The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

Anand Sivaramakrishnan; Peter Tuthill; James P. Lloyd; Alexandra Z. Greenbaum; Deepashri Thatte; Rachel A. Cooper; Thomas Vandal; Jens Kammerer; Joel Sanchez-Bermudez; Benjamin J.S. Pope; Dori Blakely; Loïc Albert; Neil J. Cook; Doug Johnstone; André R. Martel; Kevin Volk; Anthony Soulain; Étienne Artigau; David Lafrenière; Chris J. Willott; Sébastien Parmentier; K. E.Saavik Ford; Barry McKernan; M. Begoña Vila; Neil Rowlands; René Doyon; Mathilde Beaulieu; Louis Desdoigts; Alexander W. Fullerton; Matthew De Furio; Paul Goudfrooij; Sherie T. Holfeltz; Stephanie LaMassa; Michael Maszkiewicz; Michael R. Meyer; Marshall D. Perrin; Laurent Pueyo; Johannes Sahlmann; Sangmo Tony Sohn; Paula Stella Teixeira; Sheng Hai Zheng

doi:10.48550/arXiv.2210.17434

The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

Anand Sivaramakrishnan (Lead / Corresponding author), Peter Tuthill, James P. Lloyd, Alexandra Z. Greenbaum, Deepashri Thatte, Rachel A. Cooper, Thomas Vandal, Jens Kammerer, Joel Sanchez-Bermudez, Benjamin J.S. Pope, Dori Blakely, Loïc Albert, Neil J. Cook, Doug Johnstone, André R. Martel, Kevin Volk, Anthony Soulain, Étienne Artigau, David Lafrenière, Chris J. WillottSébastien Parmentier, K. E.Saavik Ford, Barry McKernan, M. Begoña Vila, Neil Rowlands, René Doyon, Mathilde Beaulieu, Louis Desdoigts, Alexander W. Fullerton, Matthew De Furio, Paul Goudfrooij, Sherie T. Holfeltz, Stephanie LaMassa, Michael Maszkiewicz, Michael R. Meyer, Marshall D. Perrin, Laurent Pueyo, Johannes Sahlmann, Sangmo Tony Sohn, Paula Stella Teixeira, Sheng Hai Zheng

Physics

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Abstract

The James Webb Space Telescope’s Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3-5 μm wavelengths, and a bright limit of ≃4 mag in W2. We describe the NIRISS Aperture Masking Interferometry (AMI) mode to help potential observers understand its underlying principles, present some sample science cases, explain its operational observing strategies, indicate how AMI proposals can be developed with data simulations, and how AMI data can be analyzed. We also present key results from commissioning AMI. Since the allied Kernel Phase Imaging (KPI) technique benefits from AMI operational strategies, we also cover NIRISS KPI methods and analysis techniques, including a new user-friendly KPI pipeline. The NIRISS KPI bright limit is ≃8 W2 (4.6 μm) magnitudes. AMI NRM and KPI achieve an inner working angle of ∼70 mas, which is well inside the ∼400 mas NIRCam inner working angle for its circular occulter coronagraphs at comparable wavelengths.

Original language	English
Publisher	arXiv
Number of pages	30
DOIs	https://doi.org/10.48550/arXiv.2210.17434
Publication status	Published - 8 Nov 2022

Keywords

instrumentation
interferometers – methods
data analysis – techniques
high angular resolution – techniques
direct imaging

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10.48550/arXiv.2210.17434Licence: CC BY

