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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)

 



What's on

 
Cycle 1 announcement PDF Print E-mail

A pre-announcement for Cycle 1 observations has appeared on the ALMA science portal.

The Joint ALMA Observatory (JAO) expects to start the next cycle of Early Science observations (Cycle 1) in January 2013. About 800 hours will be available for science projects.

The ALMA Early Science Cycle 1 anticipated capabilities will comprise:

  • Thirty two 12-m antennas in the main array, and nine 7-m antennas (for short baselines) and two 12-m antennas (for making single-dish maps) in the Atacama Compact Array (ACA)
  • Receiver bands 3, 6, 7 & 9 (wavelengths of about 3, 1.3, 0.8 and 0.45 mm)
  • Baselines up to 1km
  • Both single field interferometry and mosaics
  • Mixed correlator modes (both high and low frequency resolution in the same observation)

Use of the ACA for short baseline interferometry and single-dish observations will only be offered to complement observations with the main array, and not as a stand-alone capability. Single dish use will be limited to spectral line observations. More details will be provided in the Call for Proposals.

The key dates for Cycle 1 are given below. ALMA reserves the right to alter the given dates, should it become necessary to do so.

15 May 2012: Deadline for Notices of Intent
31 May 2012: Call for Proposals for ALMA Early Science Cycle 1, release of Observing Tool, and opening of archive for proposal submission.
12 July 2012: Proposal Deadline.
Mid November 2012: Result of the proposal review process sent to PIs
1 January 2013: Start of ALMA Cycle 1 observing.
February 2013: One month engineering period during altiplanic winter.
31 October 2013: End of ALMA Cycle 1 observing.
 
Cycle 1 Tutorial PDF Print E-mail

Tutorial per ALMA - Cycle 1

L' ARC organizza una sessione di talk per
- illustrare le novita' di ALMA per il ciclo 1 e le possibilita' offerte dallo strumento
- presentare gli strumenti di supporto disponibili per gli utenti ALMA durante tutte le fasi dei loro progetti
- mostrare quali procedure sono consigliate per la preparazione delle proposte osservative, con esempi pratici e simulazioni

Per consentire una migliore interazione tra gli utenti e una piu' rapida organizzazione, i talk saranno presentati durante una sessione di circa 3 ore trasmessa via videoconferenza, con possibilita' di interazione tra gli utenti collegati. Una ripetizione della sessione in una data diversa sara' considerata in base alla richiesta. La trasmissione sara' inoltre registrata e resa disponibile su questo sito.

La sessione (ed eventuali repliche) potranno avere luogo nelle settimane tra il 28 maggio e l'8 giugno 2012.


Dal punto di vista organizzativo sara' possibile avere un numero elevato di partecipanti collegati (i.e. ogni partecipante potrebbe in teoria seguire la presentazione dalla sua postazione di lavoro), ma per limitare il numero di persone collegate, soprattutto ai fini della buona riuscita della sessione di domande e del controllo dei collegamenti, vi invitiamo ad individuare all'interno della vostra struttura un gruppo di persone interessate all'evento o a inserirlo tra i seminari periodici. Sara' allora sufficiente individuare una persona di riferimento per il gruppo che si occupi del collegamento (i.e. al massimo scaricare ed installare un software) ed eventualmente della proiezione con un normale sistema pc+proiettore.

In caso di risposta favorevole, oltre ad indicarci i nominativi delle persone interessate a collegarsi individualmente o dei referenti dei gruppi, vi invitiamo a indagare all'interno dei vostri istituti quali giorni  sarebbero per voi i piu' indicati nelle settimane proposte sopra. Indicateci inoltre, qualora ne abbiate, quali sistemi di videoconferenza potete utilizzare.

Vi invitiamo a comunicarci il vostro interesse a partecipare entro e non oltre il 30 aprile 2012 compilando il form.

Sara' organizzata una sessione di prova di connessione circa 10 giorni prima della data fissata. I dettagli per la connessione saranno distribuiti agli interessati.
Vi aspettiamo numerosi!

Last Updated on Wednesday, 11 April 2012 09:19
 
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