Academic literature on the topic '(standard astronomical journal format)'
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Journal articles on the topic "(standard astronomical journal format)"
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Bara, Salvador. "Black-body luminance and magnitudes per square arcsecond in the Johnson-Cousins BVR photometric bands." Photonics Letters of Poland 11, no. 3 (September 30, 2019): 63. http://dx.doi.org/10.4302/plp.v11i3.926.
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A relevant amount of light pollution studies deal with the unwanted visual effects of artificial light at night, including the anthropogenic luminance of the sky that hinders the observation of the celestial bodies which are a main target of ground-based astrophysical research, and a key asset of the intangible heritage of humankind. Most quantitative measurements and numerical models, however, evaluate the anthropogenic sky radiance in any of the standard Johnson-Cousins UBVRI photometric bands, generally in the V one. Since the Johnson-Cousins V band is not identical with the visual CIE V() used to assess luminance, the conversion between these two photometric systems turns out to be spectrum-dependent. Given its interest for practical applications, in this Letter we provide the framework to perform this conversion and the transformation constants for black-body spectra of different absolute temperatures. Full Text: PDF ReferencesF. Falchi et al. "The new world atlas of artificial night sky brightness", Sci. Adv. 2, e1600377 (2016). CrossRef M. Kocifaj, "A review of the theoretical and numerical approaches to modeling skyglow: Iterative approach to RTE, MSOS, and two-stream approximation", Journal of Quantitative Spectroscopy & Radiative Transfer 181, 2 (2016). CrossRef M.S. Bessel, "UBVRI PASSBANDS", Publications of the Astronomical Society of the Pacific, 102, 1181 (1990).. CrossRef CIE, Commision Internationale de l'Éclairage. CIE 1988 2° SpectralLuminous Efficiency Function for Photopic Vision. (Vienna, Bureau Central de la CIE, 1990) DirectLink S. Bará, "Variations on a classical theme: On the formal relationship between magnitudes per square arcsecond and luminance", International Journal of Sustainable Lighting IJSL 19(2), 104 (2017). CrossRef A. Sánchez de Miguel, M. Aubé, J. Zamorano, M. Kocifaj, J. Roby, C. Tapia. "Sky Quality Meter measurements in a colour-changing world", Monthly Notices of the Royal Astronomical Society 467(3), 2966 (2017). CrossRef M.S. Bessell, "Standard Photometric Systems", Annual Reviews of Astronomy and Astrophysics, 43, 293 (2005). CrossRef J.B. Oke, "Absolute Spectral Energy Distributions for White Dwarfs", The Astrophysical Journal Suppl. Series 236(27), 21 (1974). CrossRef J.B. Oke, J.E. Gunn, "Secondary standard stars for absolute spectrophotometry", The Astrophysical Journal 266, 713 (1983). CrossRef M.R. Blanton, S. Roweis S., "K-Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared", The Astronomical Journal, 133(2), 734(2007). Table 1. CrossRef
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Hutchins, Carol. "Session 3 Overview: Management of Astronomical Pecularities." International Astronomical Union Colloquium 110 (1989): 136. http://dx.doi.org/10.1017/s0252921100003201.
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Session 3 on “Handling and Use of Special Format Materials” dealt with diverse items which are of unique importance in astronomical libraries.Preprints and reprints are important in several ways. Libraries’ collection and dissemination of information about pre-publication journal and conference papers boosts the astronomer’s awareness of current research in a timely fashion. Individual libraries’ practices range from very basic—the receipt and physical display of preprints—to the more elaborate activities including production of lists, gathering of subsequent publication information about the papers themselves, construction of local databases listing preprints, and electronic network exchange of listings.There was a consensus that the sending of reprint series is far less important than it was in years past.We heard a call for formal recognition or designation of a central clearinghouse for information about astronomy preprints.
