ORAC-DR: Overview and General Introduction 4.1-0 SUN/230.6 —Abstract Ii
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CFITSIO User's Reference Guide
CFITSIO User’s Reference Guide An Interface to FITS Format Files for C Programmers Version 3.3 HEASARC Code 662 Goddard Space Flight Center Greenbelt, MD 20771 USA February 2013 ii Contents 1 Introduction 1 1.1 ABriefOverview .................................. ... 1 1.2 Sources of FITS Software and Information . ........... 1 1.3 Acknowledgments................................. ..... 2 1.4 LegalStuff ....................................... 4 2 Creating the CFITSIO Library 5 2.1 BuildingtheLibrary .............................. ...... 5 2.1.1 UnixSystems................................... 5 2.1.2 VMS......................................... 7 2.1.3 WindowsPCs.................................... 7 2.1.4 MacintoshPCs .................................. 7 2.2 TestingtheLibrary............................... ...... 8 2.3 LinkingProgramswithCFITSIO . ....... 9 2.4 Using CFITSIO in Multi-threaded Environments . ............ 9 2.5 GettingStartedwithCFITSIO . ....... 10 2.6 ExampleProgram .................................. 10 3 A FITS Primer 13 4 Programming Guidelines 15 4.1 CFITSIODefinitions............................... ..... 15 4.2 Current Header Data Unit (CHDU) . ...... 17 4.3 Function Names and Variable Datatypes . .......... 18 4.4 Support for Unsigned Integers and Signed Bytes . ............ 20 4.5 Dealing with Character Strings . ......... 22 iii iv CONTENTS 4.6 ImplicitDataTypeConversion . ........ 23 4.7 DataScaling ..................................... 23 4.8 SupportforIEEESpecialValues . ........ 24 4.9 Error Status Values and the -
The Starlink Build System SSN/78.1 —Abstract I
SSN/78.1 Starlink Project Starlink System Note 78.1 Norman Gray, Peter W Draper, Mark B Taylor, Steven E Rankin 11 April 2005 Copyright 2004-5, Council for the Central Laboratory of the Research Councils Copyright 2007, Particle Physics and Astronomy Research Council Copyright 2007, Science and Technology Facilities Council The Starlink Build System SSN/78.1 —Abstract i Abstract This document provides an introduction to the Starlink build system. It describes how to use the Starlink versions of the GNU autotools (autoconf, automake and libtool), how to build the software set from a checkout, how to add and configure new components, and acts as a reference manual for the Starlink-specific autoconf macros and Starlink automake features. It does not describe the management of the CVS repository in detail, nor any other source maintainance patterns. It should be read in conjunction with the detailed build instructions in the README file at the top of the source tree (which takes precedence over any instructions in this document, though there should be no major disagreements), and with sun248, which additionally includes platform-specific notes. Copyright 2004-5, Council for the Central Laboratory of the Research Councils Copyright 2007, Particle Physics and Astronomy Research Council Copyright 2007, Science and Technology Facilities Council ii SSN/78.1—Contents Contents 1 Introduction 1 1.1 Quick entry-points . 2 2 Tools 3 2.1 Overview of the Autotools . 3 2.1.1 Autoconf . 5 2.1.2 Automake . 9 2.1.3 Libtool . 13 2.1.4 Autoreconf: why you don’t need to know about aclocal . -
A Cpu-Gpu Framework for Astronomical Data Reduction and Analysis
UNIVERSIDAD DE CHILE FACULTAD DE CIENCIAS F´ISICAS Y MATEMATICAS´ DEPARTAMENTO DE CIENCIAS DE LA COMPUTACION´ FADRA: A CPU-GPU FRAMEWORK FOR ASTRONOMICAL DATA REDUCTION AND ANALYSIS TESIS PARA OPTAR AL GRADO DE MAG´ISTER EN CIENCIAS, MENCION´ COMPUTACION´ FRANCISCA ANDREA CONCHA RAM´IREZ PROFESOR GU´IA: MAR´IA CECILIA RIVARA ZU´NIGA~ PROFESOR CO-GU´IA: PATRICIO ROJO RUBKE MIEMBROS DE LA COMISION:´ ALEXANDRE BERGEL JOHAN FABRY GONZALO ACUNA~ LEIVA Este trabajo ha sido parcialmente financiado por Proyecto FONDECYT 1120299 SANTIAGO DE CHILE 2016 Resumen Esta tesis establece las bases de FADRA: Framework for Astronomical Data Reduction and Analysis. El framework FADRA fue dise~nadopara ser eficiente, simple de usar, modular, expandible, y open source. Hoy en d´ıa,la astronom´ıaes inseparable de la computaci´on,pero algunos de los software m´asusados en la actualidad fueron desarrollados tres d´ecadasatr´asy no est´andise~nadospara enfrentar los actuales paradigmas de big data. El mundo del software astron´omicodebe evolucionar no solo hacia pr´acticasque comprendan y adopten la era del big data, sino tambi´enque est´enenfocadas en el trabajo colaborativo de la comunidad. El trabajo desarollado consisti´oen el dise~no e implementaci´onde los algoritmos b´asicos para el an´alisisde datos astron´omicos, dando inicio al desarrollo del framework. Esto con- sider´ola implementaci´onde estructuras de datos eficientes al trabajar con un gran n´umero de im´agenes,la implementaci´onde algoritmos para el proceso de calibraci´ono reducci´onde im´agenesastron´omicas,y el dise~noy desarrollo de algoritmos para el c´alculode fotometr´ıay la obtenci´onde curvas de luz. -
