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Annual Report
2013–14 ® 1 Annual Report ® 2013–14Annual Report Pennsylvania Historical and Museum Commission . 1 From the Chairman . 2 From the Executive Director . 3 The State Museum of Pennsylvania . 4 Pennsylvania State Archives . 8 Historic Sites and Museums . 12 Historic Preservation . 16 Management Services . 27 Pennsylvania Heritage Foundation . 28 Pennsylvania Historical and Museum Commission The Pennsylvania Historical and Museum Commission (PHMC) is the official history agency of the Commonwealth of Penn- sylvania. It was created in 1945 from the merger of three previously separate organizations: the Pennsylvania State Archives, established in 1903; the State Museum of Pennsylvania, created in 1905; and the Pennsylvania Historical Commission (PHC), organized by legislation in 1913. The responsibilities of PHMC, which are based in the Pennsylvania Constitution, are further defined in the History Code and the Administrative Code. The primary duties include the following: • the conservation of Pennsylvania’s historical and natural heritage • the preservation of public records, historic documents and objects of historic interest • the identification, restoration and preservation of architecturally and historically significant sites and structures PHMC’s programs, services and initiatives are administered by five bureaus: The State Museum of Pennsylvania, Pennsylvania State Archives, Historic Sites and Museums, Historic Preservation and Management Services. Mission Statement The Pennsylvania Historical and Museum Commission works in partnership with others to preserve the Commonwealth’s natural and cultural heritage as a steward, teacher and advocate for the people of Pennsylvania and the nation. Vision Statement The Pennsylvania Historical and Museum Commission enriches people’s lives by helping them to understand Pennsylvania’s past, to appreciate the present and to embrace the future. -
Challenges and Opportunities Women and Girls Face in Half of All S&E Bachelor’S Degrees
LEHIGH VALLEY WOMENChallenges and IN Opportunities Lin Erickson & Karen Knecht STEM April 2020 n December 19, 2019, Camille Schrier earned the title students get older, particularly in technology programs careers need to support their success and advance- (e.g. coding, robotics and video game development). ment; and 3) identify the marketing and messaging of Miss America 2020, after performing a science This decline mirrors local STEM achievement test data strategies that would be most effective in attracting (Pennsylvania State School Assessment), with female girls’ interest in Da Vinci STEM programs. The Melior demonstration, the “catalytic decomposition of hydrogen scores on standardized math and science tests drop- Group conducted five focus groups with students in ping dramatically between grades 4 and 8. grades 4-12, college students, and working women in peroxide,” live on NBC for the world to view. Her story STEM. The focus groups took place at the Da Vinci O THE RESEARCH Science Center. as a biochemist and repeat pageant winner has been viewed by The purpose of the research was to assess the needs millions. It will be shared again on PBS39 WLVR 91.3 on September of K-12 girls, undergraduate women, and women in STEM KEY FINDINGS employment and identify opportunities to enhance the The Needs Assessment Survey provided valuable in- 9, 2020 from 5:30 – 7pm. Ms. Schrier will join other distinguished STEM learning and support ecosystem for women and sights about the interests, experiences, and perceptions girls in the Lehigh Valley. of school-age students, college students, and working female leaders in science, technology, engineering, and math (STEM) women in STEM careers. -
2015 Annual Report
NOTES FROM THE FIELD 32-Page Book for 2015 Girl Scouts of Eastern Pennsylvania THIS ANNUAL REPORT BOOK IS PROPERTY OF Girl Scouts of Eastern Pennsylvania PERTINENT COORDINATES Girl Scouts of Eastern Pennsylvania 330 Manor Road, Miquon, Pennsylvania 19444 40.070206, -75.252716 FOR INITIAL RECORDS GIRL SCOUTS OF EASTERN PENNSYLVANIA, INC. (“GSEP”) OPERATES AS AN INDEPENDENT, NONPROFIT ORGANIZATION CHARTERED BY THE NATIONAL GIRL SCOUTS OF THE USA TO PROVIDE LEADERSHIP DEVELOPMENT OPPORTUNITIES FOR GIRLS IN NINE COUNTIES: BERKS, BUCKS, CARBON, CHESTER, DELAWARE, LEHIGH, MONTGOMERY, NORTHAMPTON, AND PHILADELPHIA. THE GIRL SCOUT PROMISE ON MY HONOR, I WILL TRY: TO SERVE GOD AND MY COUNTRY, TO HELP PEOPLE AT ALL TIMES, AND TO LIVE BY THE GIRL SCOUT LAW. IN THE EVENT OF MISPLACEMENT IF FOUND PLEASE CONTACT @ IS HENCE, THERE ISN’T A HANDSOME REWARD WAITING. WWW.GSEP.ORG GIRL SCOUTS OUR MISSION: GIRL SCOUTING BUILDS GIRLS OF COURAGE, CONFIDENCE, AND CHARACTER, WHO MAKE THE WORLD A BETTER PLACE. CONTENTS: 01. EXECUTIVE MESSAGE 06. TAKE THE LEAD 2015 02. MEMBERSHIP 07. THANK YOU TO OUR DONORS 03. LAND 08. BOARD OF DIRECTORS 04. CAMPAIGN FOR GIRLS 09. OUR FOOTPRINT 05. FINANCE THE GIRL SCOUT LAW: I WILL DO MY BEST TO BE HONEST AND FAIR, FRIENDLY AND HELPFUL, CONSIDERATE AND CARING, COURAGEOUS AND STRONG, AND RESPONSIBLE FOR WHAT I SAY AND DO, AND TO RESPECT MYSELF AND OTHERS, RESPECT AUTHORITY, USE RESOURCES WISELY, MAKE THE WORLD A BETTER PLACE, AND BE A SISTER TO EVERY GIRL SCOUT. GIRL SCOUTS OF EASTERN PENNSYLVANIA. PRINTED APRIL 2016. EXECUTIVE MESSAGE This has been a year marked by big changes and great accomplishments at Girl Scouts of Eastern Pennsylvania. -
Spring 2018 Contentsspring 2018
JOURNAL SPRING 2018 CONTENTSSPRING 2018 1 From the Headmaster MORAVIAN ACADEMY’S PARENT AMBASSADOR NETWORK 2 Shining Bright In conjunction with the Office of Admis- Talent Abounds at the Middle and Upper School sions, Moravian Academy created a Parent 4 Ambassador Network (PAN) of approximately Into the Woods 25 members to represent our school by 5 sharing their many and varied experiences with other families in and about the Greater 6 Thank you to our Retiring Faculty and Staff! Lehigh Valley. We know that our parents are our best advocates and tell stories about our 10 Fields and Courts Moravian community better than just about 12 Through the Looking Glass: anyone. We value and trust our relationships Moravian Academy Auction with these storytellers. Our goal for PAN is to encourage a family to visit our campus and tour our beautiful 14 Moravian Academy in the Community facilities - whether that be our downtown, 15 International Festival for All Families historic Bethlehem campus or our sprawling 120-acre Upper School campus. In order 16 Summer at the Academy Preview to assist our members, we provide litera- ture with key items such as top reasons to 17 Lehigh Valley Summerbridge choose Moravian Academy, statistics and studies supporting an independent school 18 Student Lebenslauf: “Same Difference?” education, and guidelines for answering some of the more difficult questions posed 19 Institutional Advancement News to the admissions team. We invite you to consider joining our PAN 21 Alumni News community. If you are interested, please reach out to Ingrid Gerber, Senior Director of 28 Class Notes Admissions, at [email protected]. -
A Tail Structure Associated with Protoplanetary Disk Around SU
Draft version February 28, 2019 A Preprint typeset using LTEX style emulateapj v. 12/16/11 A TAIL STRUCTURE ASSOCIATED WITH PROTOPLANETARY DISK AROUND SU AURIGAE EIJI AKIYAMA1, EDUARD I. VOROBYOV2,3, HAUYU BAOBABU LIU4,5, RUOBING DONG5,6, JEROME de LEON7, SHENG-YUAN LIU5, MOTOHIDE TAMURA7,8,9 1Institute for the Advancement of Higher Education, Hokkaido University, Kita17, Nishi8, Kita-ku, Sapporo, 060-0817, Japan; [email protected] 2Department of Astrophysics, University of Vienna, Vienna 1018, Austria 3Research Institute of Physics, Southern Federal University, Rostov-on-Don, 344090, Russia 4European Southern Observatory, Karl Schwarzschild Str 2, 85748 Garching bei M¨unchen, Germany 5Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei, 10617, Taiwan 6Department of Astronomy/Steward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA 7Department of Astronomy, The University of Tokyo, 7-3-1, Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan 8Astrobiology Center of NINS, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588, Japan 9National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588, Japan Draft version February 28, 2019 ABSTRACT We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO (J=2– 1) line emission from the protoplanetary disk around T-Tauri star SU Aurigae (hereafter SU Aur). Previous observations in optical and near infrared wavelengths find a unique structure in SU Aur. One of the highlights of the observational results is that an extended tail-like structure is associated with the disk, indicating mass transfer from or into the disk. -
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, -
2016 Annual Report
