Tony Monteiro
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[email protected] Education Current Phd Student, University of Kansas
Jonathan (Yoni) Brande - [email protected] Education ● Current PhD Student, University of Kansas, Department of Physics and Astronomy ● BS, Astronomy, with Computer Science minor, University of Maryland, College Park, Dec. 2017 Research and Employment ● 2020 - present - PhD Student and Graduate Teaching Asst. - University of Kansas Dept. Physics and Astronomy ○ Transiting exoplanet characterization through transmission spectroscopy. Advisor: Dr. Ian Crossfield ○ Fall 2020 - Graduate TA for intro physics labs. Supervisor: Prof. Jennifer Delgado ● 2018 - 2020 - NASA GSFC, Planetary Systems Lab, Exoplanets and Stellar Astrophysics Lab/University of Maryland, Dept. of Astronomy - Faculty Research Assistant - ○ Contributed to the Exoplanet Modeling and Analysis Center by developing exoplanet modeling tools, e.g. developing/refining the exoplanet-specific interface to GSFC’s Planetary Spectrum Generator tool and refining and validating intern-developed tools such as the Exoplanet Boundaries Calculator. The EMAC project is currently deployed as a community resource1. Advisor - Dr. Avi Mandell ○ Conducted research into the feasibility of using JWST’s Mid-Infrared Instrument for direct imaging of gaseous planets around nearby M-dwarfs. Developed generalized frameworks for conducting parallelized JWST simulations on the Goddard Private Cloud computing resource. Advisors - Dr. Thomas Barclay, Dr. Elisa Quintana ○ Contributed to TESS planet discovery and characterization efforts through dynamics, transit timing variation analysis of TESS targets, including the L98-59 system2. Advisors - Dr. Thomas Barclay, Dr. Elisa Quintana ● 2017 - Summer/Fall - 2018 Spring - University of Maryland, Department of Astronomy - ○ Efficient algorithms for representing the complex gravity fields of asteroids. Worked to develop novel methods for gravitational modeling of asteroids using analytic evaluations of the gravity of cubic mass elements. -
Daniel Huber
Asteroseismology & Exoplanets: A Kepler Success Story Daniel Huber SETI Institute / NASA Ames Research Center U Chicago Astronomy Colloquium April 2014 Collaborators Bill Chaplin, Andrea Miglio, Yvonne Elsworth, Tiago Campante & Rasmus Handberg (Birmingham) Jørgen Christensen-Dalsgaard, Hans Kjeldsen, Victor Silva Aguirre (Aarhus) Tim Bedding & Dennis Stello (Sydney) Ron Gilliland (PSU), Sarbani Basu (Yale), Steve Kawaler (Iowa State), Travis Metcalfe (SSI), Jaymie Matthews (UBC), Saskia Hekker (Amsterdam), Marc Pinsonneault & Jennifer Johnson (OSU), Eric Gaidos (Hawaii) Tom Barclay, Jason Rowe, Elisa Quintana & Jack Lissauer (NASA Ames / SETI) Josh Carter, Lars Buchhave, Dave Latham, Ben Montet & John Johnson (Harvard) Dan Fabrycky (Chicago) Josh Winn, Kat Deck & Roberto Sanchis-Ojeda (MIT) Andrew Howard, Howard Isaacson & Geoff Marcy (Hawaii, Berkeley) The Kepler Space Telescope • launched in March 2009 • 0.95 m aperture • 42 CCD’s , 105 sq deg FOV Borucki et al. (2008), Koch et al. (2010) Kepler Field of View Kepler Orbit Kepler obtained uninterrupted high-precision photometry of ~> 150,000 stars for 4 years to search for transiting exoplanets Asteroseismology in a Nutshell AstEroseismology? AstEroseismology? unnamed author, sometime in 1995 What causes stellar oscillations? Oscillations in cool stars are driven by turbulent surface convection (opacity in hot stars) Radial Order n displacement center surface number of nodes from the surface to the center of the star Spherical Degree l l = 0 Spherical Degree l l = 2 l = 0 Δν ~ 135 µHz for the Sun sound speed cs -1 3 1/2 Δν = (2 ∫dr/cs) ∝ (M/R ) (ω = n π c / L!) Ulrich (1986) δν ∝ ∫dcs/dr (Age) δν (individual frequencies) sound speed cs -1 3 1/2 Δν = (2 ∫dr/cs) ∝ (M/R ) (ω = n π c / L!) Ulrich (1986) νmax νmax ~ 3000 µHz for the Sun 0.5 -2 0.5 νmax ∝ νac ∝ g Teff ∝ M R Teff Brown et al. -
