{"id":688,"date":"2024-04-05T16:48:48","date_gmt":"2024-04-05T14:48:48","guid":{"rendered":"https:\/\/uscc.inaf.it\/?page_id=688"},"modified":"2026-03-27T15:37:30","modified_gmt":"2026-03-27T14:37:30","slug":"inaf-made-software","status":"publish","type":"page","link":"https:\/\/uscc.inaf.it\/en\/struttura-organizzativa\/settore-4-servizi-informatici\/inaf-made-software\/","title":{"rendered":"INAF made Software"},"content":{"rendered":"<p class=\"wp-block-paragraph\">Plenty of useful software have been made by INAF researchers. It is not always easy to find references or even know about the existence of such software. A system connect with the new <strong>INAF-CRIS<\/strong> is under development and a list of INAF software will be available soon<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><a href=\"https:\/\/uscc.inaf.it\/en\/?page_id=692\" data-type=\"page\" data-id=\"692\">The Open Source Licence suggest from INAF is GNU GPL 3<\/a><\/p>\n\n\n\n<h2 class=\"wp-block-heading has-text-color has-link-color wp-elements-a4b9fd87ccf0cd1fe8858aff3f152f53\" style=\"color:#021034;padding-top:0.4rem;padding-right:0px;padding-bottom:0px;padding-left:0rem;font-size:clamp(0.929rem, 0.929rem + ((1vw - 0.2rem) * 0.769), 1.4rem);font-style:normal;font-weight:400;letter-spacing:1px;line-height:1;text-transform:uppercase\"><em>Software with DOI \u2013 INAF<\/em><\/h2>\n\n\n\n<figure style=\"margin-bottom:var(--wp--preset--spacing--large)\" class=\"wp-block-table\"><table><tbody><tr><td>DISCOS<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00001\">10.20371\/INAF\/SW\/2019_00001<\/a><\/td><\/tr><tr><td>GOFIO<\/td><td><a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00002\">&nbsp;10.20371\/INAF\/SW\/2019_00002<\/a><\/td><\/tr><tr><td>Osservazioni Multi-Banda<\/td><td><a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00003\">&nbsp;10.20371\/INAF\/SW\/2019_00003<\/a><\/td><\/tr><tr><td>Solar System<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00004\">10.20371\/INAF\/SW\/2019_00004<\/a><\/td><\/tr><tr><td>Stability Valley<\/td><td><a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00005\">&nbsp;10.20371\/INAF\/SW\/2019_00005<\/a><\/td><\/tr><tr><td>InsideStars<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00006\">10.20371\/INAF\/SW\/2019_00006<\/a><\/td><\/tr><tr><td>geologic-symbols-qgis<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00007\">10.20371\/INAF\/SW\/2019_00007<\/a><\/td><\/tr><tr><td>Pymoondb<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00008\">10.20371\/INAF\/SW\/2019_00008<\/a><\/td><\/tr><tr><td>PacketLib<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2019_00009\">10.20371\/INAF\/SW\/2019_00009<\/a><\/td><\/tr><tr><td>SCOSpy<\/td><td><a href=\"http:\/\/dx.doi.org\/10.20371\/INAF\/SW\/2020_00001\">&nbsp;10.20371\/INAF\/SW\/2020_00001<\/a><\/td><\/tr><tr><td>SpectraPy<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/inaf\/sw\/2021_00001\">10.20371\/inaf\/sw\/2021_00001<\/a><\/td><\/tr><tr><td>SIPGI<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/inaf\/sw\/2021_00002\">10.20371\/inaf\/sw\/2021_00002<\/a><\/td><\/tr><tr><td>Starfinder<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/inaf\/sw\/2022_00001\">10.20371\/inaf\/sw\/2022_00001<\/a><\/td><\/tr><tr><td>PATCH<\/td><td>&nbsp;<a href=\"http:\/\/dx.doi.org\/10.20371\/inaf\/sw\/2022_00001\">10.20371\/inaf\/sw\/2022_00001<\/a><\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n<h2 class=\"wp-block-heading has-text-color