DOCSLIB.ORG

Juan Rafael Martínez Galarza

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Juan Rafael Martínez Galarza JUAN RAFAEL MART´INEZ GALARZA OFFICE ADDRESS CONTACT INFO Harvard-Smithsonian Center for Astrophysics Phone: +1 617 495 7027 60 Garden Stret Fax: +1 617 495 7490 Cambridge, MA 02138 [email protected] U. S. A. www.strw.leidenuniv.nl/∼martinez PROFILE Postdoctoral fellow at the Harvard-Smithsonian Center for Astrophysics. My research focuses on several aspects of galactic and extragalactic star formation. In particular, I am interested in the initial luminosity and mass distributions of masive star clusters, and the interaction of new-born massive stars with the interstellar medium. I use infrared photometry and spectroscopy performed with space-based observatories, as well as Bayesian modeling and SED fitting tools. I am also interested in infrared astronomical instrumentation, scientific outreach and education. RESEARCH EXPERIENCE Unraveling the Properties of Dense, Star-forming Clusters from Diverse Multi- wavelength Surveys Harvard-Smithsonian Center for Astrophysics, 2012 - present Multi-wavelenth studies of several galactic star-forming regions and Bayesian SED fitting of their SEDs. Development of a Virtual Observatory-comaptible fitting tool. PhD Thesis: Mid-infrared spectroscopy of starburst Leiden Observatory, 2008 - 2012 State-of-the-art physical modelling and interpretation of the Spectral Energy Distributions (SEDs) of starburts. Comparison with Spitzer data. Mid-Infrared Instrument (MIRI) for the James Webb Space Telescope Rutherford Appleton Laboratory, United Kingdom, 2008-2012 Testing and data analysis of the spectrometer performance. Responsible for the wavelength calibra- tion of the instrument. Master Research: Filamentary Star formation in ρ-Ophiuchus Leiden Observatory, 2006-2007 Radio interferometric observations of a star-forming filament in the ρ-Ophiuchus region. Analysis of high density gas tracers. Supervisor: Dr. Michiel Hogerheijde Undergrad Research: Modelling of infrared emission from λ Bootis stars Steward Observatory, University of Arizona, 2005 Modelling of the geometry and radiative properties of diffuse dust in the vicinity of chemically peculiar stars Supervisor: Dr. Kate Su, Prof. George Rieke Undergrad Research: The Nature of λ Bootis stars Space Telescope Science Institute (STScI), Baltimore, 2004-2005 Chemical abundances in the atmospheres of λ Bootis stars, via optical spectroscopy Supervisor: Dr. Inga Kamp EDUCATION Leiden University PhD in Astronomy, June 2012 Title: “Infrared Spectroscopy of Starbursts: From Spitzer-IRS to JWST-MIRI” Advisor: Dr. Bernhard Brandl Promotor: Prof. Ewine van Dishoeck Leiden University MSc in Astronomy, December 2007 Universidad Nacional de Colombia BSc in Physics, July 2005 SELECTED TALKS The Properties of Dense, Star-forming Clusters from Multi-wavelength SED Fit- ting: the Case of W43 AAS 221st Meeting Long Beach, CA, USA, January 2013 Beyond the evident: A New Bayesian Tool for Multiwavelength SED fitting of Starbursts Far Infrared 2011 Meeting University College London, United Kingdom, September 2011 Astronom´ıa en la Proxima´ Decada:´ Del Hubble al Telescocpio Espacial James Webb C´atedra de Sede Jos´eCelestino Mutis Universidad Nacional, Bogot´a, Colombia, November 2009 Astronomy Education in Colombia: Challenges for the Next Decade XXVII International Astronomical Union (IAU) General Assembly Rio de Janeiro, Brazil, June 2009 ASTRONOMICAL OBSERVATIONS High Resolution Optical Spectroscopy ESO La Silla 3.6 m Telescope, Chile Mid-Infrared Spectroscopy Spitzer Space Telescope, Infrared Spectrograph (IRS) TEACHING Undergrad Research Seminar Teaching Assistant, Spring 2011 Detection of Light Teaching Assistant, Fall 2010 Radioastronomy Teaching Assistant, Fall 2009 SERVICE & OUTREACH IAU Astronomy for Developement Proposal