Fast automatic spectrograph for transient (FAST)

José A. Araiza-Durán, Giuliano Pignata, Anna Brucalassi

Resultado de la investigación: Conference contribution

Resumen

The Fast automatic spectrograph for transient (FAST) is a valuable tool to classify resources and better characterize variable sources. FAST is a low resolution spectrograph with multiple resolving power modes (R ∼ 300 and 1000 at 6500 Å) in the VIS-UV range and with to capability to work in imaging mode. The spectrograph consist of a collimating mirror, reflective gratings, and a five-lenses design camera that offers a field of view of 10 arcmin when working in imaging mode. The instrument will be installed in the PROMPT-7 telescope which is able to operate without human intervention for the follow-up of time-variable sources. In this work, the optical design of the spectrograph, the telescope specifications, and the objects under study will be discussed.

Idioma originalEnglish
Título de la publicación alojadaGround-based and Airborne Instrumentation for Astronomy VII
EditoresLuc Simard, Luc Simard, Christopher J. Evans, Hideki Takami
EditorialSPIE
Volumen10702
ISBN (versión impresa)9781510619579
DOI
EstadoPublished - 1 ene 2018
EventoGround-based and Airborne Instrumentation for Astronomy VII 2018 - Austin, United States
Duración: 10 jun 201814 jun 2018

Conference

ConferenceGround-based and Airborne Instrumentation for Astronomy VII 2018
PaísUnited States
CiudadAustin
Período10/06/1814/06/18

Huella dactilar

Spectrographs
Spectrograph
spectrographs
Optical resolving power
Telescopes
Telescope
Imaging
telescopes
Lens Design
Imaging techniques
lens design
Optical design
Optical Design
Field of View
Gratings
field of view
Light sources
specifications
Lenses
resources

ASJC Scopus subject areas

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

Citar esto

Araiza-Durán, J. A., Pignata, G., & Brucalassi, A. (2018). Fast automatic spectrograph for transient (FAST). En L. Simard, L. Simard, C. J. Evans, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy VII (Vol. 10702). [107024P] SPIE. https://doi.org/10.1117/12.2312129
Araiza-Durán, José A. ; Pignata, Giuliano ; Brucalassi, Anna. / Fast automatic spectrograph for transient (FAST). Ground-based and Airborne Instrumentation for Astronomy VII. editor / Luc Simard ; Luc Simard ; Christopher J. Evans ; Hideki Takami. Vol. 10702 SPIE, 2018.
@inproceedings{3a851d68040b40688cf5448df0c24d50,
title = "Fast automatic spectrograph for transient (FAST)",
abstract = "The Fast automatic spectrograph for transient (FAST) is a valuable tool to classify resources and better characterize variable sources. FAST is a low resolution spectrograph with multiple resolving power modes (R ∼ 300 and 1000 at 6500 {\AA}) in the VIS-UV range and with to capability to work in imaging mode. The spectrograph consist of a collimating mirror, reflective gratings, and a five-lenses design camera that offers a field of view of 10 arcmin when working in imaging mode. The instrument will be installed in the PROMPT-7 telescope which is able to operate without human intervention for the follow-up of time-variable sources. In this work, the optical design of the spectrograph, the telescope specifications, and the objects under study will be discussed.",
keywords = "Low-Resolution, Robotic telescope, Spectrograph, Transient",
author = "Araiza-Dur{\'a}n, {Jos{\'e} A.} and Giuliano Pignata and Anna Brucalassi",
year = "2018",
month = "1",
day = "1",
doi = "10.1117/12.2312129",
language = "English",
isbn = "9781510619579",
volume = "10702",
editor = "Luc Simard and Luc Simard and Evans, {Christopher J.} and Hideki Takami",
booktitle = "Ground-based and Airborne Instrumentation for Astronomy VII",
publisher = "SPIE",
address = "United States",

}

Araiza-Durán, JA, Pignata, G & Brucalassi, A 2018, Fast automatic spectrograph for transient (FAST). En L Simard, L Simard, CJ Evans & H Takami (eds.), Ground-based and Airborne Instrumentation for Astronomy VII. vol. 10702, 107024P, SPIE, Ground-based and Airborne Instrumentation for Astronomy VII 2018, Austin, United States, 10/06/18. https://doi.org/10.1117/12.2312129

Fast automatic spectrograph for transient (FAST). / Araiza-Durán, José A.; Pignata, Giuliano; Brucalassi, Anna.

Ground-based and Airborne Instrumentation for Astronomy VII. ed. / Luc Simard; Luc Simard; Christopher J. Evans; Hideki Takami. Vol. 10702 SPIE, 2018. 107024P.

Resultado de la investigación: Conference contribution

TY - GEN

T1 - Fast automatic spectrograph for transient (FAST)

AU - Araiza-Durán, José A.

AU - Pignata, Giuliano

AU - Brucalassi, Anna

PY - 2018/1/1

Y1 - 2018/1/1

N2 - The Fast automatic spectrograph for transient (FAST) is a valuable tool to classify resources and better characterize variable sources. FAST is a low resolution spectrograph with multiple resolving power modes (R ∼ 300 and 1000 at 6500 Å) in the VIS-UV range and with to capability to work in imaging mode. The spectrograph consist of a collimating mirror, reflective gratings, and a five-lenses design camera that offers a field of view of 10 arcmin when working in imaging mode. The instrument will be installed in the PROMPT-7 telescope which is able to operate without human intervention for the follow-up of time-variable sources. In this work, the optical design of the spectrograph, the telescope specifications, and the objects under study will be discussed.

AB - The Fast automatic spectrograph for transient (FAST) is a valuable tool to classify resources and better characterize variable sources. FAST is a low resolution spectrograph with multiple resolving power modes (R ∼ 300 and 1000 at 6500 Å) in the VIS-UV range and with to capability to work in imaging mode. The spectrograph consist of a collimating mirror, reflective gratings, and a five-lenses design camera that offers a field of view of 10 arcmin when working in imaging mode. The instrument will be installed in the PROMPT-7 telescope which is able to operate without human intervention for the follow-up of time-variable sources. In this work, the optical design of the spectrograph, the telescope specifications, and the objects under study will be discussed.

KW - Low-Resolution

KW - Robotic telescope

KW - Spectrograph

KW - Transient

UR - http://www.scopus.com/inward/record.url?scp=85052632498&partnerID=8YFLogxK

U2 - 10.1117/12.2312129

DO - 10.1117/12.2312129

M3 - Conference contribution

SN - 9781510619579

VL - 10702

BT - Ground-based and Airborne Instrumentation for Astronomy VII

A2 - Simard, Luc

A2 - Simard, Luc

A2 - Evans, Christopher J.

A2 - Takami, Hideki

PB - SPIE

ER -

Araiza-Durán JA, Pignata G, Brucalassi A. Fast automatic spectrograph for transient (FAST). En Simard L, Simard L, Evans CJ, Takami H, editores, Ground-based and Airborne Instrumentation for Astronomy VII. Vol. 10702. SPIE. 2018. 107024P https://doi.org/10.1117/12.2312129