Galaxy&forma+on&simula+ons& done&with&ART&(I)&hipacc.ucsc.edu/html/HIPACCLectures/Ceverino_1.pdf ·...
Transcript of Galaxy&forma+on&simula+ons& done&with&ART&(I)&hipacc.ucsc.edu/html/HIPACCLectures/Ceverino_1.pdf ·...
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Galaxy forma+on simula+ons done with ART (I)
Daniel Ceverino
Santa Cruz school, 2010
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Lectures
• Tuesday: Descrip+on of projects
• Wednesday: Physical models for galaxy forma+on in ART
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PROJECTS
• Main Goal: Get experience and skills with… – running ART – dealing with the raw data from simula+ons – doing analysis of ART outputs
• Beyond simple homeworks
• Scien+fically relevant (and open) projects.
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3 layers of complexity
• Run the test-‐case + Run the extract-‐ART code + analysis of the generated outputs
• Run the extract-‐ART code + analysis
• Analysis of the provided outputs, from the ‘galaxy A’ run described in Ceverino, Dekel and Bournaud (2010)
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre(on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac(on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba(c contrac(on? Density
profiles of gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema(cs of gas: disk rota(on curve, dispersion-‐dominated
galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema(cs of stars: bulge/disk decomposi(on, origin of bulge
stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma(on and evolu(on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre(on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouZlows • 12. Sta+s+cs of global galaxy proper+es: Mv, Mb=Mg+Ms, Mdisk (select
n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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List of projects • 1. Accre+on rate onto halos and onto galaxies: DM, gas, stars • 2. Merger rate • 3. Interac+on of Streams and Disk. • 4. Angular momentum: in streams vs disk • 5. Structure of high-‐z galaxies: Adiaba+c contrac+on? Density profiles of
gas, stars, DM. f_b? • 6. Kinema+cs of gas: disk rota+on curve, dispersion-‐dominated galaxies,… • 7. Kinema+cs of stars: bulge/disk decomposi+on, origin of bulge stars,… • 8. Globular cluster forma+on and evolu+on. • 9. SFR vs. Accre+on rate • 10. The SSFR plateau (fixed mass) at z>2 • 11. Gas ouglows • 12. Sta(s(cs of global galaxy proper(es: Mv, Mb=Mg+Ms, Mdisk
(select n,T, v_tan>f*|v|), Mbulge SFR, Mdot V, sigma R_0.5 Z
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How to run ART?
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How to run ART?
• Untar the code version*.tar in an empty directory at $HOME
• Untar the inicial condi+ons package (*.tar) in a different directory, where you will actually run the simula+on.
• Compile the code: edit the makefile and select the proper fortran and c compiler. Type make
• Place the executable (hartCSF.x) with the files for ini+al condi+ons and the input files
• Execute ./hartCSF.x > screen & (check first if the environment variable OMP_NUM_THREADS=#cores)
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control.dat
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sf.dat
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Details of the test-‐Run
• Target halo mass Max. reso. dm Mass reso. Box
• 1.12 10^11 Msun (z=0) 35-‐70 pc 7 10^5 Msun 10 Mpc/h
• Advance snapshots at z=2, 1, 0.6
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How to run extract data from ART snapshots?
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How to run extract data from ART snapshots?
• Untarfile: analysisRec.tar • Compile it: make –f MakeAnaR (select compiler first in MakeAnaR
• Input files: control.dat & schedule_R.dat, plus ana.R.exe and snapshots.
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How to run extract data from ART snapshots?
• Untarfile: analysisRec.tar • Compile it: make –f MakeAnaR (select compiler first in MakeAnaR
• Input files: control.dat & schedule_R.dat • Output files: fortran unformaved binary files
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How to run the extrac+ng code?
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Summary
• Run the test-‐case + Run the extract-‐ART code + analysis of the generated outputs (RUN)
• Run the extract-‐ART code + analysis (snapshots_RUN)
• Analysis of the provided outputs (outputs_CDB)
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Bibliography
• Some documenta+on about the physical model implemented in ART:
hvp://astronomy.nmsu.edu/danielcv/PhDCeverino.pdf
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thanks