has-link-color wp-elements-c1cb0e0582da75bc13ce583cac61a6ad\" style=\"color:#021034;padding-top:0.4rem;padding-right:0px;padding-bottom:0px;padding-left:0rem;font-size:clamp(0.929rem, 0.929rem + ((1vw - 0.2rem) * 0.769), 1.4rem);font-style:normal;font-weight:400;letter-spacing:1px;line-height:1;text-transform:uppercase\"><em>Other softwares from<\/em> <em>INAF<\/em><\/h2>\n\n\n\n<figure class=\"wp-block-table\"><table class=\"has-fixed-layout\"><tbody><tr><td><em><strong>Nome<\/strong><\/em><\/td><td><em><strong>Link<\/strong><\/em><\/td><td><em><strong>Refered Person<\/strong><\/em><\/td><td><em><strong>info<\/strong><\/em><\/td><\/tr><tr><td>AETEC<\/td><td><a href=\"http:\/\/aetc.oapd.inaf.it\/\">aetc.oapd.inaf.it<\/a><\/td><td>D. Fantinel<\/td><td>The Advanced Exposure Time Calculator (AETC) is a tool to simulate images of astrophysical objects obtained with any combination of telescope, instrument and given passband using a suitable set of parameters that define the configuration of the equipment used for the observations<\/td><\/tr><tr><td>APHOT<\/td><td><a href=\"https:\/\/www.oa-roma.inaf.it\/merlin\/2019\/05\/01\/a-phot\/\">https:\/\/www.oa-roma.inaf.it\/merlin\/2019\/05\/01\/a-phot\/<\/a><\/td><td>E. Merlin<\/td><td>fotometria in apertura di campi fondi extragalattic<\/td><\/tr><tr><td>APOGEO<\/td><td><a href=\"https:\/\/www.ia2.inaf.it\/index.php\/13-software\/35-apogeo\">https:\/\/www.ia2.inaf.it\/index.php\/13-software\/35-apogeo<\/a><\/td><td>S. Zorba<\/td><td>&nbsp;<\/td><\/tr><tr><td>Astrocook<\/td><td><a href=\"https:\/\/github.com\/DAS-OATs\/astrocook\">https:\/\/github.com\/DAS-OATs\/astrocook<\/a><\/td><td>G. Cupani<\/td><td>Quasar Spectral Analysis with GUI<\/td><\/tr><tr><td>Bayesfit<\/td><td><a href=\"http:\/\/www.brera.mi.astro.it\/~stefano.andreon\/BayesianMethodsForThePhysicalSciences\/\">http:\/\/www.brera.mi.astro.it\/~stefano.andreon\/BayesianMethodsForThePhysicalSciences\/<\/a>&nbsp;(cliccare su &#8220;model&#8221;)<\/td><td>S. Andreon<\/td><td>library of fit Bayesian models for fitting astronomical data<\/td><\/tr><tr><td>CARACal<\/td><td><a href=\"https:\/\/github.com\/caracal-pipeline\/caracal\">https:\/\/github.com\/caracal-pipeline\/caracal<\/a><\/td><td>P. Serra<\/td><td>&nbsp;pipeline for radio interferometry data reduction&nbsp;<br><a href=\"https:\/\/caracal.readthedocs.io\/\">link to HomePage<\/a><\/td><\/tr><tr><td>DIAMONDS<\/td><td><a class=\"\" href=\"https:\/\/github.com\/EnricoCorsaro\/DIAMONDS\">https:\/\/github.com\/EnricoCorsaro\/DIAMONDS<\/a>&nbsp;e ha anche un sito web di documentazione, incluso un manuale guida per utente e tutorial.<a class=\"\" href=\"https:\/\/diamonds.readthedocs.io\/\">https:\/\/diamonds.readthedocs.io<\/a><\/td><td>&nbsp;E. Corsaro<\/td><td>&nbsp;Il sistema&nbsp;<strong>DIAMONDS<\/strong>&nbsp;(high-<strong>DI<\/strong>mensional&nbsp;<strong>A<\/strong>nd multi-<strong>MO<\/strong>dal&nbsp;<strong>N<\/strong>este<strong>D<\/strong>&nbsp;<strong>S<\/strong>ampling) code performs a Bayesian parameter estimation and model comparison by means of the nested sampling Monte Carlo (NSMC) algorithm.<\/td><\/tr><tr><td>DIF<\/td><td><a href=\"https:\/\/github.com\/lnicastro\/DIF\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/github.com\/lnicastro\/DIF<\/a><\/td><td>L. Nicastro<\/td><td>A set of tools that use HTM and HEALPix to implement an indexing system for astronomical catalogs and other data with spherical coordinates stored in MySQL \/ MariaDB.