Project Cyclops : a Design Study of a System for Detecting
^^^^m•i.j . --f'v.i^ "^y^-!^ A Design Study of a System for Detecting Extraterrestrial Intelligent Life '• >..-, i,C%' PREPARED UNDER STANFORD /NASA /AMES RESEARCH CENTER >J^1t> 1971 SUMMER FACULTY FELLOWSHIP PROGRAM IN ENGINEERING SYSTEMS DESIGr CR 114445 (Revised Edition 7/73) Available to the public rB' ^ A Design Study of a System for Detecting Extraterrestrial Intelligent Life PREPARED UNDER STANFORD/ NASA/AMES RESEARCH CENTER 1971 SUMMER FACULTY FELLOWSHIP PROGRAM IN ENGINEERING SYSTEMS DESIGN Further copies of this report may be obtained by writing to Dr. John Billingham NASA/ Ames Research Center, Code LT Moffett Field, California 94035 weixesunr colligc LWRART CYCLOPS PEOPLE Co-Directors: Bernard M. Oliver Stanford University (Summer appointment) John Billingham Ames Research Center, NASA System Design and Advisory Group: James Adams Stanford University Edwin L. Duckworth San Francisco City College Charles L. Seeger New Mexico State University George Swenson University of Illinois Antenna Structures Group: Lawrence S. Hill California State College L.A. John Minor New Mexico State University Ronald L. Sack University of Idaho Harvey B. Sharfstein San Jose State College Pennsylvania Alan 1. Soler University of Receiver Group: Washington Ward J. Helms University of William Hord Southern Illinois University Pierce Johnson University of Missouri C. ReedPredmore Rice University Transmission and Control Group: Marvin Siegel Michigan State University Jon A. Soper Michigan Technological University Henry J. Stalzer, Jr. Cooper Union Signal Processing Group: Jonnie B. Bednar University of Tulsa Douglas B. Brumm Michigan Technological University James H. Cook Cleveland State University Robert S. Dixon Ohio State University Johnson Luh Purdue University Francis Yu Wayne State University /./ la J C, /o ) •»• < . -
Radio Astronomy
Edition of 2013 HANDBOOK ON RADIO ASTRONOMY International Telecommunication Union Sales and Marketing Division Place des Nations *38650* CH-1211 Geneva 20 Switzerland Fax: +41 22 730 5194 Printed in Switzerland Tel.: +41 22 730 6141 Geneva, 2013 E-mail: [email protected] ISBN: 978-92-61-14481-4 Edition of 2013 Web: www.itu.int/publications Photo credit: ATCA David Smyth HANDBOOK ON RADIO ASTRONOMY Radiocommunication Bureau Handbook on Radio Astronomy Third Edition EDITION OF 2013 RADIOCOMMUNICATION BUREAU Cover photo: Six identical 22-m antennas make up CSIRO's Australia Telescope Compact Array, an earth-rotation synthesis telescope located at the Paul Wild Observatory. Credit: David Smyth. ITU 2013 All rights reserved. No part of this publication may be reproduced, by any means whatsoever, without the prior written permission of ITU. - iii - Introduction to the third edition by the Chairman of ITU-R Working Party 7D (Radio Astronomy) It is an honour and privilege to present the third edition of the Handbook – Radio Astronomy, and I do so with great pleasure. The Handbook is not intended as a source book on radio astronomy, but is concerned principally with those aspects of radio astronomy that are relevant to frequency coordination, that is, the management of radio spectrum usage in order to minimize interference between radiocommunication services. Radio astronomy does not involve the transmission of radiowaves in the frequency bands allocated for its operation, and cannot cause harmful interference to other services. On the other hand, the received cosmic signals are usually extremely weak, and transmissions of other services can interfere with such signals. -
The Origins and Development of the Search for Extraterrestrial Intelligence, 1959-1971 Sierra E
