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Musical Composition Graduate Portfolio
University of Northern Iowa UNI ScholarWorks Dissertations and Theses @ UNI Student Work 2021 Musical composition graduate portfolio Juan Marulanda University of Northern Iowa Let us know how access to this document benefits ouy Copyright ©2021 Juan Marulanda Follow this and additional works at: https://scholarworks.uni.edu/etd Recommended Citation Marulanda, Juan, "Musical composition graduate portfolio" (2021). Dissertations and Theses @ UNI. 1102. https://scholarworks.uni.edu/etd/1102 This Open Access Thesis is brought to you for free and open access by the Student Work at UNI ScholarWorks. It has been accepted for inclusion in Dissertations and Theses @ UNI by an authorized administrator of UNI ScholarWorks. For more information, please contact [email protected]. Copyright by JUAN MARULANDA 2021 All Rights Reserved MUSICAL COMPOSITION GRADUATE PORTFOLIO An Abstract Submitted in Partial Fulfillment of the Requirements for the Degree Master of Music Juan Marulanda University of Northern Iowa May 2021 This Study By: Juan Carlos Marulanda Entitled: Musical Composition Graduate Portfolio has been approved as meeting the thesis requirement for the Degree of Master of Music: Composition Date Dr. Daniel Swilley, Chair, Recital Committee Date Dr. Michael Conrad, Recital Committee Member Date Dr. Jonathan Schwabe, Recital Committee Member Date Dr. Jennifer Waldron, Dean, Graduate College This Recital Performance By: Juan Marulanda Entitled: Musical Composition Graduate Portfolio has been approved as meeting the thesis requirement for the Degree of Master of Music: Composition Date Dr. Daniel Swilley, Chair, Recital Committee Date Dr. Michael Conrad, Recital Committee Member Date Dr. Jonathan Schwabe, Recital Committee Member Date Dr. Jennifer Waldron, Dean, Graduate College ABSTRACT The musical works included in this portfolio were composed between Fall 2019 and Spring 2021. -
Curriculum Vitae - 24 March 2020
Dr. Eric E. Mamajek Curriculum Vitae - 24 March 2020 Jet Propulsion Laboratory Phone: (818) 354-2153 4800 Oak Grove Drive FAX: (818) 393-4950 MS 321-162 [email protected] Pasadena, CA 91109-8099 https://science.jpl.nasa.gov/people/Mamajek/ Positions 2020- Discipline Program Manager - Exoplanets, Astro. & Physics Directorate, JPL/Caltech 2016- Deputy Program Chief Scientist, NASA Exoplanet Exploration Program, JPL/Caltech 2017- Professor of Physics & Astronomy (Research), University of Rochester 2016-2017 Visiting Professor, Physics & Astronomy, University of Rochester 2016 Professor, Physics & Astronomy, University of Rochester 2013-2016 Associate Professor, Physics & Astronomy, University of Rochester 2011-2012 Associate Astronomer, NOAO, Cerro Tololo Inter-American Observatory 2008-2013 Assistant Professor, Physics & Astronomy, University of Rochester (on leave 2011-2012) 2004-2008 Clay Postdoctoral Fellow, Harvard-Smithsonian Center for Astrophysics 2000-2004 Graduate Research Assistant, University of Arizona, Astronomy 1999-2000 Graduate Teaching Assistant, University of Arizona, Astronomy 1998-1999 J. William Fulbright Fellow, Australia, ADFA/UNSW School of Physics Languages English (native), Spanish (advanced) Education 2004 Ph.D. The University of Arizona, Astronomy 2001 M.S. The University of Arizona, Astronomy 2000 M.Sc. The University of New South Wales, ADFA, Physics 1998 B.S. The Pennsylvania State University, Astronomy & Astrophysics, Physics 1993 H.S. Bethel Park High School Research Interests Formation and Evolution -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
October 2017 BRAS Newsletter
October 2017 Issue Next Meeting: Monday, October 9th at 7PM at HRPO nd (2 Mondays, Highland Road Park Observatory) October Program: BRAS President John Nagle will. reveal how he researches and puts together his Observing Notes column for our newsletter each. month. What's In This Issue? HRPO’s Great American Eclipse Event Summary (Page 2) President’s Message Secretary's Summary Outreach Report - FAE Light Pollution Committee Report Recent Forum Entries 20/20 Vision Campaign Messages from the HRPO Spooky Spectrum Observe The Moon Night Natural Sky Conference HRPO 20th Anniversary Observing Notes – Phoenix & Mythology Like this newsletter? See past issues