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Pysynphot interface control document with the ETC: |
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=ETC-Pysynphot interface:= |
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The ETC will access pysynphot functionality by communicating with a |
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pysynphot TCP server running on the local ETC machine. |
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The ETC application will start the pysynphot server when the |
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application starts up. |
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The ETC will submit requests to the pysynphot server as character |
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strings identical (in most cases) to those used to submit synphot requests. |
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(This item may be revisited for cycle 18, when there is no longer a |
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need to maintain compatibility with synphot syntax.) |
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The ETC will receive responses from the pysynphot server as character |
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strings, typically consisting of numbers and filenames. The exact |
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syntax may vary for each task. |
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The pysynphot server must catch all exceptions raised by the pysynphot |
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code, and return useful error messages to the ETC. |
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The pysynphot server must be able to report the version of pysynphot |
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that it is running. |
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=Pysynphot Functionality= |
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==Requirements for 17.0== |
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(reverse-engineered from what was delivered): |
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Purpose of this release: Support COS ETC |
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Pysynphot builds: 0.3.x |
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Acceptance defined as: COS team accepts ETC regression test results. |
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- Parse a syntactically correct synphot expression to produce a |
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spectrum. The expression may include the following functions: |
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'spec', 'unit', 'box', 'bb', 'pl', 'em', 'icat', |
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'rn', 'z', 'ebmvx', 'band' |
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The spectrum may be specified in the following units: |
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'photlam', 'flam', 'counts', 'vegamag' |
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'fnu', 'photnu', 'abmag', 'stmag', 'obmag', 'jy', 'mjy' |
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and the following wavelength units: |
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Angstroms nm micron mm cm m hz |
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Renormalization may be specified in either |
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'flam' 'vegamag' (see below) |
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Extinction may be specified with the following reddening laws: |
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'gal1', 'gal2', 'gal3', 'smc', 'lmc', 'xgal' |
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Specifically, in the following order: |
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- construct a spectrum by either: |
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- reading it from a text or FITS file, |
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- interpolating it from a supported atlas, |
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- constructing a blackbody, powerlaw, gaussian, or flat spectrum |
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- summing any combination of the above |
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- apply reddening to the spectrum |
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- redshift the spectrum |
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- renormalize the spectrum either: |
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within a Band to a value specified in vegamag, or, |
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within a Box to a value specified in flam |
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- apply reddening to the spectrum (either before or after but not both) |
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- Parse a syntactically correct and complete obsmode string (without |
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parameterized keywords), supported by the current graph and component |
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tables to produce a bandpass. |
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- Multiply a spectrum and a bandpass together to produce an observation, |
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using the binned wavelength set specified in the wavecat.dat file for |
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the obsmode. |
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- Write a spectrum or an observation to a FITS file. |
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- Compute the countrate and effective wavelength of an observation. |
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== Requirements for 17.1==: |
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Purpose of this release: Improve support for COS ETC |
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Pysynphot builds: 0.4.x |
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Acceptance defined as: ETC regression tests pass |
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- Update the graph, component, and thermal component tables. |
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- Show the full file specifications being used in the computation of a |
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bandpass. |
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- Report the version of pysynphot being used. |
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== Requirements for 17.2==: |
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Purpose of this release: Bugfixes & improved robustness to |
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user-supplied spectra |
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Pysynphot builds: 0.4.x |
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Acceptance defined as: ETC regression tests pass |
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== Requirements for 18.0==: |
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Purpose of this release: Support all ETCs |
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Pysynphot builds: 0.6.x |
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{ current regression tests pass & agree with synphot |
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Acceptance defined as: { OR |
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{ instrument teams accept synphot & ETC test results |
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- Support parameterized keywords. |
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- Compute the thermal background for an obsmode that includes support |
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for thermal calculations in the graph table. |
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- Support spectral elements in descending wavelength order(* Or: |
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modify the offending files in CDBS so that they are ascending.) |
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== Requirements for UI for 18.0== |
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Purpose of this release: provide direct access to pysynphot for ETC |
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users to perform analysis related to their ETC requests |
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Pysynphot builds: 0.7.x |
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Acceptance defined as: ?? |
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- All the above functionality via OO UI |
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- Documentation |
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- Tutorial |
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- Plot a spectrum or spectral element |
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- Fully support renormalization in the standard set of units |
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- Make .thermback() a method on an ObsBandpass |
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- Support calcphot.effstim with an Observation.effstim() method that |
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supports the full set of units |
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- Provide capability to modify "refdata" functionality |
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- Provide obsmode capability |
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