James Madison University JMU Scholarly Commons Masters Theses The Graduate School Spring 2012 "A cosmic Rorschach test": The origins and development of the search for extraterrestrial intelligence, 1959-1971 Sierra E. Smith James Madison University Follow this and additional works at: https://commons.lib.jmu.edu/master201019 Part of the History Commons Recommended Citation Smith, Sierra E., ""A cosmic Rorschach test": The origins and development of the search for extraterrestrial intelligence, 1959-1971" (2012). Masters Theses. 334. https://commons.lib.jmu.edu/master201019/334 This Thesis is brought to you for free and open access by the The Graduate School at JMU Scholarly Commons. It has been accepted for inclusion in Masters Theses by an authorized administrator of JMU Scholarly Commons. For more information, please contact [email protected]. “A Cosmic Rorschach Test”: The Origins and Development of the Search for Extraterrestrial Intelligence, 1959-1971 Sierra E. Smith A thesis submitted to the Graduate Faculty of JAMES MADISON UNIVERSITY In Partial Fulfillment of the Requirements for the degree of Master of Arts History May 2012 Acknowledgements First and foremost, I would like to thank my thesis committee who has gone above and beyond the call of duty to guide me through this process. Despite being dragged into the twentieth century, Dr. Alison Sandman, my thesis director, helped articulate the ideas for my project far better than I could have alone. Thought-provoking conversations with Dr. Kevin Borg ensured that I thought broadly and deeply about both my project and my future plans. Dr. Steven Guerrier’s open door and enthusiasm for my project has been a constant throughout my graduate experience. -
Billy L. Quarles – Research Scientist
Billy L. Quarles | Research Scientist 837 State Street – Atlanta, GA 30332 B [email protected] • Í www.billyquarles.com Education University of Texas at Arlington Physics Doctor of Philosophy 2008–2012 Stephen F. Austin State University Physics Master of Science 2006–2008 Texas Christian University Physics & Astronomy Bachelor of Science 2002–2006 PhD Dissertation Title: Selected studies of celestial dynamics and habitability of extrasolar planetary systems Supervisors: Professor Zdzislaw Musielak & Associate Professor Manfred Cuntz Research Interests Theory: Gravitational Dynamics, Planetary Spin Dynamics, Planet Formation, Planetary Habitability Observation: Exoplanets in Binary Stars, Multiple Planet Systems Research Experience Georgia Institute of Technology Atlanta, GA Research Scientist August 2018 – present { Investigate the occurrence of circumbinary planets using data from the Transiting Exoplanet Survey Satellite. { Performed an investigation of the changes in climate for exoplanets in binary systems due evolution of planetary spin. { Improved the characterization of warm, large exoplanets using Gaussian Process based methods of noise characterization University of Oklahoma Norman, OK Postdoctoral Research Associate September 2016 – August 2018 { Performed an investigation of stability for multiple planets that may exist binary star systems. { Identified the possible compositions of the TRAPPIST-1 planets based upon system stability. { Implemented a new code to take advantage of GPUs to understand the processes of giant planet migration in the early Solar System. University of Idaho Moscow, ID Postdoctoral Research Associate May 2016 – August 2016 { Investigated the stability of obliquity in exoplanet systems. San Diego State University San Diego, CA Technical Consultant September 2015 – August 2016 { Implemented new computational methods that improve the efficiency of planet detection in binary systems. -
Search for Extraterrestrial Intelligence (SETI) - the Next Steps (34Th Symposium) (IAA.1.1) (A4.) SETI I - Technical Aspects (1.)
