Search this site
Skip to main content
Skip to navigation
ACO
Home
Project
ESR Thesis subjects
ESR 1
ESR 2
ESR 3
ESR 4
ESR 5
ESR 6
ESR 7
ESR 8
ESR 9
ESR 10
ESR 11
ESR 12
ESR 13
ESR 14
ESR 15
ESR 16
ESR 17
ACO in a nutshell
ACO Science
ACO Objectives
Events
ACO Meetings
ACO Supervisory Board Meeting 2023
ACO Network meeting Year3
ACO Schools
ACO Year 3 School
ACO Virtual Reality School
ACO Year 2 School
ACO Year 1 School
Program
ACO Congresses
ACO Congress Year 2
ACO Congress Year 4
ACO Organized Events
FAUST @ IPAG, Sep 2022
FAUST meeting venue
Hotels in Grenoble
FAUST participants
ACO Trainings
Team
People
Organization
ACO recruited ESRs
ACO public datasets
ASTRONOMICAL OBSERVATIONS
CHESS observations
ASAI observations
SOLIS observations
FAUST observations
THEORETICAL CHEMISTRY CALCULATIONS
Cations structures Scripts
Software Packages
Atomic coordinates of the periodic amorphous ice grain model
Atomic coordinates of the structures of iCOMs adsorbed at the surface of a
Atomic coordinates of the structures of iCOMs adsorbed at the surface of an
Absolute reactive cross sections for the reactions of methanimine radical c
GFN2-xTB structures of iCOM adsorbed on a cluster model of water molecules
Structures and Properties of Known and Postulated Interstellar Cations
Where does the energy go during the interstellar NH3 formation on water ice
Harmonic vibrational frequencies of the structures of iCOMs adsorbed at the
Amorphous grain model of interstellar icy grains
ACO-FROST: generation of icy grain models and adsorption of molecules
Ammonia Binding Energy distribution at Interstellar Icy Grains
Reactivity of N(2D) atoms and of the cyano radical (CN) with vinyl cyanide
Cyanoacetylene gas-phase chemistry of relevance in interstellar objects, co
Combined crossed molecular beams and computational study on the N(2D) + HCC
A Combined Crossed Molecular Beam and Theoretical Investigation of the CN(X
Acetaldehyde binding energies: a coupled experimental and theoretical study
Trajectory files for "Where does the energy go during the interstellar NH3
Diffusion jump structures for H, N and O atoms
The GRETOBAPE gas-phase reaction network: the importance of being exothermi
Theoretical water binding energy distribution and snowline in protoplanetar
Infrared action spectroscopy as tool for probing gas-phase dynamics: Proton
Optical constants of CO and CO2 in the IR ans THz ranges and code to calcul
Optical constants of CO and CO2 in the IR ans THz ranges and code to calcul
Optimized structures of the stationary points on the potential energy surfa
Optimized structures of the stationary points on the potential energy surfa
Optimized structures of the stationary points on the potential energy surfa
Astrochemical reaction networks: bringing order to chaos
Formation of Complex Organic Molecules on Interstellar CO Ices? Insights fr
Formation Of Interstellar Complex Organic Molecules On Water-rich Ices Trig
Optimized stationary points on the potential energy surface of the reaction
Optimized stationary points on the potential energy surfaces of the N(2D)+
Optimized stationary points on the potential energy surfaces of the S+(4S)
Optimized stationary points on the potential energy surfaces of the N(2D) +
Optimized structures of selected stationary points on the potential energy
ASTROCHEMICAL MODELS
Referred Publications
Press Releases
Outreach products
Contact & Credits
ACO
Home
Project
ESR Thesis subjects
ESR 1
ESR 2
ESR 3
ESR 4
ESR 5
ESR 6
ESR 7
ESR 8
ESR 9
ESR 10
ESR 11
ESR 12
ESR 13
ESR 14
ESR 15
ESR 16
ESR 17
ACO in a nutshell
ACO Science
ACO Objectives
Events
ACO Meetings
ACO Supervisory Board Meeting 2023
ACO Network meeting Year3
ACO Schools
ACO Year 3 School
ACO Virtual Reality School
ACO Year 2 School
ACO Year 1 School
Program
ACO Congresses
ACO Congress Year 2
ACO Congress Year 4
ACO Organized Events
FAUST @ IPAG, Sep 2022
FAUST meeting venue
Hotels in Grenoble
FAUST participants
ACO Trainings
Team
People
Organization
ACO recruited ESRs
ACO public datasets
ASTRONOMICAL OBSERVATIONS
CHESS observations
ASAI observations
SOLIS observations
FAUST observations
THEORETICAL CHEMISTRY CALCULATIONS
Cations structures Scripts
Software Packages
Atomic coordinates of the periodic amorphous ice grain model
Atomic coordinates of the structures of iCOMs adsorbed at the surface of a
Atomic coordinates of the structures of iCOMs adsorbed at the surface of an
Absolute reactive cross sections for the reactions of methanimine radical c
GFN2-xTB structures of iCOM adsorbed on a cluster model of water molecules
Structures and Properties of Known and Postulated Interstellar Cations
Where does the energy go during the interstellar NH3 formation on water ice
Harmonic vibrational frequencies of the structures of iCOMs adsorbed at the
Amorphous grain model of interstellar icy grains
ACO-FROST: generation of icy grain models and adsorption of molecules
Ammonia Binding Energy distribution at Interstellar Icy Grains
Reactivity of N(2D) atoms and of the cyano radical (CN) with vinyl cyanide
Cyanoacetylene gas-phase chemistry of relevance in interstellar objects, co
Combined crossed molecular beams and computational study on the N(2D) + HCC
