NSF IRES 2009 Shashi M. Kanbur SUNY Oswego May-August 2009
Introduction 3 weeks here, 6 weeks in Brazil. May 26 th -June12th: July 10 th -Aug 20 th. Oswego: AM: Portuguese, PM: talks/Chimera/Astro projects. This PM: get ID cards, parking, computer accounts, sign papers to get stipends, deliver Visa plus other other forms to OIEP. Have intro talk on Chimera?
Chimera Chimera is a robotic telescope control system. Ubuntu 10.8 on laptop. Download subversion, download source, use install script. Install Chimera on laptop with setup.py Currently at version 453. Upgrade from version 415.
LNA
UFSC, Antonio Kanaan, Paulo Henrique da Silva Its tough to get time on telescopes. Need long periods of time. mapas.html mapas.html mapas.html
Chimera Software system to robotically control a telescope. Much of it written. Need to work on photometry/extinction/seeing modules. Mainly testing these and the rest of Chimera.
Photometry CCD: Charge Coupled Device: rely on photoelectric effect. Point telescope to star: add up the “signal” centered around the star – this is aperture photometry. Extinction: how does the “signal” from a given star vary during the night? Seeing: FWHM.
Cepheid Variables Pulsating stars, periods of the order of days. Period is related to their absolute magnitude. m-M = 5log(d) – 5 Relation between M and logP is the Period-Luminosity (PL) relation. Fundamental way to measure distances in the Universe.
Why? Hubble’s law: v = Hd Get v from Doppler shift of spectral lines. Get d from extra-galactic distance ladder. Slope gives H, Hubble’s constant – most fundamental constant in Astrophysics. Sets size scale, age scale and fate/past of Universe. Know it to 10% precision, want to know it to < 1% precision.
Cepheid PL relation M = a+blogP But is it linear? My work suggests it is nonlinear, at least in the LMC. All astrophysics projects have this as motivation: further testing, impact on H, theoretical modeling, data analysis.
Projects Multiphase PC/PL relations. Impact on H of linear/nonlinear PL relation using OGLE III data. M3/M15 Oosterhoff dichotomy for RR Lyraes. Astronomical data reduction of a large new set of data. Statistical analysis of existing data.
Multiphase PC/PL
Compare with models.
Impact on H Calibrate the SNIa diagram. With OGLE II data, difference in H of about 1-2%. With OGLE III data, difference in H of about 5%. Check!!! Work on multiphase OGLE III data, compare with observations.
NGC 4258 Water maser galaxy for which an accurate geometric distance exists. Have the data for Cepheids in this galaxy. Is the Cepheid PL relation in NGC 4258 linear or non-linear. Write program to analyze data. Apply F test, testimator, SIC etc. to investigate linearity/nonlinearity.
Oosterhoff dichotomy in M3/M15 Study data and theoretical models for RR Lyraes in M3/M15. Investigate Oosterhoff dichotomy in terms of PC/AC relations. Does Oosterhoff dichotomy manifest itself in PC/AC relations as a function of phase. PC relation flat at minimum light? Use as a reddening indicator?
Data Reduction Work through IRAF data reduction procedures and daophot photometry procedures for a large (330Gb data set) of Cepheid observations for the LMC in IR. Work on Sloan data set. Produce documentation and cookbook. Primary standards/secondary standards.
Statistical Analysis of Data Cubic polynomial fits to M33 data. Testimator as a test of heteroskedasticity. Fourier/PCA analysis of other variable star datasets. PC/PL relation linear in M31/M33? IRAC bands PL relations.
Expectations Learn Python, OOP. Become familiar with Chimera, its structure and operation. Work on Chimera and work on one of the research projects. Need to write a report plus powerpoint poster on the Chimera work at the end of the project. Right now, become familiar with chimera and OOP. Play around with it. Work.
Schedule AM: Portuguese. Lunch. PM (talks by me or by other faculty) Tuesday May 26 th : PM: Admin Wednesday May 27 th : Chimera Intro plus projects. Thursday May 28 th : 2pm Dr. Alex Pantaleev: Object Orientated Programming. Friday May 29 th : PM: Chimera plus projects. Monday June 8 th : PM: Gravitational Wave Astronomy. Tuesday June 9 th : PM: Physical Chemistry.