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Javier Peralta Calvillo Generated From: Editor CVN De FECYT Date of Document: 24/01/2021 V 1.4.3 4154B7e2be6a86b67f637261e4ad3d11
Javier Peralta Calvillo Generated from: Editor CVN de FECYT Date of document: 24/01/2021 v 1.4.3 4154b7e2be6a86b67f637261e4ad3d11 This electronic file (PDF) has embedded CVN technology (CVN-XML). The CVN technology of this file allows you to export and import curricular data from and to any compatible data base. List of adapted databases available at: http://cvn.fecyt.es/ 4154b7e2be6a86b67f637261e4ad3d11 General quality indicators of scientific research This section describes briefly the main quality indicators of scientific production (periods of research activity, experience in supervising doctoral theses, total citations, articles in journals of the first quartile, H index...). It also includes other important aspects or peculiarities. My name is Javier Peralta and I was born in Algeciras (1979, Spain). I graduated in Physics at the University of La Laguna (Spain) in 2003, specializing in the fields of Astrophysics and Applied Physics. In 2009, I got an European PhD degree in Physics at the University of the Basque Country (Spain) with the highest qualification ("Cum Laude") . My PhD research, supervised by Professors Agustín Sánchez-Lavega and Ricardo Hueso, focused on the atmospheric dynamics of the planet Venus using data from the space missions Galileo and Venus Express. As a result, 6 articles were published in international peer review journals (4 of them as first author) along with more than 80 citations which allowed to be awarded in 2012 with the “Extraordinary Prize of Doctorate” granted by the University of the Basque Country. After my PhD, I spent the last 10 years (2009-2019) working in different research institutions as postdoctoral researcher: 2 years at IAA/CSIC in Granada (Spain), 3 years at the Astronomical Observatory of Lisbon (CAAUL/OAL, Portugal) and 5 years at the Institute of Space and Astronautical Science of Japan (ISAS/JAXA), funded by JAXA's International Top Young Fellowship (ITYF). -
David Charbonneau Refereed Publications As of May 2015
David Charbonneau Refereed Publications as of May 2015 160. Low False Positive Rate of Kepler Candidates Estimated From A Combination Of Spitzer And Follow-Up Observations Désert, Jean-Michel; Charbonneau, David; Torres, Guillermo; Fressin, François; Ballard, Sarah; Bryson, Stephen T.; Knutson, Heather A.; Batalha, Natalie M.; Borucki, William J.; Brown, Timothy M.; Deming, Drake; Ford, Eric B.; Fortney, Jonathan J.; Gilliland, Ronald L.; Latham, David W.; Seager, Sara The Astrophysical Journal, Volume 804, Issue 1, article id. 59 (2015). 159. The Mass of Kepler-93b and The Composition of Terrestrial Planets Dressing, Courtney D.; Charbonneau, David; Dumusque, Xavier; Gettel, Sara; Pepe, Francesco; Collier Cameron, Andrew; Latham, David W.; Molinari, Emilio; Udry, Stéphane; Affer, Laura; Bonomo, Aldo S.; Buchhave, Lars A.; Cosentino, Rosario; Figueira, Pedro; Fiorenzano, Aldo F. M.; Harutyunyan, Avet; Haywood, Raphaëlle D.; Johnson, John Asher; Lopez-Morales, Mercedes; Lovis, Christophe; Malavolta, Luca; Mayor, Michel; Micela, Giusi; Motalebi, Fatemeh; Nascimbeni, Valerio; Phillips, David F.; Piotto, Giampaolo; Pollacco, Don; Queloz, Didier; Rice, Ken; Sasselov, Dimitar; Ségransan, Damien; Sozzetti, Alessandro; Szentgyorgyi, Andrew; Watson, Chris The Astrophysical Journal, Volume 800, Issue 2, article id. 135 (2015). 158. An Empirical Calibration to Estimate Cool Dwarf Fundamental Parameters from H-band Spectra Newton, Elisabeth R.; Charbonneau, David; Irwin, Jonathan; Mann, Andrew W. The Astrophysical Journal, Volume 800, Issue 2, article -
TESS Discovery of a Super-Earth and Three Sub-Neptunes Hosted by the Bright, Sun-Like Star HD 108236
