activity
20022026
most citedThe peculiar nova V1309 Sco/Nova Sco 2008: A candidate twin of V838 Mon

61 citations · 406 across the 31 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2026

Cataclysmic Variables Photometric Periods from TESS

S. O. Kepler, Alejandra Daniela Romero, Larissa Luciano Amorim +1

We present a sample of coherent and stable photometric period determinations for cataclysmic variables, based on TESS photometry through sector 102. We analyzed a total of 1554 cat…

astro-ph.SR2023

A grid of Non-LTE line-blanketed atmosphere structures and synthetic spectra for subdwarfs

Thayse A. Pacheco, Ronaldo S. Levenhagen, Marcos P. Diaz +1

We present an update of the grid of detailed atmosphere models and homogeneous synthetic spectra for hot, high-gravity subdwarf stars. High-resolution spectra and synthetic photome…

astro-ph.IM2022★ 1 cited

The CUBES Science Case

Chris Evans, Stefano Cristiani, Cyrielle Opitom +51

We introduce the scientific motivations for the development of the Cassegrain U-Band Efficient Spectrograph (CUBES) that is now in construction for the Very Large Telescope. The as…

astro-ph.SR2022★ 11 cited

Detached eclipsing binaries from the Kepler field: radii and photometric masses of components in short-period systems

Patricia Cruz, John F. Aguilar, Hernán E. Garrido +2

The characterisation of detached eclipsing binaries with low mass components has become important when verifying the role of convection in stellar evolutionary models, which requir…

astro-ph.SR2021★ 6 cited

A Grid of Synthetic Spectra for Subdwarfs: Non-LTE line-blanketed atmosphere models

Thayse A. Pacheco, Marcos P. Diaz, Ronaldo S. Levenhagen +1

A new grid of detailed atmosphere model spectra for hot and moderately cool subdwarf stars is presented. High-resolution spectra and synthetic photometry are calculated in the rang…

astro-ph.SR2020★ 4 cited

The H line emission of the Be star Psc: the last 40 years

Ronaldo S. Levenhagen, Marcos P. Diaz, Eduardo B. Amôres +1

A study on the photosphere and disc of the Be star Psc is presented. We recover almost 40 years of high-resolution spectroscopic observations and additional data gathered from…