... For spectra a transformation from wavelength to frequency is used to identify spectral regions which follow a power law. This transformation is given by . ... Whereas the transforms mentioned above only perform a non--linear rebinning of the data, the Fourier transform converts a spatial image into the frequency domain. ... As an example of using Fourier transforms to extract information from a frame, an azimuthal intensity profile of the spiral galaxy A0526--16 is shown in Figure . ...

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• Background estimate by filtering
• Background Estimates

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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Next: Results Up: High Resolution Measurements from Previous: Introduction . The first step in PSA is to Fourier transform the image and calculate the square modulus of the FT to generate the power spectrum, . ... Specifically, one excludes the very lowest frequencies where the large scale nonuniformities in the image have the greatest effect, and one limits the fit to a frequency range where the SNR is sufficiently high. ...

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• Dark Backgrounds
• J. Boia RИsumИ
• ACS Data Handbook

. Next slide . Back to first slide . View graphic version .

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• Background estimation
• Source Operations

grdfft - Perform mathematical operations on grdfiles in the frequency domain grdfft in _ grdfile -G out _ grdfile [ -A azimuth ] [ -C zlevel ] [ -D [ scale |g ] ] [ -E [ x|y ][ w ] ] [ -F [ x | ... The horizontal dimensions of the grdfiles are assumed to be in meters. ... Append a scale to multiply by (kr * scale ) instead. Alternatively, append g to indicate that your data are geoid heights in meters and output should be gravity anomalies in mGal. Default is no scale]. ...

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• Galactic Gravitational Wave Background
• Critical Frequencies and Gravitational Wave Detector Halfwidth for
• Gravitational wave background from nearby galaxies

Program: TRANSFORM Purpose: Transform a (sub)set using rotation, scaling, translation etc. ... This set will be transformed to OUTSET=, using a concatenation of simple operations like rotation, scaling, translation etc. ... POS= Enter position of centre: [0,0] All operations are defined with respect to a central point. ... If, for example, you want to rotate an object about its centre, then determine the position of this centre (e.g. -6.2 8.5) and enter these numbers here (e.g. POS= -6.2 8.5). ...

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• http://www.atnf.csiro.au/projects/askap/techdocs/LOFAR_technology.pdf
• http://www.atnf.csiro.au/management/atuc/2002nov/LOFAR-technologies.pdf
• http://www.atnf.csiro.au/observers/planning/Universities_Operations.pdf

... The Time shift for April, 17-18 20 April 1999 . ... The INTMINS April 1999 operations schedule was done on the base of the MIR ground track long-term prediction using the MIR's orbital elements status on 29/03/99 . ... The investigation of the time shift behaviour was began before 29/03/99 on the base of the different orbital elements determined (by KIAM RAN) 22/03/99, 25/03/99 and continued on the base of the orbital elements determined at 31/03/99, 5/04/99. ... Modified 20 April 1999  ...

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• IKI SSC INTMINS
• W o r k s h o p H E N D - 2003 'The Second year of HEND operations on the NASA

Next: NOVIDAS and UVPROC II-Data Archive and Reduction System for Nobeyama Millimeter Array . ... The RATAN-600 radio telescope allows us to carry out simultaneous multi-frequency observations using wide-band radiometers. ... Using these features a flexible astronomical data processing system (FADPS), operating on different UNIX platforms, was created. ... FADPS commands may be executed directly in UNIX, in scripts, or using a special shell for our data processing system in the X-Window system. ...

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• Heuristic Estimates of Weighted Binomial Statistics for Use in Detecting Rare
• Automated Programming and Simulations of Signal Compression from the Cosmic
• Correction of Systematic Errors in Differential Photometry

The Cosmic Background Imager T. J. Pearson et al. California Institute of Technology The Cosmic Background Imager (CBI) is an instrument designed to make images of the cosmic microwave background radiation and to measure its statistical properties on angular scales from 5 arc minutes to one degree (spherical harmonic scales from l  3000 down to l  300). The CBI is a 13-element interferometer mounted on a 6 meter platform operating in ten 1-GHz frequency bands from 26 GHz to 36 GHz. ...

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• Astrophysics Group VSA
• Astrophysics Group Cosmic Microwave Background (CMB)
• PPEUC Programme - Cosmic Microwave Background Workshop

; 31 October 2006, 14 November 2006, 30 January 2007 EDUC ATIONAL · BACKGROUND: University of Texas at Austin, Austin, TX, 1967 NASA EXPERIENCE: NASA Manned Spacecraft Center /Lyndon B. Johnson Space Center , Houston, TX (19672004) · Systems Engineer, Recovery Systems Branch, Landing and Recovery Division , Flight Operations Directorate (1967-1970) · Systems Engineer, Operations Development Section, Systems ...

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• http://www.jsc.nasa.gov/history/oral_histories/PaceCW/PaceCW_Bio.pdf
• http://www.jsc.nasa.gov/history/oral_histories/DavisLD/DavisLD_Bio.pdf
• http://www.jsc.nasa.gov/history/oral_histories/KnightJ/KnightJ_Bio.pdf

... The Russian Federation State Program "Physics of Condenced Matter", the "Superconductivity" division , Project code "Generation-2" . ... The multielement josephson structures are known to allow implementation of the unique properties of the Josephson junctions as electromagnetic waves sources with high change rate of generation frequency, working in the millimeter and submillimeter wavelength diapasones. ... Even the optimal type of the junction electrodynamic interconnection isn't chosen. ...

