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The Italian ARC is hosted by the Istituto di Radioastronomia in Bologna and is one of the seven nodes that constitute the European network that will provide technical and scientific support to ALMA users. The nodes will be operating in close collaboration with each other and with the central node at ESO, Garching. Each node contributes its own specific expertise, in order to ensure that maximum advantage is taken of the European competences in the field of mm-astronomy and interferometry.

Our ARC node staff will support the ALMA users in all the steps of their projects, by helping in

  • using the ALMA tools for proposal preparation and submission
  • improving the observing strategy
  • tracking the project status
  • reducing data with CASA
  • analizing data in continuum, spectral lines, mosaic, polarization
  • archive mining
  • handling ALMA large amount of data (also through GRID)

 



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mm workshop PDF Print E-mail

Secondo Workshop sull'Astronomia millimetrica e submillimetrica in Italia

L'ALMA Regional Centre italiano, ospitato dall'INAF-Istituto di Radioastronomia, organizza il "Secondo Workshop sull'Astronomia millimetrica e submillimetrica in Italia" presso l'Area della Ricerca del CNR a Bologna, il 2-3 Aprile 2012.

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Last Updated on Tuesday, 24 January 2012 16:56
 
Alma Opens its Eyes PDF Print E-mail

The Atacama Large Millimetre/Submillimetre Array (ALMA) is now open for all astronomers. After the call for proposals for the so-called Early Science Cycle 0 in March 2011, more than 900 proposals from astronomers worldwide were submitted. During the last few months a team of over 70 astronomers rated these for technical feasibility and scientific merit. 112 proposals were ranked with highest-priority, and are scheduled to be observed during the Cycle 0 phase, which officially started on Friday 30 September and was accompanied by the public release of an image of the Antennae Galaxies on 3 October 2011.

In the Early Science Cycle 0 only 16 antennas are used, but nevertheless ALMA is already the most powerful instrument of its kind. Alongside the first scientific observations, the build up of the Array will continue. After completion of construction, which is planned to be reached in 2013, ALMA will consist of 66 antennas.

Click here to read the official ESO Press Release

Last Updated on Thursday, 06 October 2011 08:39
 
ALMA Phase 2 PDF Print E-mail

Submission of proposals for ALMA Early Science Cycle 0 closed on June 30. The astronomical community responded enthusiastically to the first ever ALMA Call for Proposals: 919 unique proposals were received. Their distribution across the four ALMA science categories is as follows:

  1. Cosmology and the high redshift universe: 20%;
  2. Galaxies and galactic nuclei: 27%;
  3. ISM, star formation/protoplanetary disks and their astrochemistry, exoplanets: 40%;
  4. Stellar evolution, the Sun and the solar system: 13%.

The scientific and technical assessment of the 919 proposals submitted for ALMA Early Science Cycle 0 has been completed. Fifty science assessors and 25 technical assessors from all over the world have considered the expected scientific value and technical feasibility of all the proposals submitted. As a result, the most promising proposals have been selected as those most likely for completion using the initial 16-antenna ALMA capabilities.

The 112 highest-priority projects cover a wide range of science:
  1. Cosmology and the high redshift universe: 18.8%;
  2. Galaxies and galactic nuclei: 25.9%;
  3. ISM, star formation/protoplanetary disks and their astrochemistry, exoplanets: 44.6%;
  4. Stellar evolution, the Sun and the solar system: 10.7%.
In addition, several filler projects have been identified among the best lower-priority ones.

The observations to collect the data required to complete these projects are expected to start on 30 September or soon after. However, the construction and operation of ALMA - one of the world’s largest and most complex observatories, at an altitude higher than any other ongoing human activity - continues to be very challenging, and changes to the plan may still be necessary.

Principal Investigators (PIs) of the proposals have been notified of the outcome of the proposal review process by email.

The initial Phase II products will be generated by ALMA staff. PIs of highly rated proposals will be contacted by a scientist from their supporting ALMA Regional Centre (ARC) to review these Phase II products.

Phase II is the process by which an approved proposal is made executable and submitted to the observing queue in order to be subsequently run at the telescope (subject to various scheduling constraints). The main part of this is the automatic generation of the Scheduling Blocks that are used to control the telescopes during the observations.

Completion of Phase II by the PI is required for any ALMA project that is approved for admission to the observing queue with a grade A or B. Phase II must be completed within a period of September 1st - 30th, 2011, immediately following the conclusion of the PRP. The Observatory may also additionally require that Phase II for highly-ranked projects be completed early in that period. Projects awarded grade C will overfill the observing queue to accommodate weather variations, and completion of Phase II for such projects may be deemed optional by the Observatory.

PIs will be contacted by their supporting ALMA Regional Centre (ARC) and provided with the name of a contact scientist to help PIs prepare their Phase II products. Each PI will then work with his/her ARC contact to ensure that the Phase II products are successfully prepared within the one-month window. This will be done using the ALMA Observing Tool, and will include the accommodation of any changes to the project mandated by the results of the PRP. The full details of the process and policies for handling all changes to projects from Phase II onwards will be made available in additional forthcoming documentation. Priority for ARC support for Phase II will also follow the A, B, C proposal ranking.


Last Updated on Friday, 16 September 2011 10:01