<\/td><\/tr><tr><td>DPI<\/td><td><a href=\"http:\/\/arxes.iaps.inaf.it\/DownloadSoftware\/dpi-1_0.tar.gz\">http:\/\/arxes.iaps.inaf.it\/DownloadSoftware\/dpi-1_0.tar.gz<\/a><\/td><td>D. Turrini<\/td><td>a Fortran library implementing the symplectic mapping for binary star systems for the&nbsp;<strong>Mercury<\/strong>&nbsp;6 N-Body software package<\/td><\/tr><tr><td>EasyLife<\/td><td><a href=\"https:\/\/www.iasf-milano.inaf.it\/software\/\">https:\/\/www.iasf-milano.inaf.it\/software\/<\/a><\/td><td>M. Scodeggio<\/td><td>&nbsp;<\/td><\/tr><tr><td>SNOoPY<\/td><td><a href=\"http:\/\/sngroup.oapd.inaf.it\/snoopy.html\">http:\/\/sngroup.oapd.inaf.it\/snoopy.html<\/a><\/td><td>E. Cappellaro<\/td><td>&nbsp;SNOoPY (SuperNOva PhotometrY) is a package designed to facilitate the task of producing SN light curves from multi-band photometric observations obtained with a generic collection of telescopes.<\/td><\/tr><tr><td>FAMA<\/td><td><a href=\"https:\/\/ascl.net\/1402.016\">https:\/\/ascl.net\/1402.016<\/a><\/td><td>L. Magrini<\/td><td>Fast Automatic MOOG Analysis<\/td><\/tr><tr><td>FAMED<\/td><td><a class=\"\" href=\"https:\/\/github.com\/EnricoCorsaro\/FAMED\">https:\/\/github.com\/EnricoCorsaro\/FAMED<\/a>&nbsp;con sito web di documentazione e tutorial<a class=\"\" href=\"https:\/\/famed.readthedocs.io\/\">https:\/\/famed.readthedocs.io<\/a><\/td><td>E. Corsaro<\/td><td>Il sistema&nbsp;<strong>FAMED<\/strong>&nbsp;(<strong>F<\/strong>ast and&nbsp;<strong>A<\/strong>uto-<strong>M<\/strong>ated p<strong>E<\/strong>ak bagging with&nbsp;<strong>D<\/strong>iamonds) pipeline is a multi-platform parallelized software to perform an automated extraction and mode identification of oscillation frequencies for solar-like pulsators.<\/td><\/tr><tr><td>foscgui<\/td><td><a href=\"http:\/\/sngroup.oapd.inaf.it\/foscgui.html\">http:\/\/sngroup.oapd.inaf.it\/foscgui.html<\/a><\/td><td>E. Cappellaro<\/td><td>Foscgui is a graphic user interface aimed at extracting SN spectra and photometry obtained with a fosc-like instrument. In the current version two instruments are implemented AFOSC@182cm Asiago, ALFOSC@NOT La Palma<\/td><\/tr><tr><td>GalNest<\/td><td>&nbsp;<\/td><td>M. Rivi<\/td><td>Rilevazione sorgenti da survey nella banda radio, analizzando direttamente le visibilit\u00e0 radio.<\/td><\/tr><tr><td>GHATS<\/td><td><a href=\"http:\/\/www.brera.inaf.it\/utenti\/belloni\/GHATS_Package\/Home.html\">http:\/\/www.brera.inaf.it\/utenti\/belloni\/GHATS_Package\/Home.html<\/a><\/td><td>T. Belloni<\/td><td>analisi temporale aperiodica di dati X.<\/td><\/tr><tr><td>HENDRICS<\/td><td><a href=\"https:\/\/github.com\/stingraysoftware\/hendrics\">https:\/\/github.com\/stingraysoftware\/hendrics<\/a><\/td><td>M. Bachetti<\/td><td>&nbsp;<\/td><\/tr><tr><td>Ice Thickness Calculator<\/td><td><mark>TB<\/mark><mark>D<\/mark><\/td><td>C. Scire&#8217;<\/td><td>interfaccia&nbsp;software disponibile online per il calcolo dello spessore di sottili strati di ghiacci depositati su un substrato<\/td><\/tr><tr><td>Intranet<\/td><td><a href=\"http:\/\/intranet.ifc.inaf.it\">http:\/\/intranet.ifc.inaf.it<\/a><\/td><td>F. D&#8217;Anna<\/td><td>sw di gestione sito d&#8217;istituto<\/td><\/tr><tr><td>jExact<\/td><td><a href=\"https:\/\/github.com\/RomoloPoliti\/jExact\">https:\/\/github.com\/RomoloPoliti\/jExact<\/a><\/td><td>R. Politi<\/td><td>interfaccia java per l&#8217;accesso alla webapp&nbsp;exact<\/td><\/tr><tr><td>JoXSZ<\/td><td><a href=\"https:\/\/www.google.com\/url?q=https:\/\/github.com\/fcastagna\/JoXSZ&amp;sa=D&amp;ust=1591614642879000&amp;usg=AOvVaw3Qrbcl5FI87erctDE7hmSk\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/github.com\/fcastagna\/JoXSZ<\/a>(<a href=\"https:\/\/www.google.com\/url?q=https:\/\/arxiv.org\/abs\/2005.12315&amp;sa=D&amp;ust=1591614642879000&amp;usg=AOvVaw3a_YVAcqXmvrenZHxYSaPF\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/arxiv.org\/abs\/2005.12315<\/a>).