Swarthmore College Works Physics & Astronomy Faculty Works Physics & Astronomy 2-1-2021 TESS Discovery Of A Super-Earth And Three Sub-Neptunes Hosted By The Bright, Sun-Like Star HD 108236 T. Daylan K. Pinglé J. Wright M. N. Günther K. G. Stassun Follow this and additional works at: https://works.swarthmore.edu/fac-physics See P nextart of page the forAstr additionalophysics andauthors Astr onomy Commons Let us know how access to these works benefits ouy Recommended Citation T. Daylan, K. Pinglé, J. Wright, M. N. Günther, K. G. Stassun, S. R. Kane, A. Vanderburg, D. Jontof-Hutter, J. E. Rodriguez, A. Shporer, C. X. Huang, T. Mikal-Evans, M. Badenas-Agusti, K. A. Collins, B. V. Rackham, S. N. Quinn, R. Cloutier, K. I. Collins, P. Guerra, Eric L.N. Jensen, J. F. Kielkopf, B. Massey, R. P. Schwarz, D. Charbonneau, J. J. Lissauer, J. M. Irwin, Ö Baştürk, B. Fulton, A. Soubkiou, B. Zouhair, S. B. Howell, C. Ziegler, C. Briceño, N. Law, A. W. Mann, N. Scott, E. Furlan, D. R. Ciardi, R. Matson, C. Hellier, D. R. Anderson, R. P. Butler, J. D. Crane, J. K. Teske, S. A. Shectman, M. H. Kristiansen, I. A. Terentev, H. M. Schwengeler, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, Z. K. Berta-Thompson, L. G. Bouma, W. Fong, G. Furesz, C. E. Henze, E. H. Morgan, E. Quintana, E. B. Ting, and J. D. Twicken. (2021). "TESS Discovery Of A Super-Earth And Three Sub-Neptunes Hosted By The Bright, Sun-Like Star HD 108236". -
David Charbonneau Curriculum Vitae (December 2013)
David Charbonneau Curriculum vitae (December 2013) Harvard University, Department of Astronomy, 60 Garden St., Cambridge, MA 02138 Email: [email protected] Web: www.cfa.harvard.edu/~dcharbon Office: 617 496 6515 Fax: 617 495 7049 Current Position Professor of Astronomy, Harvard University Education Harvard University, A. M. (Astronomy, 1999), Ph. D. (Astronomy, 2001) U. of Toronto, Honors B. Sc. with high distinction (Math, Physics, & Astronomy, 1996) Previous Positions Thomas D. Cabot Associate Professor of Astronomy, 2008-2009, Harvard University Assistant Professor of Astronomy, 2004-2007, Harvard University R. A. Millikan Postdoctoral Scholar in Astronomy, 2001-2004, California Institute of Technology Research Focus Detection and characterization of exoplanets with the goal of studying inhabited worlds Selected Awards The Raymond and Beverly Sackler Prize in the Physical Sciences, 2012 UC Alumni of Influence Award, University of Toronto, 2012 Fannie Cox Prize for Excellence in Science Teaching, Harvard University, 2011 Alan T. Waterman Award, National Science Foundation, 2009 Scientist of the Year, Discover Magazine, 2007 David and Lucile Packard Fellowship for Science and Engineering, 2006 – 2011 NASA Exceptional Scientific Achievement Medal, 2006 Alfred P. Sloan Research Fellow, 2006 – 2008 Robert J. Trumpler Award, Astronomical Society of the Pacific, 2004 Bart J. Bok Prize in Astronomy, Harvard University, 2004 Fireman Award for PhD Thesis in Astronomy, Harvard University, 2000 Merit Fellowship, Harvard University, -
Table of Contents
AAS Newsletter November/December 2012, Issue 167 - Published for the Members of the American Astronomical Society Table of Contents 2 President’s Column 23 Committee on Employment 3 From the Executive Office 24 Committee on the Status of Women in 4 On the Waterfront: AAS Returns to Long Astronomy Beach 25 Bringing Sustainability into Your Institution 5 2012 Kavli Lecturers 27 Calendar of Events 7 HAD News 28 Announcements 8 JWST Update 29 United Nations Basic Space Science Initiative 12 Candidate Statements (UNBSSI) 1991-2012 21 News from NSF Division of Astronomical Sciences (AST) Back page Washington News 22 News from the Astronomical Society of the Pacific (ASP) A A S American Astronomical Society President's Column AAS Officers David J. Helfand, President David J. Helfand, [email protected] Debra M. Elmegreen, Past President Nicholas B. Suntzeff, Vice-President Edward B. Churchwell, Vice-President Paula Szkody, Vice-President From close-up pictures of water-sculpted pebbles on Hervey (Peter) Stockman, Treasurer G. Fritz Benedict, Secretary Mars, to the detection of galaxies at the boundary of Anne P. Cowley, Publications Board Chair the Dark Ages, discoveries in our field continue to Edward E. Prather, Education Officer advance our understanding of the Universe and to Councilors fascinate legions of the public who support our inquiry. Bruce Balick Nancy S. Brickhouse Unfortunately, we do not see similar progress in the Eileen D. Friel political sphere, even now that the consequences have Edward F. Guinan been spelled out of allowing budget sequestration to hit Todd J. Henry Steven D. Kawaler every government agency in January. -
Jason A. Dittmann 51 Pegasi B Postdoctoral Fellow
Jason A. Dittmann 51 Pegasi b Postdoctoral Fellow Contact Massachusetts Institute of Technology MIT Kavli Institute: 37-438f 617-258-5928 (office) 70 Vassar St. 520-820-0928 (cell) Cambridge, MA 02139 [email protected] Education Harvard University, Cambridge, MA PhD, Astronomy and Astrophysics, May 2016 Advisor: David Charbonneau, PhD • University of Arizona, Tucson, AZ BS, Astronomy, Physics, May 2010 Advisor: Laird Close, PhD • Recent 51 Pegasi b Postdoctoral Fellow July 2017 – Present Research Earth and Planetary Science Department, MIT Positions Faculty Contact: Sara Seager Postdoctoral Researcher Feb 2017 – June 2017 Kavli Institute, MIT Supervisor: Sarah Ballard Postdoctoral Researcher July 2016 – Jan 2017 Center for Astrophysics, Harvard University Supervisor: David Charbonneau Research Assistant Sep 2010 – May 2016 Center for Astrophysics, Harvard University Advisors: David Charbonneau Publication 16 first and second authored publications Summary 22 additional co-authored publications 1 first-authored publication in Nature 1 co-authored publication in Nature Selected 51 Pegasi b Postdoctoral Fellowship 2017 – Present Awards and Pierce Fellowship 2010 – 2013 Honors Certificate of Distinction in Teaching 2012 Best Project Award, Physics Ugrd. Research Symp. 2009 Best Undergraduate Research (Steward Observatory) 2009 – 2010 Grants Principal Investigator, Hubble Space Telescope 2017, 10 orbits Awarded “Initial Reconaissance of a Transiting Rocky (maximum award) Planet in a Nearby M-Dwarf’s Habitable Zone” Principal Investigator, -
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars Origins | Climate | Discovery Jacob Bean (University of Chicago) Presented on behalf of the FINESSE/CASE science team: Mark Swain (PI), Nicholas Cowan, Jonathan Fortney, Caitlin Griffith, Tiffany Kataria, Eliza Kempton, Laura Kreidberg, David Latham, Michael Line, Suvrath Mahadevan, Jorge Melendez, Julianne Moses, Vivien Parmentier, Gael Roudier, Evgenya Shkolnik, Adam Showman, Kevin Stevenson, Yuk Yung, & Robert Zellem Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars **Candidate NASA MIDEX mission for launch in 2023** Objectives FINESSE will test theories of planetary origins and climate, transform comparative planetology, and open up exoplanet discovery space by performing a comprehensive, statistical, and uniform survey of transiting exoplanet atmospheres. Strategy • Transmission spectroscopy of 500 planets: Mp = few – 1,000 MEarth • Phase-resolved emission spectroscopy of a subset of 100 planets: Teq > 700 K • Focus on synergistic science with JWST: homogeneous survey, broader context, population properties, and bright stars Hardware • 75 cm aluminum Cassegrain telescope at L2 • 0.5 – 5.0 μm high-throughput prism spectrometer with R > 80 • Single HgCdTe detector with JWST heritage for science and guiding Origins | Climate | Discovery Advantages of Fast Infrared -
Arxiv:2010.15996V1 [Astro-Ph.IM] 29 Oct 2020 Keywords: ARIEL, Exoplanets, Transit Photometry, Light Curves, Stellar Spots, Machine Learning
Draft version November 2, 2020 Typeset using LATEX default style in AASTeX63 Lessons Learned from the 1st ARIEL Machine Learning Challenge: Correcting Transiting Exoplanet Light Curves for Stellar Spots Nikolaos Nikolaou ,1 Ingo P. Waldmann ,1 Angelos Tsiaras ,1 Mario Morvan ,1 Billy Edwards ,1 Kai Hou Yip ,1 Giovanna Tinetti ,1 Subhajit Sarkar,2 James M. Dawson,2 Vadim Borisov,3 Gjergji Kasneci,3 Matej Petkovic,´ 4 Tomaˇz Stepiˇsnik,4 Tarek Al-Ubaidi,5, 6 Rachel Louise Bailey ,6 Michael Granitzer ,7 Sahib Julka ,7 Roman Kern,8 Patrick Ofner ,8 Stefan Wagner,9 Lukas Heppe ,10 Mirko Bunse ,10 and Katharina Morik 10 1Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK 2School of Physics and Astronomy, Cardiff University, The Parade, Cardiff, CF24 3AA, UK 3Department of Computer Science, University of Tuebingen, Tuebingen, Germany 4Joˇzef Stefan Institute, Ljubljana, Slovenia 5DCCS, Austria 6Space Research Institute, Austrian Academy of Sciences, Austria 7Chair of Data Science, University of Passau, Germany 8Know-Center GmbH - Research Center for Data-Driven Business & Big Data Analytics, Austria 9Commission for Astronomy, Austrian Academy of Sciences, Graz, Austria 10Artificial Intelligence Group, TU Dortmund University, Germany Submitted to ApJ ABSTRACT The last decade has witnessed a rapid growth of the field of exoplanet discovery and characterisation. However, several big challenges remain, many of which could be addressed using machine learning methodology. For instance, the most prolific method for detecting exoplanets and inferring several of their characteristics, transit photometry, is very sensitive to the presence of stellar spots. The current practice in the literature is to identify the effects of spots visually and correct for them manually or discard the affected data. -
