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The Astronomy Theory, Observations and Methods (ATOM) Journal
Robotic Telescopes, Student Research and Education (RTSRE) Proceedings Conference Proceedings, Hilo, Hawaii, USA, Jul 23-27, 2018 Fitzgerald, M., Bartlett, S., Salimpour, S., Eds. Vol. 2, No. 1, (2019) ISBN 978-0-6483996-1-2 / doi : 10.32374/rtsre.2019.003 / CC BY-NC-ND license Peer Reviewed Article. rtsre.org/ojs Rationale for a New Journal: the Astronomy Theory, Observations and Methods (ATOM) Journal Michael Fitzgerald1* Abstract In this article, the rationale behind the creation of a new journal, Astronomy Theory, Observa- tions and Methods (ATOM) journal, currently hosted at rtsre.org is provided. It aims to fill a niche in the community for papers on any general topic in astronomy that may not find their place in top tier astronomical journals. The article outlines the thinking behind why there is a gap to be filled with regards to current scholarly metrics and the nature of other journals of similar scope and impact. The journal aims to be accessible to new and novice scientific authors, as well as those more established, through accessible developmental peer review and an explicit aim to avoid using publication metrics as a barrier to publication selection. The scope, which accepts more broader articles than most, of the journal and considerations on behalf of a potential author are also outlined. Keywords Scientific publishing — Amateur Astronomy — Student Research — Scientometrics 1School of Education, Edith Cowan University *Corresponding author: psyfi[email protected] journal, such as MNRAS, ApJ, AJ or AA, PASP or PASA. The “race to the top” for mainstream astron- Introduction omy journals means that the journals in the middle Part of the rationale for many astronomy student to top range of impact factor, such as those men- research projects (e.g. -
Introductory Guide for Authors This Guide Is for Early-Career Researchers Who Are Beginning to Write Papers for Publication
Introductory guide for authors This guide is for early-career researchers who are beginning to write papers for publication. publishingsupport.iopscience.org publishingsupport.iopscience.org This guide is for early-career researchers who are beginning to write papers for publication. Academic publishing is rapidly changing, with new technologies and publication models giving authors much more choice over where and how to publish their work. Whether you are writing up the results of a PhD chapter or submitting your first paper, knowing how to prepare your work for publication is essential. This guide will provide an overview of academic publishing and advice on how to make the most of the process for sharing your research. For more information and to download a digital version of this guide go to publishingsupport.iopscience.org. c o n t e n t s Page Choosing where to submit your paper 4 Writing and formatting 6 Peer-review process 8 Revising and responding to referee reports 10 Acceptance and publication 12 Promoting your published work 13 Copyright and ethical integrity 14 Frequently asked questions 15 Publishing glossary 16 IOP publications 18 Introductory guide for authors 3 publishingsupport.iopscience.org Choosing where to submit your paper It can be tempting to begin writing a paper before giving much thought to where it might be published. However, choosing a journal to target before you begin to prepare your paper will enable you to tailor your writing to the journal’s audience and format your paper according to its specific guidelines, which you may find on the journal’s website. -
Open Infrastructure and Community: the Case of Astronomy