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• Lab234 - Development of the superconducting elements for operation at
• Project 1 - SfP - Ovsyannikov, Supersensitive high-Tc superconducting
• Report on Cosmic Call 1999

... SITE SAFETY PLAN . ... Prepared by: Ben Harris, Site Safety Officer . ... INTRODUCTION . SECTION I . APO SAFETY POLICY . ... RESPONSIBILITIES . ... 2.2 Site Safety Officer . ... REPORTING SAFETY CONCERNS . ... 4.3 General Requirements . 4.4 General Responsibilities . ... Figure 1 - Notice of Incident-State of New Mexico . ... 5.3 National Fire Protection Association Codes (NFPA) . ... 6.1 Background . ... OFFICE SAFETY . ... Figure 9 - Back Safety Tips . ... PERSONAL PROTECTIVE EQUIPMENT . ...

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• MILT Description
• Untitled Document
• APO Job Announcements

... From left to right, the columns list the machine acronym, the present access of the machines to outside users, the operating mode, total bandwidth (MHz), number of frequency channels, bandwidth per channel (kHz), shortest sampling interval (us), number of bits recorded per sample, number of polarizations recorded and the data storage method. ... Disk . ... Timing . ... Baseband . ... Data sampling: 4-bit in search mode, 6-bit in timing mode . ... Mode(s) of operation: baseband recording and timing ....

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• Operations
• measured_operating_values
• arecibo technical and operations memo series (atoms)

... The operators will be explained as they are used. The general notion to keep in mind is that any combination of these operators results in a 2- D affine coordinate transformation in the TF plane, which may be represented using the homogeneous coordinates often used in computer graphicsfoley. ... S _t_c,f_c = g_t_c,f_c,(_t) | ... We denote a time shift to the position , with an operator that has a multiplicative law of composition : (Table 1). ... Note that these two operators do not commute. ...

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• CONCLUSION
• Mean power spectrum
• INTRODUCTION

. The enclosure for the Solar Fourier Transform Spectrometer, commonly called the FTS Tank, at the McMath-Pierce Solar Facility on Kitt Peak. The tank is shown open, with some of the equipment racks required to operate the FTS visible in the background. Credit: Tom Eglin, Mark Hanna/NOAO/AURA/NSF

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. Use white text, and mess with the opacity. Probably not the same as Federico's Watermark timp.

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• Query Operations
• APOD: 2013 March 25 - Planck Maps the Microwave Background
• APOD: 2002 February 6 - The Cosmic Infrared Background

... Product of two Gaussians · g = N(µ,2) N(µ,2) exp [-(x-µ)І/2І - (x-µ)І/2І] · µ = (µІ+µІ) / (І+І) ; І = ІІ / (І+І) for , µ µ and · g = (1/2) exp [-(x-µ)І/2І] (1/2(І+І)) exp [(µ-µ)І/2(І+І)] Bayesian Aperture Photometry (Gaussian) · Measurements: Background in an area AB = rAS: fB ± B M ( Source + Background ) in an area AS: fM ± · Priors: p(b) = N(b;f0B,0BІ) p(s) = N(s;f0S,0SІ) · Likelihoods: f(fB,B|b,r) exp [-(rb-fB)І/2BІ] ...

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• The AstroStat Slog background
• The AstroStat Slog Blog Archive Background Subtraction, the Sequel [Eqn]
• The AstroStat Slog background marginalization

... Getting to Armagh . ... An Airbus service operates every 30 minutes, Monday to Saturday, between Belfast International Airport and the Europa Buscentre in Belfast, and at 30 or 60 minute intervals on a Sunday. ... The journey from the airport to Belfast takes about 30 minutes. The Ulsterbus express bus between Belfast Europa Buscentre and Armagh takes about 1 hour. ... It is possible to take a bus from Dublin Airport to Newry and then take a taxi to Armagh. ... Belfast International Airport . ...

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• HISTORICAL BACKGROUND
• Historical Background
• Background

dfos = Data Flow Operations System, the common tool set for DFO make printable . Some parts of the daily workflow can be performed day by day in an automatic way. Let us recall the Table 1 from the simple model , now with the processing mode updated: . ... CALIB/SCIENCE . ... workflow steps 1-3 . ... day1 . ... day2 . ... createAB -m CALIB -d day1; createJob -m CALIB -d day1 . ... 4 : Mapping of the daily workflow into three working days for the optimized workflow. [1-3] is short for days1-3. ...

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• Operations with DFOS: daily cronjobs
• ESO - Thesis Topic: Foreground emission and Cosmic Microwave background
• ESO - La Silla Science Operations

Automatic Detection of NEOs in CCD Frames . ... CCD frames obtained with modern telescopes with robotic operation allow carrying out standard observation programs for detection of peculiar objects on stellar backgrounds, as is the case of Near Earth Objects (NEOs). ... In this paper, we present original algorithms for automatically detecting dim NEO images in telescope frames, considering both sidereal and differential tracking [2]. ...

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• IAA EOP Service