Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT)

Andrew Szentgyorgyi; Sagi Ben-Ami; Jae Sok Oh; Chan Park; Daniel Baldwin; Jacob Bean; Alex Bichkovsky; Patricia Brennan; Daniel Catropa; Chueh Yi Chou; Moo Yung Chun; Laird Close; Jeffrey D. Crane; Peter Doherty; Daniel Durusky; Jason Eastman; Harland Epps; Ian N. Evans; Vitor Hartmann; Ofir Hershko; Bi Ho Jang; Jeong Gyun Jang; Ueejeong Jeong; Andres Jordan; Colby Jurgenson; Jan Kansky; Jihun Kim; Kang Min Kim; Sanghyuk Kim; Yunjong Kim; Sungho Lee; Matthew Leung; Hung Hsu Ling; Henrique Lupinari; Jared R. Males; Kenneth McCracken; Claudia Mendes de Oliveira; Rafael Millan-Gabet; Mark Mueller; Heeyoung Oh; Cem Onyuksel; Byeong Gon Park; Sung Joon Park; Woojin Park; William Podgorski; Andreas Seifahrt; Matthew Smith; Yahel Sofer-Rimalt; Shiang Yu Wang; Abigail Unger; Alan Uomoto; Young Sam Yu

doi:10.1117/12.3018439

Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT)

Andrew Szentgyorgyi
, Sagi Ben-Ami
, Jae Sok Oh
, Chan Park
, Daniel Baldwin
, Jacob Bean
, Alex Bichkovsky
, Patricia Brennan
, Daniel Catropa
, Chueh Yi Chou
, Moo Yung Chun
, Laird Close
, Jeffrey D. Crane
, Peter Doherty
, Daniel Durusky
, Jason Eastman
, Harland Epps
, Ian N. Evans
, Vitor Hartmann
, Ofir Hershko

Bi Ho Jang, Jeong Gyun Jang, Ueejeong Jeong, Andres Jordan, Colby Jurgenson, Jan Kansky, Jihun Kim, Kang Min Kim, Sanghyuk Kim, Yunjong Kim, Sungho Lee, Matthew Leung, Hung Hsu Ling, Henrique Lupinari, Jared R. Males, Kenneth McCracken, Claudia Mendes de Oliveira, Rafael Millan-Gabet, Mark Mueller, Heeyoung Oh, Cem Onyuksel, Byeong Gon Park, Sung Joon Park, Woojin Park, William Podgorski, Andreas Seifahrt, Matthew Smith, Yahel Sofer-Rimalt, Shiang Yu Wang, Abigail Unger, Alan Uomoto, Young Sam Yu

Facultad de Ingeniería y Ciencias

Producción científica: Capítulo del libro/informe/acta de congreso › Contribución a la conferencia › revisión exhaustiva

9 Citas (Scopus)

Resumen

The discovery of a fair sample of Earth-analogues (Earth 2.0's), i.e. rocky, Earth-mass exoplanets orbiting a Solar-type star in that host star's habitable zone, and a subsequent search of evidence of bioactivity on those Earth 2.0's by the detection of biogenically produced molecules in those exoplanetary atmospheres, are two of the most urgent observational programs in astrophysics and science in general. To identify an Earth 2.0, it is necessary to measure the reflex motion radial velocity amplitude of the host star at the 10 cm/sec level, a precision considerably below that which is currently achievable with existing instruments. The follow-on project to search for the biomarkers in an Earth 2.0's atmosphere may require an effective planet/star contrast of 10^-10, again well below the currently achievable level. In this paper, we discuss technical innovations in the implementation of the GMT-Consortium Large Earth Finder (G-CLEF) spectrograph that will enable these observational objectives. We discuss plans to operate G-CLEF at the Magellan Clay telescope with the MagAO-X adaptive optics system and subsequently with GMagAO-X at the Giant Magellan Telescope (GMT).