SPECIALISED PORTALS, ONLINE INFORMATION SERVICES, SCHOLARLY ONLINE NETWORKS: THE IMPACT OF E-INFRASTRUCTURES ON SCIENCE COMMUNICATION AND SCHOLARLY COMMUNITY BUILDING Open infrastructure and community: the case of astronomy Niels Taubert Abstract This comment focuses on an early case of an open infrastructure that emerged in the 1990s in international astronomy. It targets the reasons for this infrastructure’s tremendous success and starts with a few comments on the term ‘digital infrastructure’. Subsequently, it provides a brief description of the most important components of the infrastructure in astronomy. In a third step, the use of one component — the arXiv, an open access repository for manuscripts — is analyzed. It concludes with some considerations about the success and acceptance of this infrastructure in astronomy. Keywords Scholarly communication; Science communication: theory and models DOI https://doi.org/10.22323/2.17020302 Introduction The creation and establishment of a discipline-specific digital infrastructure is challenging. In many cases it is highly questionable before or during its development whether the requirements of the targeted user group [Van Zundert, 2012] will be met, and when completed whether the extent of its utilization may stay behind the initial expectations [Kaltenbrunner, 2017, p. 303] often due to nebulous reasons. The aim of this comment is to approach at least some of the difficulties of the development of a digital infrastructure in science by drawing on a successful case: the digital infrastructure in international astronomy. In a first step, a heuristic model is given. It illustrates that the development of an infrastructure is not merely a technical task, but a creation of a complex arrangement that includes a two-sided social embedding of the technology. -
Vitae-Balonek-Full-2019 May 13
Thomas J. Balonek Professor of Physics and Astronomy Department of Physics and Astronomy Colgate University 13 Oak Drive, Hamilton, NY 13346 (315) 228-7767 [email protected] EDUCATIONAL BACKGROUND Ph.D. (Astronomy) University of Massachusetts, Amherst, MA, 1982 M.S. (Astronomy) University of Massachusetts, Amherst, MA, 1977 B.A. (Physics) Cornell University, Ithaca, NY, 1974 PROFESSIONAL BACKGROUND Professor of Physics and Astronomy, Colgate University, Hamilton, NY (2002-present) Chair, Department of Physics and Astronomy, Colgate University, Hamilton, NY (2008-2011) Visiting Research Scientist, National Astronomy and Ionosphere Center, Cornell University, Ithaca, NY (2006-2007) Associate Professor of Physics and Astronomy, Colgate University, Hamilton, NY (1991-2002) Chair, Department of Physics and Astronomy, Colgate University, Hamilton, NY (1995-1998) Chair, New York Astronomical Corporation (1995-1998) Visiting Research Scientist, National Radio Astronomy Observatory, Tucson, AZ (1992-1993) Assistant Professor of Physics and Astronomy, Colgate University, Hamilton, NY (1985-1991) Visiting Assistant Professor of Astronomy, Williams College, Williamstown, MA (1983-1985) NASA-ASEE (National Aeronautics and Space Administration and American Society for Engineering Education) Summer Faculty Fellow, NASA-Ames Research Center, Moffett Field, CA (1983, 1984) Post-Doctoral Research Associate and Lecturer I, University of New Mexico, Albuquerque, NM (1982-1983) Planetarium Lecturer, Basset Planetarium, Amherst College, Amherst, MA (1979-1981) -
High-Sensitivity Radio Astronomy
High-Sensitivity Radio Astronomy Proceedings of a meeting held at Jodrell Bank, University of Manchester January 22-26, 1996 Edited by N. Jackson R. J. Davis Jodrell Bank, Nuffield Radio Astronomy Laboratories, University of Manchester CAMBRIDGE UNIVERSITY PRESS Contents Participants xi Preface xv Foreword xvii Acknowledgements xviii Planets, stars and pulsars Longitudinal asymmetry of Jupiter's radiation belts after the encounter with comet D/Shoemaker-Levy 9 Richard Strom, Imke de Pater and Floris van der Tak 2 Pulsars at the highest radio frequencies Richard Wielebinski 6 Present and future pulsar searches F. Camilo 14 The study of stellar radio emission with very large aperture radio telescopes E.R. Seaquist 23 High-resolution. MERLIN maps of the radio emission from Nova Cygni 1992 and Nova Cassiopeiae 1993 Stewart Eyres, Richard Davis, Mike Bode and Huw Lloyd 33 Orbital motion and a model for HM Sge H.T. Kenny, A.R. Taylor, S. Kwok, S.P.S. Eyres and R.J. Davis 37 Variable sources and jets in Cepheus A V.A. Hughes 42 A radio survey of southern X-ray binary stars R.E. Spencer, A.K. Tzioumis, L.R. Ball, 5.J. Newell and V. Migenes 46 MERLIN astrometry of radio stars S.T. Garrington, R.J. Davis, L.V. Morrison and R.W. Argyle 50 High-sensitivity radio observations of the 8.665-GHz 3He+ hyperfme line emission from planetary nebulae D.S. Balser, T.M. Bania, R.T. Rood and T.L. Wilson 53 High-resolution observations of young planetary nebulae M. Bryce, A. Pedlar, T. Muxlow, P. -