New Master Leases for Mauna Kea Science Reserve & Related Facilities & Easements
AGENCY ACTIONS SECTION 343-5(B), HRS PUBLICATION FORM (FEBRUARY 2013 REVISION) Project Name: New Master Lease for the Mauna Kea Science Reserve and Related Facilities and Easements Island: Hawai‘i District: Hāmākua TMK: 4-4-015:009 (Mauna Kea Science Reserve), 4-4-015:012 (Halepōhaku Mid-Level Facility), and 4-4-015:001 por. (Mauna Kea Access Road Easement) Permits: Issuance of New Leases for the Mauna Kea Science Reserve, or a portion of it, and Halepōhaku Mid-Level Facility and amendment of the Grant of Easement for the Mauna Kea Access Road. Proposing/Determination Agency: University of Hawai‘i at Hilo 200 W. Kawili Street Hilo, Hawai‘i 96720 Donald Stranley (808) 932-7348 Accepting Authority: Governor of the State of Hawai‘i 415 South Beretania Street #5 Honolulu, Hawaii 96813 (808) 586-0034 Consultant: Planning Solutions, Inc. 210 Ward Avenue, Suite 330 Honolulu, Hawai‘i 96814 Status (check one only): __DEA-AFNSI Submit the proposing agency notice of determination/transmittal on agency letterhead, a hard copy of DEA, a completed OEQC publication form, along with an electronic word processing summary and a PDF copy (you may send both summary and PDF to [email protected]); a 30-day comment period ensues upon publication in the periodic bulletin. __FEA-FONSI Submit the proposing agency notice of determination/transmittal on agency letterhead, a hard copy of the FEA, an OEQC publication form, along with an electronic word processing summary and a PDF copy (send both summary and PDF to [email protected]); no comment period ensues upon publication in the periodic bulletin. -
ORAC-DR: a Generic Data Reduction Pipeline Infrastructure✩
Astronomy and Computing 9 (2015) 40–48 Contents lists available at ScienceDirect Astronomy and Computing journal homepage: www.elsevier.com/locate/ascom Full length article ORAC-DR: A generic data reduction pipeline infrastructureI Tim Jenness ∗, Frossie Economou 1 Joint Astronomy Centre, 660 N. A`ohok¯ u¯ Place, Hilo, HI 96720, USA article info a b s t r a c t Article history: ORAC-DR is a general purpose data reduction pipeline system designed to be instrument and observatory Received 5 September 2014 agnostic. The pipeline works with instruments as varied as infrared integral field units, imaging arrays Accepted 27 October 2014 and spectrographs, and sub-millimeter heterodyne arrays and continuum cameras. This paper describes Available online 1 November 2014 the architecture of the pipeline system and the implementation of the core infrastructure. We finish by discussing the lessons learned since the initial deployment of the pipeline system in the late 1990s. Keywords: ' 2014 The Authors. Published by Elsevier B.V. Data reduction pipelines This is an open access article under the CC BY license Techniques: miscellaneous Methods: data analysis (http://creativecommons.org/licenses/by/3.0/). 1. Introduction The Observatory Reduction and Acquisition Control Data Re- duction pipeline (orac-dr; Cavanagh et al., 2008; Economou et al., In the early 1990s each instrument delivered to the United King- 1999; ascl:1310.001) was the resulting system. In the sections that dom Infrared Telescope (UKIRT) and the James Clerk Maxwell Tele- follow we present an overview of the architectural design and scope (JCMT) came with its own distinct data reduction system that then describe the pipeline implementation. -
MKCMP Decommissioning Plan for Mauna Kea Observatories
DECOMMISSIONING PLAN FOR THE MAUNA KEA OBSERVATORIES A Sub-Plan of the Mauna Kea Comprehensive Management Plan January 2010 Prepared for: Office of Mauna Kea Management University of Hawai‘i-Hilo Prepared by: Sustainable Resources Group Intn’l, Inc. DECOMMISSIONING PLAN FOR THE MAUNA KEA OBSERVATORIES A Sub-Plan of the Mauna Kea Comprehensive Management Plan January 2010 Prepared for: Office of Mauna Kea Management University of Hawai‘i - Hilo 200 W. Kawili Street Hilo, Hawaii 96720 www.malamamaunakea.org Prepared by: Sustainable Resources Group Intn’l, Inc. 111 Hekili Street, Suite A373 Kailua, HI 96734 www.srgii.com Executive Summary The Decommissioning Plan for Mauna Kea Observatories (Decommissioning Plan) is a sub-plan of the Mauna Kea Comprehensive Management Plan (CMP). It was required as a condition of approval of the CMP by the Board of Land and