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Results (101 - 200 of 212)

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Ticket Summary Status Owner Type Priority Milestone
#87 test Mie code accepted peter task minor
#88 cosmic ray excitation of forbidden transitions new enhancement minor
#99 crash with non-conservation new nobody defect - convergence minor
#101 get uncertainties of optimized parameters new peter enhancement minor C13 branch
#104 sink terms in n-level atoms new nobody enhancement minor
#141 make number of LAMDA levels adjustable with command new enhancement minor database infrastructure
#150 atomic data for S II new enhancement minor
#186 grid aborts due to element non-conservation new peter defect - convergence minor C13 branch
#194 determine the amount of hydrogen ionizing radiation absorbed by the grains new peter enhancement minor C13 branch
#209 update N II effective recombination rate coefficients new nobody enhancement minor
#217 llvm 3.0 (tags/Apple/clang-211.12) (based on LLVM 3.0svn) segfault new nobody defect - FPE minor
#225 error in input script results in obscure crash new nobody defect - failed assert minor C13 branch
#337 atomic model for Mg I new nobody enhancement minor
#389 we do not report Inwd component of emergent intensities new nobody enhancement minor C19_branch
#32 "compile stars" should work when run from any directory new nobody enhancement trivial
#15 Cloudy should be able to save state and allow restart from an arbitrary saved state new nobody enhancement good to do
#129 H - O charge exchange new enhancement good to do C13 branch
#130 H- + P -> 2H0* (10 eV) rate update new enhancement good to do
#136 review O I collision data new enhancement good to do C13 branch
#142 2020 Feb arXiv paper on Fe DR - including fits new enhancement good to do C13 branch
#171 update OI, CI excitation by H0 new enhancement good to do C13 branch
#173 HD chemistry, cooling new enhancement good to do
#192 paper on "Broyden's method" for solution of RT new nobody enhancement good to do Radiative transfer
#195 H3+ orto para chemistry network new nobody enhancement good to do C13 branch
#198 Ne III collision strength update new nobody enhancement good to do C13 branch
#199 update to UMIST numerical fits to chemistry rates new nobody enhancement good to do database infrastructure
#201 add ACH2 and BE refractive index data from Zubko new peter enhancement good to do C13 branch
#202 chemi ionization of H - solve Lya/Hb problem in agn? new nobody enhancement good to do
#212 Ni inner shell atomic data new nobody enhancement good to do
#213 predict gamma ray line spectrum new nobody enhancement good to do
#219 new chemistry data base - UMIST successor? new nobody enhancement good to do
#227 Auger spectrum new nobody enhancement good to do
#228 H2 formation on grain surface, two recent publications new nobody enhancement good to do
#230 atomic data summary paper new nobody enhancement good to do
#231 atomic data summary paper new nobody enhancement good to do
#232 support accurate synthetic photometry new peter enhancement good to do
#234 chemical heating, cosmic rays, and molecular gas new nobody physics good to do
#235 opacities in dense warm gas new nobody physics good to do
#236 hydrogen ionization, cosmic rays, and molecular gas new nobody physics good to do
#238 Saha Equation Normalized to Total Atomic Number new nobody physics good to do
#239 C II line formation in ISM new nobody physics good to do
#240 Move Cloudy routines into a project namespace new nobody enhancement good to do
#241 H2 ortho para rate Lique+ 2012 new nobody enhancement good to do
#249 coupled escape probabilities - gives implementation details new nobody enhancement good to do
#251 move block of cobalt blue translated BLOCK DATA into external file new nobody enhancement good to do
#252 attenuation of cosmic rays vs column density new nobody enhancement good to do
#256 update N_2 photodissociation rate new nobody enhancement good to do
#257 treatment of scattering around H I Lyman lines new nobody enhancement good to do
#261 three-body H2 formation rate update new nobody enhancement good to do
#262 review detailed level dependent H2 rates in this paper new nobody enhancement good to do
#263 dust heating - photon absorption vs electron collisions new peter physics good to do
#264 N chemistry in ISM new nobody enhancement good to do
#265 updated H electron collisions new nobody enhancement good to do
#266 update Si CX ionization new nobody enhancement good to do
#268 autoionization following collisional ionization new nobody enhancement good to do
#273 update CO photodissociation rate new nobody enhancement good to do
#274 H2 formation pumping new nobody enhancement good to do
#275 stark broadening of optical He I lines new nobody enhancement good to do
#276 chemistry of metastable He I 2 ^3S new nobody enhancement good to do
#277 collisional ionization rate coefficients new nobody enhancement good to do
#283 ortho para as separate species - are we happy with this? new nobody enhancement good to do
#285 AtomPy: An Open Atomic Data Curation Environment for Astrophysical Applications new nobody enhancement good to do
#286 update H2 ortho para rates new nobody enhancement good to do
#287 3He hyperfine collision rate update new nobody enhancement good to do
#288 DR for Fe12 + forming Fe11+ new nobody enhancement good to do
#290 atomic data for Be seq new nobody enhancement good to do
#293 update O III to new storey / badnell paper new nobody enhancement good to do
#294 inconsistency between two sums of the total continuum new nobody defect - wrong answer good to do
#295 He CX recombination data file, currently unused new nobody enhancement good to do
#296 Fe XIV atomic data new nobody enhancement good to do database infrastructure
#297 H2 formation on grains with temperature fluctuations new nobody enhancement good to do
#316 direct yahoo links in hazy & source to q&a if that is what we want to do new nobody task good to do C19_branch
#317 H2 ice formation new nobody enhancement good to do
#318 Si III data update new nobody enhancement good to do
#321 transition probabilities for noble gas first ion FS lines new nobody enhancement good to do
#322 update C I atomic H collision rates new nobody enhancement good to do
#327 line convergence at outer boundary of large column density clouds new nobody defect - convergence good to do
#329 rationalize the STOP COLUMN DENSITY commands new nobody enhancement good to do C19_branch
#334 LAMDA level energies are approximate and cannot be used to derive line energies new nobody defect - wrong answer good to do database infrastructure
#338 trans probs for forbidden lines within ground term new nobody enhancement good to do
#339 atomic data, esp recombination, update new nobody enhancement good to do
#343 new version of Chianti released new nobody defect - convergence good to do
#344 Particle Swarm Optimization algorithm new nobody enhancement good to do
#353 collision strengths for H-like 13 ? Z ? 42 new nobody enhancement good to do
#354 treatment of continuum lowering new nobody enhancement good to do
#356 H2+ and primordial chemistry new nobody enhancement good to do
#357 H3+ chemistry network new nobody physics good to do
#359 Fe X determining magnetic fields new nobody enhancement good to do
#361 low temperature Ne 2, 3 collision strengths new nobody enhancement good to do
#362 Analytic H i-to-H2 Photodissociation Transition Profiles new nobody enhancement good to do
#363 H2 - H2 collisional dissociation new nobody enhancement good to do
#364 He like energy levels, TPs new nobody enhancement good to do
#365 g-bar collision strengths for Rydberg levels new nobody enhancement good to do
#366 PDR chemistry on grain surfaces new nobody enhancement good to do
#368 X-ray CX code we could study new nobody enhancement good to do
#369 fast H2 OP conversion on grains new nobody enhancement good to do
#370 Rayleigh scattering treatment new nobody enhancement good to do
#371 H atom collisions new nobody enhancement good to do
#372 discussion of atomic data for O IV and Si OV new nobody enhancement good to do
#373 review of collisional ionization for light elements new nobody enhancement good to do
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