papers

Publications (8)

astro-ph.SR2018

Fundamental parameter accuracy of DA and DB white dwarfs in Gaia Data Release 2

P. -E. Tremblay, E. Cukanovaite, N. P. Gentile Fusillo +2

We report on a comparison of spectroscopic analyses for hydrogen (DA) and helium atmosphere (DB) white dwarfs with Gaia Data Release 2 (DR2) parallaxes and photometry. We assume a…

astro-ph.SR2023

Main sequence companions to white dwarfs II: the age-activity-rotation relation from a sample of Gaia common proper motion pairs

A. Rebassa-Mansergas, J. Maldonado, R. Raddi +8

Magnetic activity and rotation are related to the age of low-mass main sequence stars. To further constrain these relations, we study a sample of 574 main sequence stars members of…

astro-ph.SR2022

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.SR2020

white dwarfs within 40 pc I: spectroscopic observations of new candidates

P. -E. Tremblay, M. A. Hollands, N. P. Gentile Fusillo +30

We present a spectroscopic survey of 230 white dwarf candidates within 40 pc of the Sun from the William Herschel Telescope and Gran Telescopio Canarias. All candidates were select…

astro-ph.SR2022

Kinematic properties of white dwarfs. Galactic orbital parameters and age-velocity dispersion relation

R. Raddi, S. Torres, A. Rebassa-Mansergas +9

We present the first detailed 3D kinematic analysis of a sample of 3133 white dwarfs that use Gaia astrometry plus radial velocities, which were measured either by Gaia or by groun…

math-ph2023

Singularities and asymptotic distribution of resonances for Schrödinger operators in one dimension

T. J. Christiansen, T. Cunningham

We obtain new results about the high-energy distribution of resonances for the one-dimensional Schrödinger operator. Our primary result is an upper bound on the density of resonan…