The Simons Observatory: Beam Characterization for the Small Aperture Telescopes

We use time-domain simulations of Jupiter observations to test and develop a beam reconstruction pipeline for the Simons Observatory Small Aperture Telescopes. The method relies on a mapmaker that estimates and subtracts correlated atmospheric noise and a beam fitting code designed to compensate for...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2024-01, Vol.961 (1)
Hauptverfasser: Dachlythra, Nadia, Duivenvoorden, Adriaan J., Gudmundsson, Jon E., Hasselfield, Matthew, Coppi, Gabriele, Adler, Alexandre E., Alonso, David, Azzoni, Susanna, Chesmore, Grace. E., Fabbian, Giulio, Ganga, Ken, Gerras, Remington G., Jaffe, Andrew H., Johnson, Bradley R., Keating, Brian, Keskitalo, Reijo, Kisner, Theodore S., Krachmalnicoffork, Nicoletta, Lungu, Marius, Matsuda, Frederick, Naess, Sigurd, Page, Lyman, Puddu, Roberto, Puglisi, Giuseppe, Simon, Sara M., Teply, Grant, Tsan, Tran, Wollack, Edward J., Wolz, Kevin, Xu, Zhilei
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 1
container_start_page
container_title The Astrophysical journal
container_volume 961
creator Dachlythra, Nadia
Duivenvoorden, Adriaan J.
Gudmundsson, Jon E.
Hasselfield, Matthew
Coppi, Gabriele
Adler, Alexandre E.
Alonso, David
Azzoni, Susanna
Chesmore, Grace. E.
Fabbian, Giulio
Ganga, Ken
Gerras, Remington G.
Jaffe, Andrew H.
Johnson, Bradley R.
Keating, Brian
Keskitalo, Reijo
Kisner, Theodore S.
Krachmalnicoffork, Nicoletta
Lungu, Marius
Matsuda, Frederick
Naess, Sigurd
Page, Lyman
Puddu, Roberto
Puglisi, Giuseppe
Simon, Sara M.
Teply, Grant
Tsan, Tran
Wollack, Edward J.
Wolz, Kevin
Xu, Zhilei
description We use time-domain simulations of Jupiter observations to test and develop a beam reconstruction pipeline for the Simons Observatory Small Aperture Telescopes. The method relies on a mapmaker that estimates and subtracts correlated atmospheric noise and a beam fitting code designed to compensate for the bias caused by the mapmaker. We test our reconstruction performance for four different frequency bands against various algorithmic parameters, atmospheric conditions, and input beams. We additionally show the reconstruction quality as a function of the number of available observations and investigate how different calibration strategies affect the beam uncertainty. For all of the cases considered, we find good agreement between the fitted results and the input beam model within an ∼1.5% error for a multipole range ℓ = 30–700 and an ∼0.5% error for a multipole range ℓ = 50–200. We conclude by using a harmonic-domain component separation algorithm to verify that the beam reconstruction errors and biases observed in our analysis do not significantly bias the Simons Observatory r-measurement.
doi_str_mv 10.3847/1538-4357/ad0969.