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Delacour, Thomas, Soizick Lesteven, Gilles Landais, Aline Eisele, Magali Neuville, Evelyne Son, and Philippe Vonflie. "Bibliographical references: From publishers to SIMBAD." EPJ Web of Conferences 186 (2018): 12004. http://dx.doi.org/10.1051/epjconf/201818612004.
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The SIMBAD astronomical database hosted by the CDS provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system. The CDS receives the bibliographic meta-data of the articles published in the main astronomical journals directly from the publishers. How we receive the data and their format vary from one publisher to the next. These data are first extracted and stored in files with a standardised format. Then, to avoid errors or misprints, we perform different tests on these data: - Author names are compared to a reference list maintained at CDS, and the keywords are compared with the AAS list - Astronomical objects are verified by checking their name in the SIMBAD database - A completion test checks that all of articles of a journal volume are present The next step identifies whether an astronomical object appears inside a title, a keyword or an abstract, and if so, we add a link to the object in SIMBAD. Once all of the verifications and corrections have been made we add the meta-data into SIMBAD. We also add other information such as the number of different astronomical objects studied in the paper, the presence tables and their links to VizieR, any new acronyms, as well as some comments. New developments are in progress to automatically extract the data from the tables in the articles (that have not been processed by, or provided to VizieR) . In addition, each night automatic checks are executed to list the new data and to test the coherence of these data in SIMBAD.
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ANISYA, ANISYA, INDRA WARMAN, and DEDE WIRA TRISE PUTRA. "SUNTINGAN DOKUMEN BERBASIS WEB." Edik Informatika 7, no. 2 (June 11, 2021): 21–28. http://dx.doi.org/10.22202/ei.2021.v7i2.4818.
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Web-based document editing is a system for making scientific papers without having to adjust the format of writing scientific papers. Where in this system has provided a framework for entering journal contents. Journal article creation must follow the format already in place in the organization, such as font size, edge size, and so on. Often in writing journals, writers experience difficulties or constraints in the format of writing, so they often experience errors in writing journal articles. For this reason, it is necessary to have a standard web journal writing program, which provides a framework for the format of journal writing. The process carried out in designing this application is by looking at the guidelines for journal manuscript writing, with these guidelines the writer can know how the journal format will be translated into a program script. The purpose of this research is to design a standard web program for editing documents in journals and to assist journal authors / journal authors in making scientific papers online. In this research, the writer made a document editing system for scientific journal writing format using PHP and MySQL in the application system. Where in the system designed the author only includes the entries of each input in the journal framework. In this system all the input that is filled in is stored in a database with different tables. And when the author sees the contents of the journal, the display on the journal contents automatically matches the journal template.
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W, Diaz-Merced, Oppelt T, Mockiewicz J, and Agata H. "Accessibility of astronomy journal papers." Caribbean Journal of Science and Technology 10, no. 02 (2022): 31–41. http://dx.doi.org/10.55434/cbi.2022.20105.
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The Working Group on Accessibility and Disability (WGAD) of the American Astronomical Society published a comprehensive list of accessibility recommendations for professional astronomy journals, based on the first-hand experience of both higher education students and professional astronomers. The recommendations include accessibility strategies intended to improve access for a wide range of disabled and neurodiverse readers, with particular attention to the way readers with visual, motor, and cognitive disabilities cope with information in a digital interface. In this paper we use the tools of critical discourse analysis (CDA) to compare the recommended strategies to the digital discursive modes currently employed by leading astronomy journals. Raters analyzed discourse modes for a sample of 256 astronomy journal articles, including the usage of linguistic indicators, digital architecture, and information display. We identify emergent categories of access barriers faced by disabled astronomers, and identify strategies in the journal papers addressing those emergent categories. We compare the discourse modes currently used in astronomy publications with the access barriers and recommended strategies described by the WGAD document. Our analysis found that discourses in astronomical publications were typically constituted with the expectation of various shared commonalities between the author and the reader, including: 1. Same sensorial modality of interaction; 2. Same experiential knowledge as authors; 3. Same access to information as authors; 4. Same linguistic knowledge as authors; 5. Same cognitive strategies as authors; 6. Same socioeconomic status and background. This case study may serve as a baseline for future studies on how inaccessible textual discourse, digital architecture, and digital display in STEM journals enhance professional inequalities. Examining how current standard journal standards impact the transition to different professional career stages would help to identify alternate discursive strategies which would improve accessibility.
