MIRI MRS Simultaneous Imaging

Simultaneous use of the JWST MIRI imager and the medium resolution spectrometer (MRS) modes is offered for all observations where the MRS is the primary observing mode. Astrometry of stars in the imager field will result in more accurate data cube construction.

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Main article: MIRI Medium-Resolution Spectroscopy
See also: MIRI Imaging 

The MIRI imager can be used for mid-infrared imaging simultaneously with the MIRI medium resolution spectrometer. This is referred to as "simultaneous imaging." It is the default operational mode for MRS observations, and is highly recommended that simultaneous imaging be specified for all MRS observations as there are no data volume issues when using the imager and the MRS simultaneously; MRS observations cannot be part of coordinated parallels with other instruments (see the list of coordinated parallel options). Therefore, the only instance where simultaneous imaging should be turned off is if saturation of the imager would occur due to a long MRS observation or if a bright target is in the imager field of view.

MIRI simultaneous imaging is not considered a parallel imaging mode.



Purpose

Since the MIRI MRS has an extremely small field of view (FOV), its absolute astrometric solution cannot always be tied to an external reference frame using MRS data alone. If data are taken without a prior target acquisition observation (for instance, when mapping an extended, diffuse source) the absolute astrometry of a given visit may be in error by 0.5" or more. This poses a challenge to combining exposures across multiple different visits, and also for comparing source locations against extant multi-wavelength data. The simultaneous imaging mode helps to alleviate this problem by obtaining data across the much larger MIRI imaging field of view that can be used offline (in combination with the well-known relation between the imaging and MRS fields) to improve the astrometric solution of individual MRS exposures by cross-matching multiple sources in the imaging field against known catalog positions.

Science applications 

Simultaneous imaging can also be used to obtain additional science observations of an extended object. For example, MRS observations of a small portion of a nebula can be complemented by simultaneous imaging of adjacent regions of the nebula (depending on the roll of the observatory, which is significantly constrained for JWST). Figure 1 shows the spacing and orientation of the imager and MRS FOVs. Specific examples of simultaneous imaging science applications can be found in the descriptions of the GTO and ERS programs.

Figure 1. Spacing and orientation of the imager and MRS FOVs

Image from the Aladdin viewer in APT of the MIRI imager FOV (large rectangle) and the MRS FOVs for each channel (off the top right corner of the MIRI imager FOV).


Selecting simultaneous imaging in APT

See also: MIRI MRS APT TemplateMIRI Medium Resolution Spectroscopy Template Parameters

Figure 2 shows how to select simultaneous imaging when MIRI Medium Resolution Spectroscopy1 is selected as the primary observing template.

MRS parameters cannot be specified when MIRI Imaging is selected as the primary observing template.

Figure 2. Selecting simultaneous imaging in the MIRI Medium Resolution Spectroscopy APT template

In the MIRI Medium Resolution Spectroscopy APT observation template's MRS Parameters panel, select YES or NO under the Simultaneous Imaging drop-down menu. The default, and recommended selection, is YES. All MIRI imaging subarray options are available under the Imager Subarray drop-down menu.

Selecting multiple simultaneous imaging filters

See also: MIRI Filters and Dispersers

A different imaging filter can be selected for each exposure in a given observation. For instance, if an observation contained three exposures (one each for the MRS Wavelength Ranges SHORT, MEDIUM, and LONG, thereby covering the entire MRS wavelength range), then simultaneous imaging could correspondingly be obtained in three different filters.

Long wavelength filter warning

Selecting the F1280W, F1500W, F1800W, F2100W, or F2550W filters for simultaneous imaging will result in the following warning message: "Warning (Form): Imager Filter overlap." This is due to the large size of the PSF FWHM in those filters compared to the smallest of the MRS dither patterns; executing a small dither for the MRS will result in the PSFs of point sources in the imager overlapping between subsequent exposures, which can be problematic when performing image subtraction.

Simultaneous imaging and target acquisition

See also: MIRI MRS Target AcquisitionMIRI Imaging Target AcquisitionMIRI Detector Subarrays

MRS target acquisition (TA) uses the FULL subarray of the MIRI imager. If TA is selected, the FULL imager subarray should also be selected for simultaneous imaging (Fig. 2), otherwise APT will generate a warning that the imager data quality may be adversely affected. If no MRS TA is selected (option available starting in APT 25.4.2), there is no restriction on the subarray mode available for simultaneous imaging.

Simultaneous imaging overheads

See also: MIRI Overheads

If simultaneous imaging is selected, there will be an additional small overhead for each dither position. For example, if a 4-point dither is selected, and observations are set up with all three Wavelength Ranges, this results in 12 dithers and each of those dithers incurs its own small overhead.

Bold italics style indicates words that are also parameters or buttons in software tools like the APT and ETC. Similarly, a bold style represents menu items and panels.




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Latest updates
  •   
    Updated Figure 1 to match APT 27.0.1 and removed Figure 2

  •  
    Updated exposure creation for multiple filters, and for no-TA options in APT 25.4.2.
    Figures replaced to match APT 25.4.2.