Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora: Carme Jordi NebotThis is a research study on how the open clusters parallax measurements can be affected by different biases using the precision of Gaia satellite. In order to carry on this project, NGC6705 and NGC2682 data has been used. As a result, there are some deviations between observed and true parallax when magnitude and = o cutoffs are applied from different observation distances
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
We derive Bayesian distances for all stars in the radial velocity sample of Gaia DR2, and use the st...
Context. The early-third Gaia data release (EDR3) parallaxes constitute the most detailed and accura...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: ...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2015, Tutor: J...
Context. With the third release of the high-precision optical-wavelength Gaia survey, we are in a be...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
Aims. This paper has two main objectives: (1) To determine the intrinsic properties of 16 faint and ...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: ...
© 2017 ESO. Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS)...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
© 2017 ESO. Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS)...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
We derive Bayesian distances for all stars in the radial velocity sample of Gaia DR2, and use the st...
Context. The early-third Gaia data release (EDR3) parallaxes constitute the most detailed and accura...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: ...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2015, Tutor: J...
Context. With the third release of the high-precision optical-wavelength Gaia survey, we are in a be...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
Aims. This paper has two main objectives: (1) To determine the intrinsic properties of 16 faint and ...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: ...
© 2017 ESO. Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS)...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...
© 2017 ESO. Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS)...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a ...