vlbiplanobs 5.0

Observaiton Planner for VLBI observations

Thank you everyone for the wait! PlanObs is back with tons of new features. That also imply that for the time being it may contain some minor bugs, and a few features may be missing. They will be back incrementally during the upcoming updates.

EVN Observation Planner

The EVN Observation Planner is a tool to determine the visibility of a given astronomical source when planning very-long-baseline-interferometry (VLBI) observations. The tool is specially written for the preparation of observations with the European VLBI Network (EVN), but it can be used for any kind of VLBI observations than can be currently arranged (e.g. with the Very Long Baseline Array, VLBA; the Australian Long Baseline Array, LBA; eMERLIN; or the global mm-VLBI array, for example). An ad-doc VLBI array can also be quickly configured.

In addition to the determination of the source visibility by the different antennas, the EVN Observation Planner would provide an estimation of the expected rms noise level (sensitivity) reached during the planned observations, and an estimation of the resolution. The EVN Observation Planner can thus be used while preparing an observing proposal. Note that the EVN Observation Planner has been designed as a more complete version of the previous EVN Calculator.

It runs both online and locally!

You can make use of the EVN Observation Planner just by going to the online tool hosted at JIVE, without installing anything.

But if you want to run it in your local machine, you can also install the package via pip:

python3 -m pip install vlbiplanobs

Once you have it installed, you can simply run it by typing planobs-server in the terminal. It will start to run the server and you will be able to access it in your browser by following the typed url (likely http://0.0.0.0:8050/).

**But PlanObs also has a lovely command-line interface!

The EVN Observation Planner can also be used through the terminal or inside your own Python program without the need of running a server.

Command-line interface (CLI)

This is great for when you want to plan, or verify the feasibility of, a VLBI observation quickly, or you have multiple sources to observe already defined.

You only need to type:

planobs

In your terminal to encounter all options.

Example cases

1. You want to know when a source (e.g. 'Altair') can be observed by a given VLBI network (e.g. the EVN and eMERLIN). It is as easy as:

planobs -b 6cm -t 'Altair' --network EVN eMERLIN

If you want to specify an epoch and some particular stations, you can do:

planobs --band 6cm --target 'Altair' --stations Ef Hh Ir Mc Tr Hh T6 O8 Wb Cm --starttime '2020-06-15 20:00' --duration 12
    --no-gui   # if you don't want to visualize the plots in the browser but only within the terminal

Station additions

The information about each station is stored in an independent file under data/stations_catalog.inp (following a Python configuration file format). Then, the addition or update of a new station is extremely straightforward. You can manually add a new station by introducing a new entry in the file with the following fields and syntax:

[Station Name]

station = Station Name
code = # An unique code to identify the station (it can be the abbreviation of the full station name).
network = # If the station belongs to one of the known VLBI Networks, or 'Other' otherwise.
possible_networks = # a comma-separated list of possible VLBI Networks that the station can join to observe.
country =  # Country where the station is located.
diameter =  # station diameter in free format (e.g. '30 m' or '30 x 20 m' is often used for the case of interferometers composed of 30 20-m antennas).
position = X, Y, Z  # Geocentric coordinates of the station.
min_elevation = XX  # minimum elevation the station can observe, in degrees. By default it is 10 deg if not specified.
real_time = no/yes  #  In case the station can participate in real-time correlation observations (e.g. e-EVN). By default 'no'.
SEFD_YY = ZZ   # Multiple inputs providing the estimated System Equivalent Flux Density (SEFD) of the station (ZZ measured in Jy) at the observing wavelength YY in cm. There should be one entry per observing band.
# The lack of entries would be understood as the station is unable to observe at such band.

We are more than glad to integrate any additional station that can be relevant to the purposes of this program.

If you have any suggestion, please open an issue in the GitHub repository, or contact the author.