Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Xavier Luri CarrascosoAn improvement in the estimation of distance and distance modulus cannot be achieved by only an enhancement of the precision of the trigonometric parallax, but with the correct statistical treatment of the parallaxes to derive these parameters. We aim to provide a recommendation regarding the distance estimators to be used for Gaia DR2 and onwards, as well as to rise awareness about the practice of unquestioningly inverting the parallax. We test the performance of two Bayesian and a frequentist methods over a simulated sample of 107 Gaia DR2 stars, using a specifically developed Python software. We conclude that the use ...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora:...
We study the kinematics of a sample of classical Cepheids younger than 120 Myr. For these stars, the...
Context. The early-third Gaia data release (EDR3) parallaxes constitute the most detailed and accura...
We derive Bayesian distances for all stars in the radial velocity sample of Gaia DR2, and use the st...
Context. The second Gaia.data release (Gaia DR2 ) provides precise five-parameter astrometric data (...
International audienceContext. The second Gaia data release (Gaia DR2) provides precise five-paramet...
Context. The second Gaia data release (Gaia DR2) provides precise five-parameter astrometric data (p...
For the vast majority of stars in the second Gaia data release, reliable distances cannot be obtaine...
In this thesis, we present distance measurements to embedded stars by using the wealth of astrometri...
We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc...
The datasets are described in https://arxiv.org/abs/1902.02355 , which is submitted to MNRAS. Each ...
The Gaia spacecraft has just released a large set of parallaxes, including 41 novae for which the fr...
The Gaia mission measures accurate proper motions and parallax distances to millions of stars, inclu...
Context. Estimating the distances to asymptotic giant branch (AGB) stars using optical measurements ...
Distance estimates used by "Gaia Early Data Release 3: The Galactic anticentre", Gaia Collaboration,...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora:...
We study the kinematics of a sample of classical Cepheids younger than 120 Myr. For these stars, the...
Context. The early-third Gaia data release (EDR3) parallaxes constitute the most detailed and accura...
We derive Bayesian distances for all stars in the radial velocity sample of Gaia DR2, and use the st...
Context. The second Gaia.data release (Gaia DR2 ) provides precise five-parameter astrometric data (...
International audienceContext. The second Gaia data release (Gaia DR2) provides precise five-paramet...
Context. The second Gaia data release (Gaia DR2) provides precise five-parameter astrometric data (p...
For the vast majority of stars in the second Gaia data release, reliable distances cannot be obtaine...
In this thesis, we present distance measurements to embedded stars by using the wealth of astrometri...
We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc...
The datasets are described in https://arxiv.org/abs/1902.02355 , which is submitted to MNRAS. Each ...
The Gaia spacecraft has just released a large set of parallaxes, including 41 novae for which the fr...
The Gaia mission measures accurate proper motions and parallax distances to millions of stars, inclu...
Context. Estimating the distances to asymptotic giant branch (AGB) stars using optical measurements ...
Distance estimates used by "Gaia Early Data Release 3: The Galactic anticentre", Gaia Collaboration,...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora:...
We study the kinematics of a sample of classical Cepheids younger than 120 Myr. For these stars, the...
Context. The early-third Gaia data release (EDR3) parallaxes constitute the most detailed and accura...