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Puschmann, Paul, and Luciana Quaranta. "Editorial." Historical Life Course Studies 5 (January 11, 2018): 1–2. http://dx.doi.org/10.51964/hlcs9333.
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Historical Life Course Studies, a journal in population studies, aims to stimulate and facilitate the implementation of IDS (Intermediate Data Structure, a standard data format for large historical databases), and to publish the results from (comparative) research with the help of large historical databases. The journal publishes not only empirical articles, but also descriptions (of the construction) of new and existing large historical databases, as well as articles dealing with database documentation, the transformation of existing databases into the IDS format, the development of algorithms and extraction software and all other issues related to the methodology of large historical databases.
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Matthijs, Koen, and Paul Puschmann. "Editorial." Historical Life Course Studies 2 (May 11, 2015): 37. http://dx.doi.org/10.51964/hlcs9357.
Full textAbstract:
Historical Life Course Studies, a journal in population studies, aims to stimulate and facilitate the implementation of IDS (Intermediate Data Structure, a standard data format for large historical databases), and to publish the results from (comparative) research with the help of large historical databases. The journal publishes not only empirical articles, but also descriptions (of the construction) of new and existing large historical databases, as well as articles dealing with database documentation, the transformation of existing databases into the IDS format, the development of algorithms and extraction software and all other issues related to the methodology of large historical databases.
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Coelho, Richard J., and Jan La Forge. "Preparing a Journal Manuscript: A Guide for Rehabilitation Counselor Practitioners." Journal of Applied Rehabilitation Counseling 27, no. 3 (September 1, 1996): 37–41. http://dx.doi.org/10.1891/0047-2220.27.3.37.
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Encouraging rehabilitation counseling practitioners to enter the arena of journal-writing is an ongoing concern of the profession. This article intends to help authors, especially practitioners who have not submitted previously, organize research materials for writing articles. A model of organizing standard components of a professional journal article is presented and discussed. The guidelines presented also provide a summary of the manuscript format and editorial review process. Suggestions presented provide a basis for assisting the rehabilitation counselor practitioner who is considering writing a journal article.
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Coelho, Richard J., and Jan La Forge. "Preparing a Journal Manuscript: A Guide for Rehabilitation Counsellor Practitioners." Australian Journal of Rehabilitation Counselling 3, no. 1 (1997): 1–8. http://dx.doi.org/10.1017/s1323892200001563.
Full textAbstract:
Encouraging rehabilitation counselling practitioners to enter the arena of journal-writing is an ongoing concern of the profession. This article intends to help authors, especially practitioners who have not submitted previously, organise research materials for writing articles. A model of organising standard components of a professional journal article is presented and discussed. The guidelines presented also provide a summary of the manuscript format and editorial review process. Suggestions presented provide a basis for assisting the rehabilitation counsellor practitioner who is considering writing a journal article.
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Hotan, A. W., W. van Straten, and R. N. Manchester. "psrchive and psrfits: An Open Approach to Radio Pulsar Data Storage and Analysis." Publications of the Astronomical Society of Australia 21, no. 3 (2004): 302–9. http://dx.doi.org/10.1071/as04022.