Idioma original	Inglés
Título de la publicación alojada	Ground-Based and Airborne Instrumentation for Astronomy X
Editores	Julia J. Bryant, Kentaro Motohara, Joel R. Vernet
Editorial	SPIE
ISBN (versión digital)	9781510675155
DOI	https://doi.org/10.1117/12.3018439
Estado	Publicada - 2024
Evento	Ground-Based and Airborne Instrumentation for Astronomy X 2024 - Yokohama, Japón Duración: 16 jun 2024 → 21 jun 2024

Serie de la publicación

Nombre	Proceedings of SPIE - The International Society for Optical Engineering
Volumen	13096
ISSN (versión impresa)	0277-786X
ISSN (versión digital)	1996-756X

Conferencia

Conferencia	Ground-Based and Airborne Instrumentation for Astronomy X 2024
País/Territorio	Japón
Ciudad	Yokohama
Período	16/06/24 → 21/06/24

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10.1117/12.3018439

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Szentgyorgyi, A., Ben-Ami, S., Oh, J. S., Park, C., Baldwin, D., Bean, J., Bichkovsky, A., Brennan, P., Catropa, D., Chou, C. Y., Chun, M. Y., Close, L., Crane, J. D., Doherty, P., Durusky, D., Eastman, J., Epps, H., Evans, I. N., Hartmann, V., ... Yu, Y. S. (2024). Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT). En J. J. Bryant, K. Motohara, & J. R. Vernet (Eds.), Ground-Based and Airborne Instrumentation for Astronomy X Artículo 130960Z (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 13096). SPIE. https://doi.org/10.1117/12.3018439

Szentgyorgyi, Andrew ; Ben-Ami, Sagi ; Oh, Jae Sok et al. / Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT). Ground-Based and Airborne Instrumentation for Astronomy X. editor / Julia J. Bryant ; Kentaro Motohara ; Joel R. Vernet. SPIE, 2024. (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{c282bda196cc4027822051e0b16e9f7a,

title = "Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT)",

abstract = "The discovery of a fair sample of Earth-analogues (Earth 2.0's), i.e. rocky, Earth-mass exoplanets orbiting a Solar-type star in that host star's habitable zone, and a subsequent search of evidence of bioactivity on those Earth 2.0's by the detection of biogenically produced molecules in those exoplanetary atmospheres, are two of the most urgent observational programs in astrophysics and science in general. To identify an Earth 2.0, it is necessary to measure the reflex motion radial velocity amplitude of the host star at the 10 cm/sec level, a precision considerably below that which is currently achievable with existing instruments. The follow-on project to search for the biomarkers in an Earth 2.0's atmosphere may require an effective planet/star contrast of 10-10, again well below the currently achievable level. In this paper, we discuss technical innovations in the implementation of the GMT-Consortium Large Earth Finder (G-CLEF) spectrograph that will enable these observational objectives. We discuss plans to operate G-CLEF at the Magellan Clay telescope with the MagAO-X adaptive optics system and subsequently with GMagAO-X at the Giant Magellan Telescope (GMT).",

keywords = "High dispersion spectroscopy, exoplanets, precision radial velocity measurements",

author = "Andrew Szentgyorgyi and Sagi Ben-Ami and Oh, \{Jae Sok\} and Chan Park and Daniel Baldwin and Jacob Bean and Alex Bichkovsky and Patricia Brennan and Daniel Catropa and Chou, \{Chueh Yi\} and Chun, \{Moo Yung\} and Laird Close and Crane, \{Jeffrey D.\} and Peter Doherty and Daniel Durusky and Jason Eastman and Harland Epps and Evans, \{Ian N.\} and Vitor Hartmann and Ofir Hershko and Jang, \{Bi Ho\} and Jang, \{Jeong Gyun\} and Ueejeong Jeong and Andres Jordan and Colby Jurgenson and Jan Kansky and Jihun Kim and Kim, \{Kang Min\} and Sanghyuk Kim and Yunjong Kim and Sungho Lee and Matthew Leung and Ling, \{Hung Hsu\} and Henrique Lupinari and Males, \{Jared R.\} and Kenneth McCracken and \{Mendes de Oliveira\}, Claudia and Rafael Millan-Gabet and Mark Mueller and Heeyoung Oh and Cem Onyuksel and Park, \{Byeong Gon\} and Park, \{Sung Joon\} and Woojin Park and William Podgorski and Andreas Seifahrt and Matthew Smith and Yahel Sofer-Rimalt and Wang, \{Shiang Yu\} and Abigail Unger and Alan Uomoto and Yu, \{Young Sam\}",

