SAO/NASA ADS Help Pages
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
A Comparison of Researcher's Reference Management Software
Journal of Economics and Behavioral Studies Vol. 6, No. 7, pp. 561-568, July 2014 (ISSN: 2220-6140) A Comparison of Researcher’s Reference Management Software: Refworks, Mendeley, and EndNote Sujit Kumar Basak Durban University of Technology, South Africa [email protected] Abstract: This paper aimed to present a comparison of researcher’s reference management software such as RefWorks, Mendeley, and EndNote. This aim was achieved by comparing three software. The main results of this paper were concluded by comparing three software based on the experiment. The novelty of this paper is the comparison of researcher’s reference management software and it has showed that Mendeley reference management software can import more data from the Google Scholar for researchers. This finding could help to know researchers to use the reference management software. Keywords: Reference management software, comparison and researchers 1. Introduction Reference management software maintains a database to references and creates bibliographies and the reference lists for the written works. It makes easy to read and to record the elements for the reference comprises such as the author’s name, year of publication, and the title of an article, etc. (Reiss & Reiss, 2002). Reference Management Software is usually used by researchers, technologists, scientists, and authors, etc. to keep their records and utilize the bibliographic citations; hence it is one of the most complicated aspects among researchers. Formatting references as a matter of fact depends on a variety of citation styles which have been made the citation manager very essential for researchers at all levels (Gilmour & Cobus-Kuo, 2011). Reference management software is popularly known as bibliographic software, citation management software or personal bibliographic file managers (Nashelsky & Earley, 1991). -
Spaces Determined by Point-Countable Covers
Pacific Journal of Mathematics SPACES DETERMINED BY POINT-COUNTABLE COVERS GARY FRED GRUENHAGE,ERNEST A. MICHAEL AND YOSHIO TANAKA Vol. 113, No. 2 April 1984 PACIFIC JOURNAL OF MATHEMATICS Vol. 113, No. 2,1984 SPACES DETERMINED BY POINT-COUNTABLE COVERS G. GRUENHAGE, E. MICHAEL AND Y. TANAKA Recall that a collection 9 of subsets of X is point-countable if every x G X is in at most countably many ?Gf. Such collections have been studied from several points of view. First, in characterizing various kinds of j-images of metric spaces, second, to construct conditions which imply that compact spaces and some of their generalizations are metrizable, and finally, in the context of meta-Lindelόf spaces. This paper will make some contributions to all of these areas. 1. Introduction. A space1 X is determined by a cover £P, or 9 determines X,2 if U C X is open (closed) in X if and only if U Π P is relatively open (relatively closed) in P for every P E <•?. (For example, X is determined by <$ if <$ is locally finite or if {P°: P E <3>} covers X.) We will explore this notion in the context of point-countable covers. Within the class of λ -spaces, spaces determined by point-countable covers turn out to be related to spaces having a point-countable Λ -net- work. Recall that a cover ζP of X is a k-network for X if, whenever K C U with K compact and U open in X9 then K C U φ C U for some finite ^C^. -
“Merging Libraries” & “Export Your Library with RIS”
“Merging libraries” & “Export your library with RIS” Export library with RIS To convert your EndNote X6 library for other applications (like Zotero, Mendeley, Reference Manager or ProCite etc.): - In EndNote X6, go to the drop-down output style list on the toolbar, and choose Select Another Style. Highlight and select the appropriate output style: - Select the RefMan (RIS) style. - From the File menu, select Export to export your library to a plain text file. - Now you can import the file into your application To import RIS file from another application into EndNote: 1 Library Wissenschaftspark Albert Einstein A