BMarcote (bmarcote)

bmarcote

Geek Repo

Company:JIVE (Joint Institute for VLBI ERIC)

Home Page:bmarcote@github.io

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BMarcote's repositories

gmrt_pipeline

CASA-based Pipeline for uGMRT Data Reduction

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vex

Parser to read and save VEX files.

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vlbi_calculator

Sensitivity, elevation, and uv coverage calculator for a given VLBI observation

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evn_support

Collection of scripts and other tasks used by the EVN Support Scientists to process EVN data after the correlation and before the data is delivered.

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seffers

SEarch for Fringe-FindERS (for a given VLBI observation)

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evn_postprocess

Master script to run a semi interactive post-processing of EVN data

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vastrostuff

Singularity container of radio (specially VLBI) data tools

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binaries

Useful scripts to work with astrophysical binary systems

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casa_pipeline

CAPI: Pipeline to reduce radio data (VLBI and GMRT) in CASA

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measurements

Extends astropy.Quantity to support uncertainties associated to the values.

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antisafelinks

annihilating Microsoft Safelinks from emails and Milder folders

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aplpy

Astronomical Plotting Library in Python (note that APLpy 1.0 is now developed in the v1.x branch - see README.rst for more details)

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casa-vlbi

Scripts to assist VLBI data reduction in CASA

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Code-Refinery-GitHub-Workshop

Hands On repository.

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coderefinery-documentation-example-project

Example project for coderefinery documentation lesson

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coderefinery-workshop-day2-testcodes

A public repo to play with Git and GitHub

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conf_files

Configuration files for common programs.

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jiveplot

Python based plotting package for CASA MeasurementSet

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jupyter-casa

A Jupyter kernel for CASA

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PolConvert

Advanced polarization calibration of linear feeds in VLBI observations.

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sched

Fork of NRAO SCHED

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tools-osx

A small collection of command line tools for Mac OS X, incl.: clipcat, dict, eject, ql, swuser, trash & with.

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tps

Transient phase space diagram as seen in Nimmo et al. 2021 (https://arxiv.org/pdf/2105.11446.pdf), heavily inspired by Evan Keane's TPS code.

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VLBI-utilities

Utilities that can be used at stations to help with VLBI observations.

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