Name: Fifth Workshop on Millimetre Astronomy in Italy
Start: 2023-06-12T13:30:00+02:00
End: 2023-06-14T18:00:00+02:00
Location: Bologna

Fifth Workshop on Millimetre Astronomy in Italy

from Monday, 12 June 2023 (13:30) to Wednesday, 14 June 2023 (18:00)

Monday, 12 June 2023

13:30 Jan Brand, Matteo Bonato, Tiziana Venturi - Welcome speech
Jan Brand, Matteo Bonato, Tiziana Venturi - Welcome speech
13:30 - 13:35
Introductory speech

13:35 Federica Govoni - Perspectives for observations at high radio frequencies with the Italian facilities (Invited)
Federica Govoni - Perspectives for observations at high radio frequencies with the Italian facilities (Invited)
13:35 - 13:50
I will present the status of the radio astronomical facilities in Italy and the future perspectives for observations at high frequencies.

13:50 Anna Miotello - ALMA updates and new capabilities (Invited)
Anna Miotello - ALMA updates and new capabilities (Invited)
13:50 - 14:00
In this talk, an overview of ALMA will be provided, with updates and explanation of the new capabilities
14:00
14:00 - 15:30
Contributions

14:00 Viviana Casasola - The Interstellar Medium in nearby galaxies (Review invited)

14:30 Alice Concas - Molecular gas and dust extinction relation revealed by ALMAQUEST

14:50 Francesco Salvestrini - Investigating molecular gas scaling relations in the local Universe: What drives the cycle of star formation?

15:10 Simone Bianchi - Exploring the mm-to-cm SED of nearby spirals
15:30
15:30 - 15:41
Contributions

15:30 Eleonora Torresi - Cold molecular gas and nuclear activity in radio galaxies: Linking properties on macro and micro scales

15:31 Elena Redaelli - The core population and kinematics of a massive clump: an ALMA view of AG14.49

15:32 Farideh S. Tabatabaei - Unveiling the interplay between magnetic ﬁelds and accretion in a young protocluster

15:33 Vincenzo Galluzzi - A multi-frequency polarimetric study of the Radio Galaxy "Pictor A"

15:34 Fabrizio Gentile - Radio-Selected NIR-Dark galaxies: the ALMA view behind the dust

15:35 Cleo Whitcombe - Millimetre-wave spectroscopy of pyrrole: a model for astrophysical searches

15:36 Wentao Song - Rotational spectroscopic study of cysteamine

15:37 Alice Nucara - The Rosetta-Stone project: a comparison between observations and simulations to investigate the star-formation mechanism in massive regions

15:38 Andrea Maggio - Free jet millimeter wave torsion-rotation spectrum of a silicon containing molecule: dimethylsylane

15:39 Meriem Behiri - Discovering unexplored SHORES of the radio Universe

15:40 Alice Somigliana - A way to disentangle between viscous and MHD evolution in protoplanetary discs
15:41 Coffee break
Coffee break
15:41 - 16:10
16:10
16:10 - 17:30
Contributions

16:10 Davide Belfiori - Studying magnetic fields structure of the starburst galaxy NGC253 through ALMA polarization observations

16:30 Federico Esposito - Modelling molecular clouds and CO excitation in AGN-host galaxies

16:50 Ilaria Ruffa - Molecular gas kinematics in local early-type galaxies with ALMA

