2010 June GBT KFPA Call for Proposals The K band Focal Plan Array Receiver (KFPA) was successfully commissioned in March and April 2010. Initial results of these...
2011 February GBT KFPA Call for Proposals The K band Focal Plan Array Receiver (KFPA) was successfully re commissioned in August and September 2010. Results of t...
2012A GBT Call for Proposals KFPA The K band Focal Plan Array Receiver (KFPA) share risk observations were successful in Winter 2010/2011. The KFPA is now av...
Single Pixel Testing Laboratory * Single Pixel Laboratory Tests: September 04/05, 2008 * LO1 power level requirements on GBT * Lab noise temperature...
16: Mapping and Calibration: 2010 April 19 Ran tests of nodding spectra with all beams. Seemed OK. Ran some maps of TMC, Orion and M33, which looked reasonable....
Monitor and Control of the K band Focal Plane Array Overview The GBT M C System The GBT monitor and control (M C) system, named Ygor, is a distributed object or...
KFPA M C Software Integration Path to a Common User Backend KFPA M C Manager The creation of a Manager and microcontroller firmware is the first step and handl...
Purpose The purpose of this page is to serve as a primer for discussion about designing a scalable M C software package for the K band FPA receiver. Introduction...
KFPA Axial Ratio Tests The KFPA axial ratio is specified to be 1 dB maximum. Axial ratio tests were completed 14 Jan 2009 on the KFPA single beam receiver. A lin...
Main.BobSimon 03 Nov 2008 TKFPA29SEP08 Ward, Simon Testing the KFPA receiver in the lab Setup: Cold KFPA 1 pixel receiver with 300k waveguide load on feed window ...
Comments Supporting Box Rotation Capabilities Comments Against Box Rotation Capabilities * Most of the effects of box rotation can be accomplished with intel...
Main.BobSimon 2010 08 25 Changes/Fixes to be made in hardware and software: Misc control screen: Should look like: * CalControl.pdf Cryo LNA control screen:...
Main.StevenWhite 07 Jun 2007 2.1.1 Pixel Cryogenics System #8211; This is a small single pixel dewar that will be used to test the first prototype pixel on the ...
Conceptual Design Review CDR Final Report: CDR Panel Final Report Response to Final Report: Email to Committee Members Panel Members Name Affiliation ...
It should be a goal, if not a spec, to provide reasonable total power continuum performance; I would suggest the quantitative goal that the RMS of 1 second integr...
Main.BobSimon 2010 01 27 * cooldown_01_07_10.pdf: Eight wraps of Super Insulation added and temperatures sensors moved. No significant difference over prior c...
Final Report: kfpa_cdr_finalreport2.pdf: February 11, 2009 Final Response: KFPA Critical Design Review Response.pdf :February 26, 2009. Dates: January 30 and 31...
Thermal Loading Calculations (Updated January 12, 2009) The thermal loads are calculated and shown in the file ThermalLoadTotals7pixel.XLS with the 15K to 300 K a...
* Pipeline progress review * The pdf version of the Minutes_October_20_2009.pdf * The pdf version of the September 23, 2009_KFPA_Pipeline_conference * T...
Rob Taggart is the administrator of drawing numbers for the K band FPA project. A read only drawing log file is available on the network for assigned drawing num...
Main.StevenWhite 07 Jun 2007 1.1 Electrical Design and Specs #8211; The overall system architecture must be finalized and specifications written. There are sev...
!Engineering Planning Table of Contents Seven Pixel Tests * Post Commissioning Tests * Commissioning Stability Tests March 26 and April 19, 2010: 800 MHz...
Existing GBT K band Data There have been 167 projects that have used the existing K band receiver on the GBT. They are listed here. Of these, 134 have used the ...
J. Bally, University of Colorado J. DiFrancesco, HIA, Victoria A. Goodman, Harvard/CfA M. Heyer, University of Massachusetts M. Hollis, NASA/GSFC J. Jackson, Bost...
* Is it possible to get the upper frequency limit pushed to 27.5GHz? At 27.478 GHz, there's the ammonia (9,9) line located. It is third lowest ortho ammonia trans...
Frequency Switched Pipeline Calibration Plan Note that much of the content of this documentation is out of date. Please refer to the GBT Pipeline documentation ...