PreprintSubmitted manuscript, 1.73 MBLicence: CC BY

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The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry
Sivaramakrishnan, A. (Lead / Corresponding author), Tuthill, P., Lloyd, J. P., Greenbaum, A. Z., Thatte, D., Cooper, R. A., Vandal, T., Kammerer, J., Sanchez-Bermudez, J., Pope, B. J. S., Blakely, D., Albert, L., Cook, N. J., Johnstone, D., Martel, A. R., Volk, K., Soulain, A., Artigau, É., Lafrenière, D. & Willott, C. J. & 21 others, Parmentier, S., Ford, K. E. S., McKernan, B., Vila, M. B., Rowlands, N., Doyon, R., Beaulieu, M., Desdoigts, L., Fullerton, A. W., De Furio, M., Goudfrooij, P., Holfeltz, S. T., LaMassa, S., Maszkiewicz, M., Meyer, M. R., Perrin, M. D., Pueyo, L., Sahlmann, J., Sohn, S. T., Teixeira, P. S. & Zheng, S. H., 8 Jan 2023, In: Publications of the Astronomical Society of the Pacific. 135, 1043, 20 p., 015003.
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Sivaramakrishnan, A., Tuthill, P., Lloyd, J. P., Greenbaum, A. Z., Thatte, D., Cooper, R. A., Vandal, T., Kammerer, J., Sanchez-Bermudez, J., Pope, B. J. S., Blakely, D., Albert, L., Cook, N. J., Johnstone, D., Martel, A. R., Volk, K., Soulain, A., Artigau, É., Lafrenière, D., ... Zheng, S. H. (2022). The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry. arXiv. https://doi.org/10.48550/arXiv.2210.17434

@techreport{6290021b0817462fa8a34d25a8ef376f,

title = "The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry",

abstract = "The James Webb Space Telescope{\textquoteright}s Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3-5 μm wavelengths, and a bright limit of ≃4 mag in W2. We describe the NIRISS Aperture Masking Interferometry (AMI) mode to help potential observers understand its underlying principles, present some sample science cases, explain its operational observing strategies, indicate how AMI proposals can be developed with data simulations, and how AMI data can be analyzed. We also present key results from commissioning AMI. Since the allied Kernel Phase Imaging (KPI) technique benefits from AMI operational strategies, we also cover NIRISS KPI methods and analysis techniques, including a new user-friendly KPI pipeline. The NIRISS KPI bright limit is ≃8 W2 (4.6 μm) magnitudes. AMI NRM and KPI achieve an inner working angle of ∼70 mas, which is well inside the ∼400 mas NIRCam inner working angle for its circular occulter coronagraphs at comparable wavelengths.",

keywords = "instrumentation, interferometers – methods, data analysis – techniques, high angular resolution – techniques, direct imaging",

author = "Anand Sivaramakrishnan and Peter Tuthill and Lloyd, {James P.} and Greenbaum, {Alexandra Z.} and Deepashri Thatte and Cooper, {Rachel A.} and Thomas Vandal and Jens Kammerer and Joel Sanchez-Bermudez and Pope, {Benjamin J.S.} and Dori Blakely and Lo{\"i}c Albert and Cook, {Neil J.} and Doug Johnstone and Martel, {Andr{\'e} R.} and Kevin Volk and Anthony Soulain and {\'E}tienne Artigau and David Lafreni{\`e}re and Willott, {Chris J.} and S{\'e}bastien Parmentier and Ford, {K. E.Saavik} and Barry McKernan and Vila, {M. Bego{\~n}a} and Neil Rowlands and Ren{\'e} Doyon and Mathilde Beaulieu and Louis Desdoigts and Fullerton, {Alexander W.} and Furio, {Matthew De} and Paul Goudfrooij and Holfeltz, {Sherie T.} and Stephanie LaMassa and Michael Maszkiewicz and Meyer, {Michael R.} and Perrin, {Marshall D.} and Laurent Pueyo and Johannes Sahlmann and Sohn, {Sangmo Tony} and Teixeira, {Paula Stella} and Zheng, {Sheng Hai}",

year = "2022",

month = nov,

day = "8",

doi = "10.48550/arXiv.2210.17434",

language = "English",

publisher = "arXiv",

type = "WorkingPaper",

institution = "arXiv",

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Sivaramakrishnan, A, Tuthill, P, Lloyd, JP, Greenbaum, AZ, Thatte, D, Cooper, RA, Vandal, T, Kammerer, J, Sanchez-Bermudez, J, Pope, BJS, Blakely, D, Albert, L, Cook, NJ, Johnstone, D, Martel, AR, Volk, K, Soulain, A, Artigau, É, Lafrenière, D, Willott, CJ, Parmentier, S, Ford, KES, McKernan, B, Vila, MB, Rowlands, N, Doyon, R, Beaulieu, M, Desdoigts, L, Fullerton, AW, Furio, MD, Goudfrooij, P, Holfeltz, ST, LaMassa, S, Maszkiewicz, M, Meyer, MR, Perrin, MD, Pueyo, L, Sahlmann, J, Sohn, ST, Teixeira, PS & Zheng, SH 2022 'The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry' arXiv. https://doi.org/10.48550/arXiv.2210.17434