<\/td><td>F.&nbsp;Castagna<\/td><td>fit sulle propriet\u00e0 termodinamiche degli ammassi di galassie considerando congiuntamente dati in X e in SZ (effetto Sunyaev-Zeldovich).<\/td><\/tr><tr><td>LIRA<\/td><td><a href=\"https:\/\/cran.r-project.org\/web\/packages\/lira\/index.html\">https:\/\/cran.r-project.org\/web\/packages\/lira\/index.html<\/a><\/td><td>M. Sereno<\/td><td>Linear Regression in Atronomy<\/td><\/tr><tr><td>MCS<\/td><td><a href=\"https:\/\/github.com\/gcalderone\/MCS\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/github.com\/gcalderone\/MCS<\/a><\/td><td>L. Nicastro<br>G. Calderone<\/td><td>Multi-purpose, MySQL oriented classes aimed at implementing astronomical applications in (almost) any language.<\/td><\/tr><tr><td>MeerKATHI<\/td><td>&nbsp;<a href=\"https:\/\/meerkathi.readthedocs.io\/en\/latest\/index.html\">https:\/\/meerkathi.readthedocs.io\/en\/latest\/index.html<\/a><\/td><td>P. Serra<\/td><td>radio interferometry pipeline<\/td><\/tr><tr><td>Mercury-Arxes<\/td><td><a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ab18f5\/meta\">Turrini et al. 2019, ApJ, 877, 50<\/a><\/td><td>D. Turrini<\/td><td>a Fortran parallel implementation of the hybrid symplectic algorithm of the&nbsp;<strong>Mercury<\/strong>&nbsp;6 N-Body software package<\/td><\/tr><tr><td>MyRO<\/td><td><a href=\"https:\/\/github.com\/lnicastro\/MyRO\">https:\/\/github.com\/lnicastro\/MyRO<\/a><\/td><td>L. Nicastro<\/td><td>A set of tools aimed at implementing a per-record privilege system on MySQL databases similar to that of a unix file system.<\/td><\/tr><tr><td>NADIR<\/td><td><a href=\"https:\/\/www.ia2.inaf.it\/index.php\/13-software\/32-ia2-software-2\">https:\/\/www.ia2.inaf.it\/index.php\/13-software\/32-ia2-software-2<\/a><\/td><td>C. Knapic<\/td><td>archive management<\/td><\/tr><tr><td>PaketLib<\/td><td><a href=\"https:\/\/github.com\/ASTRO-BO\/PacketLib\">https:\/\/github.com\/ASTRO-BO\/PacketLib<\/a><\/td><td>A. Bulgarelli<\/td><td>PacketLib is a C++ open-source software library for writing applications which deal with satellite telemetry source packets, provided that the packets are compliant with the CCSDS Telemetry and Telecommand Standards.<\/td><\/tr><tr><td>PASSATA<\/td><td><a href=\"http:\/\/aowiki.arcetri.inaf.it\/Public\/PassataSoftPublic\">http:\/\/aowiki.arcetri.inaf.it\/Public\/PassataSoftPublic<\/a> <\/td><td>G. Agapito<\/td><td>ibreria IDL per simulazioni end-to-end di sistemi di Ottica Adattiva<\/td><\/tr><tr><td>PI GCS<\/td><td><a href=\"https:\/\/github.com\/lbusoni\/pi_gcs\">https:\/\/github.com\/lbusoni\/pi_gcs<\/a><\/td><td>L. Busoni<\/td><td>Python wrapper&nbsp;for Physik Instrument&nbsp;General Command Set API.<\/td><\/tr><tr><td>Pinocchio<\/td><td><a href=\"https:\/\/github.com\/pigimonaco\/Pinocchio\">https:\/\/github.com\/pigimonaco\/Pinocchio<\/a><\/td><td>P. Monaco<\/td><td>metodo approssimato per le simulazioni cosmologiche<\/td><\/tr><tr><td>Plico<\/td><td><a href=\"https:\/\/github.com\/lbusoni\/plico\">https:\/\/github.com\/lbusoni\/plico<\/a><\/td><td>L. Busoni<\/td><td>Python Laboratory Instrumentation COntrol. Provides a framework client\/server to interface devices and expose control over the network.