note = "Publisher Copyright: {\textcopyright} 2024 SPIE.; Ground-Based and Airborne Instrumentation for Astronomy X 2024 ; Conference date: 16-06-2024 Through 21-06-2024",

year = "2024",

doi = "10.1117/12.3018439",

language = "English",

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

publisher = "SPIE",

editor = "Bryant, \{Julia J.\} and Kentaro Motohara and Vernet, \{Joel R.\}",

booktitle = "Ground-Based and Airborne Instrumentation for Astronomy X",

}

Szentgyorgyi, A, Ben-Ami, S, Oh, JS, Park, C, Baldwin, D, Bean, J, Bichkovsky, A, Brennan, P, Catropa, D, Chou, CY, Chun, MY, Close, L, Crane, JD, Doherty, P, Durusky, D, Eastman, J, Epps, H, Evans, IN, Hartmann, V, Hershko, O, Jang, BH, Jang, JG, Jeong, U, Jordan, A, Jurgenson, C, Kansky, J, Kim, J, Kim, KM, Kim, S, Kim, Y, Lee, S, Leung, M, Ling, HH, Lupinari, H, Males, JR, McCracken, K, Mendes de Oliveira, C, Millan-Gabet, R, Mueller, M, Oh, H, Onyuksel, C, Park, BG, Park, SJ, Park, W, Podgorski, W, Seifahrt, A, Smith, M, Sofer-Rimalt, Y, Wang, SY, Unger, A, Uomoto, A & Yu, YS 2024, Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT). En JJ Bryant, K Motohara & JR Vernet (eds.), Ground-Based and Airborne Instrumentation for Astronomy X., 130960Z, Proceedings of SPIE - The International Society for Optical Engineering, vol. 13096, SPIE, Ground-Based and Airborne Instrumentation for Astronomy X 2024, Yokohama, Japón, 16/06/24. https://doi.org/10.1117/12.3018439

Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT). / Szentgyorgyi, Andrew; Ben-Ami, Sagi; Oh, Jae Sok et al.
Ground-Based and Airborne Instrumentation for Astronomy X. ed. / Julia J. Bryant; Kentaro Motohara; Joel R. Vernet. SPIE, 2024. 130960Z (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 13096).

Producción científica: Capítulo del libro/informe/acta de congreso › Contribución a la conferencia › revisión exhaustiva

TY - GEN

T1 - Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT)

AU - Szentgyorgyi, Andrew

AU - Ben-Ami, Sagi

AU - Oh, Jae Sok

AU - Park, Chan

AU - Baldwin, Daniel

AU - Bean, Jacob

AU - Bichkovsky, Alex

AU - Brennan, Patricia

AU - Catropa, Daniel

AU - Chou, Chueh Yi

AU - Chun, Moo Yung

AU - Close, Laird

AU - Crane, Jeffrey D.

AU - Doherty, Peter

AU - Durusky, Daniel

AU - Eastman, Jason

AU - Epps, Harland

AU - Evans, Ian N.

AU - Hartmann, Vitor

AU - Hershko, Ofir

AU - Jang, Bi Ho

AU - Jang, Jeong Gyun

AU - Jeong, Ueejeong

AU - Jordan, Andres

AU - Jurgenson, Colby

AU - Kansky, Jan

AU - Kim, Jihun

AU - Kim, Kang Min

AU - Kim, Sanghyuk

AU - Kim, Yunjong

AU - Lee, Sungho

AU - Leung, Matthew

AU - Ling, Hung Hsu

AU - Lupinari, Henrique

AU - Males, Jared R.

