Project | PI | Institute | Rate | Subj. | Contact | |
K008 | C.Carilli | NRAO | A | GAL | E.Dartois | dartois@iram.fr |
K00f | L.Tacconi | MPE | A | GAL | A.Dutrey | dutrey@iram.fr |
K015 | E.Falgarone | ENS | B | MOL | L.Loinard | loinard@iram.fr |
K004 | M.Sempere | CSIC | B | GAL | R.Moreno | moreno@iram.fr |
K017 | R.Barvainis | NSF | B | GAL | H.Wiesemeyer | wiesemey@iram.fr |
For the 30m telescope, the highest rating ``A'' was given to 34
proposals, 27 proposals were rated ``B'', i.e. were given backup status.
The remaining proposals, although scientifically valuable in most
cases, were rated ``C''. The individual ratings are listed in the
attached table. All A proposals will be scheduled on the 30m
telescope, although some with less time than requested. We expect that
less than half of the B-rated programs will actually be
scheduled. The selection will take into account scientific merit,
crowding in certain right ascension ranges, and general aspects of
balance. Proposals rated ``C'' will not get telescope time.
The principal investigators of each proposal will be informed by letter which will include comments issued by the committee if there are any.
A | B | C | |||
Proposal No. | |||||
01-00 | 57-00 | 02-00 | 69-00 | 05-00 | 50-00 |
03-00 | 61-00 | 06-00 | 73-00 | 07-00 | 55-00 |
04-00 | 65-00 | 10-00 | 79-00 | 08-00 | 58-00 |
09-00 | 70-00 | 11-00 | 82-00 | 14-00 | 60-00 |
12-00 | 71-00 | 13-00 | 85-00 | 16-00 | 63-00 |
26-00 | 72-00 | 15-00 | 87-00 | 17-00 | 66-00 |
27-00 | 75-00 | 19-00 | 92-00 | 18-00 | 67-00 |
30-00 | 80-00 | 22-00 | 93-00 | 20-00 | 68-00 |
31-00 | 81-00 | 25-00 | 95-00 | 21-00 | 74-00 |
32-00 | 84-00 | 34-00 | 23-00 | 76-00 | |
33-00 | 89-00 | 35-00 | 24-00 | 77-00 | |
41-00 | 90-00 | 37-00 | 28-00 | 78-00 | |
42-00 | 94-00 | 43-00 | 29-00 | 83-00 | |
44-00 | 96-00 | 48-00 | 36-00 | 86-00 | |
46-00 | 98-00 | 49-00 | 38-00 | 88-00 | |
51-00 | 54-00 | 39-00 | 91-00 | ||
52-00 | 59-00 | 40-00 | 97-00 | ||
53-00 | 62-00 | 45-00 | 99-00 | ||
56-00 | 64-00 | 47-00 | 100-00 |
For the interferometer, the programs were classified A (accepted), B
(backup), C (rejected) and D (deferred). Programs rated A will be
scheduled in priority. Further time, if available, will go
to the B programs following the same criteria as for the 30m telescope
proposals.
D programs have been considered as unfeasible during the summer period.
Note: As a consequence of manpower limitations and safety
issues, projects for the coming season will be carried out with the
Plateau de Bure interferometer on a best effort basis only. IRAM can
therefore not guarantee to schedule all A-rated proposals. If
a project is not scheduled before the end of the summer period, it
will have to be resubmitted and it will be rated again together with
any new programs that come in for the next season.
Project | Rate | Project | Rate | Project | Rate |
K001 | B | K002 | C | K003 | C |
K004 | B | K005 | D | K006 | C |
K007 | B | K008 | A | K009 | C |
K00A | C | K00B | B | K00C | C |
K00D | C | K00E | C | K00F | A |
K010 | C | K011 | A | K012 | D |
K013 | A | K014 | B | K015 | B |
K016 | C | K017 | B | K018 | C |
K019 | B | K01A | D | K01B | C |
K01C | A | K01D | C | K01E | A |
K01F | C | K020 | A | K021 | C |
K022 | B | K023 | C | K024 | A |
Please contact your local contact as soon as possible to send him/her the setup of your project. The section ``Writing the setup of your observations'' (at http://iram.fr/PDBI/obs-setup.html) of the PdBI web page (http://iram.fr/PDBI/bure.html) provides the information needed to write the first iteration of your setup.
Not all is perfect though. Some proposals still do not have their figures incorporated in the .tex file. As the submission facility automatically creates the final postscript file from the submitted .tex file, the absence of figures is not noticed, unless they are explicitly incorporated. As an example, the following lines were used to incorporate Fig. 1 in this text:
\begin{figure}[t] \resizebox{\hsize}{!} {\rotatebox{270} {\includegraphics{histogram.eps}}} \caption[arrivals]{Number of electronic proposals which arrived per hour for the last proposal deadline. } \label{f:arrivals} \end{figure}
The submission facility allows to view the created final postscript file. Please use this viewing option to look at your proposal as it will be passed on to the program committee.
As the vast majority of proposals now arrives to the program committee in laser printer quality, the few proposals which still arrive by fax are looked at with increasing suspicion. Please be aware that this mode of submission makes a proposal significantly less competitive: Typical grey scale plots transmitted by fax loose all definition, and are equivalent to subjecting the proposal reviewer to a Rorschach test. The outcome is predictable, and has already led to flat proposal rejections.
Reading faxed text is not necessarily simpler, or what are the proposal reviewers expected to think when they read about the source | | | | 7 | | ? Of course, with a little reading on, cross-checking, and lots of prior knowledge, the assessor finds out rapidly that HH7-11 is proposed to be observed. Not all assessors however enjoy these sportive aspects of their work, particularly if there are still 100 more proposals to be read.
In view of their poor legibility we therefore plan to discontinue the acceptance of faxed proposals. A questionnaire will be sent soon to the principal investigators of all proposals which were submitted by fax or normal mail for the last deadline. They will be invited to explain the reasons why electronic submission was not used, and to suggest improvements of the facility. If no strong reasons come up, fax submission will be discontinued in the near future.