When Extrasolar Planets Transit Their Parent Stars 701
Charbonneau et al.: When Extrasolar Planets Transit Their Parent Stars 701 When Extrasolar Planets Transit Their Parent Stars David Charbonneau Harvard-Smithsonian Center for Astrophysics Timothy M. Brown High Altitude Observatory Adam Burrows University of Arizona Greg Laughlin University of California, Santa Cruz When extrasolar planets are observed to transit their parent stars, we are granted unprece- dented access to their physical properties. It is only for transiting planets that we are permitted direct estimates of the planetary masses and radii, which provide the fundamental constraints on models of their physical structure. In particular, precise determination of the radius may indicate the presence (or absence) of a core of solid material, which in turn would speak to the canonical formation model of gas accretion onto a core of ice and rock embedded in a proto- planetary disk. Furthermore, the radii of planets in close proximity to their stars are affected by tidal effects and the intense stellar radiation. As a result, some of these “hot Jupiters” are significantly larger than Jupiter in radius. Precision follow-up studies of such objects (notably with the spacebased platforms of the Hubble and Spitzer Space Telescopes) have enabled direct observation of their transmission spectra and emitted radiation. These data provide the first observational constraints on atmospheric models of these extrasolar gas giants, and permit a direct comparison with the gas giants of the solar system. Despite significant observational challenges, numerous transit surveys and quick-look radial velocity surveys are active, and promise to deliver an ever-increasing number of these precious objects. The detection of tran- sits of short-period Neptune-sized objects, whose existence was recently uncovered by the radial- velocity surveys, is eagerly anticipated. -
January 2004 Issue of the OSS Voyages Newsletter
COMMITTEE ON THE STATUS OF MINORITIES IN ASTRONOMY J ANUARY 2004 SPECTRUM A report on underrepresented minorities in astronomy INSIDE THIS ISSUE: So… What About 1 So… What About Diversity? Diversity? by Marcel Agueros Professional Organi- 1 zations of Minorities Led by a team of graduate students, the University of in Physical Sciences Washington Astronomy Department has developed a The Accountability 4 departmental plan for more effectively engaging diver- Side of Diversity sity issues through enhanced coordination of effort and improved leveraging of available resources. What’s in a Name? 6 Marcel Agueros describes how they went about it and Astronomy Faculty 9 what they learned along the way. Diversity Survey: Preliminary Results A Small First Step 10 he meeting was over. For nearly an hour the graduate students and the graduate program ad- Ph.D. Productivity of 12 visor had intensively discussed a number of Historically Black T Colleges pressing departmental issues. We were wrapping up Marcel Agueros is a when a question was casually dropped on the table: 4th-year astronomy SASS: Cultivating the 14 “What about diversity?” graduate student at the Next Generation of University of Washing- Astronomers What seemed like a simple enough question to ask ton. His dissertation NASA Space Science 16 turned out to be a very difficult question to answer. That research is on X-ray Diversity Initiatives meeting took place about a year ago, and we are still selected stars from the working our way to a good answer. However, with the RASS and SDSS Sur- Meet Dara Norman at 17 help of some friends—the Graduate Opportunities and veys under the direc- CTIO Minority Achievement Program and ADVANCE here at tion of Scott Anderson. -
Making a Massive Open Online Course (MOOC) About Astrobiology: Why? for Whom? How?
