Stout: Cloudy's Atomic and Molecular Database
arXiv:1506.01741 · doi:10.1088/0004-637X/807/2/118
Abstract
We describe a new atomic and molecular database we developed for use in the spectral synthesis code Cloudy. The design of Stout is driven by the data needs of Cloudy, which simulates molecular, atomic, and ionized gas with kinetic temperatures 2.8 K < T < 1e10 K and densities spanning the low to high-density limits. The radiation field between photon energies Ry and 100 MeV is considered, along with all atoms and ions of the lightest 30 elements, and ~100 molecules. For ease of maintenance, the data are stored in a format as close as possible to the original data sources. Few data sources include the full range of data we need. We describe how we fill in the gaps in the data or extrapolate rates beyond their tabulated range. We tabulate data sources both for the atomic spectroscopic parameters and for collision data for the next release of Cloudy. This is not intended as a review of the current status of atomic data, but rather a description of the features of the database which we will build upon.
ApJ in press
References in corpus (18)
- An atomic and molecular database for analysis of submillimetre line observations
- A PDR-Code Comparison Study
- Collisional Excitation of the [CII] Fine Structure Transition in Interstellar Clouds
- Electron impact excitation of OII fine-structure levels
- Molecular Hydrogen in Star-forming regions: implementation of its micro-physics in Cloudy
- X-ray enabled MOCASSIN: a 3D code for photoionized media
- Improved He I Emissivities in the Case B Approximation
- Corrigendum: Improved He~I Emissivities in the Case B Approximation
- Theoretical He I Emissivities in the Case B Approximation
- Inelastic Mg+H collision data for non-LTE applications in stellar atmospheres
- Electron-impact excitation of neutral oxygen
- CII in the Interstellar Medium: Excitation by H2 Revisited
- J-resolved He I emission predictions in the low-density limit
- On the Validity of Collider-Mass Scaling for Molecular Rotational Excitation
- Atomic data for S II - Toward Better Diagnostics of Chemical Evolution in High-redshift Galaxies
- Uncertainties in Theoretical HeI Emissivities: HII Regions, Primordial Abundance, and Cosmological Recombination
- Radiative cooling in collisionally and photo ionized plasmas
- Atomic data for Zn II - Improving Spectral Diagnostics of Chemical Evolution in High-redshift Galaxies
Cited by in corpus (19)
- Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b
- A constraint on light primordial black holes from the interstellar medium temperature
- Investigation of the environment around close-in transiting exoplanets using CLOUDY
- Atomic Data Revisions for Transitions Relevant to Observations of Interstellar, Circumgalactic, and Intergalactic Matter
- The CHIANTI atomic database
- Fe III emission in quasars: evidence for a dense turbulent medium
- X-ray spectroscopy in the microcalorimeter era 4: Optical depth effects on the soft X-rays studied with CLOUDY
- Extended high-ionization [MgIV] emission tracing widespread shocks in starbursts seen by JWST /NIRSpec
- Production of photoionized plasmas in the laboratory using X-ray line radiation
- Photoionization modeling of the dusty nova V1280 Scorpii
- Polarization of Rayleigh scattered Lyα in active galactic nuclei
- New Insights with XRISM & Cloudy: A novel Column Density Diagnostic
- A recent update of gas-phase chemical reactions and molecular lines in CLOUDY: its effects on millimeter and sub-millimeter molecular line predictions
- Energy levels and radiative rates for transitions in Fe V, Co VI and Ni VII
- Fine-structure electron-impact excitation of Ne and Ne for low temperature astrophysical plasmas
- Energy levels and radiative rates for Cr-like Cu VI and Zn VII
- Creating a CLOUDY Compatible Database with CHIANTI version 10 Data
- Photoionization models of Planetary Nebulae
- Spectroscopic modelling of two high-mass X-ray binaries, Cyg X--3 and 4U 1538--522