17:10 Maria Vittoria Zanchettin - AGN driven winds and gaseous discs in local Seyfert galaxies: high resolution study of the multiphase ISM with ALMA, MUSE and JVLA
17:30 Marcella Massardi - The ALMA Science Archive development and the ARI-L project
Marcella Massardi - The ALMA Science Archive development and the ARI-L project
17:30 - 17:50
In the ALMA 2030 development roadmap a crucial role is assigned to the evolution of the ALMA Science Archive to improve the user experience and maximize the scientific exploitation of ALMA data. To date, the Archive accounts for 10 cycles of data summing up to 1.4 PB of raw data and images representative of the data content that cover all the possible science categories from solar observations to cosmology. Most of the data are still unpublished: the ALMA Science Archive is a gold mine for archival users! The expected telescope upgrade will costitute a huge challenge in the archival data management. In view of the next decade telescope development, several upgrades have already been applied to improve the Archive features and offer easy access and experience to the miners. In this talk I will present some of the already available features and examples of their application to science cases. In particular, I will focus on the results of the Additional Representative Images for Legacy (ARI-L) project that has been a European Development project for ALMA Upgrade leaded by the Italian node of the EU ARC. It increased the legacy value of the ALMA Science Archive by bringing the reduction level of ALMA data from Cycles 2-4 close to that of data from more recent Cycles processed for imaging with the ALMA Pipeline. The project produced, assessed the quality of, and delivered to the ALMA Science Archive more than 300000 images for more than 88.5% of the observational datasets from Cycles 2 to 4 processable with the ALMA Pipeline that were missing pipeline-generated images. ARI-L products are certified for quality and can be downloaded from the ALMA Science Archive as ``external products''. The ARI-L project documentation and website are publicly available through the ALMA science portal (https://almascience.org/alma-data/aril).

17:50 Michele Ginolfi - Understanding teenage galaxies at the end of cosmic reionization (Invited)
Michele Ginolfi - Understanding teenage galaxies at the end of cosmic reionization (Invited)
17:50 - 18:15
I will summarise recent and ongoing research highlights from the ALPINE survey, an ALMA large program that observed dust continuum and [CII] emission in a statistical sample of normal star-forming galaxies at z=4–6, highlighting their significance to our understanding of early galaxy evolution. Combined with ancillary data at UV through near-IR wavelengths, ALPINE provides the currently largest multi-wavelength sample of post-reionization galaxies and has advanced our understanding of (i) the interstellar medium properties and star formation activity, (ii) the gas content, (iii) outflows and metal enrichment of the circumgalactic medium and (v) the kinematics and merger rates, in galaxies at z>4. ALPINE builds the basis for more detailed measurements with the current and next generations of big telescopes, and I will show an overview of a number of legacy programs that are already being carried out with ALMA and JWST.

18:15 Maris Assimo - Paleo-spectroscopy: retrieve and complement past data for radioastronomy searches
Maris Assimo - Paleo-spectroscopy: retrieve and complement past data for radioastronomy searches
18:15 - 18:35
A plethora of microwave and millimetre wave molecular spectroscopy data are available to the radioastronomy community. However, some of it was collected several decades ago and its modelling is sometimes obsolete. Moreover, instrumental advances allow complementing the data with new measurements that extend the investigated frequency ranges and improve the quality of the spectral predictions. Therefore, retrieving and complementing past information is necessary to look for not yet detected molecules in space. Some recent cases related to molecules containing atoms of the third period will be discussed, focusing on the challenges derived by the presence of internal motions (i.e. methyl internal rotation) and preliminary searches on Alma Archive.
Tuesday, 13 June 2023
09:00
09:00 - 11:00
Contributions

09:00 Anna Miotello - The Disk Exoplanet C/Onnection (Invited)

09:25 Francesca Bacciotti - Layered molecular outflows and disk substructures: the HL Tau case

09:45 Marta De Simone - Reveal the chemical history of young protostars combining mm and cm wavelengths

10:05 Stefano Facchini - The physico-chemical connection between nascent planets and their birth environment (Invited)

10:30 DISCUSSION on planet-forming disk science led by Davide Fedele and Giovanni Rosotti
11:00 Coffee break
Coffee break
11:00 - 11:30

11:30 Andrea Possenti - Neutron stars pulsating in the mm-band: Italian perspectives (Invited)
Andrea Possenti - Neutron stars pulsating in the mm-band: Italian perspectives (Invited)
11:30 - 11:55
The pulsed radio emission from the neutron stars has usually a steep spectrum, thus making difficult their investigation in the mm band. However, the availability of new instrumentation is opening new perspectives in the field, hopefully allowing us to address some long standing and still unanswered questions in the field of the emission processes from a neutron star magnetosphere. In particular, the presentation will focus on the expectations arising from the installation of a suite of high frequency receivers at the Sardinia Radio Telescope.
11:55
11:55 - 13:05
Contributions

