The Leiden Atomic and Molecular Database (LAMDA) collects spectroscopic information and collisional rate coefficients for molecules, atoms, and ions of astrophysical and astrochemical interest. We describe the developments of the database since its inception in 2005, and outline our plans for the near future. Such a database is constrained both by the nature of its uses and by the availability of accurate data: we suggest ways to improve the synergies among users and suppliers of data. We summarize some recent developments in computation of collisional cross sections and rate coefficients. We consider atomic and molecular data that are needed to support astrophysics and astrochemistry with upcoming instruments that operate in the mid- and f...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
The BASECOL2012 database is a repository of collisional data and a web service within the Virtual At...
International audienceAnalysis of light emission from different regions of the interstellar medium a...
The Leiden Atomic and Molecular Database (LAMDA) collects spectroscopic information and collisional ...
The Leiden Atomic and Molecular Database (LAMDA) collects spectroscopic information and collisional ...
Spectroscopy has been crucial for our understanding of physical and chemical phenomena. The interpre...
Atomic and molecular (A&M) databases that contain information about species, their identities and ra...
The building of on-line atomic and molecular databases for astrophysics and for other applications f...
A large variety of atomic and molecular (A&M) data is used in astrophysics, both for the analysis of...
Atomic and molecular data for the transitions of a number of astrophysically interesting species are...
CHIANTI is an atomic database and software package for modeling emission lines and continua from hot...
Atomic and molecular data for the transitions of a number of astrophysically interesting species ar...
We describe recent work at NIST to develop and maintain databases for spectra, transition probabilit...
When we began this work, very few of the atomic and molecular data used by astronomers in the analys...
The estimation of molecular abundances in interstellar clouds from spectroscopic observations requir...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
The BASECOL2012 database is a repository of collisional data and a web service within the Virtual At...
International audienceAnalysis of light emission from different regions of the interstellar medium a...
The Leiden Atomic and Molecular Database (LAMDA) collects spectroscopic information and collisional ...
The Leiden Atomic and Molecular Database (LAMDA) collects spectroscopic information and collisional ...
Spectroscopy has been crucial for our understanding of physical and chemical phenomena. The interpre...
Atomic and molecular (A&M) databases that contain information about species, their identities and ra...
The building of on-line atomic and molecular databases for astrophysics and for other applications f...
A large variety of atomic and molecular (A&M) data is used in astrophysics, both for the analysis of...
Atomic and molecular data for the transitions of a number of astrophysically interesting species are...
CHIANTI is an atomic database and software package for modeling emission lines and continua from hot...
Atomic and molecular data for the transitions of a number of astrophysically interesting species ar...
We describe recent work at NIST to develop and maintain databases for spectra, transition probabilit...
When we began this work, very few of the atomic and molecular data used by astronomers in the analys...
The estimation of molecular abundances in interstellar clouds from spectroscopic observations requir...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
The BASECOL2012 database is a repository of collisional data and a web service within the Virtual At...
International audienceAnalysis of light emission from different regions of the interstellar medium a...