1667 K Street NW, Suite 800 • Washington, DC 20006 • Aas.Org 6
6 May 2020 Dr. Lisa Nichols Office of Science and Technology Policy 1650 Pennsylvania Ave. NW Washington, DC 20504 [email protected] Re: AAS Response to OSTP Request for Information: Public Access to Peer-Reviewed Scholarly Publications, Data and Code Resulting from Federally Funded Research, FR Doc. 2020–03189, 12 February 2020 Dear Dr. Nichols: We appreciate the opportunity to have met with you on 28 February and to learn of the OSTP’s recognition of the critical role of nonprofit society publishers in advancing open access to federally funded research. We look forward to continued dialogue and engagement in this area. The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America. Its membership of over 8,000 individuals also includes physicists, mathematicians, geologists, engineers, and others whose research and educational interests lie within the broad spectrum of subjects comprising contemporary astronomy, planetary science, and heliophysics. The mission of the AAS is to enhance and share humanity’s scientific understanding of the universe. As a 501(c)(3) the AAS owns, operates, and publishes the most widely read and cited journals in the field: The Astronomical Journal (AJ), The Astrophysical Journal (ApJ), The Astrophysical Journal Letters, The Astrophysical Journal Supplement Series, and The Planetary Science Journal. The AJ was established in 1849 and came into AAS ownership 100 years later; the ApJ was established in 1895, 100 years before becoming one of the very first scholarly journals online. One of the conditions for taking ownership of the ApJ from the University of Chicago in the 1970s included a provision whereby journal proceeds were not to be used to directly fund the ongoing operations of the society. -
Annualreport
2 17 ANNUALREPORT 17 20 TABLEOFCONTENTS 1 Trustee’s Update 2 Director’s Update 3 Science Highlights 30 Technical Support Highlights 34 Development Highlights 37 Public Program Highlights 40 Putnam Collection Center Highlights 41 Communication Highlights 43 Peer-Reviewed Publications 49 Conference Proceedings & Abstracts 59 Statement of Financial Position TRUSTEE’SUPDATE By W. Lowell Putnam About a decade ago the phrase, unique, enriching and transformative “The transformational effect of the as well. We are committed to building DCT”, started being used around the on that in all that we are doing going Observatory. We were just beginning forward. to understand that a 4 meter class We are not the only growing entity telescope was going to be more in the Flagstaff area. There has seen impactful than our original, and naïve, substantial growth at NAU, at our other concept of “2x the Perkins”. Little did we partner institutions and in the number know then, and we are still learning just of high technology, for-profit business in how transforming the DCT has been. the region. This collective growth is now As you read Jeff’s report and look creating opportunities for collaboration through the rest of this report you can and partnerships that did not exist a begin to see the results in terms of decade ago. We have the potential scientific capability and productivity. to do things that we would not have The greater awareness of Lowell on considered even a few years ago. The the regional and national level has challenge will be doing them in ways also lead to the increases in the public that keep the Observatory the collegial program, and the natural progression and collaborative haven that it has to building a better visitor program and always been. -
Lowell Observatory Publications 2013 Armstrong, J. T. ; Hutter, D. J. ; Baines, E. K. ; Benson, J. A. ; Bevilacqua, R. M. ; Busc
