Control, acquisition and quick-look software for infrared spectrometers
Identifieur interne :
000141 ( PascalFrancis/Curation );
précédent :
000140;
suivant :
000142
Control, acquisition and quick-look software for infrared spectrometers
Auteurs : Emanuel Rossetti [
Italie] ;
Ernesto Oliva [
Italie] ;
Livia Origlia [
Italie]
Source :
-
Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.
RBID : Pascal:11-0004572
Descripteurs français
English descriptors
Abstract
Modern IR spectrometers must be equipped with software well suited to a wide range of purposes, starting from the low level controls and going through acquisition, handling and fast quick-look of data. Such a complex software structure can be conveniently managed by means of dedicated GUIs which allow one to access the system at different levels: from the lowest (cryogenic controls) to the highest (data acquisition and quick-look). We will briefly describe the structure of this software, whose original characteristics is in the use of SQLite. We will also show a couple of results from our quick-look procedure based on customized DS9 and IRAF. The software architecture, that we present here, is general and can be adapted to any astronomical instruments. We have specifically implemented and tested it on GIANO spectrometer.
| pA |
| A01 | 01 | 1 | | @0 0277-786X |
|---|
| A02 | 01 | | | @0 PSISDG |
|---|
| A03 | | 1 | | @0 Proc. SPIE Int. Soc. Opt. Eng. |
|---|
| A05 | | | | @2 7740 |
|---|
| A06 | | | | @3 p. 2 |
|---|
| A08 | 01 | 1 | ENG | @1 Control, acquisition and quick-look software for infrared spectrometers |
|---|
| A09 | 01 | 1 | ENG | @1 Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States |
|---|
| A11 | 01 | 1 | | @1 ROSSETTI (Emanuel) |
|---|
| A11 | 02 | 1 | | @1 OLIVA (Ernesto) |
|---|
| A11 | 03 | 1 | | @1 ORIGLIA (Livia) |
|---|
| A12 | 01 | 1 | | @1 RADZIWILL (Nicole M.) @9 ed. |
|---|
| A12 | 02 | 1 | | @1 BRIDGER (Alan) @9 ed. |
|---|
| A14 | 01 | | | @1 Universita' di Bologna, Dipartimento di Astronomia, Via Ranzani 1 @2 40127 Bologna @3 ITA @Z 1 aut. |
|---|
| A14 | 02 | | | @1 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5 @2 50125 Firenze @3 ITA @Z 2 aut. |
|---|
| A14 | 03 | | | @1 INAF, Osservatorio Astronomico di Bologna, Via Ranzani 1 @2 40127 Bologna @3 ITA @Z 3 aut. |
|---|
| A18 | 01 | 1 | | @1 SPIE @3 USA @9 org-cong. |
|---|
| A18 | 02 | 1 | | @1 American Astronomical Society @3 USA @9 org-cong. |
|---|
| A20 | | | | @2 774032.1-774032.10 |
|---|
| A21 | | | | @1 2010 |
|---|
| A23 | 01 | | | @0 ENG |
|---|
| A25 | 01 | | | @1 SPIE @2 Bellingham, Wash. |
|---|
| A26 | 01 | | | @0 978-0-8194-8230-3 |
|---|
| A26 | 02 | | | @0 0-8194-8230-7 |
|---|
| A43 | 01 | | | @1 INIST @2 21760 @5 354000174702881000 |
|---|
| A44 | | | | @0 0000 @1 © 2011 INIST-CNRS. All rights reserved. |
|---|
| A45 | | | | @0 8 ref. |
|---|
| A47 | 01 | 1 | | @0 11-0004572 |
|---|
| A60 | | | | @1 P @2 C |
|---|
| A61 | | | | @0 A |
|---|
| A64 | 01 | 1 | | @0 Proceedings of SPIE, the International Society for Optical Engineering |
|---|
| A66 | 01 | | | @0 USA |
|---|
| C01 | 01 | | ENG | @0 Modern IR spectrometers must be equipped with software well suited to a wide range of purposes, starting from the low level controls and going through acquisition, handling and fast quick-look of data. Such a complex software structure can be conveniently managed by means of dedicated GUIs which allow one to access the system at different levels: from the lowest (cryogenic controls) to the highest (data acquisition and quick-look). We will briefly describe the structure of this software, whose original characteristics is in the use of SQLite. We will also show a couple of results from our quick-look procedure based on customized DS9 and IRAF. The software architecture, that we present here, is general and can be adapted to any astronomical instruments. We have specifically implemented and tested it on GIANO spectrometer. |