format Article
fullrecord <record><control><sourceid>nasa</sourceid><recordid>TN_cdi_nasa_ntrs_20240001106</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>20240001106</sourcerecordid><originalsourceid>FETCH-nasa_ntrs_202400011063</originalsourceid><addsrcrecordid>eNqFjc0KgkAUhYcoyH4eIGgxL6COjmm2KynauchFu7jVFQ11ZO4U1NOXEG1bHc53-DiMzTzhyGUQud5CLu1ALiIXriIOY6fHrB_rM0sIEdihjI5DNiK6ddWPY4ulWYH8UNaqIZ6eCfUDjNLPFd8g1DwpQMPFoC5fYErV8Fxpbjqjhqri6xa1uWvkGVZIF9UiTdggh4pw-s0xm--2WbK3GyA4NUbTyRd-8Pn3PBHKP_Mb8_E-jA</addsrcrecordid><sourcetype>Publisher</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>The Simons Observatory: Beam Characterization for the Small Aperture Telescopes</title><source>IOP Publishing Free Content</source><source>DOAJ Directory of Open Access Journals</source><source>NASA Technical Reports Server</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Dachlythra, Nadia ; Duivenvoorden, Adriaan J. ; Gudmundsson, Jon E. ; Hasselfield, Matthew ; Coppi, Gabriele ; Adler, Alexandre E. ; Alonso, David ; Azzoni, Susanna ; Chesmore, Grace. E. ; Fabbian, Giulio ; Ganga, Ken ; Gerras, Remington G. ; Jaffe, Andrew H. ; Johnson, Bradley R. ; Keating, Brian ; Keskitalo, Reijo ; Kisner, Theodore S. ; Krachmalnicoffork, Nicoletta ; Lungu, Marius ; Matsuda, Frederick ; Naess, Sigurd ; Page, Lyman ; Puddu, Roberto ; Puglisi, Giuseppe ; Simon, Sara M. ; Teply, Grant ; Tsan, Tran ; Wollack, Edward J. ; Wolz, Kevin ; Xu, Zhilei</creator><creatorcontrib>Dachlythra, Nadia ; Duivenvoorden, Adriaan J. ; Gudmundsson, Jon E. ; Hasselfield, Matthew ; Coppi, Gabriele ; Adler, Alexandre E. ; Alonso, David ; Azzoni, Susanna ; Chesmore, Grace. E. ; Fabbian, Giulio ; Ganga, Ken ; Gerras, Remington G. ; Jaffe, Andrew H. ; Johnson, Bradley R. ; Keating, Brian ; Keskitalo, Reijo ; Kisner, Theodore S. ; Krachmalnicoffork, Nicoletta ; Lungu, Marius ; Matsuda, Frederick ; Naess, Sigurd ; Page, Lyman ; Puddu, Roberto ; Puglisi, Giuseppe ; Simon, Sara M. ; Teply, Grant ; Tsan, Tran ; Wollack, Edward J. ; Wolz, Kevin ; Xu, Zhilei</creatorcontrib><description>We use time-domain simulations of Jupiter observations to test and develop a beam reconstruction pipeline for the Simons Observatory Small Aperture Telescopes. The method relies on a mapmaker that estimates and subtracts correlated atmospheric noise and a beam fitting code designed to compensate for the bias caused by the mapmaker. We test our reconstruction performance for four different frequency bands against various algorithmic parameters, atmospheric conditions, and input beams. We additionally show the reconstruction quality as a function of the number of available observations and investigate how different calibration strategies affect the beam uncertainty. For all of the cases considered, we find good agreement between the fitted results and the input beam model within an ∼1.5% error for a multipole range ℓ = 30–700 and an ∼0.5% error for a multipole range ℓ = 50–200. We conclude by using a harmonic-domain component separation algorithm to verify that the beam reconstruction errors and biases observed in our analysis do not significantly bias the Simons Observatory r-measurement.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ad0969.