Co-author of a proposal to create a regional node in Colombia ASTROCOL Network of Colombian Astronomers Creator - Moderator Colombian Astronomy & Astrophysics Meetings (COCOA) Founding Member Kaiser Association of Astronomy Students, Leiden President, 2007 REFEREED PUBLICATIONS Ongoing Massive Star Formation in NGC 604 Mart´ınez-Galarza, J. R.; Hunter, D. Groves, B.; Brandl, B., 2012, Astrophysical Journal, 761, 3M. The Physical Conditions in Starbursts Derived from Bayesian Fitting of Mid-IR SED Models: 30 Doradus as a Template Mart´ınez-Galarza, J. R.; Groves, B.; Brandl, B.; de Messieres, G. E.; Indebetouw, R.; Dopita, M. A., 2011, Astrophysical Journal, 738, 176M. Infrared Emission by Dust Around λ Bootis Stars: Debris Disks or Thermally Emit- ting Nebulae? Mart´ınez-Galarza, J. R.; Kamp, I.; Su, K. Y. L.; G´asp´ar, A.; Rieke, G.; Mamajek, E. E., 2009, Astrophysical Journal, Volume 694, Issue 1, pp. 165-173. Modeling the Infrared Bow Shock at δ Velorum: Implications for Studies of Debris Disks and λ Bootis Stars G´asp´ar, A.; Su, K. Y. L.; Rieke, G. H.; Balog, Z.; Kamp, I.; Mart´ınez-Galarza, J. R.; Stapelfeldt, K., 2008, Astrophysical Journal, Volume 672, Issue 2, pp. 974-983 CONFERENCE PROCEEDINGS Wavelength calibration of the JWST-MIRI medium resolution spectrometer Mart´ınez-Galarza, J. R.; Glauser, A. M.; Hern´an-Caballero, A.; Azzollini, R.; Glasse, A.; Kendrew, S.; Brandl, B.; Lahuis, F., 2010, Proceedings of the SPIE Meeting, Volume 7731, pp. 77313Q-77313Q-12 First results from MIRI verification model testing With 30 co-authors, 2008, Proceedings of the SPIE Meeting, Volume 7010, pp. 70103A-70103A-12 λ Bootis stars: Current status and new insights from Spitzer Kamp, I.; Mart´ınez-Galarza, J. R.; Paunzen, E.; Su, K. Y. L.; G´asp´ar, A.; Rieke, G. H., 2008, Contributions of the Astronomical Observatory Skalnat´ePleso, vol. 38, no. 2, p. 147-156.
Load more

Recommended publications
  • Summer 2020 Re Visiting a Past Event
    REINVENTING AMERICAN DEMOCRACY FOR THE 21ST CENTURY THE INTERSECTION OF DEMOCRACY & RELIGION A Nation in Crisis SUMMER 2020 RE VISITING A PAST EVENT Policy Perspectives on Police Use of Lethal Force As America reckons with its relationship to police violence, we are reminded that progress can be slow. It has been more than five years since the deaths of Michael Brown and Eric Garner. On February 4, 2015, the Academy convened a discussion at the University of California, Berkeley, led by Andrea Roth (Assistant Professor of Law, University of California, Berkeley School of Law) and Franklin Zimring (William G. Simon Professor of Law, University of California, Berkeley School of Law) about the hundreds of people who are killed each year by police, the racial disparity among the victims, and the incomplete data that make analyzing the problem so difficult. The conversation also covered the effectiveness of various avenues for police reform. To read the full transcript of this event (published in the Spring 2015 issue of the Bulletin) and hundreds of other Stated Meetings from the last twenty years, please visit amacad.org/bulletin. A video of this event and many others can be found at youtube.com/americanacad. For more information about Academy events, please visit www.amacad.org/events. SUMMER 2020 CONTENTS Features 16 Letters from Members Letters upon election are an Academy tradition. Letters of reflection are something new. 20 Online Discussions A series of virtual programs on topics related to the COVID-19 pandemic. CONTENTS 4 Our Work 4 Reinventing American Democracy for the 21st Century 9 New Issue of Dædalus Explores the Intersection of Democracy & Religion 12 A New Profile of Humanities Departments Members 25 Noteworthy 9 Departments 3 From the President 28 From the Archives ON THE COVER: Several hundred doctors, nurses, and medical professionals gathered on June 5, 2020, in St.