Natural Resources (BLNR) in April 2009. The purpose of this Decommissioning Plan is to describe a process for decommissioning observatories on Mauna Kea, including financial planning. Although some observatories have made preliminary inquiries regarding what might be expected of them if they were to cease operations, neither the State, nor the University, have guidelines for the decommissioning of facilities. This Decommissioning Plan provides the guidelines recommended by the University. The Decommissioning Plan provides a framework that can be used by both existing and future observatories on Mauna Kea to ensure that the Department of Land and Natural Resources (DLNR) as the land owner and lessor, UH as the lessee, and the observatories as sublessees have clear expectations of the observatory decommissioning process. -
The Significant Properties of Software: a Study
The Significant Properties of Software: A Study Brian Matthews, Brian McIlwrath, David Giaretta, Esther Conway STFC Rutherford Appleton Laboratory Chilton OX11 0QX UK December 2008 Significant Properties of Software Revision History: Version Date Authors Sections Affected / Comments 0.1 18/02/2008 BMM Outline 0.5 05/03/2008 BMM First Draft 0.6 09/03/2008 DG DG added section on OAIS/CASPAR 0.7 11/03/2008 BMM Added section on StarLink + revisions. 0.8 23/03/2008 BMcI, EC, BMM Expanded use cases 1.0 28/03/2008 BMM, BMcI First Complete release version 1.1 23/12/2008 BMM Final Revision 2 Significant Properties of Software Executive Summary ...................................................................................................... 5 Recommendations ..................................................................................................................... 6 1 Background to the Study ....................................................................................... 9 1.1 Introduction ................................................................................................................... 9 1.2 Significant Properties .................................................................................................. 10 2 Scope of Study .................................................................................................... 12 2.1 Definition of Software ................................................................................................ 12 2.2 Diversity of Software ................................................................................................. -
Book of Abstracts 2009 European Week of Astronomy and Space
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SLALIB — Positional Astronomy Library Programmer's Manual
CCLRC / Rutherford Appleton Laboratory SUN/67.63 Particle Physics & Astronomy Research Council Starlink Project Starlink User Note 67.63 P. T. Wallace 21 October 2003 SLALIB — Positional Astronomy Library 2.4-13 Programmer’s Manual Abstract SLALIB is a library used by writers of positional-astronomy applications. Most of the 187 routines are concerned with astronomical position and time, but a number have wider trigono- metrical, numerical or general applications. ii Contents 1 INTRODUCTION 1 1.1 Purpose . 1 1.2 Example Application . 1 1.3 Scope . 2 1.4 Objectives . 3 1.5 Fortran Version . 4 1.6 CVersion ........................................ 4 1.7 Future Versions . 4 1.8 New Functions . 5 1.9 Acknowledgements . 5 2 LINKING 5 3 SUBPROGRAM SPECIFICATIONS 6 4 EXPLANATION AND EXAMPLES 169 4.1 Spherical Trigonometry . 169 4.2 Vectors and Matrices . 172 4.3 Celestial Coordinate Systems . 174 4.4 Precession and Nutation . 177 4.5 Mean Places . 179 4.6 Epoch . 179 4.7 Proper Motion . 180 4.8 Parallax and Radial Velocity . 180 4.9 Aberration . 181 4.10 Different Sorts of Mean Place . 182 4.11 Mean Place Transformations . 183 4.12 Mean Place to Apparent Place . 185 4.13 Apparent Place to Observed Place . 186 4.14 The Hipparcos Catalogue and the ICRS . 189 4.15 Timescales . 189 4.16 Calendars . 193 4.17 Geocentric Coordinates . 193 4.18 Ephemerides . 194 4.19 Radial Velocity and Light-Time Corrections . 203 4.20 Focal-Plane Astrometry . 204 4.21 Numerical Methods . 205 5 SUMMARY OF CALLS 208 SUN/67.63 1 1 INTRODUCTION 1.1 Purpose SLALIB1 is a library of routines intended to make accurate and reliable positional-astronomy applications easier to write. -
Arxiv:1410.7513V1 [Astro-Ph.IM] 28 Oct 2014