|---|
| C02 | 01 | X | | @0 001D02B09 |
|---|
| C03 | 01 | X | FRE | @0 Interface utilisateur @5 06 |
|---|
| C03 | 01 | X | ENG | @0 User interface @5 06 |
|---|
| C03 | 01 | X | SPA | @0 Interfase usuario @5 06 |
|---|
| C03 | 02 | X | FRE | @0 Spectromètre @5 18 |
|---|
| C03 | 02 | X | ENG | @0 Spectrometer @5 18 |
|---|
| C03 | 02 | X | SPA | @0 Espectrómetro @5 18 |
|---|
| C03 | 03 | X | FRE | @0 Personnalisation @5 19 |
|---|
| C03 | 03 | X | ENG | @0 Customization @5 19 |
|---|
| C03 | 03 | X | SPA | @0 Personalización @5 19 |
|---|
| C03 | 04 | X | FRE | @0 Astrophysique @5 20 |
|---|
| C03 | 04 | X | ENG | @0 Astrophysics @5 20 |
|---|
| C03 | 04 | X | SPA | @0 Astrofísica @5 20 |
|---|
| C03 | 05 | X | FRE | @0 Architecture logiciel @4 CD @5 96 |
|---|
| C03 | 05 | X | ENG | @0 Software architecture @4 CD @5 96 |
|---|
| C03 | 05 | X | SPA | @0 Arquitectura logicial @4 CD @5 96 |
|---|
| N21 | | | | @1 003 |
|---|
| N44 | 01 | | | @1 OTO |
|---|
| N82 | | | | @1 OTO |
|---|
|
|---|
| pR |
| A30 | 01 | 1 | ENG | @1 Software and cyberinfrastructure for astronomy @3 San Diego CA USA @4 2010 |
|---|
|
|---|
Links toward previous steps (curation, corpus...)
- to stream PascalFrancis, to step Corpus: Pour aller vers cette notice dans l'étape Curation :000104
Links to Exploration step
Pascal:11-0004572
Le document en format XML
<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Control, acquisition and quick-look software for infrared spectrometers</title>
<author><name sortKey="Rossetti, Emanuel" sort="Rossetti, Emanuel" uniqKey="Rossetti E" first="Emanuel" last="Rossetti">Emanuel Rossetti</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Universita' di Bologna, Dipartimento di Astronomia, Via Ranzani 1</s1>
<s2>40127 Bologna</s2>
<s3>ITA</s3>
<sZ>1 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><author><name sortKey="Oliva, Ernesto" sort="Oliva, Ernesto" uniqKey="Oliva E" first="Ernesto" last="Oliva">Ernesto Oliva</name>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5</s1>
<s2>50125 Firenze</s2>
<s3>ITA</s3>
<sZ>2 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><author><name sortKey="Origlia, Livia" sort="Origlia, Livia" uniqKey="Origlia L" first="Livia" last="Origlia">Livia Origlia</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF, Osservatorio Astronomico di Bologna, Via Ranzani 1</s1>
<s2>40127 Bologna</s2>
<s3>ITA</s3>
<sZ>3 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">11-0004572</idno>
<date when="2010">2010</date>
<idno type="stanalyst">PASCAL 11-0004572 INIST</idno>
<idno type="RBID">Pascal:11-0004572</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000104</idno>
<idno type="wicri:Area/PascalFrancis/Curation">000141</idno>
</publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Control, acquisition and quick-look software for infrared spectrometers</title>
<author><name sortKey="Rossetti, Emanuel" sort="Rossetti, Emanuel" uniqKey="Rossetti E" first="Emanuel" last="Rossetti">Emanuel Rossetti</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Universita' di Bologna, Dipartimento di Astronomia, Via Ranzani 1</s1>
<s2>40127 Bologna</s2>
<s3>ITA</s3>
<sZ>1 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><author><name sortKey="Oliva, Ernesto" sort="Oliva, Ernesto" uniqKey="Oliva E" first="Ernesto" last="Oliva">Ernesto Oliva</name>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5</s1>
