Pure Parallel Observations
JWST allows for separate proposals of only pure parallel observations, which are specified via select observing templates available in the Astronomer’s Proposal Tool (APT).
Purple text indicates the parameter is Limited Access.
Boldface italics type indicates the name of an APT parameter or a value for a parameter.
Red text indicates restrictions on a parameter.
Black text indicates an important note.
Brown text indicates notes for the developers.
Green text indicates the name of the parameter used by Commanding.
Items in brackets - <value> - are required values.
Items in square brackets - [<value>] - are optional.
Science pure parallel proposals do not follow JWST's standard single stream process. In the initial proposal, only example observations are specified in APT. After the proposal is approved, Pure parallel observations are crafted by the observer based on their example observations and sized to fit the pure parallel slots assigned to them.
Calibration pure parallel observations are crafted by the scheduling system to meet the requirements of their example observations.
Pure parallel slots are defined by STScI at the beginning of the observing cycle based on the contents of the approved pool of proposals whose exposures will serve as the primary observations. Each slot corresponds to a single exposure (i.e. a single dither position). Approved pure parallel observations are paired with these pure parallel slots and are then scheduled simultaneously with and according to the plan windows of the original primary visits. The pure parallel observing mode is used for science as well as calibration observing.
Note that currently the pool of pure parallel slots are only created from observations using the following templates:
- MIRI Imaging
- MIRI LRS (with FULL subarray)
- MIRI MRS
- NIRCam Imaging
- NIRCam WFSS
- NIRISS Imaging
- NIRISS WFSS
- NIRSpec Fixed Slit
- NIRSpec IFU
- NIRSpec MOS
Science Pure Parallel Proposals
To propose for science pure parallel observing, check the PURE PARALLEL PROPOSAL box on the Proposal Information form. Because pure parallel observations do not drive the pointing of the telescope, this will modify APT forms in the following ways:
- The target section is removed from the proposal.
- All templates selected will have the target automatically set to PARALLEL.
- There are no options for dithering in the observing templates.
Science Pure Parallel Observation Limitations
- Currently only four templates can be proposed for science pure parallel observing: MIRI Imaging, NIRCam Imaging, NIRISS Imaging and NIRISS WFSS.
- As with NIRCam coordinated parallel observing, certain readout modes are restricted for pure parallel observing because of data rates.
- There can only be one exposure specification in a pure parallel observation.
- EXPOSURES/DITHER must be set to 1.
- No special requirements may be specified for a science pure parallel observation.
- Some NIRCam readout patterns cannot be used with parallel observations because of data rate limitations.
- RAPID and BRIGHT2 cannot be used at any time (NIRCam prime or parallel)
- BRIGHT1 can only be used if MODULE is not ALL (NIRCam prime or parallel)
Approved Science Pure Parallel Programs
Once the TAC has approved one or more science pure parallel programs, there will be a process to divide up the available pure parallel slots between the approved science pure parallel programs and the expected needs of the calibration pure parallel suite of proposals. Once a science pure parallel program is approved and marked as such in the database the following changes will occur in the APT forms:
- A new section called "Pure Parallel Slots" will be added to the proposal. This allows the user to review the slots assigned to their proposal, sort them in various ways and create parallel slot groups. The slots in a group are similar enough that a single observation definition can be used for all of them.
- A new field called "Parallel Slot Group" will be added to the observations. This allows the user to select a parallel group. For each slot in the selected group a visit will be created using those observation parameters.
Calibration Pure Parallels
Calibration Pure Parallels are calibration observations with the PARALLEL special requirement. Templates that allow (or require) the PARALLEL special requirement are listed in Parallel and No Parallel Special Requirement Rules.
November 16, 2022
- PROPINSTJWST-91525 Added link to Par/NoPar rules in Calibration Pure Parallels section.
Version 5 (July 13, 2021)
Version 4 (June 24, 2019)
PROPINSTJWST-91352 - Added BRIGHT2 limitation to Science Pure Parallel Observation Limitations section.
Version 3 (April 16, 2019)
- Editorial change (moved change log to main article).
Version 2 (June 19, 2018)
- PR 89938 - added NIRCam readout patterns to Limitations section
Version 1 (February 8, 2018)
This is the initial version.