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AbstractA new set of software applications and libraries for use in the archival and analysis of pulsar astronomical data is introduced. Known collectively as the psrchive scheme, the code was developed in parallel with a new data storage format called psrfits, which is based on the Flexible Image Transport System (FITS). Both of these projects utilise a modular, object-oriented design philosophy. psrchive is an open source development environment that incorporates an extensive range of c++ object classes and pre-built command line and graphical utilities. These deal transparently and simultaneously with multiple data storage formats, thereby enhancing data portability and facilitating the adoption of the psrfits file format. Here, data are stored in a series of modular header–data units that provide flexibility and scope for future expansion. As it is based on FITS, various standard libraries and applications may be used for data input, output, and visualisation. Both psrchive and psrfits are made publicly available to the academic community in the hope that this will promote their widespread use and acceptance.
Dissertations / Theses on the topic "(standard astronomical journal format)"
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Bock, Douglas Carl-Johan. "Wide Field Aperture Synthesis Radio Astronomy." University of Sydney. Physics, 1998. http://hdl.handle.net/2123/377.
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This thesis is focussed on the Molonglo Observatory Synthesis Telescope (MOST), reporting on two primary areas of investigation. Firstly, it describes the recent upgrade of the MOST to perform an imaging survey of the southern sky. Secondly, it presents a MOST survey of the Vela supernova remnant and follow-up multiwavelength studies. The MOST Wide Field upgrade is the most significant instrumental upgrade of the telescope since observations began in 1981. It has made possible the nightly observation of fields with area ~5 square degrees, while retaining the operating frequency of 843 MHz and the pre-existing sensitivity to point sources and extended structure. The MOST will now be used to make a sensitive (rms approximately 1 mJy/beam) imaging survey of the sky south of declination -30°. This survey consists of two components: an extragalactic survey, which will begin in the south polar region, and a Galactic survey of latitudes |b| < 10°. These are expected to take about ten years. The upgrade has necessitated the installation of 352 new preamplifiers and phasing circuits which are controlled by 88 distributed microcontrollers, networked using optic fibre. The thesis documents the upgrade and describes the new systems, including associated testing, installation and commissioning. The thesis continues by presenting a new high-resolution radio continuum survey of the Vela supernova remnant (SNR), made with the MOST before the completion of the Wide Field upgrade. This remnant is the closest and one of the brightest SNRs. The contrast between the structures in the central pulsar-powered nebula and the synchrotron radiation shell allows the remnant to be identified morphologically as a member of the composite class. The data are the first of a composite remnant at spatial scales comparable with those available for the Cygnus Loop and the Crab Nebula, and make possible a comparison of radio, optical and soft X-ray emission from the resolved shell filaments. The survey covers an area of 50 square degrees at a resolution of 43" x 60", while imaging structures on scales up to 30'. It has been used for comparison with Wide Field observations to evaluate the performance of the upgraded MOST. The central plerion of the Vela SNR (Vela X) contains a network of complex filamentary structures. The validity of the imaging of these filaments has been confirmed with Very Large Array (VLA) observations at 1.4 GHz. Unlike the situation in the Crab Nebula, the filaments are not well correlated with H-alpha emission. Within a few parsec of the Vela pulsar the emission is much more complex than previously seen: both very sharp edges and more diffuse emission are present. It has been postulated that one of the brightest filaments in Vela X is associated with the X-ray feature (called a `jet') which appears to be emanating from the region of the pulsar. However, an analysis of the MOST and VLA data shows that this radio filament has a flat spectral index similar to another more distant filament within the plerion, indicating that it is probably unrelated to the X-ray feature.
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Bock, Douglas Carl-Johan. "Wide Field Aperture Synthesis Radio Astronomy." Thesis, The University of Sydney, 1997. http://hdl.handle.net/2123/377.