EXPANDING IMPACT Investing in Our Region EXPANDING IMPACT 2016 3145 Hamilton Blvd. Bypass Community Allentown, PA 18103 Investing in Our Region 484.664.1002 Impact Report davincisciencecenter.org Investing in Our Region Dear Friends, The Da Vinci Science Center had a record-breaking year in 2016 and we are so grateful that you were part of this milestone! We welcomed more than 140,000 visitors and program participants (a 75% increase since 2011). With new exhibits, a robust field trip schedule, and an ever-growing outreach program, we were successful in bringing science to life and lives to science for so many in our region. The Da Vinci Our outreach programs continued to bring science into our schools and the community. Science Center Our educators, volunteers, mentors, and community partners made it possible to bring a Brings Science diverse range of programs to underserved areas. We are particularly proud of the growing to Life and Lives opportunities we offered for students to connect with STEM professionals at their schools, to Science as well as at the Center. Students were able to experience science in action and learn about the educational backgrounds and career paths of scientists and engineers in our community. We believe, and research supports, that early and frequent interaction with STEM yields a more equipped future workforce. Our continued growth prompted us to consider expanding the Da Vinci Science Center experiences, culminating with our VISION announcement in November to partner with the City of Easton to explore building a $130 million Da Vinci Science City complex along To be a visionary leader the city’s scenic waterfront area. -
Orbital Refinement and Stellar Properties for the HD 9446, HD
Draft version March 6, 2020 Typeset using LATEX twocolumn style in AASTeX62 Orbital Refinement and Stellar Properties for the HD 9446, HD 43691, and HD 179079 Planetary Systems Michelle L. Hill,1 Teo Mocnik,ˇ 1 Stephen R. Kane,1 Gregory W. Henry,2 Joshua Pepper,3 Natalie R. Hinkel,4 Paul A. Dalba,1, ∗ Benjamin J. Fulton,5 Keivan G. Stassun,6 Lee J. Rosenthal,5 Andrew W. Howard,5 Steve B. Howell,7 Mark E. Everett,8 Tabetha S. Boyajian,9 Debra A. Fischer,10 Joseph E. Rodriguez,11 Thomas G. Beatty,11 and David J. James12, 13 1Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA 2Center of Excellence in Information Systems, Tennessee State University, Nashville, TN 37209, USA 3Department of Physics, Lehigh University, Bethlehem, PA 18015, USA 4Southwest Research Institute, San Antonio, TX 78238, USA 5Department of Astronomy, California Institute of Technology, Pasadena, CA 91125, USA 6Vanderbilt University, Department of Physics & Astronomy, 6301 Stevenson Center Lane, Nashville, TN 37235, USA 7NASA Ames Research Center, Moffett Field, CA 94035, USA 8National Optical Astronomy Observatory, Tucson, AZ 85719, USA 9Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803, USA 10Department of Astronomy, Yale University, New Haven, CT 06511, USA 11Department of Astronomy and Steward Observatory, University of Arizona, Tucson, AZ 85721 12Center for Astrophysics j Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA 13Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USA (Accepted Mar 04, 2020) Submitted to AJ ABSTRACT The Transit Ephemeris Refinement and Monitoring Survey (TERMS) is a project which aims to detect transits of intermediate-long period planets by refining orbital parameters of the known ra- dial velocity planets using additional data from ground based telescopes, calculating a revised tran- sit ephemeris for the planet, then monitoring the planet host star during the predicted transit win- dow. -
The Da Vinci Discovery Center of Science and Technology, Inc
THE DA VINCI DISCOVERY CENTER OF SCIENCE AND TECHNOLOGY, INC FINANCIAL REPORT June 30, 2019 THE DA VINCI DISCOVERY CENTER OF SCIENCE AND TECHNOLOGY, INC. Table of Contents June 30, 2019 and 2018 Page Independent Auditors' Report 1-2 Consolidated Financial Statements Consolidated statements of financial position 3 Consolidated statements of activities 4 Consolidated statements of functional expenses 5-6 Consolidated statements of cash flows 7-8 Notes to the consolidated financial statements 9-22 INDEPENDENT AUDITORS' REPORT To the Board of Directors of The Da Vinci Discovery Center of Science and Technology, Inc. We have audited the accompanying consolidated financial statements of The Da Vinci Discovery Center of Science and Technology, Inc. (a nonprofit organization) and subsidiaries, which comprise the consolidated statements of financial position as of June 30, 2019 and 2018, and the related consolidated statements of activities, functional expenses and cash flows for the years then ended, and the related notes to the financial statements. Management’s Responsibility for the Financial Statements Management is responsible for the preparation and fair presentation of these consolidated financial statements in accordance with accounting principles generally accepted in the United States of America; this includes the design, implementation, and maintenance of internal control relevant to the preparation and fair presentation of consolidated financial statements that are free from material misstatement, whether due to fraud or error. Auditors’ Responsibility Our responsibility is to express an opinion on these consolidated financial statements based on our audits. We conducted our audits in accordance with auditing standards generally accepted in the United States of America. -
