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Moustakas's Projects

archetypes icon archetypes

Algorithms and documentation for generating spectral archetypes. Useful for redshift fitting, spectral classification, developing target selection algorithms, and a myriad other applications.

astronomy-camp icon astronomy-camp

Code for reducing data taken during Astronomy Camp (http://astronomycamp.org).

awesome-cv icon awesome-cv

:page_facing_up: Awesome CV is LaTeX template for your outstanding job application

breyo icon breyo

Reduction and analysis pipeline for the Breyo Observatory at Siena College.

desi-highschool icon desi-highschool

An introduction to the DESI project for high schoolers, with real data!

desi-photometry icon desi-photometry

DESI Legacy Imaging Surveys Photometry for observed and potential (DESI) targets.

dsecop icon dsecop

This repository contains data science educational materials developed by DSECOP Fellows.

hizea icon hizea

Studying a remarkable sample of intermediate redshift post-starburst galaxies selected from the Sloan Digital Sky Survey

impro icon impro

A wide-ranging suite of IDL routines which observational extragalactic astronomers may find useful.

impy icon impy

Miscellaneous collection of python and R scripts.

isedfit icon isedfit

iSEDfit is a Bayesian spectral energy distribution fitting code designed to extract the physical properties of galaxies from broadband photometry.

ispec icon ispec

Code to fully reduce and calibrate 2D longslit optical spectra, and to analyze the resulting 1D galaxy emission-line and continuum spectra using stellar population synthesis models.

legacyhalos icon legacyhalos

Code and papers for a multi-faceted study of the baryonic content of dark matter halos in Legacy Survey imaging.

lslga-inspect icon lslga-inspect

Visual inspection tool for large galaxies in the Legacy Surveys (http://legacysurvey.org/).

nearly_nmf icon nearly_nmf

Methodology to handle NMF when the data can be negative.

nonnegmfpy icon nonnegmfpy

Vectorized Nonnegative Matrix Factorization with heteroscedastic uncertainties and missing data

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