PACE Members attended the IAU Symposium “Uncovering early galaxy evolution in the ALMA and JWST era”, hosted in Viana do Castelo, Portugal, from 3-7 June 2019.
This symposium brought together community of theoretical and observational experts to discuss how we can make the most of ALMA and JWST synergies in advancing our understanding of galaxy evolution in the young Universe during the next decade.
PACE members presented various posters, fostering the discussion about possible synergies between ALMA and future facilities in construction or soon available for the scientific community.
PACE member participated in the Polarization Workshop, held in Garching in the last week of May. Experts from the European ALMA Regional Center Network meet at ESO to discuss and improve the procedure to validate ALMA data observed in full polarization mode, a challenging observing technique offered by the ALMA observatory in the past Cycles. The workshop will trigger a more efficient and thorough analysis for such type of data, increasing the more and more the scientific impact of ALMA in the field of Observational Astrophysics.
On the second week of May ended the 9th SKA Pathfinder Radio Continuum Survey Group (SPARCS) meeting, which took place in Lisbon, between the 6th and 10th May 2019.
The aim of the meeting was to coordinate developments of techniques for radio data analysis and to help in the choice of area, depth, location on the sky, and other parameters, future and ongoing surveys. PACE members have been heavily involved in the meeting, participating in the discussion, and presenting their results.
On the last week of September, PACE participated to the annual meeting of the European ALMA Network, hosted this year by the Czech ARC Node. In the beautiful landscape of Prague countryside, representatives of different European Institutions discussed the status and future plans for ALMA development. With new facilities starting soon their operations, these meetings aim to assure for ALMA a future at the forefront of astronomical research for the next decades.
The annual European meeting of the ARC nodes and CoE this year will be held in the Costa de Caparica Hotel.
More than 50 scientists from the different ALMA nodes in Europe will attend this meeting to discuss the strategic lines for the future of ALMA, and the technical improvements of the official data reduction pipeline of the instrument.
The Portuguese Alma Center of Expertise (PACE) will guest the event in collaboration with the ESO-ALMA Headquarter of Garching.
This year’s YERAC will be organized and sponsored by the MPI for Radioastronomy in collaboration with its IMPRS for Astronomy and Astrophysics. As in most years since 1968, early stage radioastronomers (i.e. PhD candidates and postdocs) will meet, discuss and network in a relaxed atmosphere. Each participant is given the opportunity to give an oral talk.
Five years passed so quickly, and half a decade seems a lot in correspondence to the amount of great science ALMA has enabled thus far. As a result, the conference “Half a Decade of ALMA: Cosmic Dawns transformed” will be held on 20th-23rd September 2015 in Indian Wells, California (USA).
A list of invited speakers and topic they will cover is already online, as well as the preliminary programme layout.
Note that a pre-registration and abstract submission are now open.
Results from ALMA Long Baseline observations and from SPHERE, Gemini Planet Imager (GPI) and other high-contrast adaptive optics (AO) instruments have given a taste of what to expect over the next few years in the fields of protoplanetary and debris disks, and planet formation. For the first time observations of the regions where planets form are achievable. The workshop will discuss the state-of-the-art results, offering a panchromatic view, with a balance between observations and theory. Discussions will be scheduled on how facilities, such as JWST, E-ELT and TMT, and advances in modeling, will advance the field of planetary formation.
A conference to be held at ESA/ESTEC on 12—15 April 2016, which will cover all astrophysical aspects of water, including the water trail, from the formation of water in molecular clouds to water on planetary bodies, including in our own solar system; water as a probe of physics and and chemistry; and water in nearby to water in extra-galactic and high redshift sources.
More information at the conference website. Abstract submission deadline on 11th December.