Full textAbstract:
This thesis is focussed on the Molonglo Observatory Synthesis Telescope (MOST), reporting on two primary areas of investigation. Firstly, it describes the recent upgrade of the MOST to perform an imaging survey of the southern sky. Secondly, it presents a MOST survey of the Vela supernova remnant and follow-up multiwavelength studies. The MOST Wide Field upgrade is the most significant instrumental upgrade of the telescope since observations began in 1981. It has made possible the nightly observation of fields with area ~5 square degrees, while retaining the operating frequency of 843 MHz and the pre-existing sensitivity to point sources and extended structure. The MOST will now be used to make a sensitive (rms approximately 1 mJy/beam) imaging survey of the sky south of declination -30°. This survey consists of two components: an extragalactic survey, which will begin in the south polar region, and a Galactic survey of latitudes |b| < 10°. These are expected to take about ten years. The upgrade has necessitated the installation of 352 new preamplifiers and phasing circuits which are controlled by 88 distributed microcontrollers, networked using optic fibre. The thesis documents the upgrade and describes the new systems, including associated testing, installation and commissioning. The thesis continues by presenting a new high-resolution radio continuum survey of the Vela supernova remnant (SNR), made with the MOST before the completion of the Wide Field upgrade. This remnant is the closest and one of the brightest SNRs. The contrast between the structures in the central pulsar-powered nebula and the synchrotron radiation shell allows the remnant to be identified morphologically as a member of the composite class. The data are the first of a composite remnant at spatial scales comparable with those available for the Cygnus Loop and the Crab Nebula, and make possible a comparison of radio, optical and soft X-ray emission from the resolved shell filaments. The survey covers an area of 50 square degrees at a resolution of 43" x 60", while imaging structures on scales up to 30'. It has been used for comparison with Wide Field observations to evaluate the performance of the upgraded MOST. The central plerion of the Vela SNR (Vela X) contains a network of complex filamentary structures. The validity of the imaging of these filaments has been confirmed with Very Large Array (VLA) observations at 1.4 GHz. Unlike the situation in the Crab Nebula, the filaments are not well correlated with H-alpha emission. Within a few parsec of the Vela pulsar the emission is much more complex than previously seen: both very sharp edges and more diffuse emission are present. It has been postulated that one of the brightest filaments in Vela X is associated with the X-ray feature (called a `jet') which appears to be emanating from the region of the pulsar. However, an analysis of the MOST and VLA data shows that this radio filament has a flat spectral index similar to another more distant filament within the plerion, indicating that it is probably unrelated to the X-ray feature.
Books on the topic "(standard astronomical journal format)"
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Studios, Vismont. Aliens, Astronomical Elements - Alien Primary Story Journal to Write and Draw for Grades K-2 Kids: Standard Size, Dotted Midline, Blank Handwriting Practice Paper with Picture Space for Girls, Boys. Independently Published, 2020.
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Gumpers, Maxwell. Standard Guitar Tablature: Blank Sheet Music Notebook Manuscript Paper for Young Musicians, Wide Staff , Tabs Journal Format for Kids, Music Notations/ Notes Writing, 6 Lines Tablature Staves per Page. Independently Published, 2020.
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Gumpers, Maxwell. Standard Guitar Tablature: Blank Sheet Music Notebook Manuscript Paper for Young Musicians, Wide Staff , Tabs Journal Format for Kids, Music Notations/ Notes Writing, 6 Lines Tablature Staves per Page. Independently Published, 2020.
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Gumpers, Maxwell. Standard Guitar Tablature: Blank Sheet Music Notebook Manuscript Paper for Young Musicians, Wide Staff , Tabs Journal Format for Kids, Music Notations/ Notes Writing, 6 Lines Tablature Staves per Page. Independently Published, 2020.
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Publications, RAWRsome! Composition Journal for Kindergarten, K-2 and K-3, Primary Story Format: Lined Sketch Book with Picture Space, 5/8 Standard Rule, Dotted Mid-Line, Medium Size 8 X 10 , Cute Monster Theme. Independently Published, 2020.
Find full textBook chapters on the topic "(standard astronomical journal format)"
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Robinson, Marin S., Fredricka L. Stoller, Molly Constanza-Robinson, and James K. Jones. "Writing the Results Section." In Write Like a Chemist. Oxford University Press, 2008. http://dx.doi.org/10.1093/oso/9780195367423.003.0010.