back to 2009 at http://brastro.org/newsletters.html Newsletter of the Baton Rouge Astronomical Society October 2017 President’s Message The first Sidewalk Astronomy of the season was a success. We had a good time, and About 100 people (adult and children) attended. Ben Toman live streamed on the BRAS Facebook page. See his description in this newsletter. A copy of the proposed, revised By-Laws should be in your mail soon. Read through them, and any proposed changes need to be communicated to me before the November meeting. Wally Pursell (who wrote the original and changed by-laws) and I worked last year on getting the By-Laws updated to the current BRAS policies, and we hope the revised By-Laws will need no revisions for a long time. We need more Globe at Night observations – we are behind in the observations compared to last year at this time. We also need observations of variable stars to help in a school project by a new BRAS member, Shreya. -
CALENDARIO ASTRONOMICO Per L'anno Bisestile
CALENDARIO ASTRONOMICO per l’anno bisestile 2016 (Anno Internazionale delle Leguminose) con tabelle di Cronologia comparata con i Calendari Ortodosso, Copto, Israelita, Musulmano e Cinese Elaborato da LUCIANO UGOLINI Astrofilo di PRATO (Toscana) Componente dell’ASSOCIAZIONE ASTRONOMICA QUASAR presso CENTRO DI SCIENZE NATURALI di GALCETI – PRATO La pubblicazione di questo Calendario è sostenuta dal C.A.A.T. - Coordinamento delle Associazioni Astrofile della Toscana – www.astrocaat.it – [email protected] Il C.A.A.T. è: ollaoazioe ta gli astofili tosai, attività ossevativa, poozioe dell’astooia aatoiale ella osta egioe, incontri e seminari di aggiornamento, sensibilizzazione sul polea dell’iuiaeto luioso. Differenza ET-UT adottata per l’ao 16 = +68 secondi. Gli orari delle congiunzioni fra Luna, Pianeti e Stelle e la loro separazione angolare, si riferiscono all’istate della loro iia distaza e sono indicati per il centro della Terra. Gli orari del sorgere, culminare e tramontare del Sole e della Luna soo espressi per l’orizzote astrooio di Prato Piazza del Coue - Latitudine: ° ’ 8” Nord - Logitudie: ° ’ ” Est da Greeih. Le correzioni da apportare unicamente agli istanti del sorgere, culminare e tramontare degli astri, rispetto a quelle indicate, per altre città della Toscana, sono minime e riconducibili, al massimo, a pochi minuti in più o in meno. Gli altri orari indicati nel presete Caledario o eessitao di alua orrezioe e algoo per tutta l’Italia. Tutti i tepi soo espressi i T.M.E.C. Tepo Medio dell’Europa Cetrale he è il Tepo Ciile segato dai ostri orologi. Non viene tenuto conto dell’aueto di iuti douto all’ora estia, attualete i igore i Italia dall’ultia Doeia di Marzo all’ultia Doeia di Ottore. -
Desert Skies – October
Desert Skies Tucson Amateur Astronomy Association Volume LIV, Number 10 October, 2008 Mount Lemmon SkyCenter Learn about: ♦ Progress on TIMPA Observatory ♦ The new electronic newsletter! ♦ TAAA Astronomy Complex Update ♦ Volunteer for School star parties ♦ Articles from our members ♦ Websites: Trips On The Internet ♦ Constellation of the month Super-Skyway Desert Skies: October, 2008 2 Volume LIV, Number 10 Cover Photos: Upper left: The 24-inch telescope is enclosed atop Mount Lemmon within the dome at the left. Lower left: A 24-inch telescope was installed in the newly remodeled dome at the Mount Lemmon Sky Center in April. Right: The 24-inch Mount Lemmon Sky- Center telescope is the one the public uses in programs offered through the UA's College of Science and Steward Observatory. All pho- tos by Adam Block. TAAA Web Page: http://www.tucsonastronomy.org TAAA Phone Number: (520) 792-6414 Office/Position Name Phone E-mail Address President Ken Shaver 762-5094 [email protected] Vice President Keith Schlottman 290-5883 [email protected] Secretary Luke Scott 749-4867 [email protected] Treasurer Terri Lappin 977-1290 [email protected] Member-at-Large George Barber 822-2392 [email protected] Member-at-Large John Kalas 620-6502 [email protected] Member-at-Large Teresa Plymate 883-9113 [email protected] Chief Observer Dr. Mary Turner 586-2244 [email protected] AL Correspondent (ALCor) Nick de Mesa 797-6614 [email protected] Astro-Imaging SIG Steve -
A Review on Substellar Objects Below the Deuterium Burning Mass Limit: Planets, Brown Dwarfs Or What?