<\/td><\/tr><tr><td>PreProFit<\/td><td><a href=\"https:\/\/github.com\/fcastagna\/preprofit\">https:\/\/github.com\/fcastagna\/preprofit<\/a><\/td><td>F. Castragna<\/td><td>fit del profilo di pressione di cluster di galassie tramite un approccio bayesiano<\/td><\/tr><tr><td>Pymoondb<\/td><td><a href=\"https:\/\/ict.inaf.it\/gitlab\/alessandro.frigeri\/pymoondb\">https:\/\/www.ict.inaf.it\/gitlab\/alessandro.frigeri\/pymoondb<\/a><\/td><td>A. Frigeri<\/td><td>The Python interface to MoonDB, the online lunar sample geochemical and petrological database<\/td><\/tr><tr><td>QGIS<\/td><td><a href=\"https:\/\/github.com\/afrigeri\/geologic-symbols-qgis\">https:\/\/github.com\/afrigeri\/geologic-symbols-qgis<\/a><\/td><td>A. Frigeri<\/td><td>Geologic symbols library and development for QGIS<\/td><\/tr><tr><td>QSFit<\/td><td><a href=\"https:\/\/qsfit.inaf.it\/\">https:\/\/qsfit.inaf.it\/<\/a><\/td><td>G. Calderone<\/td><td>QSO Spectral Fitting: software package to automatically perform spectral analysis of Active Galactic Nuclei (AGN) optical\/UV spectra<\/td><\/tr><tr><td>RadioLensFit<\/td><td><a href=\"https:\/\/github.com\/marziarivi\/RadioLensfit2\">https:\/\/github.com\/marziarivi\/RadioLensfit2<\/a><\/td><td>M. Rivi<\/td><td>misura radio week lensing shear<\/td><\/tr><tr><td>SDI<\/td><td>&nbsp;<\/td><td>A. Pellizzoni<\/td><td>(Single Dish Imager), un sw scientifico di mapping radioastronomico per osservazioni single-dish<\/td><\/tr><tr><td>SID<\/td><td><a href=\"https:\/\/github.com\/lnicastro\/SID\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/github.com\/lnicastro\/SID<\/a><\/td><td>L. Nicastro<\/td><td>A set of tools that use HTM and HEALPix to implement an indexing system for astronomical catalogs and other data with spherical coordinates stored in MySQL \/ MariaDB. Mostly derived from&nbsp;<a href=\"https:\/\/github.com\/lnicastro\/DIF\" target=\"_blank\" rel=\"noreferrer noopener\">DIF<\/a>, with the main difference being its fully UDFs structure which makes it more flexible.<\/td><\/tr><tr><td>SoFiA<\/td><td><a href=\"https:\/\/github.com\/SoFiA-Admin\/SoFiA\">https:\/\/github.com\/SoFiA-Admin\/SoFiA<\/a><\/td><td>P. Serra<\/td><td>spectral line Source finder<br><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2015MNRAS.448.1922S\">Link all&#8217;articolo<\/a><\/td><\/tr><tr><td>STARFINDER<\/td><td><a href=\"https:\/\/www.oas.inaf.it\/en\/research\/m5-en\/starfinder-en\/\">https:\/\/www.oas.inaf.it\/en\/research\/m5-en\/starfinder-en\/<\/a><\/td><td>L. Schreiber<\/td><td>astro fotometria PSF di campi stellari particolarmente adatto per immagini corrette da ottica adattiva<\/td><\/tr><tr><td>Stingray<\/td><td><a href=\"https:\/\/github.com\/stingraysoftware\/stingray\">https:\/\/github.com\/stingraysoftware\/stingray<\/a><\/td><td>M. Bachetti<\/td><td>&nbsp;<\/td><\/tr><tr><td>TASMAN<\/td><td><a href=\"https:\/\/www.ia2.inaf.it\/index.php\/13-software\/36-tap-schema-manager\">https:\/\/www.ia2.inaf.it\/index.php\/13-software\/36-tap-schema-manager<\/a><\/td><td>S. Zorba<\/td><td>&nbsp;<\/td><\/tr><tr><td>TOCats<\/td><td><a href=\"https:\/\/catsweb.oas.inaf.it\/\">https:\/\/catsweb.oas.inaf.it\/<\/a> <\/td><td>L. Nicastro<\/td><td>Astronomical catalogues stored in a hierarchical tree using DIF + HEALPix schema, browsable in AladinLite and accessible either via web-form or directly via SQL. Custom users&#8217; catalogues can be hosted on request.