56th International Astronautical Congress 2005 Search for Extraterrestrial Intelligence (SETI) - The Next Steps (34th Symposium) (IAA.1.1) (A4.) SETI I - Technical Aspects (1.) Author Dr. Douglas A. Vakoch The SETI Institute, United States, [email protected] ADVANTAGES OF ACTIVE SETI Abstract This paper will examine the potential benefits of Active SETI, a prospect raised in the Project Cyclops report, which noted “if our first search of the nearest 1000 target stars produced negative results we might wish to transmit beacons to these stars for a year or more before carrying the search deeper into space” (p. 153). Renewed discussion of that possibility is particularly timely in light of the recent completion of Project Phoenix, which surveyed nearly 1000 nearby stars. It has often been argued that the young age of human civilization, when compared to the older age of any extraterrestrial civilization we may contact, justifies our reliance on passive SETI as opposed to transmitting. Because transmission is more costly and requires longer timescales to succeed, the argument goes, we should be expected to take the easier role. However, this reasoning presupposes that the motivations of extraterrestrial civilizations are sufficiently benevolent that they will transmit de novo rather than only in reciprocation, and that they choose to make contact even prior to learning that we desire contact. This paper examines an alternative scenario, in which entry into the Galactic Club requires initiative on the part of the applicant, rather than passively waiting for an invitation. It proposes a solution to the troubling possibility that many civilizations are listening but none is transmitting. -
Rocketstem • Vol. 2 No. 3 • May 2014 • Issue 7
RocketSTEMVol. 2 • No. 3 • May 2014 • Issue 7 Join the vast legions of citizen scientists at the Zooniverse 10 years of discovery for Cassini at Saturn Jim Adams aligns NASA technology for future missions All the equipment you need for doing astrophotography Discussing string theory, ice cream, and more with physicist Brian Greene the NASA sponsored Earth Day event April 22, 2014 at Union Station in Washington, DC. NASA announced the mosaic. The image is comprised of more than 36,000 individual photos submitted by people around the world. To view the entire mosaic and related images and videos, please visit: http://go.nasa.gov/1n4y8qp. Credit: NASA/Aubrey Gemignani Contents Follow us online: Brian Greene facebook.com/RocketSTEM Famed theoretical physicist and string theorist educates us on a variety of topics. twitter.com/rocketstem 06 www.rocketstem.org Astrophotography All of our issues are available via Ready to photograph the a full-screen online reader at: stars? We give you a rundown on the equipment you need. www.issuu.com/rocketstem 16 Editorial Staff Managing Editor: Chase Clark Cassini Astronomy Editor: Mike Barrett A decade of discovery and Photo Editor: J.L. Pickering images while orbiting Saturn, Contributing Writers its rings and 62 moons. Mike Barrett • Lloyd Campbell 22 Brenden Clark • Chase Clark Rich Holtzin • Joe Maness Jim Adams Sherry Valare • Amjad Zaidi During his career at NASA, Contributing Photographers Adams has been involved Paul Alers • Mike Barrett with dozens of missions. Dennis Bonilla • Brenden Clark 38 Lark Elliott • Aubrey Gemignani Dusty Hood • R. Hueso Zooniverse Bill Ingalls • Steve Jurvetson W. -
Kepler 186F - First Earth-Sized Planet Orbiting in Habitable Zone of Another Star | SETI Institute 17/04/14 22.07
Kepler 186f - First Earth-sized Planet Orbiting in Habitable Zone of Another Star | SETI Institute 17/04/14 22.07 SETI Institute Home For Scientists For Educators and Students TeamSETI.org >> Our Work Our Scientists About us Connect Donate Kepler 186f - First Earth-sized Planet Become a SETIStar Orbiting in Habitable Zone of Another Star by Elisa Quintana (/users/elisa-quintana) , Research Scientist For the past three decades, the SETI Institute has been participating in a number of scientific explorations to answer the question “Are we alone?” Today, my co-authors and I are announcing the achievement of another milestone in the exploration. We have confirmed the first Earth-sized planet orbiting in the habitable zone of a star other than the Sun. This planet is named Kepler-186f and it is one of five planets that have thus far been detected by NASA’s Kepler space telescope in orbit about the star Kepler-186. This star is smaller and cooler than the Sun, of a type called an M-dwarf or red dwarf, and all its known planets are small as well, with sizes less than 1.5 times the size of Earth. The planet Kepler-186f is the smallest, being within 10% of the size of Earth and orbits furthest from the host star, within the habitable zone. This is the region around a star within which a planet can sustain liquid water on its surface given the right atmospheric conditions. The Kepler-186 planetary system lies in the direction of the constellation Cygnus, about 500 light-years away. -
Ames in the 1970S and 1980S