Arxiv:2006.10868V2 [Astro-Ph.SR] 9 Apr 2021 Spain and Institut D’Estudis Espacials De Catalunya (IEEC), C/Gran Capit`A2-4, E-08034 2 Serenelli, Weiss, Aerts Et Al
Noname manuscript No. (will be inserted by the editor) Weighing stars from birth to death: mass determination methods across the HRD Aldo Serenelli · Achim Weiss · Conny Aerts · George C. Angelou · David Baroch · Nate Bastian · Paul G. Beck · Maria Bergemann · Joachim M. Bestenlehner · Ian Czekala · Nancy Elias-Rosa · Ana Escorza · Vincent Van Eylen · Diane K. Feuillet · Davide Gandolfi · Mark Gieles · L´eoGirardi · Yveline Lebreton · Nicolas Lodieu · Marie Martig · Marcelo M. Miller Bertolami · Joey S.G. Mombarg · Juan Carlos Morales · Andr´esMoya · Benard Nsamba · KreˇsimirPavlovski · May G. Pedersen · Ignasi Ribas · Fabian R.N. Schneider · Victor Silva Aguirre · Keivan G. Stassun · Eline Tolstoy · Pier-Emmanuel Tremblay · Konstanze Zwintz Received: date / Accepted: date A. Serenelli Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E- 08193, Spain and Institut d'Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, Barcelona, E-08034, Spain E-mail: [email protected] A. Weiss Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany C. Aerts Institute of Astronomy, Department of Physics & Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium and Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, the Netherlands G.C. Angelou Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany D. Baroch J. C. Morales I. Ribas Institute of· Space Sciences· (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E-08193, arXiv:2006.10868v2 [astro-ph.SR] 9 Apr 2021 Spain and Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capit`a2-4, E-08034 2 Serenelli, Weiss, Aerts et al. -
Vanderbilt University, Department of Physics & Astronomy VU Station B 1807, Nashville, TN 37235 Phone: 615-322-2828, FAX: 61
CURRICULUM VITAE: KEIVAN GUADALUPE STASSUN SENIOR ASSOCIATE DEAN FOR GRADUATE EDUCATION & RESEARCH, COLLEGE OF ARTS & SCIENCE Vanderbilt University, Department of Physics & Astronomy VU Station B 1807, Nashville, TN 37235 Phone: 615-322-2828, FAX: 615-343-7263 [email protected] DEGREES EARNED University of Wisconsin—Madison Degree: Ph.D. in Astronomy, 2000 Thesis: Rotation, Accretion, and Circumstellar Disks among Low-Mass Pre-Main-Sequence Stars Advisor: Robert D. Mathieu University of California at Berkeley Degree: A.B. in Physics/Astronomy (double major) with Honors, 1994 Thesis: A Simultaneous Photometric and Spectroscopic Variability Study of Classical T Tauri Stars Advisor: Gibor Basri EMPLOYMENT HISTORY Vanderbilt University Director, Vanderbilt Center for Autism & Innovation, 2017-present Stevenson Endowed Professor of Physics & Astronomy, 2016-present Senior Associate Dean for Graduate Education & Research, College of Arts & Science, 2015-18 Harvie Branscomb Distinguished Professor, 2015-16 Professor of Physics and Astronomy, 2011-present Director, Vanderbilt Initiative in Data-intensive Astrophysics (VIDA), 2007-present Co-Director, Fisk-Vanderbilt Masters-to-PhD Bridge Program, 2004-15 Associate Professor of Physics and Astronomy, 2008-11 Assistant Professor of Physics and Astronomy, 2003-08 Fisk University Adjunct Professor of Physics, 2006-present University of Wisconsin—Madison NASA Hubble Postdoctoral Research Fellow, Astronomy, 2001-03 Area: Observational Studies of Low-Mass Star Formation Mentor: Robert D. Mathieu University of Wisconsin—Madison Assistant Director and Postdoctoral Fellow, NSF Graduate K-12 Teaching Fellows Program, 2000-01 Duties: Development of fellowship program, instructor for graduate course in science education research Mentor: Terrence Millar HONORS AND AWARDS Presidential Award for Excellence in Science, Math, and Engineering Mentoring—2018 AAAS Mentor of the Year—2018 HHMI Professor—2018- Research Corporation for Science Advancement SEED Award—2017 1/29 Keivan G. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study.