11:55 Claudio Codella - Astrochemistry of Galactic regions: living ALMA, preparing SKA (Review Invited)

12:25 Giovanni Sabatini - First ALMA maps of cosmic ray ionization rate in high-mass star-forming regions

12:45 Andrea Giannetti - Methanol to the rescue: estimating volume density of molecular gas
13:05 Lunch
Lunch
13:05 - 14:00
14:00
14:00 - 15:30
Contributions

14:00 Sergio Molinari - Galaxy-wide star formation: zooming in from panoramic Galactic Plane surveys to 1000au-scale with ALMA (Review Invited)

14:30 Milena Benedettini - The Forgotten Quadrant Survey: a 12CO and 13CO (1–0) survey of the Galactic Plane in the range 220°<l<240°, -2.5°<b<0°

14:50 Alessio Traficante - The SQUALO-ALMA project: clump-fed accretion mechanism in high-mass star-forming objects

15:10 Marco Monaci - High Latitude Molecular Clouds chemodynamics using high-resolution multiline spectroscopy
15:30 Coffee break
Coffee break
15:30 - 16:00
16:00
16:00 - 17:10
Contributions

16:00 Alessandro Coletta - Fragmentations of ALMAGAL dense clumps in young protoclusters

16:20 Olga Bayandina - ALMA study of G11.92-0.61: disk-wind or YSO multiplicity?

16:40 DISCUSSION on Galactic science led by Milena Benedettini and Eleonora Bianchi
17:10
17:10 - 17:55
Contributions

17:10 Chiara Mininni - Molecular vs continuum emission: a morphological comparison in ALMAGAL clumps

17:30 Ivano Baronchelli - UMLAUT: A Data-Driven Machine Learning Approach with Automated Parameter Tuning and Outlier Detection (Invited)
20:00 Social dinner
Social dinner
20:00 - 22:00
Wednesday, 14 June 2023
09:00
09:00 - 10:30
Contributions

09:00 Andrea Ferrara - The Earliest Dusty Galaxies. Lessons from ALMA and JWST (Review Invited)

09:30 Roberto Decarli - The physics of the ISM in quasars at z>6

09:50 Laura Sommovigo - Fast and Furious: the dust enrichment of the early Universe

10:10 Cecilia Bacchini - 3D modelling of the molecular gas kinematics in optically-selected jellyfish galaxies
10:30 Sirio Belli - Cold Gas in High-Redshift Quiescent Galaxies (Invited)
Sirio Belli - Cold Gas in High-Redshift Quiescent Galaxies (Invited)
10:30 - 10:55
The most massive galaxies were the first to shut off their star formation, turning into quiescent systems when the universe was still young. This quenching process is still poorly understood, and to make progress it is crucial to study the role played by cold gas. I will present two different ways in which this can be done. Using millimetric observations with NOEMA, we detected CO line emission from three massive quiescent galaxies at z~1, and measured low gas masses. This suggests that quenching consists in the removal of cold gas rather than in the suppression of star formation efficiency. I will also present new results based on James Webb Space Telescope observations, in which we detect neutral atomic gas in a high-redshift quiescent galaxy using rest-frame optical absorption lines. I will illustrate the implications of this detection for models of galaxy quenching.

