Results 121 to 130 of about 1,692 (157)

Clusterix 2.0: A Virtual Observatory Tool to Estimate Cluster Membership Probability [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT Clusterix 2.0 is a web-based, Virtual Observatory compliant, interactive tool for the determination of membership probabilities in stellar clusters based on proper-motion data using a fully non-parametric method. In an area occupied by a cluster, the frequency function is made up of two contributions: cluster and field stars ...
Carme Jordi   +2 more
exaly   +7 more sources

Tesela: A New Virtual Observatory Tool to Determine Blank Fields for Astronomical Observations [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2011
Accepted for publication in Monthly Notices of the Royal Astronomical Society. 11 pages, 10 figures.
F M Jiménez-Esteban   +2 more
exaly   +5 more sources

Interoperability Tools for the Virtual Observatory

open access: yes, 2001
Interoperability is one of the key issues in the current efforts to build the Virtual Observatory. We present here some of the tools which already contribute to the efficient exchange of information between archives, databases, and journals.
Daniel Egret
exaly   +3 more sources

A Proper Motion Study of the Lupus Clouds Using Virtual Observatory Tools [PDF]

open access: yesAstronomy and Astrophysics, 2011
Context. The Lupus dark cloud complex is a well-known, nearby low-mass star-forming region, probably associated with the Gould Belt. In recent years, the number of stellar and substellar Lupus candidate members has been remarkably increased thanks to the Cores to Disks (c2d) Spitzer Legacy Program and other studies.
Fran Jiménez-Esteban, Enrique Solano
exaly   +2 more sources

A Search for New Hot Subdwarf Stars by Means of Virtual Observatory Tools [PDF]

open access: yesAstronomy and Astrophysics, 2011
13 pages, 7 ...
Cristina Rodriguez-Lopez   +2 more
exaly   +4 more sources

A Search for New Hot Subdwarf Stars by Means of Virtual Observatory Tools II [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
Recent massive sky surveys in different bandwidths are providing new opportunities to modern astronomy. The Virtual Observatory (VO) represents the adequate framework to handle the huge amount of information available and filter out data according to specific requirements.
Ana Ulla, Enrique Solano, R Oreiro
exaly   +4 more sources

WISE/2MASS-SDSS Brown Dwarfs Candidates Using Virtual Observatory Tools [PDF]

open access: yesAstronomy and Astrophysics, 2011
Accepted in A&A.
Enrique Solano, M Aberasturi
exaly   +3 more sources

Galaxy morphologies analysis using Virtual Observatory tools

2022
In this project we will be using observatory tools to study the photometric and spectroscopic properties of different galaxy morphologies. We will look into a little about galaxies and their different morphological classifications. We study the different aspects that affect galaxy morphology. We will learn about virtual observatory tools and how to use
Pillay, Dhersan, Bouchefry, Khadija El
openaire   +1 more source

J-Plus: Discovery and Characterisation of Ultracool Dwarfs Using Virtual Observatory Tools [PDF]

open access: yesAstronomy and Astrophysics, 2019
Context. Ultracool dwarfs are objects with spectral types equal to or later than M7. Most of them have been discovered using wide-field imaging surveys. The Virtual Observatory has proven to be very useful for efficiently exploiting these astronomical resources. Aims.
David Sobral   +2 more
exaly   +6 more sources

Multidimensional indexing tools for the virtual observatory

Astronomische Nachrichten, 2007
AbstractThe last decade has seen a dramatic change in the way astronomy is carried out. The dawn of the the new microelectronic devices, like CCDs has dramatically extended the amount of observed data. Large, in some cases all sky surveys emerged in almost all the wavelength ranges of the observable spectrum of electromagnetic waves.
I. Csabai   +7 more
openaire   +1 more source

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