geosciences Review A Review on Substellar Objects below the Deuterium Burning Mass Limit: Planets, Brown Dwarfs or What? José A. Caballero Centro de Astrobiología (CSIC-INTA), ESAC, Camino Bajo del Castillo s/n, E-28692 Villanueva de la Cañada, Madrid, Spain; [email protected] Received: 23 August 2018; Accepted: 10 September 2018; Published: 28 September 2018 Abstract: “Free-floating, non-deuterium-burning, substellar objects” are isolated bodies of a few Jupiter masses found in very young open clusters and associations, nearby young moving groups, and in the immediate vicinity of the Sun. They are neither brown dwarfs nor planets. In this paper, their nomenclature, history of discovery, sites of detection, formation mechanisms, and future directions of research are reviewed. Most free-floating, non-deuterium-burning, substellar objects share the same formation mechanism as low-mass stars and brown dwarfs, but there are still a few caveats, such as the value of the opacity mass limit, the minimum mass at which an isolated body can form via turbulent fragmentation from a cloud. The least massive free-floating substellar objects found to date have masses of about 0.004 Msol, but current and future surveys should aim at breaking this record. For that, we may need LSST, Euclid and WFIRST. Keywords: planetary systems; stars: brown dwarfs; stars: low mass; galaxy: solar neighborhood; galaxy: open clusters and associations 1. Introduction I can’t answer why (I’m not a gangstar) But I can tell you how (I’m not a flam star) We were born upside-down (I’m a star’s star) Born the wrong way ’round (I’m not a white star) I’m a blackstar, I’m not a gangstar I’m a blackstar, I’m a blackstar I’m not a pornstar, I’m not a wandering star I’m a blackstar, I’m a blackstar Blackstar, F (2016), David Bowie The tenth star of George van Biesbroeck’s catalogue of high, common, proper motion companions, vB 10, was from the end of the Second World War to the early 1980s, and had an entry on the least massive star known [1–3]. -
121012-AAS-221 Program-14-ALL, Page 253 @ Preflight
221ST MEETING OF THE AMERICAN ASTRONOMICAL SOCIETY 6-10 January 2013 LONG BEACH, CALIFORNIA Scientific sessions will be held at the: Long Beach Convention Center 300 E. Ocean Blvd. COUNCIL.......................... 2 Long Beach, CA 90802 AAS Paper Sorters EXHIBITORS..................... 4 Aubra Anthony ATTENDEE Alan Boss SERVICES.......................... 9 Blaise Canzian Joanna Corby SCHEDULE.....................12 Rupert Croft Shantanu Desai SATURDAY.....................28 Rick Fienberg Bernhard Fleck SUNDAY..........................30 Erika Grundstrom Nimish P. Hathi MONDAY........................37 Ann Hornschemeier Suzanne H. Jacoby TUESDAY........................98 Bethany Johns Sebastien Lepine WEDNESDAY.............. 158 Katharina Lodders Kevin Marvel THURSDAY.................. 213 Karen Masters Bryan Miller AUTHOR INDEX ........ 245 Nancy Morrison Judit Ries Michael Rutkowski Allyn Smith Joe Tenn Session Numbering Key 100’s Monday 200’s Tuesday 300’s Wednesday 400’s Thursday Sessions are numbered in the Program Book by day and time. Changes after 27 November 2012 are included only in the online program materials. 1 AAS Officers & Councilors Officers Councilors President (2012-2014) (2009-2012) David J. Helfand Quest Univ. Canada Edward F. Guinan Villanova Univ. [email protected] [email protected] PAST President (2012-2013) Patricia Knezek NOAO/WIYN Observatory Debra Elmegreen Vassar College [email protected] [email protected] Robert Mathieu Univ. of Wisconsin Vice President (2009-2015) [email protected] Paula Szkody University of Washington [email protected] (2011-2014) Bruce Balick Univ. of Washington Vice-President (2010-2013) [email protected] Nicholas B. Suntzeff Texas A&M Univ. suntzeff@aas.org Eileen D. Friel Boston Univ. [email protected] Vice President (2011-2014) Edward B. Churchwell Univ. of Wisconsin Angela Speck Univ. of Missouri [email protected] [email protected] Treasurer (2011-2014) (2012-2015) Hervey (Peter) Stockman STScI Nancy S. -