AU - McCracken, Kenneth

AU - Mendes de Oliveira, Claudia

AU - Millan-Gabet, Rafael

AU - Mueller, Mark

AU - Oh, Heeyoung

AU - Onyuksel, Cem

AU - Park, Byeong Gon

AU - Park, Sung Joon

AU - Park, Woojin

AU - Podgorski, William

AU - Seifahrt, Andreas

AU - Smith, Matthew

AU - Sofer-Rimalt, Yahel

AU - Wang, Shiang Yu

AU - Unger, Abigail

AU - Uomoto, Alan

AU - Yu, Young Sam

PY - 2024

Y1 - 2024

N2 - The discovery of a fair sample of Earth-analogues (Earth 2.0's), i.e. rocky, Earth-mass exoplanets orbiting a Solar-type star in that host star's habitable zone, and a subsequent search of evidence of bioactivity on those Earth 2.0's by the detection of biogenically produced molecules in those exoplanetary atmospheres, are two of the most urgent observational programs in astrophysics and science in general. To identify an Earth 2.0, it is necessary to measure the reflex motion radial velocity amplitude of the host star at the 10 cm/sec level, a precision considerably below that which is currently achievable with existing instruments. The follow-on project to search for the biomarkers in an Earth 2.0's atmosphere may require an effective planet/star contrast of 10-10, again well below the currently achievable level. In this paper, we discuss technical innovations in the implementation of the GMT-Consortium Large Earth Finder (G-CLEF) spectrograph that will enable these observational objectives. We discuss plans to operate G-CLEF at the Magellan Clay telescope with the MagAO-X adaptive optics system and subsequently with GMagAO-X at the Giant Magellan Telescope (GMT).

AB - The discovery of a fair sample of Earth-analogues (Earth 2.0's), i.e. rocky, Earth-mass exoplanets orbiting a Solar-type star in that host star's habitable zone, and a subsequent search of evidence of bioactivity on those Earth 2.0's by the detection of biogenically produced molecules in those exoplanetary atmospheres, are two of the most urgent observational programs in astrophysics and science in general. To identify an Earth 2.0, it is necessary to measure the reflex motion radial velocity amplitude of the host star at the 10 cm/sec level, a precision considerably below that which is currently achievable with existing instruments. The follow-on project to search for the biomarkers in an Earth 2.0's atmosphere may require an effective planet/star contrast of 10-10, again well below the currently achievable level. In this paper, we discuss technical innovations in the implementation of the GMT-Consortium Large Earth Finder (G-CLEF) spectrograph that will enable these observational objectives. We discuss plans to operate G-CLEF at the Magellan Clay telescope with the MagAO-X adaptive optics system and subsequently with GMagAO-X at the Giant Magellan Telescope (GMT).

KW - High dispersion spectroscopy

KW - exoplanets

KW - precision radial velocity measurements

UR - https://www.scopus.com/pages/publications/85201932728

U2 - 10.1117/12.3018439

DO - 10.1117/12.3018439

M3 - Conference contribution

AN - SCOPUS:85201932728

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

BT - Ground-Based and Airborne Instrumentation for Astronomy X

A2 - Bryant, Julia J.

A2 - Motohara, Kentaro

A2 - Vernet, Joel R.

PB - SPIE

T2 - Ground-Based and Airborne Instrumentation for Astronomy X 2024

Y2 - 16 June 2024 through 21 June 2024

ER -

Szentgyorgyi A, Ben-Ami S, Oh JS, Park C, Baldwin D, Bean J et al. Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT). En Bryant JJ, Motohara K, Vernet JR, editores, Ground-Based and Airborne Instrumentation for Astronomy X. SPIE. 2024. 130960Z. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.3018439

Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT)

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