Atmosphere of Freedom Sixty Years at the NASA Ames Research Center Wheat in crop growth chamber under red LED lights and low pressure sodium lamps. 98 Diverse Challenges Explored with Unified Spirit Chapter 3: Ames in the 1970s and 1980s Two events make 1969 the year to mark the next era in Ames history. First, Apollo 11 returned safely from its landing on the Moon, signalling the beginning of the end of the lunar landing mission that drove NASA almost from its start. NASA had yet to decide what to do for its second act, and its flurry of strategic planning took place against an uncertain political backdrop. Much of the American public— including both political conservatives concerned with rampant inflation and political liberals concerned with technocratic government—began to doubt the value of NASA’s big plans. NASA had downplayed the excitement of interplanetary exploration as it focused on the Moon. Congress and the American aerospace industry, under pressure from a resurgent European aerospace industry, began to doubt if NASA really wanted the aeronautics part of its name. NASA had to justify its budget with quicker results, better science, and relevance to earthly problems. The second major event of 1969 was the arrival of Hans Mark as Ames’ director. Mark, himself, displayed a force of personality, a breadth of Michael McGreevy holding a intellect, and an aggressive management style. More significantly, Mark arrived as rumors televised rock in his virtual hand circulated that Ames would be shut down. Thus, Ames people gave him a good amount of using the Ames EXOS Dexterous room to reshape their institution. -
An Earth-Sized Planet in the Habitable Zone of a Cool Star Authors: Elisa V
Title: An Earth-sized Planet in the Habitable Zone of a Cool Star Authors: Elisa V. Quintana1,2*, Thomas Barclay2,3, Sean N. Raymond4,5, Jason F. Rowe1,2, Emeline Bolmont4,5, Douglas A. Caldwell1,2, Steve B. Howell2, Stephen R. Kane6, Daniel Huber1,2, Justin R. Crepp7, Jack J. Lissauer2, David R. Ciardi8, Jeffrey L. Coughlin1,2, Mark E. Everett9, Christopher E. Henze2, Elliott Horch10, Howard Isaacson11, Eric B. Ford12,13, Fred C. Adams14,15, Martin Still3, Roger C. Hunter2, Billy Quarles2, Franck Selsis4,5 Affiliations: 1SETI Institute, 189 Bernardo Ave, Suite 100, Mountain View, CA 94043, USA. 2NASA Ames Research Center, Moffett Field, CA 94035, USA. 3Bay Area Environmental Research Institute, 596 1st St West Sonoma, CA 95476, USA. 4Univ. Bordeaux, Laboratoire d'Astrophysique de Bordeaux, UMR 5804, F-33270, Floirac, France. 5CNRS, Laboratoire d'Astrophysique de Bordeaux, UMR 5804, F-33270, Floirac, France. 6San Francisco State University, 1600 Holloway Avenue, San Francisco, CA 94132, USA. 7University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556, USA. 8NASA Exoplanet Science Institute, California Institute of Technology, 770 South Wilson Avenue Pasadena, CA 91125, USA. 9National Optical Astronomy Observatory, 950 N. Cherry Ave, Tucson, AZ 85719 10Southern Connecticut State University, New Haven, CT 06515 11University of California, Berkeley, CA, 94720, USA. 12Center for Exoplanets and Habitable Worlds, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA, 16802, USA 13Department of Astronomy and Astrophysics, The Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, USA 14Michigan Center for Theoretical Physics, Physics Department, University of Michigan, Ann Arbor, MI 48109, USA 15Astronomy Department, University of Michigan, Ann Arbor, MI 48109, USA *Correspondence to: [email protected] ! ! ! ! ! ! ! Abstract: The quest for Earth-like planets represents a major focus of current exoplanet research. -
"The Search for Extra-Terrestrial Life"
Portland State University PDXScholar Special Collections: Oregon Public Speakers Special Collections and University Archives 10-2-1975 "The Search for Extra-Terrestrial Life" Donald L. DeVincenzi Follow this and additional works at: https://pdxscholar.library.pdx.edu/orspeakers Part of the The Sun and the Solar System Commons Let us know how access to this document benefits ou.y Recommended Citation DeVincenzi, Donald L., ""The Search for Extra-Terrestrial Life"" (1975). Special Collections: Oregon Public Speakers. 91. https://pdxscholar.library.pdx.edu/orspeakers/91 This Article is brought to you for free and open access. It has been accepted for inclusion in Special Collections: Oregon Public Speakers by an authorized administrator of PDXScholar. Please contact us if we can make this document more accessible: [email protected]. “The Search for Extra-Terrestrial Life,” Donald L. DeVincenzi Portland State University October 2, 1975 PSU Library Special Collections and University Archives Oregon Public Speakers Collection https://pdxscholar.library.pdx.edu/orspeakers/91/ Transcribed by Kincaid Davis, April 10, 2020 Audited by Carolee Harrison, June 2020 PSU Library Special Collections and University Archives presents these recordings as part of the historical record. They reflect the recollections and opinions of the individual speakers and are not intended to be representative of the views of Portland State University. They may contain language, ideas, or stereotypes that are offensive to others. CARL DITTMER: On behalf of Portland State University, the College of Science, the Auxiliary Academic Activities Committee, the Environmental Sciences Seminar Committee, and the Division of Continuing Education, I welcome you to this lecture. It is a privilege to be able to present a speaker who will talk on a subject so vital to us as the one tonight.