2015 Clear Sky Nights by Art Rae
2015 Clear Sky Nights by Art Rae Volume 41, No. 4 Windsor Centre - Here is my tally of clear night skies for 2015 from my location near River Canard, Ontario. This is an unofficial "look out the window" count of all the nights I saw what I considered a "clear sky". Seeing doesn't enter into it. But it gives an idea of what kind of observing year we had this past year. 2015 brought my total up to 93 clear nights, about 25% of the total nightly skies for the year. If you thought we didn't get a lot of clear skies you are probably right. In some recent years we've experi- enced as high as 120 clear nights others as low as 83. 2013 showed 119 open sky nights. Well maybe we will have a better chance in 2016. This year we get an ex- tra day to count. The Royal Astronomical Society of Canada In This Issue 2015 Clear Sky Nights Cover Events / Housekeeping Items Page 2 November Meeting Minutes Page 3 and 5 At the Eyepiece Page 4 2016 Executive and Council Page 5 Member Astrophotos Page 6 1 January 2016 Calendar of Events Our next meeting… Activities... Tuesday February 16, 2016 Occultation of Aldebaran: The Moon will pass in front of 7:30 p.m. Aldebaran tonight from 9:10 - 10:30 p.m.. Get outside during the break and have a look. at Ojibway Park Nature Centre Moon, Mercury and Venus: Will make a nice trio in the morning sky on Saturday February 6th just off of the han- 5200 Matchette Road dle of the “Teapot”. -
ESO Annual Report 2004 ESO Annual Report 2004 Presented to the Council by the Director General Dr
ESO Annual Report 2004 ESO Annual Report 2004 presented to the Council by the Director General Dr. Catherine Cesarsky View of La Silla from the 3.6-m telescope. ESO is the foremost intergovernmental European Science and Technology organi- sation in the field of ground-based as- trophysics. It is supported by eleven coun- tries: Belgium, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Sweden, Switzerland and the United Kingdom. Created in 1962, ESO provides state-of- the-art research facilities to European astronomers and astrophysicists. In pur- suit of this task, ESO’s activities cover a wide spectrum including the design and construction of world-class ground-based observational facilities for the member- state scientists, large telescope projects, design of innovative scientific instruments, developing new and advanced techno- logies, furthering European co-operation and carrying out European educational programmes. ESO operates at three sites in the Ataca- ma desert region of Chile. The first site The VLT is a most unusual telescope, is at La Silla, a mountain 600 km north of based on the latest technology. It is not Santiago de Chile, at 2 400 m altitude. just one, but an array of 4 telescopes, It is equipped with several optical tele- each with a main mirror of 8.2-m diame- scopes with mirror diameters of up to ter. With one such telescope, images 3.6-metres. The 3.5-m New Technology of celestial objects as faint as magnitude Telescope (NTT) was the first in the 30 have been obtained in a one-hour ex- world to have a computer-controlled main posure. -
