Nomenclature for JWST MULTIACCUM Detector Integrations Table 5-2 from MOCD: Common Lexicon of Terms for Detector Readouts CLOCK To address a particular.

Slides:



Advertisements
Similar presentations
Methods of Enumeration Counting tools can be very important in probability … particularly if you have a finite sample space with equally likely outcomes.
Advertisements

16 January 2003STScI TIPS1 JWST's Near-Infrared Detectors: Ultra-Low Background Operation and Testing Bernie Rauscher, Don Figer, Mike Regan, Sito Balleza,
Shuvra Das University of Detroit Mercy
Discussion of CalWebb contents M. Robberto (facilitator)
CS61C L21 State Elements : Circuits that Remember (1) Spring 2007 © UCB 161 Exabytes In 2006  In 2006 we created, captured, and replicated 161 exabytes.
Detectors for the JWST Near Infrared Spectrograph (NIRSpec) B.J. Rauscher 1, P. Strada 2, M.W. Regan 3, D.F. Figer 3, P. Jakobsen 2, S.H. Moseley 1, T.
Software Design Project
4.1 Chapter 4 Digital Transmission Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
1 Ultra low background characterization of Rockwell Scientific MBE HgCdTe arrays Donald N. B. Hall, University of Hawaii, Institute for Astronomy, Honolulu,
McGraw-Hill©The McGraw-Hill Companies, Inc., 2004 Chapter 4 Digital Transmission.
Light to Electricity: lines begin and end in black (low signal level) called Blanking between blanking is the active video scanning is precisely controlled.
1D or 2D array of photosensors can record optical images projected onto it by lens system. Individual photosensor in an imaging array is called pixel.
A/D Conversion No. 1  Seattle Pacific University Analog to Digital Conversion Based on Chapter 5 of William Stallings, Data and Computer Communication.
Random signals. Histogram of the random signal Continuous Time Sinusoidal signals.
Analyzing Data Chapter 2.
Digital Images Chapter 8 Exploring the Digital Domain.
CS3350B Computer Architecture Winter 2015 Lecture 5.2: State Circuits: Circuits that Remember Marc Moreno Maza [Adapted.
Analyzing Data Chapter 2. Units & Measurement – section 1  Chemists use an internationally recognized system of units to communicate their findings.
Photon Transfer Method 1. Using two identical flat field exposures it is possible to measure the read noise of a CCD with the Photon Transfer method. Two.
6e-1 Science Data Products Daryl Swade DMS Systems Engineer S&OC System Design Review #1.
Unit 14 Derivation of State Graphs
Data Management Subsystem Jeff Valenti (STScI). DMS Context PRDS - Project Reference Database PPS - Proposal and Planning OSS - Operations Scripts FOS.
CMPD273 Multimedia System Prepared by Nazrita Ibrahim © UNITEN2002 Multimedia System Characteristic Reference: F. Fluckiger: “Understanding networked multimedia,
©Brooks/Cole, 2003 Chapter 2 Data Representation.
JWST NIRSpec Dithering Strategies (and a Cross-SI View) Jason Tumlinson JIM / TIPS Oct 15, 2009.
Detectors for Light Sources Contribution to the eXtreme Data Workshop of Nicola Tartoni Diamond Light Source.
Digital Imaging. Digital image - definition Image = “a two-dimensional function, f(x,y), where x and y are spatial coordinates, and the amplitude of f.
Coding the JWST Calibration Pipeline(s) 2010 Calibration Workshop Robert Jedrzejewski/STScI.
JWST Calibration Error Budget Jerry Kriss. 15 March 20072/14 JWST Flux & Wavelength Calibration Requirements SR-20: JWST shall be capable of achieving.
4.1 Chapter 4 Digital Transmission Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 1 Section 3 Measurement. Objectives and Questions.
Chapter 2 Fundamentals of Data and Signals
Transiting Exoplanet Working Group Nikole K. Lewis STScI 10/20/2015.
Glow Experiment Outline Brandon Hanold. Outline 1.Glow Description 2.Experiment Design 3.Acquisition Loop Variables and Keywords 4.Reduction Results 5.Reduction.
APT Overview for Transiting Exoplanet Proposals Chris Moriarty – APT Developer.
NIRISS Science Team Meeting Oct 2015 NIRISS Activities in CV3 André Martel.
Multiplexors Decoders  Decoders are used for forming separate signals for different combination of input signals.  The multiplexer circuit is a digital.
CCD Image Processing: Issues & Solutions. CCDs: noise sources dark current –signal from unexposed CCD read noise –uncertainty in counting electrons in.
1 Neutron Monitor Workshop 2(B): Neutron Monitor Digital Electronics Mahidol University June 26, 2009 Paul Evenson University of Delaware Cosray at McMurdo.
Pulse Code Modulation (PCM) Analog voice data must be translated into a series of binary digits before they can be transmitted. With Pulse Code Modulation.
DEPARTMENT OF ELECTRONICS AND COMMUNICATION ENGG.
Data Reduction Schemes for MicroBoone Wu, Jinyuan Fermilab.
Single Object Spectroscopy and Time Series Observations with NIRSpec
NIRCam Readout Pattern Considerations
Introduction to the Astronomer’s Proposal Tool (APT)
NIRSpec Time Series Observations
Quantum Array Detectors
Chapter 4. Digital Transmission
Observing Strategies and Constraints
Imaging with the James Webb Space Telescope
JWST Pipeline Overview
JWST NIRCam Time Series Observations
Detectors of JWST Near IR Instruments
Transmission Modes The term transmission mode to refer to the manner in which data is sent over the underlying medium Transmission modes can be divided.
S-D analog to digital conversion
The JWST Exposure Time Calculator
FITS Header Keywords for ground test data
FlowArm PLTW Programming
JWST Overheads Jeff Valenti S&OC Mission Scientist
ESAC 2017 JWST Workshop JWST User Documentation Hands on experience
DIGITAL DATA COMMUNICATION TECHNIQUES
Σ-D Analog to Digital Converter for CMOS Image Sensors Nonu Singh (RIT, MicroE Co-Op) Background After fabricating an imaging sensor it needs to be characterized.
Inst.eecs.berkeley.edu/~cs61c CS61C : Machine Structures Lecture #21 State Elements: Circuits that Remember Hello to James Muerle in the.
DIGITAL DATA COMMUNICATION TECHNIQUES
Detector Parameters Marco Sirianni - ESA.
DIGITAL DATA COMMUNICATION TECHNIQUES
Data Representation Chapter 2 Computer HW (Von Neumann Model) Program
Instructor: Alexander Stoytchev
Instructor: Michael Greenbaum
Introduction Communication Modes Transmission Modes
Presentation transcript:

