TolTEC is an imaging polarimeter that will be mounted on the 50m diameter Large Millimeter Telescope (LMT) in Mexico. This camera simultaneously images the focal plane at three wavebands centered at 1.1, 1.4, and 2.0mm. TolTEC combines polarization-sensitive Kinetic Inductance Detectors (KIDs) with the LMT to produce 5-10 arcmin resolution maps of the sky in both total intensity and polarization. The light from the telescope is coupled to the TolTEC instrument using three room temperature mirrors. Before entering the cryostat, the light passes through a rapid-spinning achromatic half-wave plate, and once inside it passes through a 1 K Lyot stop that controls the telescope illumination. Inside the cryostat, a series of aluminum mirrors, silicon lenses, and dichroic filters split the light into three wavelength bands and direct each band to a different detector array. We will describe the design, and performance of the optics before installation at the telescope.

The optical design and performance of TolTEC: a millimeter-wave imaging polarimeter / Lunde, Emily; Ade, Peter; Berthoud, Marc; Contente, Reid; Denigris, Nat; Doyle, Simon; Ferrusca, Daniel; Golec, Joey; Kuczarski, Stephen; Lee, Dennis; Ma, Zhiyuan; Mauskopf, Philip; Mccrackan, Michael; Mcmahon, Jeffrey; Novak, Giles; Pisano, Giampaolo; Simon, Sara M.; Souccar, Kamal; Tucker, Carole; Underhill, Matthew; Van Camp, Eric; Wilson, Grant. - (2020). (Intervento presentato al convegno Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave tenutosi a Online Only, California, United States) [10.1117/12.2562798].

The optical design and performance of TolTEC: a millimeter-wave imaging polarimeter

Philip Mauskopf;Giampaolo Pisano;
2020

Abstract

TolTEC is an imaging polarimeter that will be mounted on the 50m diameter Large Millimeter Telescope (LMT) in Mexico. This camera simultaneously images the focal plane at three wavebands centered at 1.1, 1.4, and 2.0mm. TolTEC combines polarization-sensitive Kinetic Inductance Detectors (KIDs) with the LMT to produce 5-10 arcmin resolution maps of the sky in both total intensity and polarization. The light from the telescope is coupled to the TolTEC instrument using three room temperature mirrors. Before entering the cryostat, the light passes through a rapid-spinning achromatic half-wave plate, and once inside it passes through a 1 K Lyot stop that controls the telescope illumination. Inside the cryostat, a series of aluminum mirrors, silicon lenses, and dichroic filters split the light into three wavelength bands and direct each band to a different detector array. We will describe the design, and performance of the optics before installation at the telescope.
2020
Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave
Millimetre wave astronomy, sub-millimetre astronomy, polarimetry
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
The optical design and performance of TolTEC: a millimeter-wave imaging polarimeter / Lunde, Emily; Ade, Peter; Berthoud, Marc; Contente, Reid; Denigris, Nat; Doyle, Simon; Ferrusca, Daniel; Golec, Joey; Kuczarski, Stephen; Lee, Dennis; Ma, Zhiyuan; Mauskopf, Philip; Mccrackan, Michael; Mcmahon, Jeffrey; Novak, Giles; Pisano, Giampaolo; Simon, Sara M.; Souccar, Kamal; Tucker, Carole; Underhill, Matthew; Van Camp, Eric; Wilson, Grant. - (2020). (Intervento presentato al convegno Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave tenutosi a Online Only, California, United States) [10.1117/12.2562798].
File allegati a questo prodotto
File Dimensione Formato  
Lunde_The optical design_2020.pdf

solo gestori archivio

Tipologia: Versione editoriale (versione pubblicata con il layout dell'editore)
Licenza: Tutti i diritti riservati (All rights reserved)
Dimensione 7.49 MB
Formato Adobe PDF
7.49 MB Adobe PDF   Contatta l'autore

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1487690
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 4
  • ???jsp.display-item.citation.isi??? ND
social impact