Learning from 25 years of the extensible N-Dimensional Data Format Tim Jennessa,∗, David S. Berryb, Malcolm J. Currieb, Peter W. Draperc, Frossie Economoud, Norman Graye, Brian McIlwrathf, Keith Shortridgeg, Mark B. Taylorh, Patrick T. Wallacef, Rodney F. Warren-Smithf aDepartment of Astronomy, Cornell University, Ithaca, NY 14853, USA bJoint Astronomy Centre, 660 N. A‘oh¯ok¯uPlace, Hilo, HI 96720, USA cDepartment of Physics, Institute for Computational Cosmology, University of Durham, South Road, Durham DH1 3LE, UK dLSST Project Office, 933 N. Cherry Ave, Tucson, AZ 85721, USA eSUPA School of Physics & Astronomy, University of Glasgow, Glasgow G12 8QQ, UK fRAL Space, STFC Rutherford Appleton Laboratory, Harwell Oxford, Didcot, Oxfordshire OX11 0QX, UK gAustralian Astronomical Observatory, 105 Delhi Rd, North Ryde, NSW 2113, Australia hH. H. Wills Physics Laboratory, Bristol University, Tyndall Avenue, Bristol, UK Abstract The extensible N-Dimensional Data Format (NDF) was designed and developed in the late 1980s to provide a data model suitable for use in a variety of astronomy data processing applications supported by the UK Starlink Project. Starlink applications were used extensively, primarily in the UK astronomical community, and form the basis of a number of advanced data reduction pipelines today. This paper provides an overview of the historical drivers for the development of NDF and the lessons learned from using a defined hierarchical data model for many years in data reduction software, data pipelines and in data acquisition systems. Keywords: data formats, data models, Starlink, History of computing 1. Introduction In this paper the term “data model” refers to the organization, naming and semantics of components in a hierarchy. -
Starlinksoftware Collection
SUN/1.24 Starlink Project Starlink User Note 1.24 ed. S. E. Rankin 5 August 2003 STARLINK Software Collection SUN/1.24 —Abstract ii Abstract The Starlink Software Collection is a set of software which is managed and distributed by the Starlink Project. Some of the software was written by members of the Project, but some of it comes from outside the Project. This note describes the functions of the individual items in the Collection and provides an overview of the software so that readers can identify the items they need. The software is classified into four main divisions: • Packages – are large collections of programs for people who want to analyse, convert, and display data. They are subdivided into eleven classes to help you find what you want. • Utilities – are small programs devoted to a specific purpose. For example, they help you prepare for observations, write documents, and write programs. • Subroutine Libraries – are for programmers writing astronomical software. They provide facilities such as astronomical calculations, data management and graphics. • Infrastructure – are items which are mainly of interest to people writing programs within the Starlink Software Environment. They are included for completeness. Each item is described in sufficient detail for you to decide whether or not to investigate it further. If you want to find out more about an item, follow the document references given opposite the item name. If you are using the hypertext version of this document, the most up-to-date document references can be found by following the link from the software item name. iii SUN/1.24—Contents Contents 1 Introduction 1 2 Changes since the last issue 2 2.1 New packages . -
Joint Astronomy Centre Annual Report 2005/6
Joint Astronomy Centre Annual Report 2005/6 660 North A`ohoku Place Hilo, Hawaii 96720 USA Tel: +1 808 961 3756 Fax: +1 808 961 6516 Web: http://www.jach.hawaii.edu/ Introduction by the Director Welcome to the JAC Annual Report for modern times. Over its eight-year lifetime, it accounted 2005/06. It follows the same format as for roughly 75% of all publications based on JCMT data, last year’s. The reporting period, how- and was, at one stage, ranked second only to the HST ever, has been adjusted to match the in terms of its impact on astronomy. One of its most financial year, rather than the calendar notable successes was the discovery of a large popula- year, to bring this report into synchronic- tion of massive, dust-enshrouded galaxies in the early ity with our programme reports to the Universe, a class of objects now known universally as two telescope Boards. The period has certainly been “SCUBA galaxies”. The retirement of SCUBA clearly eventful, with the JCMT in the midst of a transforma- marks the end of an era. tion to third-generation instrumentation, whilst at UKIRT, observations have commenced on a major and much- The JCMT is undergoing an extremely ambitious pro- anticipated science campaign. gramme of development in which the entire instrumenta- tion suite is being replaced. The integration of ACSIS The UKIRT highlight of 2005/06 was undoubtedly the ob- into the JCMT’s new Observatory Control System contin- servation of the impact of the NASA Deep Impact probe ued throughout the reporting period.