    [Show full text]
  • An Interview with Ewine Van Dishoeck
    Issue 52 j October 2018 . Dear Colleagues, Welcome to the 5th anniversary edition of AstroPAH! What better way to cele- brate this festive occasion with you than with a show of lasers as featured on our cover. This year’s Nobel Prize in physics went to Arthur Ashkin, Gerard´ Mourou and Donna Strickland for their ground-breaking work in creating tools made of light. As the cover reveals, this has been of utmost importance to multiple fields amongst which astronomy and chemistry. Noteworthy is that Donna Strickland is the 3rd woman ever to win a Nobel Prize in physics (and the 1st in over 50 years). We would further like to celebrate our anniversary with a tribute to our Kavli-price winner Ewine van Dishoeck, who was awarded this ”Nobel-price for astronomy” for her ”combined contributions to observational, theoretical, and laboratory astrochemistry, elucidating the life cycle of interstellar clouds and the formation of stars and planets” Enjoy our interview with her in the In Focus. Of course our newsletter itself is also ’In Focus’ with some nice numbers from your feedback, showing our impact in the community. Thanks to all of you who responded to our survey! We will take your feedback into account to improve our newsletter and continue to keep you updated on the rich field of PAH-related research. We also thank everyone who has sent their paper abstracts to us, in this issue and all previous ones. Once again, our abstract section is full of interesting papers on the- oretical, experimental, and observational studies of astronomical PAHs and so much more.
    [Show full text]
  • D:\Dropbox\Phd Leiden University\Thesis\Thesis\Cover V7
    Cover Page The handle http://hdl.handle.net/1887/58690 holds various files of this Leiden University dissertation. Author: Ligterink, N.F.W. Title: The astrochemical factory: A solid base for interstellar reactions Issue Date: 2017-12-18 Publications Published papers Protostellar and cometary detections of organohalogens • Fayolle, E.C.; Oberg,¨ Karin I.; Jørgensen, J.K.; Altwegg, K.; Calcutt, H.; Muller,¨ H.S.P.; Rubin, M.; van der Wiel, M.H.D.; Bjerkeli, P.; Bourke, T.L.; Coutens, A.; van Dishoeck, E.F.; Drozdovskaya, M.N.; Garrod, R.T.; Ligterink, N.F.W.; Persson, M.V.; Wampfler, S.F.; Rosina Team The ALMA-PILS survey: detection of CH3NCO towards the low-mass protostar • IRAS 16293–2422 and laboratory constraints on its formation Ligterink, N.F.W.; Coutens, A.; Kofman, V.; Muller,¨ H.S.P.; Garrod, R.T.; Calcutt, H.; Wampfler, S.F.; Jørgensen, J.K.; Linnartz, H.; van Dishoeck, E.F.; 2017, Monthly Notices of the Royal Astronomical Society, Volume 469, Issue 2 The (w)hole survey: An unbiased sample study of transition disk candidates based • on Spitzer catalogs van der Marel, N.; Verhaar, B. W.; van Terwisga, S.; Mern, B.; Herczeg, G.; Ligterink, N. F. W.; van Dishoeck, E. F.; 2016, Astronomy & Astrophysics, Volume 592 The ALMA-PILS survey: First detections of deuterated formamide and deuterated • isocyanic acid in the interstellar medium Coutens, A.; Jørgensen, J. K.; van der Wiel, M. H. D.; Muller,¨ H. S. P.; Lykke, J. M.; Bjerkeli, P.; Bourke, T. L.; Calcutt, H.; Drozdovskaya, M. N.; Favre, C.; Fayolle, E. C.; Garrod, R. T.; Jacobsen, S.
