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).

Introduction

 Format definitions...

Purple text indicates the parameter is Limited Access.

Boldface italics type indicates the name of an APT parameter or a value for a parameter.

(warning)Red text indicates restrictions on a parameter.

(red star) 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 at the beginning of the observing cycle based on the exposures of supported primary visits. (Currently there are four observing templates which are allowed to have pure parallels attached: MIRI Imaging, NIRCam Imaging, NIRSpec MOS, and NIRISS Imaging.) Each slot corresponds to a single exposure (i.e. a single dither position).

 Approved pure parallel observations are paired with pure parallel slots and are scheduled simultaneously with and according to the plan windows of those primary visits. The pure parallel observing mode is used for science as well as calibration observing.

 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 are legal 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 will be listed below.

Change log

 Click here to expand...

General notes

none

Change log

Version 4 (June 24, 2019)

PROPINSTJWST-91352 - Added BRIGHT2 limitation to Science Pure Parallel Observation Limitations section.


Version 3 (April 16, 2019)

  1. Editorial change (moved change log to main article).


Version 2 (June 19, 2018)

  1. PR 89938 - added NIRCam readout patterns to Limitations section


Version 1 (February 8, 2018)

This is the initial version.