KFPA Gain Compression Tests On January 14 15, 2009, gain compression tests were done on the KFPA single beam receiver. The IDM Type II prototype was used. Resul...
Main.BobSimon 09 Jan 2009 Noise performance comparing the GBT K band receiver and the KFPA receiver with type I downconverter * GBTkband_vs_kfpa.xls: GBTkband_vs...
Monitor and Control Hardware Introduction Typical GBT receivers, those with four or fewer pixels, utilize a monitor and control system based on the VLBA Standar...
Main.StevenWhite 06 Jun 2007 * Original (April 2007) Internal NRAO Proposals for the frontend, backend and potential Canadian Contributions * Initial (April...
Preparing to hoist with Ken Ward and Phillip Rittenhouse Photograph by Bob Simon GBT Turret view with Bob Goldizen, Harry Morton and Phillip Rittenhouse ...
Main.StevenWhite 14 Jun 2007 Al Wotten: "For ammonia studies, IMHO it would be useful to get several (J=K) lines to characterize temperature. To get two para lin...
A seven feed, dual polarized K band focal plane array receiver is proposed for the Green Bank Telescope. This instrument will enhance the scientific capabilities ...
Observing modes: Jeff Mangum, chair This group will describe the ways in which the array will be used on the telescope to guide considerations of telescope motion...
KFPA Beam Spacing * K band hexagonal feed spacing in the focal plane and on the sky: * The above figure shows the hexgonal close packed spacing used ...
Use the total power calibrated data, plus the information from the calibration module to arrive at the data in the units in which they will be imaged (is that alw...
Sampling rates and Efficiencies The processing of the sampled data requires a limit on the data rates. The first device in this process is the analog to digital ...
Combines the information from the various M C FITS files into a data stream that the pipeline can be used. At the moment, the online sdfits filler does this task ...
This page documents work on converting GBT sdfits file to the format used by the ACSIS gridder. The ACSIS gridder is an application in starlink. Relevant docu...
This component is deferred until later in the pipeline development. Possible flagging schemes and needs should be described here. Main.BobGarwood 2009 07 14
A design for the data pipeline for the prototype GBT K Band Focal Plane Array Introduction See the KFPA wiki for more information on the GBT K Band Focal Plane A...
A design for the data pipeline for the proposed GBT K Band Focal Plane Array Introduction See the KFPA wiki for more information on the proposed GBT K Band Foca...
This wiki page exists so that ongoing pipeline discussion issues can be maintained and commented on in a single place. The current focus is on describing the use ...
Eventually this page will contain the links to the specific use cases that the pipeline will handle. The use cases should be specific enough so that the pipeline ...
This is obviously very much a work in progress. Right now it's primarily a note pad where thoughts and questions on the KFPA use cases can be displayed quickly. P...
Scratch space for thoughts on the KFPA data pipeline and processing issues. I am attempting to turn this into a KFPA data pipeline design document prior to the re...
Please feel free to edit this page and add any topics for discussion during this workshop. Eventually these items will be folded into the agenda. Visit the Main...
GBT Data Visualization visually interacting with the ungridded data from the GBT. Requirements Examples * aips /dish relied on the viewer and msplot. See ...
Glen Langston provided the sample script and accompanying procedures attached here. These procedures are written specifically to work with two sets of mapping sc...
Main.StevenWhite 2013 02 28 An ongoing issue is the stability of the integrated noise calibration module,ICM. Occasionally the values are not loaded properly, a ...
Frequency Switched KFPA Pipeline Use Case Figure 1: JCMT 850 um infrared image of Ophiucus, showing regions images B, C and D imaged with the GBT by Friesen et a...
This page was created prior to a phone meeting scheduled for 10AM on 11 Jan 2011. Eventually this list will be associated with tracked items on Pivotal Tracker (...
KFPA Data Analysis Meeting June 23 25, 2008 Purpose and Goals This is the first face to face meeting concerning the KFPA data pipeline and data analysis nee...
KFPA Pipeline Overview Pipelines * Imperative for large focal plane arrays (high data rate). * More than just a handy quick look tool. * Defaults should...