</identifier><language>eng</language><publisher>Goddard Space Flight Center: American Astronomical Society</publisher><subject>Astronomy ; Astrophysics ; Instrumentation and Photography</subject><ispartof>The Astrophysical journal, 2024-01, Vol.961 (1)</ispartof><rights>Copyright Determination: GOV_PERMITTED</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0002-2408-9201 ; 0000-0002-8132-4896 ; 0000-0003-3155-6151 ; 0000-0001-8159-8208 ; 0000-0002-7567-4451 ; 0000-0001-5748-5182 ; 0000-0002-5736-5524 ; 0000-0002-6898-8938 ; 0000-0002-0689-4290 ; 0000-0003-3510-7134 ; 0000-0002-3255-4695 ; 0000-0003-3118-5514 ; 0000-0003-2086-1759 ; 0000-0001-9221-7802 ; 0000-0001-5112-2567 ; 0000-0002-6362-6524 ; 0000-0003-2856-2382 ; 0000-0002-4598-9719 ; 0000-0002-3800-5558 ; 0009-0006-7382-1434 ; 0000-0002-4478-7111 ; 0000-0002-5501-8449 ; 0000-0002-9828-3525 ; 0000-0001-6702-0450 ; 0000-0003-0041-6447 ; 0009-0009-0876-9168</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,800,864,27924,27925</link.rule.ids></links><search><creatorcontrib>Dachlythra, Nadia</creatorcontrib><creatorcontrib>Duivenvoorden, Adriaan J.</creatorcontrib><creatorcontrib>Gudmundsson, Jon E.</creatorcontrib><creatorcontrib>Hasselfield, Matthew</creatorcontrib><creatorcontrib>Coppi, Gabriele</creatorcontrib><creatorcontrib>Adler, Alexandre E.</creatorcontrib><creatorcontrib>Alonso, David</creatorcontrib><creatorcontrib>Azzoni, Susanna</creatorcontrib><creatorcontrib>Chesmore, Grace. E.</creatorcontrib><creatorcontrib>Fabbian, Giulio</creatorcontrib><creatorcontrib>Ganga, Ken</creatorcontrib><creatorcontrib>Gerras, Remington G.</creatorcontrib><creatorcontrib>Jaffe, Andrew H.</creatorcontrib><creatorcontrib>Johnson, Bradley R.</creatorcontrib><creatorcontrib>Keating, Brian</creatorcontrib><creatorcontrib>Keskitalo, Reijo</creatorcontrib><creatorcontrib>Kisner, Theodore S.</creatorcontrib><creatorcontrib>Krachmalnicoffork, Nicoletta</creatorcontrib><creatorcontrib>Lungu, Marius</creatorcontrib><creatorcontrib>Matsuda, Frederick</creatorcontrib><creatorcontrib>Naess, Sigurd</creatorcontrib><creatorcontrib>Page, Lyman</creatorcontrib><creatorcontrib>Puddu, Roberto</creatorcontrib><creatorcontrib>Puglisi, Giuseppe</creatorcontrib><creatorcontrib>Simon, Sara M.</creatorcontrib><creatorcontrib>Teply, Grant</creatorcontrib><creatorcontrib>Tsan, Tran</creatorcontrib><creatorcontrib>Wollack, Edward J.</creatorcontrib><creatorcontrib>Wolz, Kevin</creatorcontrib><creatorcontrib>Xu, Zhilei</creatorcontrib><title>The Simons Observatory: Beam Characterization for the Small Aperture Telescopes</title><title>The Astrophysical journal</title><description>We use time-domain simulations of Jupiter observations to test and develop a beam reconstruction pipeline for the Simons Observatory Small Aperture Telescopes. The method relies on a mapmaker that estimates and subtracts correlated atmospheric noise and a beam fitting code designed to compensate for the bias caused by the mapmaker. We test our reconstruction performance for four different frequency bands against various algorithmic parameters, atmospheric conditions, and input beams. We additionally show the reconstruction quality as a function of the number of available observations and investigate how different calibration strategies affect the beam uncertainty. For all of the cases considered, we find good agreement between the fitted results and the input beam model within an ∼1.5% error for a multipole range ℓ = 30–700 and an ∼0.5% error for a multipole range ℓ = 50–200. We conclude by using a harmonic-domain component separation algorithm to verify that the beam reconstruction errors and biases observed in our analysis do not significantly bias the Simons Observatory r-measurement.