<s2>50125 Firenze</s2>
<s3>ITA</s3>
<sZ>2 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><author><name sortKey="Origlia, Livia" sort="Origlia, Livia" uniqKey="Origlia L" first="Livia" last="Origlia">Livia Origlia</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF, Osservatorio Astronomico di Bologna, Via Ranzani 1</s1>
<s2>40127 Bologna</s2>
<s3>ITA</s3>
<sZ>3 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><series><title level="j" type="main">Proceedings of SPIE, the International Society for Optical Engineering</title>
<title level="j" type="abbreviated">Proc. SPIE Int. Soc. Opt. Eng.</title>
<idno type="ISSN">0277-786X</idno>
<imprint><date when="2010">2010</date>
</imprint><seriesStmt><title level="j" type="main">Proceedings of SPIE, the International Society for Optical Engineering</title>
<title level="j" type="abbreviated">Proc. SPIE Int. Soc. Opt. Eng.</title>
<idno type="ISSN">0277-786X</idno>
</seriesStmt><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Astrophysics</term>
<term>Customization</term>
<term>Software architecture</term>
<term>Spectrometer</term>
<term>User interface</term>
</keywords><keywords scheme="Pascal" xml:lang="fr"><term>Interface utilisateur</term>
<term>Spectromètre</term>
<term>Personnalisation</term>
<term>Astrophysique</term>
<term>Architecture logiciel</term>
</keywords><front><div type="abstract" xml:lang="en">Modern IR spectrometers must be equipped with software well suited to a wide range of purposes, starting from the low level controls and going through acquisition, handling and fast quick-look of data. Such a complex software structure can be conveniently managed by means of dedicated GUIs which allow one to access the system at different levels: from the lowest (cryogenic controls) to the highest (data acquisition and quick-look). We will briefly describe the structure of this software, whose original characteristics is in the use of SQLite. We will also show a couple of results from our quick-look procedure based on customized DS9 and IRAF. The software architecture, that we present here, is general and can be adapted to any astronomical instruments. We have specifically implemented and tested it on GIANO spectrometer.</div>
</front><inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0277-786X</s0>
</fA01><fA02 i1="01"><s0>PSISDG</s0>
</fA02><fA03 i2="1"><s0>Proc. SPIE Int. Soc. Opt. Eng.</s0>
</fA03><fA05><s2>7740</s2>
</fA05><fA06><s3>p. 2</s3>
</fA06><fA08 i1="01" i2="1" l="ENG"><s1>Control, acquisition and quick-look software for infrared spectrometers</s1>
</fA08><fA09 i1="01" i2="1" l="ENG"><s1>Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States</s1>
</fA09><fA11 i1="01" i2="1"><s1>ROSSETTI (Emanuel)</s1>
</fA11><fA11 i1="02" i2="1"><s1>OLIVA (Ernesto)</s1>
</fA11><fA11 i1="03" i2="1"><s1>ORIGLIA (Livia)</s1>
</fA11><fA12 i1="01" i2="1"><s1>RADZIWILL (Nicole M.)</s1>
<s9>ed.</s9>
</fA12><fA12 i1="02" i2="1"><s1>BRIDGER (Alan)</s1>
<s9>ed.</s9>
</fA12><fA14 i1="01"><s1>Universita' di Bologna, Dipartimento di Astronomia, Via Ranzani 1</s1>
<s2>40127 Bologna</s2>
<s3>ITA</s3>
<sZ>1 aut.</sZ>
</fA14><fA14 i1="02"><s1>INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5</s1>
<s2>50125 Firenze</s2>
<s3>ITA</s3>
<sZ>2 aut.</sZ>
</fA14><fA14 i1="03"><s1>INAF, Osservatorio Astronomico di Bologna, Via Ranzani 1</s1>
<s2>40127 Bologna</s2>
<s3>ITA</s3>
<sZ>3 aut.</sZ>
</fA14><fA18 i1="01" i2="1"><s1>SPIE</s1>
<s3>USA</s3>
<s9>org-cong.</s9>
</fA18><fA18 i1="02" i2="1"><s1>American Astronomical Society</s1>
<s3>USA</s3>
<s9>org-cong.</s9>