    [Show full text]
  • Cover Page the Handle
    Cover Page The handle http://hdl.handle.net/1887/20396 holds various files of this Leiden University dissertation. Author: Bast, Jeanette Elisabeth Title: Hot chemistry and physics in the planet-forming zones of disks Issue Date: 2013-01-10 Publications Refereed papers 1. Exploring organic chemistry in planet-forming zones Jeanette E. Bast, Fred Lahuis, Ewine F. van Dishoeck & Alexander G. G. M. Tielens; Submitted to Astronomy & Astrophysics (Chapter 5) 2. First detection of near-infrared line emission from organics in young circumstellar disks Avi M. Mandell, Jeanette E. Bast, Ewine F. van Dishoeck, Geoffrey A. Blake, Colette Salyk, Michael J. Mumma, M. & Geronimo Villanueva; 2012, The Astrophysical Journal, 747, 92 (Chapter 3) 3. Single peaked CO emission line profiles from the inner regions of protoplanetary disks Jeanette E. Bast, Joanna M. Brown, Gregory J. Herczeg, Ewine van F. Dishoeck & Klaus M. Pontoppidan; 2011, Astronomy & Astrophysics, 527, A119 (Chapter 2) 4. The abundance of SiS in circumstellar envelopes around AGB stars Fredrik L. Schöier, Jeanette E. Bast, Hans Olofsson & Michael Lindqvist; 2007, Astronomy & Astrophysics, 473, 871 Non-refereed papers Planet-forming regions at the highest spectral and spatial resolution with VLT- CRIRES Klaus M. Pontopppidan, Ewine F. van Dishoeck, Geoffrey A. Blake, Rachel Smith, Joanna M. Brown, Gregory J. Herczeg, Jeanette E. Bast, Avi M. Mandell, Alain Smette, Wing-Fai This, Edward D. Young, Mark R. Mor- ris William Dent & Hans Ulrich Käufl; 2011, Messenger, 143, 32 169 Publications Conference proceedings 1. New probes of the chemistry in the inner regions of planet-forming disks Jeanette. E. Bast, Avi M.
    [Show full text]
  • Division Vi / Commission 34 / Working Group Astrochemistry
    Transactions IAU, Volume XXVIIIA Reports on Astronomy 2009–2012 c International Astronomical Union 2012 Ian Corbett, ed. doi:10.1017/S1743921312002876 DIVISION VI / COMMISSION 34 / WORKING GROUP ASTROCHEMISTRY CHAIR E.F. van Dishoeck VICE-CHAIR E. Herbst BOARD Y. Aikawa J.H. Black G.A. Blake P. Caselli J. Cernicharo G. Garay M. Guelin U.G. Jørgensen J.P. Maier K.M. Menten T.J. Millar S. Kwok F. Salama I. Sims A. Sternberg TRIENNIAL REPORT 2009-2012 1. Introduction The study of molecules in space, known as astrochemistry or molecular astrophysics, is a rapidly growing field. Molecules exist in a wide range of environments in both gaseous and solid form, from our own solar system to the distant early universe. To astronomers, molecules are indispensable and unique probes of the physical conditions and dynamics of regions in which they are detected, especially the interstellar medium. In particular, the many stages of both low-mass and high-mass star formation are better understood today thanks to the analysis of molecular observations. Molecules can also yield a global picture of the past and present of sources. Moreover, molecules affect their environment by contributing to the heating and cooling processes that occur. Molecular observations are currently being used to study the interstellar gas and dust in diffuse interstellar clouds, dense molecular clouds, protostellar objects, maser and star-forming regions, envelopes of evolved stars, protoplanetary disks, (exo-)planetary atmospheres and comets. In addition to our own Milky Way Galaxy, molecules and solid- state features are routinely detected in interstellar regions of external galaxies ranging from the nearby Magellanic Clouds to distant starbust galaxies at redshifts of more than 6.