EPJ Web of Conferences 200, 01019 (2019) https://doi.org/10.1051/epjconf/201920001019 ISE2A 2017 Making a Massive Open Online Course (MOOC) about Astrobiology: Why? For Whom? How? Charles H. Lineweaver1,* 1Research School of Astronomy and Astrophysics and the Research School of Earth Sciences, Australian National University, Canberra, ACT 0200, Australia Abstract. Massive Open Online Courses (MOOCs) are becoming the textbooks of the 21st century. I describe what a MOOC is, and try to answer the questions: Why make a MOOC? Who are MOOCs for? and How to make a MOOC? Anxiety about MOOCs replacing teachers is largely misplaced. I describe my on-going experience of putting together an astrobiology MOOC for the Australian National University. 1 What is a MOOC? 1.1 History: from tutoring, to lecturing, to MOOCing Socrates, Plato and Aristotle participated in private tutoring and small group discussions (Fig. 1). They did not give lectures to hundreds of students. Lectures seem to have been invented by the first European universities in the 13th or 14th centuries (Fig. 2). N.B. this was before the 1440 invention of the printing press by Gutenberg. At our meeting, the International Symposium on Education in Astronomy and Astrobiology, Karen Meech recounted some of her experiences organizing workshops, schools and fieldtrips. The most rewarding permanent learning and bonding was done with “long small meaningful discussions” in the context of a community of learners in some kind of isolation from the world. She seemed agnostic about the type of isolation: Hawaiian military barracks, island monasteries, ivory towers, Walden ponds, even deserts would do. -
2024 Solar Eclipse: Totality Over Texas
2024 Solar Eclipse: Totality Over Texas April 6-9, 2024 $2,295 PER PERSON, DOUBLE OCCUPANCY, $3,895, SINGLE OCCUPANCY, PLUS AIRFARE Join MSU Professor and astronomer *Dr. Megan Donahue and experience an incredible natural phenomenon of a total eclipse. On April 8, 2024, the moon will pass between the earth and the sun and be replaced by pink flames and silver streamers that stretch across the sky. Come see the eclipse from the beautiful Lake District north of Austin, Texas. Along with Dr. Donahue, enjoy outstanding expert speakers including Dr. Doug Duncan, Dr. Steve Hawley, Chris Impey, Erica Ellingson, Nick Schneider and Dr. Emily Levesque. Accommodations are at the Hyatt Regency Austin, close to downtown Austin and where guest lectures will occur or the Horseshoe Bay Resort, in the countryside Lake District, near the centerline of where the eclipse will be viewed. A total eclipse is like Tour Inclusions: no other and one of the best viewing spots for the • 3 night’s accommodations at either the Hyatt eclipse will be on this trip. Don’t miss this chance of a Regency Austin or *Horseshoe Bay Resort. lifetime, the next total eclipse visible in the U.S. will not • Breakfast, lunch and dinner daily occur until 2045. • Internationally know guest speakers • Eclipse viewing Star Party • Night viewing with telescopes from Horseshoe Bay MSU Faculty Host which is a Dark Sky Reserve Dr. Megan Donahue is a University Distinguished Professor of • Transportation to and from the Austin International Physics and Astronomy at Michigan State University. She was Airport, as well as to and from all scheduled eclipse the President of the American sessions at the Horseshoe Bay Resort and Hyatt Astronomical Society from 2018-2020, and has been very ac- Regency Austin tive in national and international • Pair of special glasses to view the eclipse scientific advisory groups for the last 30 years.