Nomenclature for JWST MULTIACCUM Detector Integrations Table 5-2 from MOCD: Common Lexicon of Terms for Detector Readouts CLOCK To address a particular pixel. “ Clock ” is a verb. READ To clock and digitize pixels in an SCA. “ Read ’ is a verb. SAMPLEThe result of a single Analog to Digital conversion. DWELLSample a pixel multiple times before clocking to the next pixel. nsampleThe number of A/D samples per pixel. FRAMEThe result of sequentially clocking and digitizing all pixels in a rectangular area of an SCA. "Full-fame readout" means to digitize all pixels in an SCA, including reference pixels. “ Frame ” also applies to the result of clocking and digitizing a subarray on an SCA. GROUPOne or more consecutively read frames. There are no intervening resets. Frames may be averaged to form a group. nframeThe number of FRAMES per GROUP. For some SI readout patterns the frames in the group are coadded. INTEGRATIONThe end result of resetting the detector and then non-destructively sampling it one or more times over a finite period of time before resetting the detector again. This is a unit of data for which signal is proportional to intensity, and it consists of one or more GROUPS. ngroupThe number of GROUPS in an INTEGRATION. GroupgapThe number of frames skipped between groups. INTEGRATION TIMEThe time elapsed between when a pixel is first read and when it is last read in an INTEGRATION. This time interval is the time relevant for scientific analysis. Using the time variables, the integration time is t int = ngroup  t group. EXPOSUREThe end result of one or more INTEGRATIONS over a finite period of time. EXPOSURE defines the contents of a single FITS file. nintThe number of INTEGRATIONS in an EXPOSURE. For nint=1 EXPOSURE is equivalent to an INTEGRATION. EXPOSURE TIMEThe total time during an exposure spent accumulating signal from a source. The total elapsed time in an exposure is longer due to readout overheads at the end of each integration period. TOTAL ELAPSED TIME The total elapsed time during an exposure, or the “ wall clock ” time. The TOTAL ELAPSED TIME is the time interval from when the first pixel is read in the first integration to when the last pixel is read in the last integration in an exposure. Note that the actual elapsed time in an INTEGRATION is slightly longer, and it depends on the number and spacing of samples in the INTEGRATION. The extra readout overhead in the total elapsed time is nframe x t frame Unit of a.fits file

Nomenclature for JWST MULTIACCUM Detector Integrations Integration time = n group x t group Exposure time = n int x t int Group gap Averaged groups of nf are sent to SSR Data cube (x, y, t)

JWST MULTIACCUM Detector Integrations Instruments teams have pre-defined detector readout patterns (e.g., combinations of nframes, group gaps are set - users will never define new readout patterns) Instruments have set detector readout patterns: –TFI: TFIRAPID / TFI –NIRSpec: NRSRAPID / NRS / NRSSlow –MIRI: FASTMode-Short/Long, SLOWMode –NIRCam - 9 readout patterns (Rapid/Fast = no dropped frames, tframe=tgroup = MAX data volume) User Delivered exposure times will be quantized in units of the detector read group time