    [Show full text]
  • Pnas11052ackreviewers 5098..5136
    Acknowledgment of Reviewers, 2013 The PNAS editors would like to thank all the individuals who dedicated their considerable time and expertise to the journal by serving as reviewers in 2013. Their generous contribution is deeply appreciated. A Harald Ade Takaaki Akaike Heather Allen Ariel Amir Scott Aaronson Karen Adelman Katerina Akassoglou Icarus Allen Ido Amit Stuart Aaronson Zach Adelman Arne Akbar John Allen Angelika Amon Adam Abate Pia Adelroth Erol Akcay Karen Allen Hubert Amrein Abul Abbas David Adelson Mark Akeson Lisa Allen Serge Amselem Tarek Abbas Alan Aderem Anna Akhmanova Nicola Allen Derk Amsen Jonathan Abbatt Neil Adger Shizuo Akira Paul Allen Esther Amstad Shahal Abbo Noam Adir Ramesh Akkina Philip Allen I. Jonathan Amster Patrick Abbot Jess Adkins Klaus Aktories Toby Allen Ronald Amundson Albert Abbott Elizabeth Adkins-Regan Muhammad Alam James Allison Katrin Amunts Geoff Abbott Roee Admon Eric Alani Mead Allison Myron Amusia Larry Abbott Walter Adriani Pietro Alano Isabel Allona Gynheung An Nicholas Abbott Ruedi Aebersold Cedric Alaux Robin Allshire Zhiqiang An Rasha Abdel Rahman Ueli Aebi Maher Alayyoubi Abigail Allwood Ranjit Anand Zalfa Abdel-Malek Martin Aeschlimann Richard Alba Julian Allwood Beau Ances Minori Abe Ruslan Afasizhev Salim Al-Babili Eric Alm David Andelman Kathryn Abel Markus Affolter Salvatore Albani Benjamin Alman John Anderies Asa Abeliovich Dritan Agalliu Silas Alben Steven Almo Gregor Anderluh John Aber David Agard Mark Alber Douglas Almond Bogi Andersen Geoff Abers Aneel Aggarwal Reka Albert Genevieve Almouzni George Andersen Rohan Abeyaratne Anurag Agrawal R. Craig Albertson Noga Alon Gregers Andersen Susan Abmayr Arun Agrawal Roy Alcalay Uri Alon Ken Andersen Ehab Abouheif Paul Agris Antonio Alcami Claudio Alonso Olaf Andersen Soman Abraham H.
    [Show full text]
  • Alexander Dalgarno: from Atomic and Molecular Physics to Astronomy and Aeronomy Ewine F
    RETROSPECTIVE Alexander Dalgarno: From atomic and molecular physics to astronomy and aeronomy Ewine F. van Dishoecka,1, Tom Hartquistb, and Amiel Sternbergc Massey, who offered Alex a fellowship toward aLeiden Observatory, Leiden University, 2300 RA Leiden, The Netherlands; bSchool of Physics a doctorate in atomic physics. Alex accepted and Astronomy, University of Leeds, Leeds LS2 9JT, United Kingdom; and cSchool of Physics and made the switch to physics. This episode & Astronomy, Tel Aviv University, Ramat Aviv 69978, Israel highlights the importance of spotting talent at an early age. Alex himself excelled at nurturing early career researchers, and the AsSirDavidBateswrotein1988,“There is from the combination of his seminal insight “Dalgarno scientific family tree” contains no greater figure than Alex Dalgarno in the and unparalleled, boundless, and sustained 70 graduate students and 36 postdocs. Alex history of atomic-molecular-optical [AMO] productivity. His long career is described in guided and mentored all of them with the physics, and its applications” (1). Prof. Alex- his autobiographical article “A serendipitous utmost thoughtfulness and care. ander Dalgarno (Harvard) passed away peace- journey” (2) and in the books written in his After completing his doctorate in 1951, fully on April 9, 2015 at age 87 in the presence – honor (1, 3 5). Alex was offered a Lecturer position in Ap- of his long-term companion, Fern Creelan. Alex, a twin and the youngest of five plied Mathematics at the Queen’s University During a career spanning 60 years, Alex children, was born in London in 1928 and of Belfast. Together with David Bates, he built produced about 750 publications covering a grew up during the Second World War.