$ Frequency Switched : SIG switching is used and the signal and reference spectra are present in each integration. For each integration after doing the total pow...
Source Calibration notes for the Pipeline Currently (August 2009) the standard GBT IDL calibration procedures use a single (scalar) value for the Noise Diode valu...
Position Switched KFPA Pipeline Use Case Figure 1: Image of the distribution of HC7N in the Taurus Molecular Cloud (TMC) The KFPA imaging pipeline has t...
Makes use of the "cal" switching present in the data. If the CAL value does not switch between T and F an equal number of times, this step does nothing. In the c...
KFPA Weather models and Opacity calibration. This page describes the KFPA pipeline approach to calibration of the measured and model atmospheric opacity as a func...
KFPA Pipeline Weekly Meeting Agenda Next meeting Wednesday, June 16 2010 at 1:00pm in GB137 and CV331. 2010 06 16 1. Final review of agenda for Jun. 17 pipeli...
Nyquist Sampling at K band * \text{Magnification is 3, giving f/D of 3 x 0.6 = 1.9.} * \text{ Nyquist sampling (Voltage) of focal plane FWHM spacing requir...
Main.StevenWhite 29 Oct 2007 Here's my Roger Norrod promised input on the spectral baseline stability requirements: A handy GBT sensitivity calculator is at: h...
K band FPGA Single Pixel Test Report for 2008 December 28 These single pixel tests compared the (K1) performance with the current GBT K band receiver (K0). The ob...
Comparison of the GBT 4 beam and Single Pixel performance Observations were made with the 4 beam K band receiver and with the single pixel receiver in order to di...
Kfpa Commissioning Session Report 29 and 30 Kevin Christiansen systematically reduced KFPA commissioning observations of W51 and produced spectral line plots and ...
KFPA Automatic Balance of IF path Modification Request #? (C04 2009) 1. Introduction The basic observing modes for the KFPA are similar to those already used ...
KFPA Firmware Documentation 1. Intro The GBT M C Manager communicates with the underlying KFPA hardware via the firmware on a Netburner card: http://netburner.co...
KFPA LO and IF chain calculation requirements Modification Request #7 (C04 2009) 1. Introduction In order for the observers, engineers and commissioners to e...
Observation and Calibration Methods for the KFPA Modification Request #9 (C04 2009) 1. Introduction The KFPA Pipeline will monitor the GBT observing status an...
KFPA LO and IF chain calculation requirements Modification Request #? (C04 2009) 1. Introduction In order for the observers, engineers and commissioners to ef...
KFPA Observation Summary; Organized by Source All the KFPA test observations are public domain, and may be used by any one. To make finding the KFPA observations...
KFPA Astrid Pipeline Interface Modification Request #8 (C04 2009) 1. Introduction The GBT observer must communicate to the KFPA pipeline some parameters rega...
KFPA Pipeline Development Note that much of the content of this documentation is out of date. Please refer to the GBT Pipeline documentation instead!!! This web...
KFPA Pipeline Calibration and Imaging Review NRAO will hold an internal review of the KFPA imaging pipeline on Thursday June 17, starting with the science lunch d...
KFPA Astrid Pointing Modes Modification Request #? (C04 2009) 1. Introduction Effective use of the KFPA requires regular peaking on a bright radio source and ...
KFPA and Pipeline Data Reduction Guide Note that much of the content of this documentation is out of date. Please refer to the GBT Pipeline documentation instea...
KFPA Astrid Spectral Line Modes Modification Request #? (C04 2009) 1. Introduction The basic observing modes for the KFPA are similar to those already used by...
LO1A: GBT Receiver Room LO used for Doppler tracking Local Oscillators 1 A and 1 B are located in the GBT receiver room and are used for the first down conversio...
LO1B: GBT Receiver Room LO used for Doppler tracking Local Oscillators 1 A and 1 B are located in the GBT receiver room and are used for the first down conversion...
Upper LO (24.8 to 34.3 GHz) Problems * This section is intended as a reference page to document and understand the problems with the upper LO design. ...
Main.BobSimon 01 Oct 2008 *Excel spreadsheet showing LO1 synthesizer power settings vs frequency. This will give correct LO1 drive at the downconverter input....
