Dataciencia

Colección SciELO Chile

Testing and performance of IFS upgrades to GPI 2.0

Indexado

Scopus

SCOPUS_ID:85178153052

DOI

10.1117/12.2677675

Año

2023

Tipo

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

The Gemini Planet Imager (GPI), is a facility class instrument for the Gemini Observatory with the primary goal of directly detecting young Jovian planets. After spending 2013 - 2020 at Gemini South, the instrument is currently undergoing maintenance and upgrades before its transition to Gemini North as GPI 2.0. Among the upgrades are significant changes to the Integral Field Spectrograph (IFS), including the installation of new prisms, Lyot stops/apodizers, and filters. The upgrades are expected to improve overall performance in the relevant wavelengths and angular separations needed for GPI 2.0.

Revista

Revista	ISSN
Proceedings Of Spie The International Society For Optical Engineering	0277-786X

Métricas Externas

PlumX	Altmetric	Dimensions

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Dimensions: https://www.dimensions.ai/why-dimensions/

Disciplinas de Investigación

WOS
Sin Disciplinas

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

SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.

Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Peng, Dillon	Hombre	University of Notre Dame - Estados Unidos
2	Chilcote, Jeffrey K.	Hombre	University of Notre Dame - Estados Unidos
3	Konopacky, Quinn	Hombre	University of California, San Diego - Estados Unidos
4	Hamper, Randall	Hombre	University of Notre Dame - Estados Unidos
5	Burke, Joel	-	University of Notre Dame - Estados Unidos
6	Sands, Brian	Hombre	University of Notre Dame - Estados Unidos
7	Engstrom, Matthew	-	University of Notre Dame - Estados Unidos
8	Karaszewski, Abigail	-	University of Notre Dame - Estados Unidos
9	Boyle, Rebecca	-	University of Notre Dame - Estados Unidos
10	Limbach, Mary Anne	Mujer	Texas A&M University - Estados Unidos
11	Greenbaum, Alexandra	-	Infrared Processing & Analysis Center - Estados Unidos
12	Sivaramakrishnan, Anand	Hombre	Space Telescope Science Institute - Estados Unidos
13	Rizika, Alexa	-	University of Notre Dame - Estados Unidos
14	Perera, S.	-	University of California, San Diego - Estados Unidos
15	Do, Clarissa	-	University of California, San Diego - Estados Unidos
16	Nguyen, Jayke	-	University of California, San Diego - Estados Unidos
17	Macintosh, Bruce	-	University of California Observatories - Estados Unidos
18	Fitzsimmons, Joeleff	-	National Research Council Canada - Canadá
19	Marois, Christian	Hombre	National Research Council Canada - Canadá University of Victoria - Canadá
20	Rantakyrö, Fredrik	-	Gemini ObservatorySouthern Operations Center - Chile
21	Aleman, Arlene	Mujer	Kavli Institute for Particle Astrophysics and Cosmology - Estados Unidos
22	Maire, Jérôme	-	University of California, San Diego - Estados Unidos
23	De Rosa, Robert	-	European Southern Observatory Santiago - Chile
24	Por, E. H.	Hombre	Space Telescope Science Institute - Estados Unidos
25	Savransky, D.	Hombre	Cornell University College of Engineering - Estados Unidos
26	Nguyen, Meiji M.	-	Space Telescope Science Institute - Estados Unidos
27	Perrin, M.	Hombre	Space Telescope Science Institute - Estados Unidos
28	Soummer, Remi	Hombre	Space Telescope Science Institute - Estados Unidos
29	Pueyo, Laurent	Hombre	Space Telescope Science Institute - Estados Unidos
30	Nickson, Bryony	Mujer	Space Telescope Science Institute - Estados Unidos
31	Spalding, Eckhart	-	The University of Sydney - Australia

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento

Fuente
National Science Foundation
Heising-Simons Foundation
Korea Astronomy and Space Science Institute
National Research Council Canada
NSF-MRI
Ministério da Ciência, Tecnologia, Inovações e Comunicações
Agencia Nacional de Investigación y Desarrollo
Ministerio de Ciencia, Tecnología e Innovación
Inova¸cões e Comunicac¸ões

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
The GPI 2.0 project is supported by a NSF-MRI grant (award AST-1920180) and the Heising-Simons Foundation. The original GPI was supported by NSF grants AST-1411868 and AST-1518332. The international Gemini Observatory is a program of NSF’s NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. on behalf of the Gemini Observatory partnership: the National Science Foundation (United States), National Research Council (Canada), Agencia Nacional de Investigación y Desarrollo (Chile), Ministerio de Ciencia, Tecnologíae Innovación (Argentina), Ministério da Ciência, Tecnologia, Inova¸cões e Comunicac¸ões (Brazil), and Korea Astronomy and Space Science Institute (Republic of Korea).

Agradecimiento

The GPI 2.0 project is supported by a NSF-MRI grant (award AST-1920180) and the Heising-Simons Foundation. The original GPI was supported by NSF grants AST-1411868 and AST-1518332. The international Gemini Observatory is a program of NSF’s NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. on behalf of the Gemini Observatory partnership: the National Science Foundation (United States), National Research Council (Canada), Agencia Nacional de Investigación y Desarrollo (Chile), Ministerio de Ciencia, Tecnologíae Innovación (Argentina), Ministério da Ciência, Tecnologia, Inova¸cões e Comunicac¸ões (Brazil), and Korea Astronomy and Space Science Institute (Republic of Korea).