    [Show full text]
  • Astrophysics Prize 2018 Explanatory Notes
    ASTROPHYSICS PRIZE 2018 EXPLANATORY NOTES Molecules in space: the raw material for stars and planets The 2018 Kavli Prize for Astrophysics goes to Ewine van Dishoeck “for her combined contributions to observational, theoretical, and laboratory astrochemistry, elucidating the life cycle of interstellar clouds and the formation of stars and planets”. A star forms when a relatively dense region of the gas that fills the space between existing stars begins to collapse under its own gravity. As the gas is compressed it heats up, to the point where the atomic nuclei within it have enough energy to overcome their mutual repulsion and fuse. The enormous heat given off in these nuclear reactions generates a pressure that counteracts gravity, eventually resulting in a stable star that shines in the night sky. This process of fusion burning creates heavier elements from lighter ones. But the interstellar gas from which a star is ESO Photo Ambassador Babak Tafreshi snapped this remarkable image of the antennas of the Atacama Large Mil- made already contains a rich variety of limeter/submillimeter Array (ALMA), set against the splendour of the Milky Way. Ewine van Dishoeck has been molecules (in addition to molecular heavily involved in the development and use of the ALMA observatory. Credit: ESO/B. Tafreshi (twanight.org) hydrogen, by far the most abundant). Ewine van Dishoeck has studied these readily destroyed by ultraviolet starlight. hunch was vindicated when the molecules extensively, using her The density of particles within researchers first found signals from knowledge of chemistry to better interstellar clouds is higher than in ammonia molecules and then from understand how they are created, how surrounding space but would still be so water.
    [Show full text]
  • Dutch Astrochemistry Network – II
    Publication: Netherlands Organisation for Scientific Research (NWO) NWO Domain Science E: [email protected] W: www.nwo.nl/astrochemistry April 2018 Dutch Astrochemistry Network – II Netherlands Organisation for Scientific Research Colophon Text: Dutch Astrochemistry Community Coordination and editing: Sebastiaan de Vet Design: Christy Renard (Communications) Printed by: Ipskamp printing On the cover: Detail of the Galactic Plane visible from the southern hemisphere imaged during the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL). The APEX data, at a wavelength of 0.87 millimetres, shows up in red and the background blue image was imaged at shorter infrared wavelengths by the NASA Spitzer Space Telescope as part of the GLIMPSE survey. The fainter extended red structures come from complementary observations made by ESA’s Planck satellite. Credits: ESO/APEX/ATLASGAL consortium/NASA/ GLIMPSE consortium/ESA/Planck Dutch Astrochemistry Network – II The Hague, April 2018 Netherlands Organisation for Scientific Research 2 Figure 1 Illustration of the lifecycle of molecules in the interstellar medium. Chemical processes take place at every stage in this process – from the birth of molecules in circumstellar shells, their passing through the physical gauntlet of the interstellar medium ultimately fuelling star and planet formation – and this controls the organic inventory of planetary systems. Preface In 2010, the Netherlands Organisation for Scientific Research (NWO) funded the Dutch Astrochemistry Network as a coherent and integrated
    [Show full text]
  • Programme Book
    PROGRAMME 1 Programme Water in the Universe: From Clouds to Oceans COMMITTEES Scientific Organising Committee (SOC) Yuri Aikawa University of Tsukuba, Japan Ted Bergin University of Michigan, United States of America Cecilia Ceccarelli University of Grenoble, France Ewine van Dishoeck Leiden Observatory, The Netherlands Yu Gao Purple Mountain Observatory, Nanjing, China Paul Hartogh MPS, Göttingen, Germany Darek Lis LERMA, Paris, France Göran Pilbratt ESA/ESTEC, Noordwijk, The Netherlands Axel Weiss MPIfR, Bonn, Germany Local Organising Committee (LOC) The LOC consists of: Göran Pilbratt Mylène Riemens Congrex - ESA Conference Bureau 2 Programme Water in the Universe: From Clouds to Oceans PROGRAMME Tuesday 12 April 2016 08:00 – 09:00 Registration & Posters can be mounted for display 09:00 – 09:20 Introduction & Logistics Session 1: Formation and Destruction of Water and its Chemistry: Theory, Laboratory Work, and Models 09:20 Water: Past, Present, and Future Gary J. Melnick Harvard-Smithsonian Center for Astrophysics, United States of America 10:00 Interstellar Water Ice Formation: A Laboratory Perspective Sergio Ioppolo1, Thanja Lamberts2, Herma Cuppen3, Harold Linnartz4 1The Open University, United Kingdom; 2University of Stuttgart, Germany; 3Radboud University Nijmegen, Netherlands; 4Leiden University, The Netherlands 10:30 Laser Desorption Time-of-flight Mass Spectrometry Of VUV Photo- processed Ice Daniel Paardekooper, Harold Linnartz Sackler Laboratory for Astrophysics, Leiden Observatory, Leiden University, The Netherlands 10:50