Main.StevenWhite 27 Aug 2007 3.3 This task describes the assembling of all components for a seven feed receiver. This includes the mounting and cabling of all i...
Main.StevenWhite 07 Jun 2007 3.1.1 Array Cryogenics System #8211; This is the cryogenic system for the full array. Ideally it would be designed for a fully pop...
Main.StevenWhite 27 Aug 2007 This task requires a fully functional multi pixel receiver with complete software packages that is then qualified and released for ob...
Main.StevenWhite 27 Aug 2007 This is the task of providing data analysis software for mapping and calibration. This is not intended to be an optimal data analy...
Main.StevenWhite 27 Aug 2007 This task includes all software necessary to aide in setting up the instrument for all its observational modes, where data is stored ...
Main.StevenWhite 07 Jun 2007 3.2.1 IF Modules (Pixels 2 7) #8211; This is the fabrication and testing of IF Modules for pixels 2 7. 3.2.2 Bias, Monitor, and Co...
Stability Tests: April 19, 2010 Commissioning Data: * Spectral Line Mode: 800 MHz, 30 second integrations, 5 minute Scans. These are difference plots between...
Main.StevenWhite 07 Jun 2007 1.2 Mechanical Design and Specs #8211; The observatory's experience with ALMA, as well as the experience of other institutions who ...
Some open issues related to the mechanical design * For the 7 pixel there are 4 G 10 standoffs per pixel. 61 pixels will need a different arrangement. * A ...
Kfpa Commissioning Session Report 17 Observations configured for larger scale images, to test pipeline processing. Had some setup issues during these tests, wh...
Main.BobSimon 01 Oct 2008 * Results of noise temperature measurements in lab, 9/25/2008 * README92508.TXT: README92508.TXT * noise092508.xls: noise092508.x...
Main.BobSimon 01 Oct 2008 * Results of noise temperature measurements in lab, 9/26/2008 * README92608.TXT: README92608.TXT * Meas26Sep08.xls: Meas26Sep08.xls...
Main.BobSimon 05 Nov 2008 Single pixel KFPA receiver. This is a summary view of noise temperature testing as done on 9/25, 9/26, and 10/28/2008, as compared to th...
EVLA design. Fabricated in Green Bank. Assembled in Socorro by Brent Willoughby. Bob Hayward engineer. November 6, 2007 Machine shop has drawings and work orde...
K Band Focal Plane Array (KFPA) and Pipeline Observer's Guide Note that much of the content of this documentation is out of date. Please refer to the GBT Pipeli...
Communications Problems * When the KFPA Cleo Manager display are all "1 's", the control software is not communicating with the net burner card and needs to ...
Single Pixel Output Waveguide Return Loss Sponsor Response. February 24, 2009. Steven D. White, Program Manger. I have agreed to purchase the isolators and accep...
Main.BobSimon 11 Jan 2008 * Receiver room: * GBT turret: * K band Pamtech cryo isolator, picture 01 * K band Pamtech cryo isolator, picture 02: * K band f...
New Directions and Requirements for the GBT Pipeline Agenda: * Brief summary of current pipeline (Joe) 10 min * Top priority requirements (All Met) ...
Review of Pipeline Progress: 2009 December 16 Steve, Toney, Bob, Marty, John and Glen reviewed pipeline development status. * Update on Hardware status Steve...
* From the point of view of continuum, the feeds should be native circular. With no special provisions other than that (for instance, there is no need for the rec...
Change Requests (Hardware) The following table is established to track all hardware changes, issue resolution, and other requests. These includes all changes to...
Observations in the K band frequency spectrum (18 26.5 GHz) of extended sources in the spectral line require inordinate amounts of telescope time with a single pi...
The Resource estimates are driven by the target milestones for this project. Overall, we'd like this project to lead to a pipeline review. The goal of the pipelin...
Position Switched Pipeline Calibration Plan Note that much of the content of this documentation is out of date. Please refer to the GBT Pipeline documentation i...
Random Comments Put suggestions / ideas here if you cannot think of anywhere else to put them... * I understand that the dewar will be designed to hold 61 pixe...
KFPA Re commissioning Test Reports The KFPA was reworked during summer 2010 and restored to the GBT on August 21, 2010. Below we summarize the tests made to confi...