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This chapter focuses on the Results section of the journal article. The Results section makes use of both text and graphics to highlight the essential findings of a study and to tell the story of scientific discovery. In this chapter we focus on writing the text; we refer you to chapter 16 for information on formatting graphics. After reading this chapter, you should be able to do the following: ■ Distinguish between the description and interpretation of data ■ Organize and present your results in a clear, logical manner ■ Refer appropriately to a figure or graph in the text ■ Use appropriate tense, voice, and word choice ■ Prepare a properly formatted figure and table As you work through the chapter, you will write a Results section for your own paper. The Writing on Your Own tasks throughout the chapter will guide you step by step as you do the following: 4A Read the literature and review your results 4B Organize your results 4C Prepare figures and/or tables 4D Tell the story of scientific discovery 4E Practice peer review 4F Fine-tune your Results section The purpose of a Results section (the third section in the standard IMRD format) is to present the most essential data collected during a research project. A well-written Results section guides the reader’s attention back and forth between text and graphics while highlighting important features of the data and telling the story of scientific discovery. Months (possibly years) of accumulated knowledge and wisdom, and countless pages of data, are distilled into only a few pages; hence, only the essential threads of the story are included in the Results section. In many journal articles, the Results section is actually a combined Results and Discussion (R&D) section. Combined R&D sections are preferred by many scientists who want to present and discuss results in an unbroken chain of thought. The combination is often more concise because less time is spent reminding the reader which results are being discussed. Combined R&D sections are not all alike; rather, they fall on a continuum with fully separated R&D sections at one end and fully integrated R&D sections at the other.
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Robinson, Marin S., Fredricka L. Stoller, Molly Constanza-Robinson, and James K. Jones. "Writing the Methods Section." In Write Like a Chemist. Oxford University Press, 2008. http://dx.doi.org/10.1093/oso/9780195367423.003.0009.
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In this chapter, we focus on writing a Methods section for a journal-quality paper. We begin with the Methods section because this is the section that many chemists write first, in part because this section describes what they know best: the procedures they have repeated (many times) to conduct their work. Moreover, most research groups use similar methodologies for several years; hence, previously written Methods sections can serve as models for writing new Methods sections. Together, these factors make the Methods section one of the easier sections to write and an excellent place to begin our writing instruction. By the end of this chapter, you will be able to do the following: ■ Know how to address the intended audience of a Methods section ■ Recognize which details to include and exclude from a Methods section ■ Organize a Methods section following standard moves ■ Use capitalization, abbreviations, and parentheses appropriately ■ Format numbers and units correctly ■ Use verb tense and voice in conventional manners As you work through the chapter, you will write a Methods section for your own paper. The Writing on Your Own tasks throughout the chapter will guide you step by step as you do the following: 3A Read the literature 3B Describe materials 3C Describe experimental methods 3D Describe numerical methods 3E Practice peer review 3F Fine-tune your Methods section The purpose of the Methods section is to address how a particular work was conducted. Relevant information about instrumentation and experimental and/ or numerical procedures is described. The goal is to describe the information in enough detail that an expert (not a novice) could repeat the work. Usually, this section is formally called, for example, Materials and Methods or Experimental Section, but for brevity, we call it simply the Methods section. Many of you have written a Methods section previously for a college-level chemistry course. Thus, we begin with an exercise to test your current knowledge about writing a Methods section.
Conference papers on the topic "(standard astronomical journal format)"
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Choquet, Élodie, Arthur Vigan, Rémi Soummer, Gaël Chauvin, Laurent Pueyo, Marshall D. Perrin, and Dean C. Hines. "A format standard for efficient interchange of high-contrast direct imaging science products." In SPIE Astronomical Telescopes + Instrumentation, edited by Suzanne K. Ramsay, Ian S. McLean, and Hideki Takami. SPIE, 2014. http://dx.doi.org/10.1117/12.2056890.
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