</fA18><fA20><s2>774032.1-774032.10</s2>
</fA20><fA21><s1>2010</s1>
</fA21><fA23 i1="01"><s0>ENG</s0>
</fA23><fA25 i1="01"><s1>SPIE</s1>
<s2>Bellingham, Wash.</s2>
</fA25><fA26 i1="01"><s0>978-0-8194-8230-3</s0>
</fA26><fA26 i1="02"><s0>0-8194-8230-7</s0>
</fA26><fA43 i1="01"><s1>INIST</s1>
<s2>21760</s2>
<s5>354000174702881000</s5>
</fA43><fA44><s0>0000</s0>
<s1>© 2011 INIST-CNRS. All rights reserved.</s1>
</fA44><fA45><s0>8 ref.</s0>
</fA45><fA47 i1="01" i2="1"><s0>11-0004572</s0>
</fA47><fA60><s1>P</s1>
<s2>C</s2>
</fA60><fA64 i1="01" i2="1"><s0>Proceedings of SPIE, the International Society for Optical Engineering</s0>
</fA64><fA66 i1="01"><s0>USA</s0>
</fA66><fC01 i1="01" l="ENG"><s0>Modern IR spectrometers must be equipped with software well suited to a wide range of purposes, starting from the low level controls and going through acquisition, handling and fast quick-look of data. Such a complex software structure can be conveniently managed by means of dedicated GUIs which allow one to access the system at different levels: from the lowest (cryogenic controls) to the highest (data acquisition and quick-look). We will briefly describe the structure of this software, whose original characteristics is in the use of SQLite. We will also show a couple of results from our quick-look procedure based on customized DS9 and IRAF. The software architecture, that we present here, is general and can be adapted to any astronomical instruments. We have specifically implemented and tested it on GIANO spectrometer.</s0>
</fC01><fC02 i1="01" i2="X"><s0>001D02B09</s0>
</fC02><fC03 i1="01" i2="X" l="FRE"><s0>Interface utilisateur</s0>
<s5>06</s5>
</fC03><fC03 i1="01" i2="X" l="ENG"><s0>User interface</s0>
<s5>06</s5>
</fC03><fC03 i1="01" i2="X" l="SPA"><s0>Interfase usuario</s0>
<s5>06</s5>
</fC03><fC03 i1="02" i2="X" l="FRE"><s0>Spectromètre</s0>
<s5>18</s5>
</fC03><fC03 i1="02" i2="X" l="ENG"><s0>Spectrometer</s0>
<s5>18</s5>
</fC03><fC03 i1="02" i2="X" l="SPA"><s0>Espectrómetro</s0>
<s5>18</s5>
</fC03><fC03 i1="03" i2="X" l="FRE"><s0>Personnalisation</s0>
<s5>19</s5>
</fC03><fC03 i1="03" i2="X" l="ENG"><s0>Customization</s0>
<s5>19</s5>
</fC03><fC03 i1="03" i2="X" l="SPA"><s0>Personalización</s0>
<s5>19</s5>
</fC03><fC03 i1="04" i2="X" l="FRE"><s0>Astrophysique</s0>
<s5>20</s5>
</fC03><fC03 i1="04" i2="X" l="ENG"><s0>Astrophysics</s0>
<s5>20</s5>
</fC03><fC03 i1="04" i2="X" l="SPA"><s0>Astrofísica</s0>
<s5>20</s5>
</fC03><fC03 i1="05" i2="X" l="FRE"><s0>Architecture logiciel</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03><fC03 i1="05" i2="X" l="ENG"><s0>Software architecture</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03><fC03 i1="05" i2="X" l="SPA"><s0>Arquitectura logicial</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03><fN21><s1>003</s1>
</fN21><fN44 i1="01"><s1>OTO</s1>
</fN44><fN82><s1>OTO</s1>
</fN82><pR><fA30 i1="01" i2="1" l="ENG"><s1>Software and cyberinfrastructure for astronomy</s1>
<s3>San Diego CA USA</s3>
<s4>2010</s4>
</fA30>
Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Ticri/CIDE/explor/CyberinfraV1/Data/PascalFrancis/Curation
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000141 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/PascalFrancis/Curation/biblio.hfd -nk 000141 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Ticri/CIDE
|area= CyberinfraV1
|flux= PascalFrancis
|étape= Curation
|type= RBID
|clé= Pascal:11-0004572
|texte= Control, acquisition and quick-look software for infrared spectrometers
}}
| This area was generated with Dilib version V0.6.25.
Data generation: Thu Oct 27 09:30:58 2016. Site generation: Sun Mar 10 23:08:40 2024 |  |