Lowell Observatory Publications 2013 Armstrong, J. T. ; Hutter, D. J. ; Baines, E. K. ; Benson, J. A. ; Bevilacqua, R. M. ; Buschmann, T. ; Clark, J. H. ; Ghasempour, A. ; Hall, J. C. ; Hindsley, R. B. ; Johnston, K. J. ; Jorgensen, A. M. ; Mozurkewich, D. ; Muterspaugh, M. W. ; Restaino, S. R. ; Shankland, P. D. ; Schmitt, H. R. ; Tycner, C. ; van Belle, G. T. ; Zavala, R. T. (2013). The Navy Precision Optical Interferometer (NPOI): An Update. Journal of Astronomical Instrumentation, Volume 2, Issue 2, id. 1340002 Baines, Ellyn K. ; Armstrong, J. Thomas ; van Belle, Gerard T. (2013). Navy Precision Optical Interferometer Observations of the Exoplanet Host κ Coronae Borealis and Their Implications for the Star's and Planet's Masses and Ages. The Astrophysical Journal Letters, Volume 771, Issue 1, article id. L17 Baines, Ellyn K. ; McAlister, Harold A. ; ten Brummelaar, Theo A. ; Turner, Nils H. ; Sturmann, Judit ; Sturmann, Laszlo ; Farrington, Christopher D. ; Vargas, Norm ; van Belle, Gerard T. ; Ridgway, Stephen T. (2013). Characterization of the Red Giant HR 2582 Using the CHARA Array. The Astrophysical Journal, Volume 772, Issue 1, article id. 16 Baumeister, H. ; Chazelas, B. ; Delplancke, F. ; Dérie, F. ; Di Lieto, N. ; Duc, T. P. ; Fleury, M. ; Graser, U. ; Kaminski, A. ; Köhler, R. ; Lévêque, S. ; Maire, C. ; Mégevand, D. ; Mérand, A. ; Michellod, Y. ; Moresmau, J. -M. ; Mohler, M. ; Müller, A. ; Müllhaupt, P. ; Naranjo, V. ; Sache, L. ; Salvade, Y. ; Schmid, C. ; Schuhler, N. ; Schulze-Hartung, T. ; Sosnowska, D. ; Tubbs, B. ; van Belle, G. T. ; Wagner, K. ; Weber, L. ; Zago, L. ; Zimmerman, N. (2013). The ESPRI project: astrometric exoplanet search with PRIMA. I. Instrument description and performance of first light observations. -
Arxiv:2107.07531V1 [Astro-Ph.IM] 15 Jul 2021
Draft version July 19, 2021 Typeset using LATEX twocolumn style in AASTeX63 Considerations for optimizing photometric classification of supernovae from the Rubin Observatory Catarina S. Alves,1 Hiranya V. Peiris,1, 2 Michelle Lochner,3, 4, 5 Jason D. McEwen,6 Tarek Allam Jr,6 Rahul Biswas,2 and The LSST Dark Energy Science Collaboration 1Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK 2Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova University Center, Stockholm 10691, Sweden 3Department of Physics and Astronomy, University of the Western Cape, Bellville, Cape Town, 7535, South Africa 4South African Radio Astronomy Observatory (SARAO), The Park, Park Road, Pinelands, Cape Town 7405, South Africa 5African Institute for Mathematical Sciences, 6 Melrose Road, Muizenberg, 7945, South Africa 6Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK ABSTRACT Survey telescopes such as the Vera C. Rubin Observatory will increase the number of observed su- pernovae (SNe) by an order of magnitude, discovering millions of events; however, it is impossible to spectroscopically confirm the class for all the SNe discovered. Thus, photometric classification is crucial but its accuracy depends on the not-yet-finalized observing strategy of Rubin Observatory's Legacy Survey of Space and Time (LSST). We quantitatively analyze the impact of the LSST observ- ing strategy on SNe classification using the simulated multi-band light curves from the Photometric LSST Astronomical Time-Series Classification Challenge (PLAsTiCC). First, we augment the simu- lated training set to be representative of the photometric redshift distribution per supernovae class, the cadence of observations, and the flux uncertainty distribution of the test set. -
Britt F. Lundgren