joint library of the German Research Centre for Geosciences GFZ, the Potsdam Institute for Climate Impact Research, the Alfred Wegener Institute for Polar and Marine Research, Research Unit Potsdam, and the IASS Institute for Advanced Sustainability Studies Potsdam (Last update: March 2013) - Got to “File” and “Import” - Choose your file in RIS format - Use the RIS import option. - Set your preferences - Import the references 2 Library Wissenschaftspark Albert Einstein A joint library of the German Research Centre for Geosciences GFZ, the Potsdam Institute for Climate Impact Research, the Alfred Wegener Institute for Polar and Marine Research, Research Unit Potsdam, and the IASS Institute for Advanced Sustainability Studies Potsdam (Last update: March 2013) Merging libraries There are three ways to merge libraries: import one library into another, copy references from one library to another, or drag-and-drop. - (Optional) If you want to import only a subset of references from a library, first open that library and show only the references you wish to copy. -
On Compact-Covering and Sequence-Covering Images of Metric Spaces
MATEMATIQKI VESNIK originalni nauqni rad 64, 2 (2012), 97–107 research paper June 2012 ON COMPACT-COVERING AND SEQUENCE-COVERING IMAGES OF METRIC SPACES Jing Zhang Abstract. In this paper we study the characterizations of compact-covering and 1-sequence- covering (resp. 2-sequence-covering) images of metric spaces and give a positive answer to the following question: How to characterize first countable spaces whose each compact subset is metrizable by certain images of metric spaces? 1. Introduction To find internal characterizations of certain images of metric spaces is one of the central problems in General Topology. In 1973, E. Michael and K. Nagami [16] obtained a characterization of compact-covering and open images of metric spaces. It is well known that the compact-covering and open images of metric spaces are the first countable spaces whose each compact subset is metrizable. However, its inverse does not hold [16]. For the first countable spaces whose each compact subset is metrizable, how to characterize them by certain images of metric spaces? The sequence-covering maps play an important role on mapping theory about metric spaces [6, 9]. In this paper, we give the characterization of a compact- covering and 1-sequence-covering (resp. 2-sequence-covering) image of a metric space, and positively answer the question posed by S. Lin in [11, Question 2.6.5]. All spaces considered here are T2 and all maps are continuous and onto. The letter N is the set of all positive natural numbers. Readers may refer to [10] for unstated definition and terminology. 2. -
Download the AAS 2011 Annual Report
2011 ANNUAL REPORT AMERICAN ASTRONOMICAL SOCIETY aas mission and vision statement The mission of the American Astronomical Society is to enhance and share humanity’s scientific understanding of the universe. 1. The Society, through its publications, disseminates and archives the results of astronomical research. The Society also communicates and explains our understanding of the universe to the public. 2. The Society facilitates and strengthens the interactions among members through professional meetings and other means. The Society supports member divisions representing specialized research and astronomical interests. 3. The Society represents the goals of its community of members to the nation and the world. The Society also works with other scientific and educational societies to promote the advancement of science. 4. The Society, through its members, trains, mentors and supports the next generation of astronomers. The Society supports and promotes increased participation of historically underrepresented groups in astronomy. A 5. The Society assists its members to develop their skills in the fields of education and public outreach at all levels. The Society promotes broad interest in astronomy, which enhances science literacy and leads many to careers in science and engineering. Adopted 7 June 2009 A S 2011 ANNUAL REPORT - CONTENTS 4 president’s message 5 executive officer’s message 6 financial report 8 press & media 9 education & outreach 10 membership 12 charitable donors 14 AAS/division meetings 15 divisions, committees & workingA groups 16 publishing 17 public policy A18 prize winners 19 member deaths 19 society highlights Established in 1899, the American Astronomical Society (AAS) is the major organization of professional astronomers in North America. -
