***************************************************************************************** ***************************************************************************************** CURVEPOPS1 - Data Release - J.J. Eldridge - 31/10/2018 ****************************************************************************************** **************************************************************************************** Within the data-release files with "-zAAA-B-C-D" are individual stellar models where -zAAA indicates a metallicity of 0.AAA. -B is the initial primary stellar mass in Msun. -C is the initial binary mass ratio with M2/M1. -D is the initial binary period in log(P/days). This release incorperates the following data directories and files: ***************************************************************************************** readme.txt -This file. ***************************************************************************************** profiles -Directory containing all the input profiles of the stellar models for SNEC. -input-zAAA-B-C-D are the structure input file -input-comp-zAAA-B-C-D are the composition input file ***************************************************************************************** DE-input-zAAA-B-C-D -directory containing the parameter file and the output data from SNEC for -each model. The inputs and outputs are as described in the SNEC manual -(find at http://stellarcollapse.org/SNEC). The parameter files will need -the directory paths to be edited to rerun. -We note to compare to observations the "magnitudes.dat" file is most suitable -and contains the lightcurve broadband magnitudes which are: 1 - Time/seconds 2 - Effective temperature / K 3 - PTF_R_AB 4 - u 5 - g 6 - r 7 - i 8 - z 9 - U 10 - B 11 - V 12 - R 13 - I ***************************************************************************************** listofmodels.txt -this file contains a model by model summary of each progenitor model. Each model has two lines of details. First line, by column: 1 - Directory with model results. 2 - Short text of model identifier - can be used to track stellar model from BPASSv2 release. 3 - SN type: 0='Failed', 1='IIP', 2='short-IIP', 3='IIb', 4='IIL', 5='87A-like', 6='long-IIP'. 4 - Empty variable. 5 - Remnant Mass to excise, Msun. 6 - Envelope binding energy / J. 7 - Estimated explosion energy / J (convert to erg for SNEC). 8 - Total progenitor mass, Msun. 9 - Estimated nickel mass, Msun (0.03xOxygen mass in ejecta). 10 - BPASSv2.1 IMF weight of model. Second line, is the final line of output from the stellar model "sneplot-" file, same as BPASSv2 release data as in manual. We repeat here: 1 - Model timestep number 2 - Age/yrs 3 - Log10(R1/Rsun) - radius of star 1 4 - Log10(T_1eff/K) - effective temperature of star 1 5 - Log10(L1/Lsun) - luminosity of star 1 6 - Total Mass, M1/Msun - mass of star 1 (use this value not column 37). 7 - (He core mass of star 1)/Msun 8 - (CO core mass of star 1)/Msun 9 - (ONe core mass of star 1)/Msun 10 - Empty column 11 - Surface mass fractions for X 12 - Surface mass fractions for Y 13 - Surface mass fractions for C 14 - Surface mass fractions for N 15 - Surface mass fractions for O 16 - Surface mass fractions for Ne 17 - (Mass of Hydrogen in star 1)/Msun 18 - (Mass of Helium in star 1)/Msun 19 - (Mass of Carbon in star 1)/Msun 20 - (Mass of Nitrogen in star 1)/Msun 21 - (Mass of Oxygen in star 1)/Msun 22 - (Mass of Neon in star 1)/Msun 23 - (Mass of Magnesium in star 1)/Msun 24 - (Mass of Silicon in star 1)/Msun 25 - (Mass of Iron in star 1)/Msun 26 - Envelope Binding Energy / Joules 27 - Total Star binding energy / Joules 28 - M(Remnant)/Msun for weak-SNe (1e43J) 29 - M(Ejecta mass)/Msun for weak-SNe (1e43J) 30 - M(Remnant)/Msun for SNe (1e44J) 31 - M(Ejecta mass)/Msun for SNe (1e44J) 32 - M(Remnant)/Msun for super-SNe (1e45J) 33 - M(Ejecta mass)/Msun for super-SNe (1e45J) 34 - Angular momentum of binary 35 - Period of binary in years 36 - log(Separation of binary/Rsun) 37 - Mass of star 1, M1/Msun - use column 6 38 - Mass of star 2, M2/Msun 39 - Total mass of binary, MTOTAL/Msun 40 - DM1W - wind mass loss rate of star 1 (Msun/(1.989*s)) 41 - DMW2 - wind mass loss rate of star 2 (Msun/(1.989*s)) 42 - DM1A - accretion of mass (Msun/(1.989*s)) 43 - DM2A - accretion of mass (Msun/(1.989*s)) 44 - DM1R - Roche Lobe Overflow of star 1 (Msun/(1.989*s)) 45 - DM2R - Roche Lobe Overflow of star 2 (Msun/(1.989*s)) 46 - DANGJJ - Change of angular momentum 47 - DLog10(R2/Rsun) - estimated radius of star 2 48 - DLog10(T2/K) - estimated effective temperature of star 2 49 - DLog10(L2/Lsun) - estimated luminosity of star 2 50 - Roche lobe overflux of star 2 51 - modelimf - total IMF probability of stars (assuming Kroupa IMF) 52 - mixedimf - IMF probability of rejuvenated stars Following are for total absolute magnitudes and colours of both stars in binary: 53 - V-I 54 - U 55 - B 56 - V 57 - R 58 - I 59 - J 60 - H 61 - K 62 - u 63 - g 64 - r 65 - i 66 - z 67 - f300w 68 - f336w 69 - f435w 70 - f450w 71 - f555w 72 - f606w 73 - f814w Following are for the absolute magnitudes of the secondary star in the binary alone: 74 - U 75 - B 76 - V 77 - R 78 - I 79 - J 80 - H 81 - K 82 - u 83 - g 84 - r 85 - i 86 - z 87 - f300w 88 - f336w 89 - f435w 90 - f450w 91 - f555w 92 - f606w 93 - f814w *****************************************************************************************