The Istituto Nazionale di Astrofisica (INAF)
invites scientists to participate in the call for proposals of
observing time at the three national radio telescopes:
- the 32-m Medicina
- the 32-m Noto
- the 64-m Sardinia Radio
Two observing semesters are scheduled every year: 1st January to
30th June, 1st July to 31st December.
Deadlines fall in early October and early April, respectively.
Below we report the time INAF plans to award for the next semester
- Medicina: 2500 hours
- Noto: 2000 hours
- SRT: 0 hours (*)
These amounts might be subject to modification, due to
maintenance needs and to the variability of the commitments
resulting from international agreements.
(*) SRT UNAVAILABLE DUE TO MAJOR UPGRADE
SRT cannot be offered during semester 2022B due to the planned
upgrade at higher frequencies (see https://sites.google.com/a/inaf.it/pon-srt/home
Please note - As single-dish observations with
Noto cannot be carried out remotely, they may need the
inclusion of a local observer in the proposers' team. Please
contact usersupport.ira(at)inaf.it prior to submission in
order to ensure this point is addressed.
Acknowledgements - Papers including data/results
obtained with the Italian radio telescopes must contain the
appropriate acknowledgements, i.e.:
For the Sardinia Radio Telescope: "The Sardinia Radio
Telescope is funded by the Ministry of University and
Research (MIUR), Italian Space Agency (ASI), and the
Autonomous Region of Sardinia (RAS) and is operated as
National Facility by the National Institute for Astrophysics
For Medicina and/or Noto: "The Medicina[Noto] radio
telescope is funded by the Ministry of University and
Research (MIUR) and is operated as National Facility by the
National Institute for Astrophysics (INAF)."
Operational activities at the Italian radio
telescopes are partly supported by ORP (http://www.orp-h2020.eu).
The ORP project has received funding from the European Union’s
Horizon 2020 research and innovation programme under grant
agreement No 101004719.
Time Allocation Committee
Proposals will be reviewed and ranked on the basis of their
scientific merit by a Time Allocation
(TAC) of experts.
How to apply
Here is a list of useful indications and resources for those
wanting to apply for observing time:
- Consult the announcement page - taking note of the
proposal deadlines - and carefully read the general guidelines
- Refer to the offered
programs to decide which type best suits the project
you have in mind
- Visit the observational status
summary of the three radio telescopes to determine the
technical feasibility of your program, which instruments are
available or appropriate, and estimate how much time is
required to complete the observations
For inquiries and updates please contact us by writing to radioproposal
The three antennas shall be seen as a single coordinated
facility so that users can submit a single proposal to request
time at one or more than one telescope.
Please consult the following general guidelines:
- Observing with our
- Which antenna to use?
- Italian VLBI
- Recovery of lost
- MoU and LoIs policy
- EATING VLBI
- Proprietary time
- Disclosure of
The offered observing programs types are:
- Guest projects
- Large projects
- Long (multi-term) projects
- NAPA proposals
- ToO projects
All of these programs are TAC-evaluated and must be submitted
using the official proposal form. Except for ToOs, which can be
submitted at any time, all other proposals must be submitted at
the regular deadlines. ToO evaluation
and observations will be carried out quickly if the requested
telescope is available.
Users can exceptionally apply for DDT (Director Discretionary Time
outside the regular calls. This is time at the disposal of the
Directors of the institute(s) hosting the telescope(s).
INAF may also promote Legacy
. These are very large projects that address broad
scientific goals that are of interest to the scientific
community at large.
Observational Status Summary
We strongly recommend the observers read the detailed
information about the observational status of the three radio
telescopes provided via the following page, which also links to
useful tools (Exposure Time Calculator, source visibilty tool,
Here is a summary of the available receivers and back-ends: