The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities

Quinn M. Konopacky; Ashley D. Baker; Dimitri Mawet; Michael P. Fitzgerald; Nemanja Jovanovic; Charles Beichman; Garreth Ruane; Rob Bertz; Hiroshi Terada; Richard Dekany; Larry Lingvay; Marc Kassis; David Anderson; Motohide Tamura; Björn Benneke; Thomas Beatty; Tuan Do; Shogo Nishiyama; Peter Plavchan; Jason Wang; Ji Wang; Adam Burgasser; Jean Baptiste Ruffio; Huihao Zhang; Aaron Brown; Jason Fucik; Aidan Gibbs; Rose Gibson; Sam Halverson; Christopher Johnson; Sonia Karkar; Takayuki Kotani; Evan Kress; Stephanie Leifer; Kenneth Magnone; Jerome Maire; Rishi Pahuja; Michael Porter; Mitsuko Roberts; Ben Sappey; Jim Thorne; Eric Wang; Étienne Artigau; Geoffrey A. Blake; Gabriela Canalizo; Guo Chen; Greg Doppmann; René Doyon; Courtney Dressing; Min Fang; Thomas Greene; Greg Herczeg; Lynne Hillenbrand; Andrew Howard; Stephen Kane; Tiffany Kataria; Eliza Kempton; Heather Knutson; David Lafrenière; Chao Liu; Stanimir Metchev; Max Millar-Blanchaer; Norio Narita; Gajendra Pandey; S. P. Rajaguru; Paul Robertson; Colette Salyk; Bun'ei Sato; Evertt Schlawin; Sujan Sengupta; Thirupathi Sivarani; Warren Skidmore; Gautam Vasisht; Chikako Yasui; Hui Zhang

doi:10.1117/12.2681522

The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities

Quinn M. Konopacky, Ashley D. Baker, Dimitri Mawet, Michael P. Fitzgerald, Nemanja Jovanovic, Charles Beichman, Garreth Ruane, Rob Bertz, Hiroshi Terada, Richard Dekany, Larry Lingvay, Marc Kassis, David Anderson, Motohide Tamura, Björn Benneke, Thomas Beatty, Tuan Do, Shogo Nishiyama, Peter Plavchan, Jason WangJi Wang, Adam Burgasser, Jean Baptiste Ruffio, Huihao Zhang, Aaron Brown, Jason Fucik, Aidan Gibbs, Rose Gibson, Sam Halverson, Christopher Johnson, Sonia Karkar, Takayuki Kotani, Evan Kress, Stephanie Leifer, Kenneth Magnone, Jerome Maire, Rishi Pahuja, Michael Porter, Mitsuko Roberts, Ben Sappey, Jim Thorne, Eric Wang, Étienne Artigau, Geoffrey A. Blake, Gabriela Canalizo, Guo Chen, Greg Doppmann, René Doyon, Courtney Dressing, Min Fang, Thomas Greene, Greg Herczeg, Lynne Hillenbrand, Andrew Howard, Stephen Kane, Tiffany Kataria, Eliza Kempton, Heather Knutson, David Lafrenière, Chao Liu, Stanimir Metchev, Max Millar-Blanchaer, Norio Narita, Gajendra Pandey, S. P. Rajaguru, Paul Robertson, Colette Salyk, Bun'ei Sato, Evertt Schlawin, Sujan Sengupta, Thirupathi Sivarani, Warren Skidmore, Gautam Vasisht, Chikako Yasui, Hui Zhang

Steward Observatory

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

4 Scopus citations

Abstract

HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R 100,000 spectroscopy between 0.98 – 2.5 µm, HISPEC will enable spectroscopy of transiting and non-transiting exoplanets in close orbits, direct high-contrast detection and spectroscopy of spatially separated substellar companions, and exoplanet dynamical mass and orbit measurements using precision radial velocity monitoring calibrated with a suite of state-of-the-art absolute and relative wavelength references. MODHIS is the counterpart to HISPEC for the Thirty Meter Telescope and is being developed in parallel with similar scientific goals. In this proceeding, we provide a brief overview of the current design of both instruments, and the requirements for the two spectrographs as guided by the scientific goals for each. We then outline the current science case for HISPEC and MODHIS, with focuses on the science enabled for exoplanet discovery and characterization. We also provide updated sensitivity curves for both instruments, in terms of both signal-to-noise ratio and predicted radial velocity precision.

Original language	English (US)
Title of host publication	Techniques and Instrumentation for Detection of Exoplanets XI
Editors	Garreth J. Ruane
Publisher	SPIE
ISBN (Electronic)	9781510665743
DOIs	https://doi.org/10.1117/12.2681522
State	Published - 2023
Event	Techniques and Instrumentation for Detection of Exoplanets XI 2023 - San Diego, United States Duration: Aug 21 2023 → Aug 24 2023

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	12680
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Techniques and Instrumentation for Detection of Exoplanets XI 2023
Country/Territory	United States
City	San Diego
Period	8/21/23 → 8/24/23

Keywords

Exoplanet atmospheres (487)
Exoplanet detection methods (489)
Exoplanets (498)
High resolution spectroscopy (2096)
Infrared astronomy (786)
Radial velocities (1332)
Spectrometers (1554)
Spectropolarimetry (1556)

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2681522

Cite this

Konopacky, Q. M., Baker, A. D., Mawet, D., Fitzgerald, M. P., Jovanovic, N., Beichman, C., Ruane, G., Bertz, R., Terada, H., Dekany, R., Lingvay, L., Kassis, M., Anderson, D., Tamura, M., Benneke, B., Beatty, T., Do, T., Nishiyama, S., Plavchan, P., ... Zhang, H. (2023). The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities. In G. J. Ruane (Ed.), Techniques and Instrumentation for Detection of Exoplanets XI Article 1268007 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12680). SPIE. https://doi.org/10.1117/12.2681522

The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities. / Konopacky, Quinn M.; Baker, Ashley D.; Mawet, Dimitri et al.
Techniques and Instrumentation for Detection of Exoplanets XI. ed. / Garreth J. Ruane. SPIE, 2023. 1268007 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12680).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Konopacky, QM, Baker, AD, Mawet, D, Fitzgerald, MP, Jovanovic, N, Beichman, C, Ruane, G, Bertz, R, Terada, H, Dekany, R, Lingvay, L, Kassis, M, Anderson, D, Tamura, M, Benneke, B, Beatty, T, Do, T, Nishiyama, S, Plavchan, P, Wang, J, Wang, J, Burgasser, A, Ruffio, JB, Zhang, H, Brown, A, Fucik, J, Gibbs, A, Gibson, R, Halverson, S, Johnson, C, Karkar, S, Kotani, T, Kress, E, Leifer, S, Magnone, K, Maire, J, Pahuja, R, Porter, M, Roberts, M, Sappey, B, Thorne, J, Wang, E, Artigau, É, Blake, GA, Canalizo, G, Chen, G, Doppmann, G, Doyon, R, Dressing, C, Fang, M, Greene, T, Herczeg, G, Hillenbrand, L, Howard, A, Kane, S, Kataria, T, Kempton, E, Knutson, H, Lafrenière, D, Liu, C, Metchev, S, Millar-Blanchaer, M, Narita, N, Pandey, G, Rajaguru, SP, Robertson, P, Salyk, C, Sato, B, Schlawin, E, Sengupta, S, Sivarani, T, Skidmore, W, Vasisht, G, Yasui, C & Zhang, H 2023, The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities. in GJ Ruane (ed.), Techniques and Instrumentation for Detection of Exoplanets XI., 1268007, Proceedings of SPIE - The International Society for Optical Engineering, vol. 12680, SPIE, Techniques and Instrumentation for Detection of Exoplanets XI 2023, San Diego, United States, 8/21/23. https://doi.org/10.1117/12.2681522

Konopacky QM, Baker AD, Mawet D, Fitzgerald MP, Jovanovic N, Beichman C et al. The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities. In Ruane GJ, editor, Techniques and Instrumentation for Detection of Exoplanets XI. SPIE. 2023. 1268007. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2681522

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abstract = "HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R 100,000 spectroscopy between 0.98 – 2.5 µm, HISPEC will enable spectroscopy of transiting and non-transiting exoplanets in close orbits, direct high-contrast detection and spectroscopy of spatially separated substellar companions, and exoplanet dynamical mass and orbit measurements using precision radial velocity monitoring calibrated with a suite of state-of-the-art absolute and relative wavelength references. MODHIS is the counterpart to HISPEC for the Thirty Meter Telescope and is being developed in parallel with similar scientific goals. In this proceeding, we provide a brief overview of the current design of both instruments, and the requirements for the two spectrographs as guided by the scientific goals for each. We then outline the current science case for HISPEC and MODHIS, with focuses on the science enabled for exoplanet discovery and characterization. We also provide updated sensitivity curves for both instruments, in terms of both signal-to-noise ratio and predicted radial velocity precision.",

keywords = "Exoplanet atmospheres (487), Exoplanet detection methods (489), Exoplanets (498), High resolution spectroscopy (2096), Infrared astronomy (786), Radial velocities (1332), Spectrometers (1554), Spectropolarimetry (1556)",

author = "Konopacky, {Quinn M.} and Baker, {Ashley D.} and Dimitri Mawet and Fitzgerald, {Michael P.} and Nemanja Jovanovic and Charles Beichman and Garreth Ruane and Rob Bertz and Hiroshi Terada and Richard Dekany and Larry Lingvay and Marc Kassis and David Anderson and Motohide Tamura and Bj{\"o}rn Benneke and Thomas Beatty and Tuan Do and Shogo Nishiyama and Peter Plavchan and Jason Wang and Ji Wang and Adam Burgasser and Ruffio, {Jean Baptiste} and Huihao Zhang and Aaron Brown and Jason Fucik and Aidan Gibbs and Rose Gibson and Sam Halverson and Christopher Johnson and Sonia Karkar and Takayuki Kotani and Evan Kress and Stephanie Leifer and Kenneth Magnone and Jerome Maire and Rishi Pahuja and Michael Porter and Mitsuko Roberts and Ben Sappey and Jim Thorne and Eric Wang and {\'E}tienne Artigau and Blake, {Geoffrey A.} and Gabriela Canalizo and Guo Chen and Greg Doppmann and Ren{\'e} Doyon and Courtney Dressing and Min Fang and Thomas Greene and Greg Herczeg and Lynne Hillenbrand and Andrew Howard and Stephen Kane and Tiffany Kataria and Eliza Kempton and Heather Knutson and David Lafreni{\`e}re and Chao Liu and Stanimir Metchev and Max Millar-Blanchaer and Norio Narita and Gajendra Pandey and Rajaguru, {S. P.} and Paul Robertson and Colette Salyk and Bun'ei Sato and Evertt Schlawin and Sujan Sengupta and Thirupathi Sivarani and Warren Skidmore and Gautam Vasisht and Chikako Yasui and Hui Zhang",

note = "Publisher Copyright: {\textcopyright} 2023 SPIE.; Techniques and Instrumentation for Detection of Exoplanets XI 2023 ; Conference date: 21-08-2023 Through 24-08-2023",

year = "2023",

doi = "10.1117/12.2681522",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

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T2 - Techniques and Instrumentation for Detection of Exoplanets XI 2023

AU - Konopacky, Quinn M.

AU - Baker, Ashley D.

AU - Mawet, Dimitri

AU - Fitzgerald, Michael P.

AU - Jovanovic, Nemanja

AU - Beichman, Charles

AU - Ruane, Garreth

AU - Bertz, Rob

AU - Terada, Hiroshi

AU - Dekany, Richard

AU - Lingvay, Larry

AU - Kassis, Marc

AU - Anderson, David

AU - Tamura, Motohide

AU - Benneke, Björn

AU - Beatty, Thomas

AU - Do, Tuan

AU - Nishiyama, Shogo

AU - Plavchan, Peter

AU - Wang, Jason

AU - Wang, Ji

AU - Burgasser, Adam

AU - Ruffio, Jean Baptiste

AU - Zhang, Huihao

AU - Brown, Aaron

AU - Fucik, Jason

AU - Gibbs, Aidan

AU - Gibson, Rose

AU - Halverson, Sam

AU - Johnson, Christopher

AU - Karkar, Sonia

AU - Kotani, Takayuki

AU - Kress, Evan

AU - Leifer, Stephanie

AU - Magnone, Kenneth

AU - Maire, Jerome

AU - Pahuja, Rishi

AU - Porter, Michael

AU - Roberts, Mitsuko

AU - Sappey, Ben

AU - Thorne, Jim

AU - Wang, Eric

AU - Artigau, Étienne

AU - Blake, Geoffrey A.