Britt F. Lundgren Contact Information Address: 1 University Heights, CPO 2430, Asheville, NC, 28804, USA Phone: +1 (828) 255-7130 email: [email protected] Education Sept 2009 Ph.D. in Astronomy University of Illinois, Urbana-Champaign, IL Thesis: “The Origins and Environments of Quasar Absorption Lines in the Sloan Digital Sky Survey” | Advisor: Prof. Robert Brunner Coursework: astrophysics, computational methods, phil. of science / education June 2003 A.B. in Physics (Astrophysics Concentration) with Honors University of Chicago, Chicago, IL Honors Thesis Advisor: Prof. Donald G. York Coursework: physics, astrophysics, education and public policy, liberal arts core Professional Appointments Aug 2016 - Assistant Professor of Physics and Astronomy Present University of North Carolina Asheville − Asheville, NC Developing and teaching undergraduate courses in physics and astronomy. Combining observations from the Hubble Space Telescope and the Sloan Digital Sky Survey (SDSS) to explore the content and distribution of gas surrounding galaxies in the distant universe. Taught 12 credit hours per semester and developed 7 new undergraduate astronomy courses, including the diversity-intensive: ”Indigenous Perspectives on the Sky”; Cottrell Scholar; Serving as Co-Chair of Education and Public Outreach for the SDSS-IV Collabo- ration; Advisory Board President for the North Carolina Space Grant. Aug 2015 - AAAS Science and Technology Policy Fellow in Big Data & Analytics Jul 2016 Division of Undergraduate Education, National Science Foundation, Arlington, VA Researched and evaluated NSF programs aiming to improve science, technology, en- gineering, and math (STEM) educational opportunities and outcomes for low-income students. Served as the Executive Secretary for the Interagency Working Group on STEM Engagement, formed by the National Science and Technology Council’s Committee on STEM Education. -
CAS Dean for Thursday, Dr. Stefi Baum 8:45 Escorted from Hotel to Building 44 9
CAS Dean for Thursday, Dr. Stefi Baum 8:45 Escorted from Hotel to Building 44 9: AM-9:50 Continental Breakfast with CAS Chairs (Conference Room Building 44, Room 307C) 10:00 -10:30 am Meet with Provost Bain (Provost’s Office 3rd floor, Building 39) 10:30 -11:30 am Meet with the Interim Dean and Staff (4th floor CAS Dean Suite, Building 41) 11:30 -12:15 pm Meet with Faculty of CAS (Room A03, Building 44) 12:15- 1:00 pm Meet with Search Committee over lunch (Small Board Room, Building 39) 1:15 - 2:00 pm University Community & Students (Room A03, Building 41) 2:00 - 2:30 pm President Sessoms (President’s Office 3rd floor, building 39) 2:30 - 3:30 pm Deans-SBPA, LRD, GRAD, CAUSES( Conference Room Building 44, Room 307C) 3:30 – 4:30 pm Meet with Provost (Provost’s Office 3rd floor, Building 39) ! ! ! ! ! "#$%&!'(&)*+!,-./! Radcliffe Institute for Advanced Harvard University Byerly Hall, 8 Garden Street Cambridge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
Royal Astronomical Society Annual Report and Accounts 31 December
Royal Astronomical Society Annual Report and Accounts 31 December 2016 Charity Registration Number 226545 Contents Reports Reference and administrative details of the charity, its trustees and advisers 1 Trustees’ report 4 Including: Executive Summary 4 Objectives 11 Significant achievements 12 Public engagement ♦ Celebrating Women ♦ RAS 200: Sky and Earth ♦ Transit of Mercury ♦ Other Education and Outreach projects Public policy ♦ Post Referendum on Europe Governance ♦ Code of Conduct and review of other documentation ♦ Occupancy of Burlington House ♦ Elections to Council 2016/2017 Ongoing significant achievements Other achievements 25 Risks 30 Structure, Governance and Management 32 Events since year end and plans for the future 34 Activities 37 Financial Review 46 Independent auditor’s report 51 Statement of financial activities 53 Balance sheet 54 Statement of cash flows 55 Principal accounting policies 56 Notes to the accounts 63 Royal Astronomical Society Reference and administrative details of the charity, its trustees and advisers Patron Her Majesty the Queen Trustees The Council members who served during 2016 were: Professor Martin Barstow (President until May 2016, A, University of Leicester) Professor John Zarnecki (President elect from May 2015 and President from May 2016, G, Open University) Professor Mike Edmunds (Vice-President until May 2016, A, University of Cardiff) Professor Yvonne Elsworth (Vice President, G, University of Birmingham) Professor Don Kurtz (Vice President, A, University of Central Lancashire) Professor