KIDA is a database of kinetic data of interest for astrochemical (interstellar medium and planetary atmospheres) studies.
Indicate a species (ex: H3O+) or a couple of species (ex: C + H2)
Warning : Second letter of 2-letters elements have to be lowercase, eg Si
Use the generic names of the species, avoid the cyclic or linear forms (ex: for c-C3H indicate C3H) , the isotopic numbers (for (13)C indicate C, except for deuterium), or the excited states (for C(1D) indicate C). You will be able to choose these forms in the next step.
Warning : Second letter of 2-letters elements have to be lowercase, eg Si
Use the generic names of the species, avoid the cyclic or linear forms (ex: for c-C3H indicate C3H) , the isotopic numbers (for (13)C indicate C, except for deuterium), or the excited states (for C(1D) indicate C). You will be able to choose these forms in the next step.
22:32, May 11
RT @GreenBankObserv : Sorry we're late, did someone ask for an uncropped map of ammonia in the Orion Nebula? https://t.co/BvK13XUwWw
11:42, Apr 14
RT @hitran : The line list for 14NH3 in HITRAN has been updated in the following ways.
1. 7400-8600 cm-1 spectral region was up… https://t.co/pdAGOfDzVM
10:11, Apr 13
RT @hitran : In addition, line shape parameters for both air and self broadening of N2O lines were revised (largely based on the… https://t.co/TB2xL1UNIp
10:10, Apr 13
Addition of a warning for the use of the deuterated network from Majumdar et al. stored in KIDA (https://t.co/dnxbFgeIFW)
10:07, Apr 13
RT @lamda_database : Updated spectroscopy for A-type CH3OH. Thanks Martin Cordiner & Nathan Roth (NASA GSFC)