Main.StevenWhite 27 Aug 2007 Monitor and Control for single pixel. This provides the monitor and control functions through a CLEO screen. This software should i...
Main.StevenWhite 07 Jun 2007 Once the single pixel receiver and backend is complete, the unit will be tested on the telescope. This task accounts for the work ne...
Software for the K band Focal Plane Array (KFPA) GBT software improvements and extensions are a critical part of the KFPA project, which will enable important new...
* External Committee Members * Internal Working Group * 2007 September (.pdf) * 2007 April (.pdf) * Exact frequency coverage of the front end. Is this o...
GBT K Band Focal Plane Array Science and Data Pipeline Workshop, Nov 26 28, 2007 Introduction This is a workspace to facilitate the organization of the GBT K B...
September 28th 2007 Focal Plane Array Discussion Meeting Overview The GBT is a superb telescope with excellent performance at frequencies up to 50 GHz (wavelengt...
Seven Pixel K band Focal Plane Array Commissioning We present summaries of initial commissioning tests of the KFPA 7 pixel tests in March and April 2010. These te...
First K band Focal Plane Array Pixel Testing The first step in developing the full 61 pixel array is prototyping the first pixel hardware. The development of the ...
A large number of laboratory tests were performed before putting the receiver on the antenna. These include: * Gain curves over frequency band * Noise temp...
SkyFreq: Sky Frequency of the center of the observing band For each GBT backend, the observer generally is concerned with placing the frequency of interest in the...
Software WBS for KFPA Reference Documentation * Example WBS's from the DSS project: * https://staff.nrao.edu/wiki/bin/view/GB/DssSoftwareWbs (current)...
Main.BobSimon 04 Nov 2008 Date: 10/28/2008, Simon From Langston's GBT observations ,we are trying to understand why Glen reported higher than expected system temp...
* System Specifications: Word Document * IFsystemLoss.pdf: 28 Aug 2007, Calculates required front end gain * KFPABeamSpacing.pdf: 6 Feb 2008, Table of beam ...
First Pixel tests with Feed at offset locations On October 6, 2008 from midnight to 8:00 AM, Steve White, Bob Simon and Glen Langston ran tests of the first pixel...
Thermal Gaps: Two options for thermal gaps are the annular choke and the photonic crystal joint (PCJ). The EVLA annular choke and a PCJ were modeled with the K b...
KFPA Test TKFPA_30: 2010 September 6 The final observing session for KFPA recommissioning had a number of observing goals: * Check the intra beam calibration b...
KFPA Re commissioning Test Reports The KFPA was completed and put on the antenna for pre observing tests on October 13, 2010. Below we summarize the tests made to...
KFPA hardware and software checks during "Shared Risk" observations TKFPA_40, December 15, 2010: Calibration check observations of 3C48 and the Moon Performed Da...
KFPA hardware and software tests TKFPA_75, August 31, 2011: Repeated Spectral line band scans for stability test * Nod observations while telescope stowed du...
KFPA Calibration and Test Observations, continuued KFPA calibration observations are presented for Autumn 2011. The primary calibration observations were made t...
IF Spectrums IDM Type I * spurs.xls: Spreadsheet with IDM Type I output spectrums. IDM Type II The IDM Type II prototype gain flatness was measured by detect...
Useful Old KFPA Links and Documentation * GBT K band Beam Spacing (Receiver Independent) * Actual KFPA Feed and Pointing Offsets * LNA and Receiver Noise...
Prerequisites * A set of typical array observing modes: Project Scientist. * Expected data rates and volumes/scan lengths: Project Scientist. * A def...
Main.StevenWhite 07 Jun 2007 2.2.1 Integrated Downconverter Module (Pixel 1) #8211; The Integrated Downconverter Module will comprise the warm part of the pixel...
Window Types The window material is chosen from the leak rate measurement results, out gassing measurement results, and electrical characteristics as many other r...
K band Phased Array Feed This wiki was co opted from the previous KbandFPA project. To find those links, go to the Old Web Home Overview The intent of this web i...
KPAF Web Preferences The following settings are web preferences of the KPAF web. These preferences overwrite the site level preferences in . and , and can...