Facilities > VLBA > Documentation > Manuals > VLBA Observational Status Summary 2020A > Proposal Preparation, Submission, & Review

Proposal Preparation, Submission, & Review

by Jonathan Romney last modified May 14, 2019 by Anna Kapinska

Observing time on the VLBA is scheduled on a semester basis, with each semester lasting six months.  Proposal deadlines are February 1 and August 1, with the February 1 proposal deadline nominally covering time to be scheduled during the following August through January, and the August 1 deadline covering time to be scheduled from February through July.   Time can be requested over multiple semesters if scientifically justified.

A Call for Proposals (see the latest VLBA proposal preparation and submission document for more information) is published approximately four weeks in advance of each semester submission deadline.  Proposals must be prepared and submitted using the NRAO Proposal Submission Tool (PST), available via NRAO Interactive Services.  Observing proposals may specify the VLBA alone, or in the various extended arrays described in Section 14.

Submitted proposals are reviewed by a Science Review Panel (SRP) in relevant subdisciplines (e.g., solar system, stellar, Galactic, extragalactic, etc.).  The SRP's comments and rating are strongly advisory to the Time Allocation Committee (TAC), and the comments of both groups are passed on to the proposers soon after each semi-annual meeting of the TAC, and prior to the next proposal submission deadline.  A detailed description of the time allocation process is available.

Approved programs are scheduled by the VLBA scheduling officers, who may be contacted at .  A "Guide to Using the VLBA" is available, aimed specifically at inexperienced users but also useful to fill in knowledge gaps for more experienced observe

The VLBA SCHED program (Walker 2011) can be used to determine the Greenwich Sidereal Time range during which the VLBI target sources are visible at various stations.  This program can also be used to evaluate the u-v plane coverage and synthesized beams provided by the selected array.

An accurate source position service is available to obtain positions accurate enough for correlation. This should be requested simultaneously with the proposal, if not earlier.