    [Show full text]
  • Report for the Academic Year 2017–2018
    Institute for Advanced Study Re port for 2 0 1 7–2 0 INSTITUTE FOR ADVANCED STUDY 1 8 EINSTEIN DRIVE PRINCETON, NEW JERSEY 08540 Report for the Academic Year (609) 734-8000 www.ias.edu 2017–2018 Cover: SHATEMA THREADCRAFT, Ralph E. and Doris M. Hansmann Member in the School of Social Science (right), gives a talk moderated by DIDIER FASSIN (left), James D. Wolfensohn Professor, on spectacular black death at Ideas 2017–18. Opposite: Fuld Hall COVER PHOTO: DAN KOMODA Table of Contents DAN KOMODA DAN Reports of the Chair and the Director 4 The Institute for Advanced Study 6 School of Historical Studies 8 School of Mathematics 20 School of Natural Sciences 30 School of Social Science 40 Special Programs and Outreach 48 Record of Events 57 80 Acknowledgments 88 Founders, Trustees, and Officers of the Board and of the Corporation 89 Administration 90 Present and Past Directors and Faculty 91 Independent Auditors’ Report THOMAS CLARKE REPORT OF THE CHAIR The Institute for Advanced Study’s independence and excellence led by Sanjeev Arora, Visiting Professor in the School require the dedication of many benefactors, and in 2017–18, of Mathematics. we celebrated the retirements of our venerable Vice Chairs The Board was delighted to welcome new Trustees Mark Shelby White and Jim Simons, whose extraordinary service has Heising, Founder and Managing Director of the San Francisco enhanced the Institute beyond measure. I am immensely grateful investment firm Medley Partners, and Dutch astronomer and and feel exceptionally privileged to have worked with both chemist Ewine Fleur van Dishoeck, Professor of Molecular Shelby and Jim in shaping and guiding the Institute into the Astrophysics at the University of Leiden.
    [Show full text]
  • Leiden Observatory Workshop: Photodissociation in Astrochemistry
    Leiden Observatory workshop: Photodissociation in astrochemistry 3–5 February, 2015 Kasteel Oud Poelgeest, Leiden Webpage: www.strw.leidenuniv.nl/cms/web/2015/20150203/info.php3?wsid=36 Contact: Alan Heays (email: [email protected], telephone: +31 6 5944 8367) Ewine van Dishoeck (email: [email protected]) 1 Overview This focussed workshop seeks to clarify the outstanding questions and priorities relevant to the forthcoming era of astrochemistry, and evaluate the present and future capabilities of spectroscopists and chemical physicists. We hope to encourage the investigation of photodissociation problems of immediate interest to astrochemistry. The format of the meeting is in the spirit of a true workshop, with plenty of time for discussions and interactions. The proposed topics for discussion are: Problems in astrochemical photodissociation • Which molecules are present in clouds, disks, and planet atmospheres exposed to intense UV radiation; how do they photodissociate: through lines or continuum; how do they (observably) influence their surroundings? • What are the important ranges of temperature, density, extinction magnitudes, and UV wavelengths? • What is the most useful kind of data? A completely assigned and modelled spectrum, raw experimental cross sections and linelists, superb accuracy over a small wavelength range (e.g., Ly alpha) or lower accuracy over a much larger range? Importance of self- and mutual shielding and tabulation of shielding functions; isotope selective processes? • Photolysis in the gas phase vs ices; small versus large molecules (PAHs) • Contributions to public databases: – Mainz UV/VIS database – Leiden photodissociation database of astrophysical molecules – PHIDRATES photoionisation and photodissociation rates – KIDA (KInetic Database for Astrochemistry) Capabilities and challenges of laboratory experiments • The generation of UV radiation: synchrotrons, lasers, plasmas, or electron excitation.
    [Show full text]