INAF Arcetri Journal
The monthly newsletter of the INAF Astrophysical Observatory of Arcetri
Jan 30th - Published the Final Report on the projects related to the Fundamental Research 2024 call. In the list below you can find the funded projects and their Principal Inevestigators. Link: http://www.inaf.it/it/notizie-inaf/pubblicata-la-graduatoria-della-valutazione-progetti-rf2024
TRICEPS: luminous and dark matter in massive galaxies at z=4-5 (Federico Lelli)
Laboratory investigations to assess the astrobiological relevance of the Martian samples collected on Mars by the NASA Mars 2020 Perseverance rover for future return to Earth (Teresa Fornaro)
ICES: Tracking the history of ices from the cradles of planets to comets (Linda Podio)
A JWST/MIRI MIRACLE: Mid-IR Activity of Circumnuclear Line Emission (Giovanni Cresci)
The JWST high-resolution view of low-metallicity dwarf starbursts (Leslie Hunt)
Accurate measurements of metallicity in galaxies with a new approach to photoionization modelling (Alessandro Marconi)
SCARFACE 2: Star Clusters As cosmic Ray FACtoriEs II (Giovanni Morlino)
2DISCHEM: Modelling atmospheric disequilibrium chemistry in 2D (Lorenzo Pino)
PIPID: Probing Ionisation Processes In Discs (Daniele Galli)
Bridging space- and ground-based efforts with JWST and ERIS to resolve AGN-driven ionized winds up to the onset of cosmic dawn (Elena Bertola)
Dust emission and optical extinction as gas tracers in star forming galaxies (Evangelos Paspaliaris)
The pc-scale view of HII regions in M33 (Anna Feltre)
MACE_WINDU: MoleculAr ComponEnts of WINds from protoplanetary Disks Unveiled (Thomas Nony)
BASC: Building the Ariel mission Stellar Catalogue: a public homogeneous catalogue for the whole stellar and exoplanet community (Camilla Danielski)
ENERGIA: ExploriNg low-Energy cosmic Rays throuGh theoretical InvestigAtions at INAF (Marco Padovani)
DiSKA: Seeing the unseen with SKA, how dust grains grow up to be planets (Davide Fedele)
ProDisCo 2.0: statistical comparison of molecular abundances in comets and proto-planetary disks (Manuela Lippi)
BINCAT: Binary Catalog for AO Sytems Performace Evaluation (Pietro Ferraiuolo)
SHINE: Space telescope High-precision Ion-beam Nm polishing Equipment (Matteo Menessini)
Pietro Bolli (Technical Director) and Ugo Di Giammatteo (Project Manager) during the Site Acceptance Test witnessing at the Meerkat site, indicate the position where the receiver will be located.
The PNRR-funded STILES project foresees the installation of 64 new receivers (covering the frequency band called 5B, between 8.4 and 15.3 GHz) in the MeerKAT antennas. These radio telescopes are operated by the South Africa Radio Astronomy Observatory and will be integrated in SKA-MID in the coming years.
The Max Planck Institute for Radio Astronomy (MPIfR) has been awarded by INAF for the supply of 64 (+ 2 spare) receivers. The MeerKAT Band 5B receiver is composed of a chain of microwave components mainly consisting of a passive feed-system (circular horn antenna, marker coupler and ortho-mode transducer), two low noise amplifiers (one for each polarization) and a section for further RF conditioning of the signals.
The passive components and the two low noise amplifiers of the front-end are inserted in a cryogenic environment to ensure excellent receiver noise temperature performance. The aggressive schedule of the PNRR funding scheme dictated the acceptance of the first receiver to be executed by the end of 2024. The first receiver was first validated at the MPIfR laboratory during the Factory Acceptance Test (middle November) and then at the operational site in South Africa at the Site Acceptance Test (middle December, see picture below). The MPIfR is now proceeding with the series production to deliver all receivers at the site by November 2025.
Technical Director: Pietro Bolli
Testing activities are started in the ADONI optical laboratory on the LATT mirror! The LATT is a prototype of an active mirror for space telescopes, controlled by 19 voice coil actuators. The working principle is shared with its bigger brothers the LBT and VLT adaptive mirrors, based on an optical surface "floating" in front of the support when in operation.
Laboratory tests include electromechanical and optical characterization at different "floating" distances (or gap) and, more important, in rough vacuum. Air shall in facts be removed from the gap to reduce the mechanical coupling with the support; to this purpose, a stylish plexiglass vacuum chamber (the Vacquarium) has been procured and installed in the lab, housing the LATT.
You are welcome to come and participate to the tests, but please do not slam the doors!
Coordinator: Runa Briguglio
Il gruppo di lavoro nasce attorno al tema del contrasto alla violenza sulle donne e alla violenza/discriminazione in genere. Lo scopo del gruppo è quello di organizzare iniziative che informino e sensibilizzino il personale su questi argomenti e forniscano ove/quando possibile un aiuto concreto alle associazioni che operano sul territorio in questo campo.
This working group is focused on contrasting violence against women and all kinds of violence and discrimination. Our goal is to organize events to inform and raise awareness among staff about these issues, and, whenever we can, offer practical help to local associations working on these problems.
Elena Amato, Valentin Brunn, Antonella Gasperini, Elena Masciadri (coord.), Lorenzo Pino, Silvestra Smeraldi, Marco Xompero, Alessandra Zanazzi.
Firenze | January 2025 | Contacts