TY - UNPB

T1 - The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

AU - Sivaramakrishnan, Anand

AU - Tuthill, Peter

AU - Lloyd, James P.

AU - Greenbaum, Alexandra Z.

AU - Thatte, Deepashri

AU - Cooper, Rachel A.

AU - Vandal, Thomas

AU - Kammerer, Jens

AU - Sanchez-Bermudez, Joel

AU - Pope, Benjamin J.S.

AU - Blakely, Dori

AU - Albert, Loïc

AU - Cook, Neil J.

AU - Johnstone, Doug

AU - Martel, André R.

AU - Volk, Kevin

AU - Soulain, Anthony

AU - Artigau, Étienne

AU - Lafrenière, David

AU - Willott, Chris J.

AU - Parmentier, Sébastien

AU - Ford, K. E.Saavik

AU - McKernan, Barry

AU - Vila, M. Begoña

AU - Rowlands, Neil

AU - Doyon, René

AU - Beaulieu, Mathilde

AU - Desdoigts, Louis

AU - Fullerton, Alexander W.

AU - Furio, Matthew De

AU - Goudfrooij, Paul

AU - Holfeltz, Sherie T.

AU - LaMassa, Stephanie

AU - Maszkiewicz, Michael

AU - Meyer, Michael R.

AU - Perrin, Marshall D.

AU - Pueyo, Laurent

AU - Sahlmann, Johannes

AU - Sohn, Sangmo Tony

AU - Teixeira, Paula Stella

AU - Zheng, Sheng Hai

PY - 2022/11/8

Y1 - 2022/11/8

N2 - The James Webb Space Telescope’s Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3-5 μm wavelengths, and a bright limit of ≃4 mag in W2. We describe the NIRISS Aperture Masking Interferometry (AMI) mode to help potential observers understand its underlying principles, present some sample science cases, explain its operational observing strategies, indicate how AMI proposals can be developed with data simulations, and how AMI data can be analyzed. We also present key results from commissioning AMI. Since the allied Kernel Phase Imaging (KPI) technique benefits from AMI operational strategies, we also cover NIRISS KPI methods and analysis techniques, including a new user-friendly KPI pipeline. The NIRISS KPI bright limit is ≃8 W2 (4.6 μm) magnitudes. AMI NRM and KPI achieve an inner working angle of ∼70 mas, which is well inside the ∼400 mas NIRCam inner working angle for its circular occulter coronagraphs at comparable wavelengths.

AB - The James Webb Space Telescope’s Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3-5 μm wavelengths, and a bright limit of ≃4 mag in W2. We describe the NIRISS Aperture Masking Interferometry (AMI) mode to help potential observers understand its underlying principles, present some sample science cases, explain its operational observing strategies, indicate how AMI proposals can be developed with data simulations, and how AMI data can be analyzed. We also present key results from commissioning AMI. Since the allied Kernel Phase Imaging (KPI) technique benefits from AMI operational strategies, we also cover NIRISS KPI methods and analysis techniques, including a new user-friendly KPI pipeline. The NIRISS KPI bright limit is ≃8 W2 (4.6 μm) magnitudes. AMI NRM and KPI achieve an inner working angle of ∼70 mas, which is well inside the ∼400 mas NIRCam inner working angle for its circular occulter coronagraphs at comparable wavelengths.

KW - instrumentation

KW - interferometers – methods

KW - data analysis – techniques

KW - high angular resolution – techniques

KW - direct imaging

U2 - 10.48550/arXiv.2210.17434

DO - 10.48550/arXiv.2210.17434

M3 - Preprint

BT - The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

PB - arXiv

ER -

The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

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Keywords

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The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

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