Calibration Against Spectral Types and VK Color Subm
Draft version July 19, 2021 Typeset using LATEX default style in AASTeX63 Direct Measurements of Giant Star Effective Temperatures and Linear Radii: Calibration Against Spectral Types and V-K Color Gerard T. van Belle,1 Kaspar von Braun,1 David R. Ciardi,2 Genady Pilyavsky,3 Ryan S. Buckingham,1 Andrew F. Boden,4 Catherine A. Clark,1, 5 Zachary Hartman,1, 6 Gerald van Belle,7 William Bucknew,1 and Gary Cole8, ∗ 1Lowell Observatory 1400 West Mars Hill Road Flagstaff, AZ 86001, USA 2California Institute of Technology, NASA Exoplanet Science Institute Mail Code 100-22 1200 East California Blvd. Pasadena, CA 91125, USA 3Systems & Technology Research 600 West Cummings Park Woburn, MA 01801, USA 4California Institute of Technology Mail Code 11-17 1200 East California Blvd. Pasadena, CA 91125, USA 5Northern Arizona University Department of Astronomy and Planetary Science NAU Box 6010 Flagstaff, Arizona 86011, USA 6Georgia State University Department of Physics and Astronomy P.O. Box 5060 Atlanta, GA 30302, USA 7University of Washington Department of Biostatistics Box 357232 Seattle, WA 98195-7232, USA 8Starphysics Observatory 14280 W. Windriver Lane Reno, NV 89511, USA (Received April 18, 2021; Revised June 23, 2021; Accepted July 15, 2021) Submitted to ApJ ABSTRACT We calculate directly determined values for effective temperature (TEFF) and radius (R) for 191 giant stars based upon high resolution angular size measurements from optical interferometry at the Palomar Testbed Interferometer. Narrow- to wide-band photometry data for the giants are used to establish bolometric fluxes and luminosities through spectral energy distribution fitting, which allow for homogeneously establishing an assessment of spectral type and dereddened V0 − K0 color; these two parameters are used as calibration indices for establishing trends in TEFF and R. -
Arxiv:2106.01477V1 [Astro-Ph.IM] 2 Jun 2021 Document in Their Instructions to Authors
Draft version June 4, 2021 Typeset using LATEX twocolumn style in AASTeX63 Best Practices for Data Publication in the Astronomical Literature Tracy X. Chen,1 Marion Schmitz,1 Joseph M. Mazzarella,1 Xiuqin Wu,1 Julian C. van Eyken,2 Alberto Accomazzi,3 Rachel L. Akeson,2 Mark Allen,4 Rachael Beaton,5 G. Bruce Berriman,2 Andrew W. Boyle,2 Marianne Brouty,4 Ben Chan,1 Jessie L. Christiansen,2 David R. Ciardi,2 David Cook,1 Raffaele D'Abrusco,3 Rick Ebert,1 Cren Frayer,1 Benjamin J. Fulton,2 Christopher Gelino,2 George Helou,1 Calen B. Henderson,2 Justin Howell,6 Joyce Kim,1 Gilles Landais,4 Tak Lo,1 Cecile Loup,4 Barry Madore,7, 8 Giacomo Monari,4 August Muench,9 Anais Oberto,4 Pierre Ocvirk,4 Joshua E. G. Peek,10, 11 Emmanuelle Perret,4 Olga Pevunova,1 Solange V. Ramirez,7 Luisa Rebull,6 Ohad Shemmer,12 Alan Smale,13 Raymond Tam,2 Scott Terek,1 Doug Van Orsow,13, 14 Patricia Vannier,4 and Shin-Ywan Wang1 1Caltech/IPAC-NED, Mail Code 100-22, Caltech, 1200 E. California Blvd., Pasadena, CA 91125, USA 2Caltech/IPAC-NExScI, Mail Code 100-22, Caltech, 1200 E. California Blvd., Pasadena, CA 91125, USA 3Center for Astrophysics j Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA 4Centre de Donn´eesastronomiques de Strasbourg, Observatoire de Strasbourg, 11, rue de l'Universit´e,67000 STRASBOURG, France 5Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA 6Caltech/IPAC-IRSA, Mail Code 100-22, Caltech, 1200 E. -
Filltex: Automatic Queries to ADS and INSPIRE Databases to Fill Latex Bibliography