<\/td><\/tr><tr><td>TOSC<\/td><td><a href=\"https:\/\/www.aanda.org\/articles\/aa\/full_html\/2017\/10\/aa30966-17\/aa30966-17.html\">https:\/\/www.aanda.org\/articles\/aa\/full_html\/2017\/10\/aa30966-17\/aa30966-17.html<\/a><\/td><td>S. Scandariato<\/td><td>an algorithm for the tomography of spotted transit chords<\/td><\/tr><tr><td>TPHOT<\/td><td><a href=\"https:\/\/www.oa-roma.inaf.it\/merlin\/2019\/04\/15\/t-phot\/\">https:\/\/www.oa-roma.inaf.it\/merlin\/2019\/04\/15\/t-phot\/<\/a><\/td><td>E. Merlin<\/td><td>fotometria template-fitting&nbsp; di campi fondi extragalattic<\/td><\/tr><tr><td>VAPE<\/td><td><a href=\"https:\/\/www.ia2.inaf.it\/index.php\/13-software\/34-vape\">https:\/\/www.ia2.inaf.it\/index.php\/13-software\/34-vape<\/a><\/td><td>M. Molinaro<\/td><td>&nbsp;<\/td><\/tr><tr><td>VIRTISpy<\/td><td><a href=\"https:\/\/github.com\/VIRTIS-VEX\/VIRTISpy\">https:\/\/github.com\/VIRTIS-VEX\/VIRTISpy<\/a><\/td><td>R. Politi<\/td><td>classe python per la lettura dei dati raccolti dallo strumento VIRTIS a bordo della sonda Venus Express<\/td><\/tr><tr><td>VO-Dance<\/td><td><a href=\"https:\/\/www.ia2.inaf.it\/index.php\/13-software\/33-vo-dance\">https:\/\/www.ia2.inaf.it\/index.php\/13-software\/33-vo-dance<\/a><\/td><td>M. Molinaro<\/td><td>VO&nbsp;<\/td><\/tr><tr><td>XNS<\/td><td><a href=\"http:\/\/www.arcetri.inaf.it\/science\/ahead\/XNS\/\">http:\/\/www.arcetri.inaf.it\/science\/ahead\/XNS\/<\/a><\/td><td>N. Bucciantini<\/td><td>modelli teorici di Neuron Star in GR<\/td><\/tr><tr><td>zmxIDL<\/td><td><a href=\"https:\/\/github.com\/lbusoni\/zmxIDL\">https:\/\/github.com\/lbusoni\/zmxIDL<\/a><\/td><td>L. Busoni<\/td><td>Interface to control \/ script Zemax from IDL<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n<div style=\"height:100px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>","protected":false},"excerpt":{"rendered":"<p>Moltissimi software di grande utilit\u00e0 sono stati realizzati dai ricercatori dell&#8217;INAF. Tuttavia, non \u00e8 sempre facile trovarne i riferimenti o persino essere a conoscenza della loro esistenza. \u00c8 attualmente in fase di sviluppo un sistema collegato al nuovo INAF-CRIS e presto sar\u00e0 disponibile un elenco completo dei software prodotti dall&#8217;ente. La licenza Open Source suggerita [&hellip;]<\/p>\n","protected":false},"author":7,"featured_media":2417,"parent":99,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"uscc-pages","meta":{"_acf_changed":false,"footnotes":""},"categories":[],"tags":[],"class_list":["post-688","page","type-page","status-publish","has-post-thumbnail","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/pages\/688","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/users\/7"}],"replies":[{"embeddable":true,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/comments?post=688"}],"version-history":[{"count":14,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/pages\/688\/revisions"}],"predecessor-version":[{"id":2489,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/pages\/688\/revisions\/2489"}],"up":[{"embeddable":true,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/pages\/99"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/media\/2417"}],"wp:attachment":[{"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=688"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=688"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/uscc.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=688"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}