A Combined Crossed Molecular Beam and Theoretical Investigation of the CN(X
Acetaldehyde binding energies: a coupled experimental and theoretical study
Trajectory files for "Where does the energy go during the interstellar NH3
Diffusion jump structures for H, N and O atoms
The GRETOBAPE gas-phase reaction network: the importance of being exothermi
Theoretical water binding energy distribution and snowline in protoplanetar
Infrared action spectroscopy as tool for probing gas-phase dynamics: Proton
Optical constants of CO and CO2 in the IR ans THz ranges and code to calcul
Optical constants of CO and CO2 in the IR ans THz ranges and code to calcul
Optimized structures of the stationary points on the potential energy surfa
Optimized structures of the stationary points on the potential energy surfa
Optimized structures of the stationary points on the potential energy surfa
Astrochemical reaction networks: bringing order to chaos
Formation of Complex Organic Molecules on Interstellar CO Ices? Insights fr
Formation Of Interstellar Complex Organic Molecules On Water-rich Ices Trig
Optimized stationary points on the potential energy surface of the reaction
Optimized stationary points on the potential energy surfaces of the N(2D)+
Optimized stationary points on the potential energy surfaces of the S+(4S)
Optimized stationary points on the potential energy surfaces of the N(2D) +
Optimized structures of selected stationary points on the potential energy
ASTROCHEMICAL MODELS
Referred Publications
Press Releases
Outreach products
Contact & Credits
More
Home
Project
ESR Thesis subjects
ESR 1
ESR 2
ESR 3
ESR 4
ESR 5
ESR 6
ESR 7
ESR 8
ESR 9
ESR 10
ESR 11
ESR 12
ESR 13
ESR 14
ESR 15
ESR 16
ESR 17
ACO in a nutshell
ACO Science
ACO Objectives
Events
ACO Meetings
ACO Supervisory Board Meeting 2023
ACO Network meeting Year3
ACO Schools
ACO Year 3 School
ACO Virtual Reality School
ACO Year 2 School
ACO Year 1 School
Program
ACO Congresses
ACO Congress Year 2
ACO Congress Year 4
ACO Organized Events
FAUST @ IPAG, Sep 2022
FAUST meeting venue
Hotels in Grenoble
FAUST participants
ACO Trainings
Team
People
Organization
ACO recruited ESRs
ACO public datasets
ASTRONOMICAL OBSERVATIONS
CHESS observations
ASAI observations
SOLIS observations
FAUST observations
THEORETICAL CHEMISTRY CALCULATIONS
Cations structures Scripts
Software Packages
Atomic coordinates of the periodic amorphous ice grain model
Atomic coordinates of the structures of iCOMs adsorbed at the surface of a
Atomic coordinates of the structures of iCOMs adsorbed at the surface of an
Absolute reactive cross sections for the reactions of methanimine radical c
GFN2-xTB structures of iCOM adsorbed on a cluster model of water molecules
Structures and Properties of Known and Postulated Interstellar Cations
Where does the energy go during the interstellar NH3 formation on water ice
Harmonic vibrational frequencies of the structures of iCOMs adsorbed at the
Amorphous grain model of interstellar icy grains
ACO-FROST: generation of icy grain models and adsorption of molecules
Ammonia Binding Energy distribution at Interstellar Icy Grains
Reactivity of N(2D) atoms and of the cyano radical (CN) with vinyl cyanide
Cyanoacetylene gas-phase chemistry of relevance in interstellar objects, co
Combined crossed molecular beams and computational study on the N(2D) + HCC
A Combined Crossed Molecular Beam and Theoretical Investigation of the CN(X
Acetaldehyde binding energies: a coupled experimental and theoretical study
Trajectory files for "Where does the energy go during the interstellar NH3
Diffusion jump structures for H, N and O atoms
The GRETOBAPE gas-phase reaction network: the importance of being exothermi
Theoretical water binding energy distribution and snowline in protoplanetar
Infrared action spectroscopy as tool for probing gas-phase dynamics: Proton
Optical constants of CO and CO2 in the IR ans THz ranges and code to calcul
Optical constants of CO and CO2 in the IR ans THz ranges and code to calcul
Optimized structures of the stationary points on the potential energy surfa
Optimized structures of the stationary points on the potential energy surfa
Optimized structures of the stationary points on the potential energy surfa
Astrochemical reaction networks: bringing order to chaos
Formation of Complex Organic Molecules on Interstellar CO Ices? Insights fr
Formation Of Interstellar Complex Organic Molecules On Water-rich Ices Trig
Optimized stationary points on the potential energy surface of the reaction
Optimized stationary points on the potential energy surfaces of the N(2D)+
Optimized stationary points on the potential energy surfaces of the S+(4S)
Optimized stationary points on the potential energy surfaces of the N(2D) +
Optimized structures of selected stationary points on the potential energy
ASTROCHEMICAL MODELS
Referred Publications
Press Releases
Outreach products
Contact & Credits
quabs- Optical constants of CO and CO2 in the IR/THz ranges and code to calculate the opacity f icy grains
quabs-Optical constants of CO and CO2 in the IR and THz ranges and code to calculate the opacity of icy interstellar grain
s
(Zenodo link)
Report abuse
Report abuse