The Fixed Stars Report Frederic Chopin
The Fixed Stars Report by Tara Cochrane for Frederic Chopin March 1, 1810 6:00 PM Warsaw, Poland Calculated for: Local Mean Time, Time Zone 0 hours West Latitude: 52 N 15 Longitude: 21 E 00 Your Company Name 1234 N. Your Address City, State 123456 Phone: 1-555-555-5555 [email protected] Introduction Report and Text Copyright 2009 Cosmic Patterns Software, Inc. The contents of this report are protected by Copyright law. By purchasing this report you agree to comply with this Copyright. This report interprets conjunctions of nearly every fixed star that has been given an astrological name to the planets, Asc, MC, 7th house cusp, and 4th cusp. Each interpretation given in this report is based on extensive research on the historical astrological meanings and myths associated with the fixed stars. A list of notable people who have the same conjunction aspect as you do is also given. This comprehensive analysis of the influence of the fixed stars combined with a list of notable people who also have this aspect provides you with extensive information, and hopefully astrologers who use this report can use this information to develop an even more refined and clearer understanding of the meaning of every fixed stars. Interpretations of the Fixed Stars Moon conjunct Dheneb, Orb: 0 deg 55 min Bold, willful, courageous, combative, astute, focused and unyielding characteristics may be indicated. Ascension to a position of leadership and renown is possible. There may be a great deal of personal charisma and emotional intensity, as well as an inclination towards obsession. -
A Terrestrial Planet Candidate in a Temperate Orbit Around Proxima Centauri
A terrestrial planet candidate in a temperate orbit around Proxima Centauri Guillem Anglada-Escude´1∗, Pedro J. Amado2, John Barnes3, Zaira M. Berdinas˜ 2, R. Paul Butler4, Gavin A. L. Coleman1, Ignacio de la Cueva5, Stefan Dreizler6, Michael Endl7, Benjamin Giesers6, Sandra V. Jeffers6, James S. Jenkins8, Hugh R. A. Jones9, Marcin Kiraga10, Martin Kurster¨ 11, Mar´ıa J. Lopez-Gonz´ alez´ 2, Christopher J. Marvin6, Nicolas´ Morales2, Julien Morin12, Richard P. Nelson1, Jose´ L. Ortiz2, Aviv Ofir13, Sijme-Jan Paardekooper1, Ansgar Reiners6, Eloy Rodr´ıguez2, Cristina Rodr´ıguez-Lopez´ 2, Luis F. Sarmiento6, John P. Strachan1, Yiannis Tsapras14, Mikko Tuomi9, Mathias Zechmeister6. July 13, 2016 1School of Physics and Astronomy, Queen Mary University of London, 327 Mile End Road, London E1 4NS, UK 2Instituto de Astrofsica de Andaluca - CSIC, Glorieta de la Astronoma S/N, E-18008 Granada, Spain 3Department of Physical Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK 4Carnegie Institution of Washington, Department of Terrestrial Magnetism 5241 Broad Branch Rd. NW, Washington, DC 20015, USA 5Astroimagen, Ibiza, Spain 6Institut fur¨ Astrophysik, Georg-August-Universitat¨ Gottingen¨ Friedrich-Hund-Platz 1, 37077 Gottingen,¨ Germany 7The University of Texas at Austin and Department of Astronomy and McDonald Observatory 2515 Speedway, C1400, Austin, TX 78712, USA 8Departamento de Astronoma, Universidad de Chile Camino El Observatorio 1515, Las Condes, Santiago, Chile 9Centre for Astrophysics Research, Science & Technology Research Institute, University of Hert- fordshire, Hatfield AL10 9AB, UK 10Warsaw University Observatory, Aleje Ujazdowskie 4, Warszawa, Poland 11Max-Planck-Institut fur¨ Astronomie Konigstuhl¨ 17, 69117 Heidelberg, Germany 12Laboratoire Univers et Particules de Montpellier, Universit de Montpellier, Pl.