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Instrumentation and Photography</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNqFjc0KgkAUhYcoyH4eIGgxL6COjmm2KynauchFu7jVFQ11ZO4U1NOXEG1bHc53-DiMzTzhyGUQud5CLu1ALiIXriIOY6fHrB_rM0sIEdihjI5DNiK6ddWPY4ulWYH8UNaqIZ6eCfUDjNLPFd8g1DwpQMPFoC5fYErV8Fxpbjqjhqri6xa1uWvkGVZIF9UiTdggh4pw-s0xm--2WbK3GyA4NUbTyRd-8Pn3PBHKP_Mb8_E-jA</recordid><startdate>20240119</startdate><enddate>20240119</enddate><creator>Dachlythra, Nadia</creator><creator>Duivenvoorden, Adriaan J.</creator><creator>Gudmundsson, Jon E.</creator><creator>Hasselfield, Matthew</creator><creator>Coppi, Gabriele</creator><creator>Adler, Alexandre E.</creator><creator>Alonso, David</creator><creator>Azzoni, Susanna</creator><creator>Chesmore, Grace. E.</creator><creator>Fabbian, Giulio</creator><creator>Ganga, Ken</creator><creator>Gerras, Remington G.</creator><creator>Jaffe, Andrew H.</creator><creator>Johnson, Bradley R.</creator><creator>Keating, Brian</creator><creator>Keskitalo, Reijo</creator><creator>Kisner, Theodore S.</creator><creator>Krachmalnicoffork, Nicoletta</creator><creator>Lungu, Marius</creator><creator>Matsuda, Frederick</creator><creator>Naess, Sigurd</creator><creator>Page, Lyman</creator><creator>Puddu, Roberto</creator><creator>Puglisi, Giuseppe</creator><creator>Simon, Sara M.</creator><creator>Teply, Grant</creator><creator>Tsan, Tran</creator><creator>Wollack, Edward J.</creator><creator>Wolz, Kevin</creator><creator>Xu, Zhilei</creator><general>American Astronomical Society</general><scope>CYE</scope><scope>CYI</scope><orcidid>https://orcid.org/0000-0002-2408-9201</orcidid><orcidid>https://orcid.org/0000-0002-8132-4896</orcidid><orcidid>https://orcid.org/0000-0003-3155-6151</orcidid><orcidid>https://orcid.org/0000-0001-8159-8208</orcidid><orcidid>https://orcid.org/0000-0002-7567-4451</orcidid><orcidid>https://orcid.org/0000-0001-5748-5182</orcidid><orcidid>https://orcid.org/0000-0002-5736-5524</orcidid><orcidid>https://orcid.org/0000-0002-6898-8938</orcidid><orcidid>https://orcid.org/0000-0002-0689-4290</orcidid><orcidid>https://orcid.org/0000-0003-3510-7134</orcidid><orcidid>https://orcid.org/0000-0002-3255-4695</orcidid><orcidid>https://orcid.org/0000-0003-3118-5514</orcidid><orcidid>https://orcid.org/0000-0003-2086-1759</orcidid><orcidid>https://orcid.org/0000-0001-9221-7802</orcidid><orcidid>https://orcid.org/0000-0001-5112-2567</orcidid><orcidid>https://orcid.org/0000-0002-6362-6524</orcidid><orcidid>https://orcid.org/0000-0003-2856-2382</orcidid><orcidid>https://orcid.org/0000-0002-4598-9719</orcidid><orcidid>https://orcid.org/0000-0002-3800-5558</orcidid><orcidid>https://orcid.org/0009-0006-7382-1434</orcidid><orcidid>https://orcid.org/0000-0002-4478-7111</orcidid><orcidid>https://orcid.org/0000-0002-5501-8449</orcidid><orcidid>https://orcid.org/0000-0002-9828-3525</orcidid><orcidid>https://orcid.org/0000-0001-6702-0450</orcidid><orcidid>https://orcid.org/0000-0003-0041-6447</orcidid><orcidid>https://orcid.org/0009-0009-0876-9168</orcidid></search><sort><creationdate>20240119</creationdate><title>The Simons Observatory: Beam Characterization for the Small Aperture Telescopes</title><author>Dachlythra, Nadia ; Duivenvoorden, Adriaan J. ; Gudmundsson, Jon E. ; Hasselfield, Matthew ; Coppi, Gabriele ; Adler, Alexandre