SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment
SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS will offer simultaneous wavelength coverage from 0.35 to 2.0 {\mu}m and will be dedicated to the study of transient and variable sources. While nom...
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| creator | Sanchez, Ricardo Zanmar Aliverti, Matteo Munari, Matteo Campana, Sergio Claudi, Riccardo Schipani, Pietro Baruffolo, Andrea Ben-Ami, Sagi Biondi, Federico Capasso, Giulio Cosentino, Rosario D'Alessio, Francesco D'Avanzo, Paolo Hershko, Ofir Kuncarayakti, Hanindyo Landoni, Marco Pignata, Giuliano Rubin, Adam Scuderi, Salvatore Vitali, Fabrizio Young, David Achrén, Jani Araiza-Duran, José Antonio Arcavi, Iair Brucalassi, Anna Bruch, Rachel Cappellaro, Enrico Colapietro, Mirko Della Valle, Massimo de Pascale, Marco di Benedetto, Rosario D'Orsi, Sergio Gal-Yam, Avishay Genoni, Matteo Hernandez, Marcos Kotilainen, Jari Causi, Gianluca Li Mattila, Seppo Rappaport, Michael Radhakrishnan, Kalyan Ricci, Davide Riva, Marco Salasnich, Bernardo Smartt, Stephen Stritzinger, Maximilian Ventura, Hector |
| description | SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph
to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS
will offer simultaneous wavelength coverage from 0.35 to 2.0 {\mu}m and will be
dedicated to the study of transient and variable sources. While nominal optical
performances of the system were presented in previous proceedings
(arXiv:1809.01521), we here present a set of further analyses aimed to identify
and quantify optical effects, due to changes in temperature and orientation of
the instrument during alignment and operations. |
| doi_str_mv | 10.48550/arxiv.2012.12680 |
| format | Article |
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to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS
will offer simultaneous wavelength coverage from 0.35 to 2.0 {\mu}m and will be
dedicated to the study of transient and variable sources. While nominal optical
performances of the system were presented in previous proceedings
(arXiv:1809.01521), we here present a set of further analyses aimed to identify
and quantify optical effects, due to changes in temperature and orientation of
the instrument during alignment and operations.</description><identifier>DOI: 10.48550/arxiv.2012.12680</identifier><language>eng</language><subject>Physics - Instrumentation and Methods for Astrophysics</subject><creationdate>2020-12</creationdate><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2012.12680$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2012.12680$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Sanchez, Ricardo Zanmar</creatorcontrib><creatorcontrib>Aliverti, Matteo</creatorcontrib><creatorcontrib>Munari, Matteo</creatorcontrib><creatorcontrib>Campana, Sergio</creatorcontrib><creatorcontrib>Claudi, Riccardo</creatorcontrib><creatorcontrib>Schipani, Pietro</creatorcontrib><creatorcontrib>Baruffolo, Andrea</creatorcontrib><creatorcontrib>Ben-Ami, Sagi</creatorcontrib><creatorcontrib>Biondi, Federico</creatorcontrib><creatorcontrib>Capasso, Giulio</creatorcontrib><creatorcontrib>Cosentino, Rosario</creatorcontrib><creatorcontrib>D'Alessio, Francesco</creatorcontrib><creatorcontrib>D'Avanzo, Paolo</creatorcontrib><creatorcontrib>Hershko, Ofir</creatorcontrib><creatorcontrib>Kuncarayakti, Hanindyo</creatorcontrib><creatorcontrib>Landoni, Marco</creatorcontrib><creatorcontrib>Pignata, Giuliano</creatorcontrib><creatorcontrib>Rubin, Adam</creatorcontrib><creatorcontrib>Scuderi, Salvatore</creatorcontrib><creatorcontrib>Vitali, Fabrizio</creatorcontrib><creatorcontrib>Young, David</creatorcontrib><creatorcontrib>Achrén, Jani</creatorcontrib><creatorcontrib>Araiza-Duran, José Antonio</creatorcontrib><creatorcontrib>Arcavi, Iair</creatorcontrib><creatorcontrib>Brucalassi, Anna</creatorcontrib><creatorcontrib>Bruch, Rachel</creatorcontrib><creatorcontrib>Cappellaro, Enrico</creatorcontrib><creatorcontrib>Colapietro, Mirko</creatorcontrib><creatorcontrib>Della Valle, Massimo</creatorcontrib><creatorcontrib>de Pascale, Marco</creatorcontrib><creatorcontrib>di Benedetto, Rosario</creatorcontrib><creatorcontrib>D'Orsi, Sergio</creatorcontrib><creatorcontrib>Gal-Yam, Avishay</creatorcontrib><creatorcontrib>Genoni, Matteo</creatorcontrib><creatorcontrib>Hernandez, Marcos</creatorcontrib><creatorcontrib>Kotilainen, Jari</creatorcontrib><creatorcontrib>Causi, Gianluca Li</creatorcontrib><creatorcontrib>Mattila, Seppo</creatorcontrib><creatorcontrib>Rappaport, Michael</creatorcontrib><creatorcontrib>Radhakrishnan, Kalyan</creatorcontrib><creatorcontrib>Ricci, Davide</creatorcontrib><creatorcontrib>Riva, Marco</creatorcontrib><creatorcontrib>Salasnich, Bernardo</creatorcontrib><creatorcontrib>Smartt, Stephen</creatorcontrib><creatorcontrib>Stritzinger, Maximilian</creatorcontrib><creatorcontrib>Ventura, Hector</creatorcontrib><title>SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment</title><description>SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph
to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS
will offer simultaneous wavelength coverage from 0.35 to 2.0 {\mu}m and will be
dedicated to the study of transient and variable sources. While nominal optical
performances of the system were presented in previous proceedings
(arXiv:1809.01521), we here present a set of further analyses aimed to identify
and quantify optical effects, due to changes in temperature and orientation of
the instrument during alignment and operations.</description><subject>Physics - Instrumentation and Methods for Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj8tqwzAURLXpoqT9gK6iD6hd-SmruxLSBwSySBbdmSvpOghsy0iyif--atrVMMNh4BDylLG0bKqKvYC7miXNWZanWV437J7Y0_H79Er3XYcqeGpHaqdgFPR0QtdZN8Co0FM9Iw2WXhwsJqy06_E6O_TPNOAQQQix0QWcgWDsGHcYNfWz9KuPhKfQm8s44BgeyF0HvcfH_9yQ8_v-vPtMDsePr93bIYGas6RpRME1MFahEiVnXAgteF3KpmS5RqFRx5Si1LUUMpporhUCU0qBglwWG7L9u70Zt5MzA7i1_TVvb-bFD_iIVpU</recordid><startdate>20201223</startdate><enddate>20201223</enddate><creator>Sanchez, Ricardo Zanmar</creator><creator>Aliverti, Matteo</creator><creator>Munari, Matteo</creator><creator>Campana, Sergio</creator><creator>Claudi, Riccardo</creator><creator>Schipani, Pietro</creator><creator>Baruffolo, Andrea</creator><creator>Ben-Ami, Sagi</creator><creator>Biondi, Federico</creator><creator>Capasso, Giulio</creator><creator>Cosentino, Rosario</creator><creator>D'Alessio, Francesco</creator><creator>D'Avanzo, Paolo</creator><creator>Hershko, Ofir</creator><creator>Kuncarayakti, Hanindyo</creator><creator>Landoni, Marco</creator><creator>Pignata, Giuliano</creator><creator>Rubin, Adam</creator><creator>Scuderi, Salvatore</creator><creator>Vitali, Fabrizio</creator><creator>Young, David</creator><creator>Achrén, Jani</creator><creator>Araiza-Duran, José Antonio</creator><creator>Arcavi, Iair</creator><creator>Brucalassi, Anna</creator><creator>Bruch, Rachel</creator><creator>Cappellaro, Enrico</creator><creator>Colapietro, Mirko</creator><creator>Della Valle, Massimo</creator><creator>de Pascale, Marco</creator><creator>di Benedetto, Rosario</creator><creator>D'Orsi, Sergio</creator><creator>Gal-Yam, Avishay</creator><creator>Genoni, Matteo</creator><creator>Hernandez, Marcos</creator><creator>Kotilainen, Jari</creator><creator>Causi, Gianluca Li</creator><creator>Mattila, Seppo</creator><creator>Rappaport, Michael</creator><creator>Radhakrishnan, Kalyan</creator><creator>Ricci, Davide</creator><creator>Riva, Marco</creator><creator>Salasnich, Bernardo</creator><creator>Smartt, Stephen</creator><creator>Stritzinger, Maximilian</creator><creator>Ventura, Hector</creator><scope>GOX</scope></search><sort><creationdate>20201223</creationdate><title>SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment</title><author>Sanchez, Ricardo Zanmar ; Aliverti, Matteo ; Munari, Matteo ; Campana, Sergio ; Claudi, Riccardo ; Schipani, Pietro ; Baruffolo, Andrea ; Ben-Ami, Sagi ; Biondi, Federico ; Capasso, Giulio ; Cosentino, Rosario ; D'Alessio, Francesco ; D'Avanzo, Paolo ; Hershko, Ofir ; Kuncarayakti, Hanindyo ; Landoni, Marco ; Pignata, Giuliano ; Rubin, Adam ; Scuderi, Salvatore ; Vitali, Fabrizio ; Young, David ; Achrén, Jani ; Araiza-Duran, José Antonio ; Arcavi, Iair ; Brucalassi, Anna ; Bruch, Rachel ; Cappellaro, Enrico ; Colapietro, Mirko ; Della Valle, Massimo ; de Pascale, Marco ; di Benedetto, Rosario ; D'Orsi, Sergio ; Gal-Yam, Avishay ; Genoni, Matteo ; Hernandez, Marcos ; Kotilainen, Jari ; Causi, Gianluca Li ; Mattila, Seppo ; Rappaport, Michael ; Radhakrishnan, Kalyan ; Ricci, Davide ; Riva, Marco ; Salasnich, Bernardo ; Smartt, Stephen ; Stritzinger, Maximilian ; Ventura, Hector</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a670-88937da005ec9470799d9764b8402de9ded02db94d6b9b268d7dcea0cccaca2b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Physics - 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to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS
will offer simultaneous wavelength coverage from 0.35 to 2.0 {\mu}m and will be
dedicated to the study of transient and variable sources. While nominal optical
performances of the system were presented in previous proceedings
(arXiv:1809.01521), we here present a set of further analyses aimed to identify
and quantify optical effects, due to changes in temperature and orientation of
the instrument during alignment and operations.</abstract><doi>10.48550/arxiv.2012.12680</doi><oa>free_for_read</oa></addata></record> |
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| identifier | DOI: 10.48550/arxiv.2012.12680 |
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| subjects | Physics - Instrumentation and Methods for Astrophysics |
| title | SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment |
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