INSTRUCTIONS FOR ORAL PRESENTATIONS - Each team is expected to present a 10 minutes talk. The talk will be followed by 3 minutes of general questions. WE WILL ADHERE STRICTLY TO THE TIME ALLOCATION, SO PLEASE MAKE SURE YOUR PRESENTATION FITS IN 10 MINUTES. Please make an appointment with Rongfeng to transfer your talk to the classroom console and test it by 7 pm on the eve of your talk, as there will be no time to set up individual laptops on the day of the talk. In the unlikely event that during the test, we find that your presentation is incompatible with the console setup or OS, we will make an exception and allow you to use your individual laptop. We will also use the copy of your talk supplied on the eve of your presentation for grading purposes - The talk is to be given by one of member chosen by the team, or it can be split between several speakers. Rongfeng has already sent each team the email of team members so you can communicate. Questions at the end of the talk will be addressed to the team as a whole, and those who are not making the oral presentation should take this opportunity to speak. - Each team member will have a 10 minute interview with the professor to discuss what he/she has learnt about the talk topic and answer a few basic questions. A sign up sheet is available in Char Burke's office (RLM 15.222). PLEASE SIGN UP BY THURSDAY APRIL 24. - Your talks should cover some of the following points and whatever else you might find interesting: a) Where is the facility located and why? When is it expected to be operational? Who are the partner and institutions? b) What are the capabilities of the new facility e.g., operating wavelengths, field of view, spatial resolution, collecting area, no of telescopes, any other relevant unique feature. c) Which of these capabilities are particularly important in allowing this facility to probe unchartered territories ? What new science questions on GALAXIES in particular will this facility allow us to address? Try to illustrate your answer WITH ONE OR MORE SIMPLE EQUATIONS OR QUANTITATIVE ARGUMENTS. Many such arguments have been made in class regarding the spatial resolution or seeing, processes traced at different wavelengths, Wien's law, the age and angular diameter distance at different redshifts, etc d) What are limitations of this facility? SCHEDULE OF TALKS Tu Apr 29 Giant Magellan Telescope (GMT) 1) Auslender, David Matthew 2) Chairez, Diana Eugenia 3) Davis, Ashley Elise 4) Degelia, James Patrick James Webb Space Telescope (JWST) 5) Duncan, Brian Takeo 6) Graf, Stephen Boyer 7) Ippolito, Joseph 8) Juarez, Aaron Javier Atacama Large Millimeter Array (ALMA) 9) Kang, Sung Ju 10) Kuehner, Dillon Baker 11) Lundgren, Rex Oliver 12) Maller, Kara Marie The Expanded Very Large Array Project (EVLA) 13) Marouni, Oren Natan 14) Prasla, Farah 15) Reaves, Jamieson N. Square Kilometer Array (SKA) 16) Smartt, Jonathan Ryan 17) Smith, Krista Lynne 18) Won, Yoo Jai