E. ; Alonso, David ; Azzoni, Susanna ; Chesmore, Grace. E. ; Fabbian, Giulio ; Ganga, Ken ; Gerras, Remington G. ; Jaffe, Andrew H. ; Johnson, Bradley R. ; Keating, Brian ; Keskitalo, Reijo ; Kisner, Theodore S. ; Krachmalnicoffork, Nicoletta ; Lungu, Marius ; Matsuda, Frederick ; Naess, Sigurd ; Page, Lyman ; Puddu, Roberto ; Puglisi, Giuseppe ; Simon, Sara M. ; Teply, Grant ; Tsan, Tran ; Wollack, Edward J. ; Wolz, Kevin ; Xu, Zhilei</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-nasa_ntrs_202400011063</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Instrumentation and Photography</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dachlythra, Nadia</creatorcontrib><creatorcontrib>Duivenvoorden, Adriaan J.</creatorcontrib><creatorcontrib>Gudmundsson, Jon E.</creatorcontrib><creatorcontrib>Hasselfield, Matthew</creatorcontrib><creatorcontrib>Coppi, Gabriele</creatorcontrib><creatorcontrib>Adler, Alexandre E.</creatorcontrib><creatorcontrib>Alonso, David</creatorcontrib><creatorcontrib>Azzoni, Susanna</creatorcontrib><creatorcontrib>Chesmore, Grace. E.</creatorcontrib><creatorcontrib>Fabbian, Giulio</creatorcontrib><creatorcontrib>Ganga, Ken</creatorcontrib><creatorcontrib>Gerras, Remington G.</creatorcontrib><creatorcontrib>Jaffe, Andrew H.</creatorcontrib><creatorcontrib>Johnson, Bradley R.</creatorcontrib><creatorcontrib>Keating, Brian</creatorcontrib><creatorcontrib>Keskitalo, Reijo</creatorcontrib><creatorcontrib>Kisner, Theodore S.</creatorcontrib><creatorcontrib>Krachmalnicoffork, Nicoletta</creatorcontrib><creatorcontrib>Lungu, Marius</creatorcontrib><creatorcontrib>Matsuda, Frederick</creatorcontrib><creatorcontrib>Naess, Sigurd</creatorcontrib><creatorcontrib>Page, Lyman</creatorcontrib><creatorcontrib>Puddu, Roberto</creatorcontrib><creatorcontrib>Puglisi, Giuseppe</creatorcontrib><creatorcontrib>Simon, Sara M.</creatorcontrib><creatorcontrib>Teply, Grant</creatorcontrib><creatorcontrib>Tsan, Tran</creatorcontrib><creatorcontrib>Wollack, Edward J.</creatorcontrib><creatorcontrib>Wolz, Kevin</creatorcontrib><creatorcontrib>Xu, Zhilei</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dachlythra, Nadia</au><au>Duivenvoorden, Adriaan J.</au><au>Gudmundsson, Jon E.</au><au>Hasselfield, Matthew</au><au>Coppi, Gabriele</au><au>Adler, Alexandre E.</au><au>Alonso, David</au><au>Azzoni, Susanna</au><au>Chesmore, Grace. E.</au><au>Fabbian, Giulio</au><au>Ganga, Ken</au><au>Gerras, Remington G.</au><au>Jaffe, Andrew H.</au><au>Johnson, Bradley R.</au><au>Keating, Brian</au><au>Keskitalo, Reijo</au><au>Kisner, Theodore S.</au><au>Krachmalnicoffork, Nicoletta</au><au>Lungu, Marius</au><au>Matsuda, Frederick</au><au>Naess, Sigurd</au><au>Page, Lyman</au><au>Puddu, Roberto</au><au>Puglisi, Giuseppe</au><au>Simon, Sara M.</au><au>Teply, Grant</au><au>Tsan, Tran</au><au>Wollack, Edward J.</au><au>Wolz, Kevin</au><au>Xu, Zhilei</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Simons Observatory: Beam Characterization for the Small Aperture Telescopes</atitle><jtitle>The Astrophysical journal</jtitle><date>2024-01-19</date><risdate>2024</risdate><volume>961</volume><issue>1</issue><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We use time-domain simulations of Jupiter observations to test and develop a beam reconstruction pipeline for the Simons Observatory Small Aperture Telescopes. The method relies on a mapmaker that estimates and subtracts correlated atmospheric