10:55 Coffee break
Coffee break
10:55 - 11:25
11:25
11:25 - 12:05
Contributions

11:25 Stefano Carniani - CGM enrichment by quasar-driven outflows

11:45 Federico Lelli - Cold gas dynamics in high-z galaxies
12:05 Violette Impellizzeri - EHT & ALMA: a view of the local Universe (Invited)
Violette Impellizzeri - EHT & ALMA: a view of the local Universe (Invited)
12:05 - 12:30
MmVLBI has revolutionised our view of black holes and have provided some of the most striking, high resolution images obtained by mmVLBI, like the first images of a supermassive black hole obtained by the Event Horizon Telescope collaboration (EHTC). But beyond these two best studied targets, M87 and SgrA*, the EHTC has been exploring a variety of nearby AGN allowing to study different local environments and jet properties. In this talk I will present an overview of the AGN that are targeted with mmVLBI at 1.3mm and 3mm, highlighting some of the recent results that have been obtained. MmVLBI is a powerful tool not only for observations of the accreting material at tens of muas resolution, but will be critical - especially as more baselines become available around the globe - to study jet launching mechanisms and how these connect to the more extended jet material which is studied with cmVLBI at mas resolution.

12:30 Discussion on extragalactic science led by Laura Pentericci and Livia Vallini
Discussion on extragalactic science led by Laura Pentericci and Livia Vallini
12:30 - 13:00

13:00 Lunch
Lunch
13:00 - 14:00

14:00 Andrea Lapi - GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies
Andrea Lapi - GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies
14:00 - 14:20
A key issue in galaxy formation and evolution is to deepen our understanding of the complex (astro)physical processes that govern the properties of galaxies on different spatial and time scales. One powerful method for achieving this task is to model the spectral energy distribution (SED) observed from galaxies at different stages of their evolution along cosmic history. To this purpose, we have developed GalaPy, a new library for modelling and fitting galactic SEDs from the X-ray to the radio band, as well as the evolution of their components and dust attenuation/reradiation. On the physical side, GalaPy incorporates both empirical and physically-motivated star formation histories, state-of-the-art single stellar population synthesis libraries, a two-component dust model for extinction, an age-dependent energy conservation algorithm to compute dust reradiation, and additional sources of stellar continuum such as synchrotron, nebular/free-free and X-ray emission from low and high mass binary stars. On the computational side, GalaPy implements a hybrid approach that combines the high performance of C++ with the user-friendly flexibility of Python, and exploits an object-oriented design via new-generation programming techniques. GalaPy is the fastest SED generation tool of its kind, with a peak performance of almost 1000 SEDs per second. It exploits fully Bayesian parameter space sampling, which allows for the inference of parameter posteriors and thus facilitates the study of the correlations between the free parameters and the other physical quantities that can be derived from modelling. The API and functions of GalaPy are under continuous development, with planned extensions in the near future. In this talk, I will introduce the project and showcase the photometric SED fitting tools that are already available to users, with particular focus on the performance on local and high-z dusty star-forming galaxies featuring prominent emission in the mm band.
14:20
14:20 - 15:40
Contributions

14:20 Toby Devereaux - Star-forming clumps and their molecular gas content

14:40 Francesca Perrotta - H2O emission lines in a strongly lensed dusty star-forming galaxy at z ∼ 3.1

15:00 Gayathri Gururajan - Probing the gas reservoirs of high-redshift lensed dusty

15:20 Marika Giulietti - Synergistic Study of High-z Strongly Lensed Dusty Star-Forming Galaxies with ALMA: Insights into Galaxy/AGN Co-evolution
15:40 Coffee break
Coffee break
15:40 - 16:10
16:10
16:10 - 17:30
Contributions

16:10 Claudia Di Cesare - Metal enrichment in the CGM around high-z merging galaxies

16:30 Eleonora Parlanti - Evidences for turbulent disk galaxies at z > 5

16:50 Luca Di Mascolo - Detection of forming intracluster gas in a galaxy protocluster at z~2.16

17:10 Giovanni Gandolfi - At the frontiers of cosmic history: How ALMA and JWST Team Up to Confirm High-Redshift Galaxy Candidates
17:30 Discussion on "user needs and requests" led by Rosita Paladino and Elisabetta Liuzzo
Discussion on "user needs and requests" led by Rosita Paladino and Elisabetta Liuzzo
17:30 - 18:00

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