Call for Science Verification Proposals for SEPIA Band 9
SEPIA (Swedish ESO PI receiver for Apex) is a new instrument at APEX, the Atacama Pathfinder Experiment. SEPIA is offered in Band 9 (conditional on the anticipated successful commissioning) for a Science Verification (SV) phase. First light has been successfully achieved (Feb 2016) and commissioning will start in April 2016.
The SEPIA band 9 receiver is an identifical copy of the ALMA band 9 receiver. An extensive description is given here. The receiver is a double sideband (DSB) receiver, which covers the RF frequency range from 600 to 722 GHz. Only 4 GHz bandwidth of one of the sidebands is recorded, but in dual polarization. The receiver is connected to the XFFTS backend which provides a fixed number of 65536 channels per 2.5 GHz sub band. At 660 GHz, this corresponds to a spectral resolution of 0.0173 km/s. The offered observing patters are On-Off observations, Raster maps, and On-the-fly (OTF) mapping. The data will be taken in either beam-switching or position switching mode. At 660 GHz, the beam size is 9.5 arcsec. An important constraint for observations at band 9 is the atmospheric transparency (see below). Generally, PWV<0.7mm conditions are required, though at some frequencies, even better conditions will be required. Note that these good to excellent conditions statistically occur 40% of the time.
Here is a (non-exhaustive) list of science cases that can be studied with SEPIA Band 9
- Water or SiO Masers Around O-rich Evolved Stars
- HCN and SiS Masers in C-rich Stars
- CO J=6-5 observations of stars (d<1 kpc)
- H-Recombination Masers
- SiO masers toward star-forming regions
- 658 GHz water maser emission in nearby galaxies
- High redshift Fine Structure Lines surveys
Science Verification proposals invited
The purpose of the Science Verification observations for SEPIA Band 9 is to execute programmes testing a various number of science cases for which the instrument was designed. Those programmes will be chosen also to test the various modes of operation.
Observing time available, suggested time limit per proposal
We expect that up to 20 hours will be available in total for Science Verification of SEPIA Band 9. We envisage approving for execution proposals ranging in total length from 0.5 to 4 hours.
The deadline for submission is Friday 11 March 2016, 12:00 CET.
Proposals received after this time will not be considered.
How to submit
Please use the latex template "SEPIA Band 9 Science Verification". All proposals should be submitted as a single PDF file. All proposals should be sent to "firstname.lastname@example.org" with "SEPIA Science Verification Proposal" in the subject line.
OTC available online
The online execution time estimator must be used for both SV and normal proposals. It can be found here:
- ON/OFF estimator: http://www.apex-telescope.org/heterodyne/calculator/V5.3/ITC/index.php
- OTF estimator: http://www.apex-telescope.org/heterodyne/calculator/otf/V7.4/
In order to use the estimator, first use the "Heterodyne receiver" menu to select "SEPIA".
SV data will be reviewed for "science quality". Once they have passed that review they will be placed in the archive and will be released immediately.
|Call for Proposals release||18.02.16|
|Proposal submission deadline||11.03.16|
|Phase 2 deadline||31.03.16|
|SV observing start||04.04.16
|SV observing end||02.06.16
Policies for Science Verification
No proprietary time
There will be no proprietary time for those data. I.e. in case your proposal is accepted and executed the data will become freely available as soon as they are released.
Notification and execution
We will notify all applicants as to whether their proposal was accepted. There is no guarantee that accepted SV will be executed. We will do our best to send notifications if/when a proposal has been executed, but we cannot guarantee to do this in real time.
Execution time and observing strategies
We may have to change execution time or observing strategy of individual projects during the SV execution campaign. As far as possible we will try to stay in contact with the proposers on those issues, but this may not always be possible.
SV and normal ESO proposals will all be reviewed for duplications as per usual ESO procedure. In case those are simply "self duplications" (as described in sub-section "No target change" below), then the rules listed in that sub-section will be followed. In case of duplications by another group, standard ESO duplication policies will be strictly followed.
No target change
Precise target coordinates must be provided in the proposal template. Change of target will not in general be possible.
If you submit SV and ESO Normal proposals for the same target
You may submit both an SV and a normal proposal for the same target, either for the same or for similar observations. If you do then please take note of the following policies:
- SV data have no proprietary time even if a normal proposal was accepted for the same observations.
- If SV data have already been obtained then identical or similar observations in your normal proposal will not be re-executed, but will be marked as "completed".
Keeping track online
The titles of all accepted SV proposals will be made available online. Exact target coordinates will be made available *only* in case actual data are taken and released. The titles, and lists of successful observations will be listed in this page.