure: High Precision Studies with the Microlensing and Transit Methods (Repost)

Exomoons to Galactic Structure: High Precision Studies with the Microlensing and Transit Methods By Supachai Awiphan
English | PDF,EPUB | 2018 | 206 Pages | ISBN : 3319909568 | 19.09 MB

This book presents three major studies covering exomoon and exoplanet detection and characterisation. Firstly, it reports the observations and analysis of the atmosphere of the hot Neptune GJ3470b, one of the lowest-mass planets with a measured atmosphere, using transmission spectroscopy techniques. The result provided improved measurements of Rayleigh scattering in the atmosphere and the first limits on additional planetary companions in the system.
Exomoons to Galactic Structure: High Precision Studies with the Microlensing and Transit Methods

Exomoons to Galactic Structure: High Precision Studies with the Microlensing and Transit Methods By Supachai Awiphan
English | PDF,EPUB | 2018 | 206 Pages | ISBN : 3319909568 | 19.09 MB

This book presents three major studies covering exomoon and exoplanet detection and characterisation. Firstly, it reports the observations and analysis of the atmosphere of the hot Neptune GJ3470b, one of the lowest-mass planets with a measured atmosphere, using transmission spectroscopy techniques. The result provided improved measurements of Rayleigh scattering in the atmosphere and the first limits on additional planetary companions in the system.