JWST's NIRISS Single-Object Slitless Spectroscopy (SOSS) imaging template, available in the Astronomer’s Proposal Tool (APT ), has parameters for specifying and scheduling observations.
The NIRISS Single-Object Slitless Spectroscopy (SOSS) template is used for the SOSS mode of NIRISS, and this article describes allowed values for all parameters. Advice on how to choose values which optimize your science can be found in the NIRISS Single-Object Slitless Spectroscopy APT Template.
The NIRISS SOSS template
consists of the following parameters:
|assign observation number|
|Observation Label||provide observation label||text||optional|
|provide observation comments||text||optional|
|select Target Name||choose from list||from Target List|
|specify ETC Workbook Calculation ID||number||for science exposures (optional) and target acquisition exposures|
|specify special requirements||choose from list||if needed|
|Template Specific Information|
|Target Acquisition Exposure|
|select acquisition target|
choose from list
|Acquisition Filter||default value||F480M|
|select acquisition mode|
|select acquisition readout pattern|
|select number of groups per integration|
choose from list
choose from list
|select readout pattern|
choose from list
|specify number of groups per integration|
|specify number of integrations per exposure|
Note for developer: This template cannot be used in parallel and cannot have parallels attached to it; the NO PARALLEL special requirement should be added. The TIME SERIES OBSERVATION special requirement should also be added.
Target Acquisition Exposure
If an offset star is to be used for the target acquisition observation, select the ACQUISITION TARGET [TACQ TARGET] from the list of targets previously entered. When the science target is a Solar System target, the acquisition target MUST be the science target. Or, if no target acquisition is needed, select ACQUISITION TARGET to be NONE; the latter option is only allowed if SUBARRAY is FULL (see Subarray ).
Note for developers: For APT, the ACQUISITION TARGET name field should always be present, but should be defaulted to the SAME TARGET AS OBSERVATION.
Note for developers: If the acquisition target is different from the science target, APT should provide an error if the distance between the ACQ and Science targets is greater than the Visit splitting distance found in the PRD. Also, if there are multiple pointings within a visit, then the rules have to apply to the greatest separation between acq target and pointing within the visit.
Note for developers: If the observation target is a fixed target, remove solar system targets from the acquisition target options. If the observation target is a Solar system target, remove all options from the acquisition target list except for the observation target and NONE.
The Target Acquisition FILTER is F480M.
ACQUISITION MODE [TACQ MODE] = SOSSBRIGHT, SOSSFAIN
This field specifies the target acquisition mode to be used to obtain the acquisition data for a “bright” or “faint” target. In this context, "bright" refers to M-band magnitudes in the range 3.0 ≤ M ≤ 6.1 (in the Vegamag system), while "faint" refers to 6.1 ≤ M ≤ 14.5.
Acquisition Readout Pattern
READOUT PATTERN [TACQ PATTERN] = NIS, NISRAPI
This field specifies the readout pattern to be used to obtain the acquisition data.
Note for developer: The NIS option is only available when TACQ MODE = SOSSFAINT.
Acquisition Number of Groups/Integration
NUMBER OF GROUPS/INTEGRATION [TACQ NGROUPS] = 3, 5, 7, 9, 11, 13, 15, 17, 19
This parameter specifies the number of groups in an integration. Note that the NUMBER OF INTEGRATIONS/EXPOSURE is set to 1 for target acquisition observations.
For each exposure specify the SUBARRAY, READOUT PATTERN, NUMBER OF GROUPS/INTEGRATION, and NUMBER OF INTEGRATIONS/EXPOSURE.
Note developers: there is only 1 exposure allowed in an observation.
SUBARRAY [SUBARRAY] = SUBSTRIP256 (default), SUBSTRIP96, FULL
This parameter specifies the region of the SCA detector that is to be read out. For more details about these subarrays,
READOUT PATTERN [READOUT PATTERN] = NISRAPID (default), NIS
This field specifies the readout pattern to be used to obtain the SOSS science data. Note that NIS is only available when SUBARRAY = FULL.
Number of Groups/Integration
NUMBER OF GROUPS/INTEGRATION [NGROUPS] specifies the number of groups in each integration. For readout pattern NIS, the range is 1-200, while for NISRAPID the range is 1-30
Number of Integrations/Exposure
NUMBER OF INTEGRATIONS/EXPOSURE [NINTS] field specifies the number of times the integration is repeated. The range is 1-65535.
Note that the following parameters have only one option, and are therefore not included in the template:
The initial version of this chapter was provided by Lily Liu.
Version 7 (April 18, 2019)
- Editorial change (moved change log to main article).
Version 6 (December 21, 2018)
- PROPINSTJWST-91122 - Added developer note in Acquisition Target section restricting acquisition target options for fixed vs. solar system observations.
Version 5 (December 27, 2017)
- PR 89483 - added restriction on Acq Target for SS observations
- PR 88411 - added developer note about TSO and NO PARALLEL requirements
Version 4 (November 15, 2017)
- PR 87895 - updated Exposure field labels to Groups/Integration and Integrations/Exposure
- PR 87961 - updated TA Readout Pattern options to include NIS
- PR 87198 - added note that NIS is only available when SUBARRAY=FULL
- PR 88816 - updated text for Acquisition Mode
Version 3 (February 21, 2017)
PR 87071 - removed mosaics option
Version 2 (December 20, 2016)
- PR 85863 - updated developer note for Acquisition Target
- PR 85608 - removed statement about Acq Flux, and added new section to state default Acq Filter
Version 1 (March 29, 2016)
This is the converted Word File from Chapter 42.
Other NIRISS Science Templates:
Other Spectroscopic Templates:
NIRISS Engineering Templates:
JWST NIRISS Single-Object Slitless Spectroscopy Template
JWST NIRISS Single-Object Slitless Spectroscopy template parameters