noise and a beam fitting code designed to compensate for the bias caused by the mapmaker. We test our reconstruction performance for four different frequency bands against various algorithmic parameters, atmospheric conditions, and input beams. We additionally show the reconstruction quality as a function of the number of available observations and investigate how different calibration strategies affect the beam uncertainty. For all of the cases considered, we find good agreement between the fitted results and the input beam model within an ∼1.5% error for a multipole range ℓ = 30–700 and an ∼0.5% error for a multipole range ℓ = 50–200. We conclude by using a harmonic-domain component separation algorithm to verify that the beam reconstruction errors and biases observed in our analysis do not significantly bias the Simons Observatory r-measurement.</abstract><cop>Goddard Space Flight Center</cop><pub>American Astronomical Society</pub><doi>10.3847/1538-4357/ad0969.</doi><orcidid>https://orcid.org/0000-0002-2408-9201</orcidid><orcidid>https://orcid.org/0000-0002-8132-4896</orcidid><orcidid>https://orcid.org/0000-0003-3155-6151</orcidid><orcidid>https://orcid.org/0000-0001-8159-8208</orcidid><orcidid>https://orcid.org/0000-0002-7567-4451</orcidid><orcidid>https://orcid.org/0000-0001-5748-5182</orcidid><orcidid>https://orcid.org/0000-0002-5736-5524</orcidid><orcidid>https://orcid.org/0000-0002-6898-8938</orcidid><orcidid>https://orcid.org/0000-0002-0689-4290</orcidid><orcidid>https://orcid.org/0000-0003-3510-7134</orcidid><orcidid>https://orcid.org/0000-0002-3255-4695</orcidid><orcidid>https://orcid.org/0000-0003-3118-5514</orcidid><orcidid>https://orcid.org/0000-0003-2086-1759</orcidid><orcidid>https://orcid.org/0000-0001-9221-7802</orcidid><orcidid>https://orcid.org/0000-0001-5112-2567</orcidid><orcidid>https://orcid.org/0000-0002-6362-6524</orcidid><orcidid>https://orcid.org/0000-0003-2856-2382</orcidid><orcidid>https://orcid.org/0000-0002-4598-9719</orcidid><orcidid>https://orcid.org/0000-0002-3800-5558</orcidid><orcidid>https://orcid.org/0009-0006-7382-1434</orcidid><orcidid>https://orcid.org/0000-0002-4478-7111</orcidid><orcidid>https://orcid.org/0000-0002-5501-8449</orcidid><orcidid>https://orcid.org/0000-0002-9828-3525</orcidid><orcidid>https://orcid.org/0000-0001-6702-0450</orcidid><orcidid>https://orcid.org/0000-0003-0041-6447</orcidid><orcidid>https://orcid.org/0009-0009-0876-9168</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2024-01, Vol.961 (1)
issn 0004-637X
1538-4357
language eng
recordid cdi_nasa_ntrs_20240001106
source IOP Publishing Free Content; DOAJ Directory of Open Access Journals; NASA Technical Reports Server; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
subjects Astronomy
Astrophysics
Instrumentation and Photography
title The Simons Observatory: Beam Characterization for the Small Aperture Telescopes
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-26T17%3A21%3A32IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-nasa&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Simons%20Observatory:%20Beam%20Characterization%20for%20the%20Small%20Aperture%20Telescopes&rft.jtitle=The%20Astrophysical%20journal&rft.au=Dachlythra,%20Nadia&rft.date=2024-01-19&rft.volume=961&rft.issue=1&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/ad0969.&rft_dat=%3Cnasa%3E20240001106%3C/nasa%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true