AU - Canalizo, Gabriela

AU - Chen, Guo

AU - Doppmann, Greg

AU - Doyon, René

AU - Dressing, Courtney

AU - Fang, Min

AU - Greene, Thomas

AU - Herczeg, Greg

AU - Hillenbrand, Lynne

AU - Howard, Andrew

AU - Kane, Stephen

AU - Kataria, Tiffany

AU - Kempton, Eliza

AU - Knutson, Heather

AU - Lafrenière, David

AU - Liu, Chao

AU - Metchev, Stanimir

AU - Millar-Blanchaer, Max

AU - Narita, Norio

AU - Pandey, Gajendra

AU - Rajaguru, S. P.

AU - Robertson, Paul

AU - Salyk, Colette

AU - Sato, Bun'ei

AU - Schlawin, Evertt

AU - Sengupta, Sujan

AU - Sivarani, Thirupathi

AU - Skidmore, Warren

AU - Vasisht, Gautam

AU - Yasui, Chikako

AU - Zhang, Hui

PY - 2023

Y1 - 2023

N2 - HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R 100,000 spectroscopy between 0.98 – 2.5 µm, HISPEC will enable spectroscopy of transiting and non-transiting exoplanets in close orbits, direct high-contrast detection and spectroscopy of spatially separated substellar companions, and exoplanet dynamical mass and orbit measurements using precision radial velocity monitoring calibrated with a suite of state-of-the-art absolute and relative wavelength references. MODHIS is the counterpart to HISPEC for the Thirty Meter Telescope and is being developed in parallel with similar scientific goals. In this proceeding, we provide a brief overview of the current design of both instruments, and the requirements for the two spectrographs as guided by the scientific goals for each. We then outline the current science case for HISPEC and MODHIS, with focuses on the science enabled for exoplanet discovery and characterization. We also provide updated sensitivity curves for both instruments, in terms of both signal-to-noise ratio and predicted radial velocity precision.

AB - HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R 100,000 spectroscopy between 0.98 – 2.5 µm, HISPEC will enable spectroscopy of transiting and non-transiting exoplanets in close orbits, direct high-contrast detection and spectroscopy of spatially separated substellar companions, and exoplanet dynamical mass and orbit measurements using precision radial velocity monitoring calibrated with a suite of state-of-the-art absolute and relative wavelength references. MODHIS is the counterpart to HISPEC for the Thirty Meter Telescope and is being developed in parallel with similar scientific goals. In this proceeding, we provide a brief overview of the current design of both instruments, and the requirements for the two spectrographs as guided by the scientific goals for each. We then outline the current science case for HISPEC and MODHIS, with focuses on the science enabled for exoplanet discovery and characterization. We also provide updated sensitivity curves for both instruments, in terms of both signal-to-noise ratio and predicted radial velocity precision.

KW - Exoplanet atmospheres (487)

KW - Exoplanet detection methods (489)

KW - Exoplanets (498)

KW - High resolution spectroscopy (2096)

KW - Infrared astronomy (786)

KW - Radial velocities (1332)

KW - Spectrometers (1554)

KW - Spectropolarimetry (1556)

UR - http://www.scopus.com/inward/record.url?scp=85178136008&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85178136008&partnerID=8YFLogxK

U2 - 10.1117/12.2681522

DO - 10.1117/12.2681522

M3 - Conference contribution

AN - SCOPUS:85178136008

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Techniques and Instrumentation for Detection of Exoplanets XI

A2 - Ruane, Garreth J.

PB - SPIE

Y2 - 21 August 2023 through 24 August 2023

ER -

The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities

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