filltex: Automatic queries to ADS and INSPIRE databases to fill LaTex bibliography Davide Gerosa1 and Michele Vallisneri1,2 1 TAPIR 350-17, California Institute of Technology, 1200 E California Boulevard, Pasadena, CA 91125, USA 2 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, DOI: 10.21105/joss.00222 Pasadena, CA 91109, USA Software • Review Summary • Repository • Archive filltex is a simple tool to fill LaTex reference lists with records from the ADS andIN- Licence SPIRE databases. ADS (“SAO/Nasa Astrophysics Data System,” n.d.) and INSPIRE Authors of JOSS papers retain (“High-Energy Physics Literature Database,” n.d.) are the most common databases copyright and release the work un- used among the theoretical physics and astronomy scientific communities, respectively. der a Creative Commons Attri- filltex automatically looks for all citation labels present in a tex document and, by bution 4.0 International License means of web-scraping, downloads all the required citation records from either of the (CC-BY). two databases. filltex significantly speeds up the LaTex scientific writing workflow, as all required actions (compile the tex file, fill the bibliography, compile the bibliography, compile the tex file again) are automated in a single command. We also provide anin- tegration of filltex for the macOS LaTex editor TexShop (“Cocoa Tex Previewer for macOS,” n.d.). References “Cocoa Tex Previewer for macOS.” n.d. http://pages.uoregon.edu/koch/texshop. “High-Energy Physics Literature Database.” n.d. http://inspirehep.net. “SAO/Nasa Astrophysics Data System.” n.d. http://adsabs.harvard.edu. Gerosa et al., (2017). filltex: Automatic queries to ADS and INSPIRE databases to fill LaTex bibliography. -
Aigaion: a Web-Based Open Source Software for Managing the Bibliographic References
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by E-LIS repository Aigaion: A Web-based Open Source Software for Managing the Bibliographic References Sanjo Jose ([email protected]) Francis Jayakanth ([email protected]) National Centre for Science Information, Indian Institute of Science, Bangalore – 560 012 Abstract Publishing research papers is an integral part of a researcher's professional life. Every research article will invariably provide large number of citations/bibliographic references of the papers that are being cited in that article. All such citations are to be rendered in the citation style specified by a publisher and they should be accurate. Researchers, over a period of time, accumulate a large number of bibliographic references that are relevant to their research and cite relevant references in their own publications. Efficient management of bibliographic references is therefore an important task for every researcher and it will save considerable amount of researchers' time in locating the required citations and in the correct rendering of citation details. In this paper, we are reporting the features of Aigaion, a web-based, open-source software for reference management. 1. Introduction A citation or bibliographic citation is a reference to a book, article, web page, or any other published item. The reference will contain adequate details to facilitate the readers to locate the publication. Different citation systems and styles are being used in different disciplines like science, social science, humanities, etc. Referencing is also a standardised method of acknowledging the original source of information or idea. -
Exportación a Otros Pgb
EXPORTACIÓN A OTROS PGB CÓMO EXPORTAR DE ZOTERO A ENDNOTE En Zotero una colección concreta -> botón derecho del ratón , exportar y guardar en formato RIS o Refer/BibIX En EndNote: File -> Import -> Reference Manager (RIS) o Refer/BibIX ENDNOTEWEB En Zotero guardar como .RIS En EndNoteweb importar con el filtro RefMan (RIS) PROCITE En Zotero guardar en formato RIS En Procite, Tools -> Import Text file -> Open Import file -> Nombre: Mi biblioteca.ris. Tipo ->All files REFERENCE MANAGER En Zotero guardar Mi biblioteca como .ris En Reference Manager- en File New Database u Open Database -> En File -> Import Text file->el que queremos “Mi biblioteca.ris”->Filter RIS REFWORK En Zotero guardar como .ris En RefWorks-> Importar-> Filtro RIS UTF-8 CÓMO EXPORTAR DE ENDNOTE A ZOTERO En EndNote -> File -> Export -> My EndNote Library -> en .txt. Output Style - > RefMan (RIS) En Zotero -> importar -> Tipo RIS ENDNOTEWEB En EndNote -> Tools-> Connect EndNote Web PROCITE En Procite Tools -> Convert file->elegir el archivo de EndNote y guardar con otro nombre REFERENCE MANAGER En EndNote File Export filtro refinan (RIS) export, como archivo .txt En Reference Manager, File Import Text file REFWORK De EndNote v.8 o superior exportación directa. Si falla en otras versiones ver Ayuda de RefWorks CÓMO EXPORTAR DE ENDNOTEWEB A ENDNOTE ZOTERO PROCITE REFERENCE MANAGER REFWORK Elegir exportar como RIS y seleccionar esta opción al importar a los progrmas CÓMO EXPORTAR DE PROCITE A ENDNOTE En Procite guardar cualquier archivo en Procite. En EndNote File -> Open library elegir el archivo de Procite-> File of type -> Procite ZOTERO En Procite, si no tenemos el filtro EndNote-RIS importarlo de www.procite.com . -
Fasciculi Mathemat
FASCICULIMATHEMATICI Nr 55 2015 DOI:10.1515/fascmath-2015-0024 Luong Quoc Tuyen MAPPING THEOREMS ON SPACES WITH sn-NETWORK g-FUNCTIONS Abstract. Let ∆ be the sets of all topological spaces satisfying the following conditions. (1) Each compact subset of X is metrizable; (2) There exists an sn-network g-function g on X such that if xn ! x and yn 2 g(n; xn) for all n 2 N, then x is a cluster point of fyng. In this paper, we prove that if X 2 ∆, then each sequentially- quotient boundary-compact map on X is pseudo-sequence-cove- ring; if X 2 ∆ and X has a point-countable sn-network, then each sequence-covering boundary-compact map on X is 1-sequence-covering. As the applications, we give that each sequentially-quotient boundary-compact map on g-metrizable spaces is pseudo-sequence-covering, and each sequence-covering boundary-compact on g-metrizable spaces is 1-sequence-covering. Key words: sn-networks, sn-network g-functions, g-metrizable spaces, boundary-compact maps, sequentially-quotient maps, pseudo-sequence-covering maps, sequence-covering maps, 1-se- quence-covering maps. AMS Mathematics Subject Classification: 54C10, 54E40, 54E99. 1. Introduction and preliminaries A study of images of topological spaces under certain sequence-covering maps is an important question in general topology. In 2001, S. Lin and P. Yan proved that each sequence-covering and compact map on metric spaces is 1-sequence-covering ([15]). Furthermore, S. Lin proved that each sequentially-quotient compact maps on metric spaces is pseudo-sequence- covering, and there exists a sequentially-quotient π-map on metric spaces is not pseudo-sequence-covering ([14]). -
The 10 Parsec Sample in the Gaia Era?,?? C
A&A 650, A201 (2021) Astronomy https://doi.org/10.1051/0004-6361/202140985 & c C. Reylé et al. 2021 Astrophysics The 10 parsec sample in the Gaia era?,?? C. Reylé1 , K. Jardine2 , P. Fouqué3 , J. A. Caballero4 , R. L. Smart5 , and A. Sozzetti5 1 Institut UTINAM, CNRS UMR6213, Univ. Bourgogne Franche-Comté, OSU THETA Franche-Comté-Bourgogne, Observatoire de Besançon, BP 1615, 25010 Besançon Cedex, France e-mail: [email protected] 2 Radagast Solutions, Simon Vestdijkpad 24, 2321 WD Leiden, The Netherlands 3 IRAP, Université de Toulouse, CNRS, 14 av. E. Belin, 31400 Toulouse, France 4 Centro de Astrobiología (CSIC-INTA), ESAC, Camino bajo del castillo s/n, 28692 Villanueva de la Cañada, Madrid, Spain 5 INAF – Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy Received 2 April 2021 / Accepted 23 April 2021 ABSTRACT Context. The nearest stars provide a fundamental constraint for our understanding of stellar physics and the Galaxy. The nearby sample serves as an anchor where all objects can be seen and understood with precise data. This work is triggered by the most recent data release of the astrometric space mission Gaia and uses its unprecedented high precision parallax measurements to review the census of objects within 10 pc. Aims. The first aim of this work was to compile all stars and brown dwarfs within 10 pc observable by Gaia and compare it with the Gaia Catalogue of Nearby Stars as a quality assurance test. We complement the list to get a full 10 pc census, including bright stars, brown dwarfs, and exoplanets.