Kurucz/Papers I am learning how to deal with the figures. I have never done figures in the text and many of my figures are 11x17 inch (6000x10000 bitmaps) that cannot be reduced on normal laserprinters and maintain legiblity. They are photographically reduced for publication. I may have to put an individual postscript file for each figure in the subdirectory with the postscript file for the text. directory [PAPERS] logical name PAPERS: subdirectory [PAPERS.logical name] logical name AFEWTHINGS 1999 A few things we do not know about the Sun and F stars and G stars ANGRADOSREIS 1992 Model atmospheres for population synthesis BRUSSELSLINES 1995 An atomic and molecular data bank for stellar spectroscopy BRUSSELSSOLAR 1995 The solar spectrum:atlases and line identifications BRUSSELSSIRIUS 1995 The spectrum of Sirius from 307 to 1040 nm BUENOSAIRES 1993 New model atmospheres for modelling binaries and disks CARACASATOM 1992 Atomic and molecular data for opacity calculations CARACAS 1992 "Finding" the "missing" solar ultraviolet opacity CARACASPROB 1992 Remaining line opacity problems for the solar spectrum COOLGREEN 1999 The cool, green hills of earth COPENHAGEN 1994 Computation of opacities for diatomic molecules DEUTERIUM 1995 If deuterium is not primordial, where does it come from? ELEMENTARY 2006 Elementary physics in the cellular automaton universe. FANTASY 2003 The age of fantasy and the age of responsibility. FERMAT 2002 A simple proof of Fermat's Last Theorem GAMMA 1992 Gamma ray bursts produced by free comets GATLINBURG 2002 Atomic and molecular data needs for astrophysics GEDANKEN 1992 Gedanken astrophysics: the universe since recombination GEDANKENVEGA 1997 Gedanken astrophysics: Vegan astrophysics GIANTPLANETS 2001 The "Extra-Solar Giant Planets" are brown dwarfs THEHAGUE 1995 The Kurucz atomic and molecular database TRANSMISSION 2005 High resolution irradiance spectrum from 300 to 1000 nm IRRADIANCE 1998 Solar irradiance by computation ISOTOPES 1992 Significant effects produced by isotopic splitting ISOHYPER 1993 Atomic data for interpreting stellar spectra: isotopic and hyperfine KYOTOLTE 1997 LTE models LIFE 2000 The formation of life LITHIUM 1995 The primordial lithium abundance MADRID 1997 Progress on model atmospheres and line data MILLENIUM 2000 The millenium and the calendar MILLENNIUM 2000 The millennium and the calendar OPACITYCALC 1996 Rapid calculation of line opacity NEUTRINOS 1992 Solution of the solar neutrino problem NICELINES 2005 Including all the lines PPREACTION 1999 A correction to the pp reaction PUERTOVALLARTA 2001 A few things we do not know about stars and model atmospheres. RADIATIVELY 2000 An outline of radiatively-driven cosmology. 1991 and 1997 versions removed RADCELLULAR 2006 Radiatively-driven cosmology in the cellular automaton universe. SAO309 1970 ATLAS: A computer program for calculating model stellar atmospheres. SAO Special Report No. 309. SYDNEY 1997 Progress on model atmospheres and line data TRANSMISSION 2005 High resolution irradiance spectrum from 300 to 1000 nm TRIESTE 1993 A new opacity-sampling model atmosphere program for arbitrary abundances TRIESTEATLAS12 2005 ATLAS12, SYNTHE, ATLAS9, WIDTH9, et cetera TRIESTELIMITS 2005 Physical, numerical, and computational limits for Kurucz codes TRIESTELINES 2005 Including all the lines TRIESTERAPID 2005 Rapid computation of line opacity in SYNTHE and DFSYNTHE TRIESTESOLAR 2005 New atlases for solar flux, irradiacne, central intensity, and limb intensity VIENNACONV 1996 Model stellar atmospheres and real stellar atmospheres VIENNAIAU176 1995 A new opacity-sampling model atmosphere program for arbitrary abundances VIENNAATLAS12 1996 Status of the ATLAS12 opacity sampling program and of new programs for Rosseland and for distribution function opacity VICTORIA 1998 Semiempirical calculation of gf values for all elements (abstract)