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  • šŸ‘‹ I am an observational astrophysicist. I got my PhD from Universite de Montpellier II in 2007. I did a postdoc at the University of Barcelona (UB): calibration of the photometric instrument of the Gaia space telescope (2008-2010). In Fall 2010, I joined the department of Physics and Astronomy at NDU university, Lebanon where I was the chairperson of the department. I am now an Associate professor at Saint Mary's College, Notre Dame, INDIANA, USA.

  • šŸ‘€ My research interests include the chemical composition of stars, synthetic spectra, binary stars, HgMn stars, model atmospheres, and numerical methods for astrophysics.

  • šŸŒ± Iā€™m currently invistigating ML/DL techniques to be applied to stellar spectroscopy in order to characterize stars from large survey

  • šŸ’žļø Iā€™m looking to collaborate on all ML/DL techniques that could be used in Astronomy

  • šŸ“« [email protected]

Marwan Gebran's Projects

astronomical icon astronomical

An interactive dashboard for visualisation, integration and classification of data using Active Learning.

basicatlas icon basicatlas

Python wrapper for running basic ATLAS-9/SYNTHE stellar models quickly and easily

blase icon blase

Hybrid data/model-driven approach to astronomical echelle spectroscopy data built on PyTorch

jupyter icon jupyter

Here I put all my nootboks that I have used when learning ML and DL

kaggle-courses icon kaggle-courses

Kaggle courses and tutorials to get you started in the Data Science world.

mgebran icon mgebran

Config files for my GitHub profile.

smelib icon smelib

Spectroscopy Made Easy Source Library

synple icon synple

An Easy-to-Use Wrapper for the Spectral Synthesis Code Synspec

tensorflow icon tensorflow

Project containig related material for my TensorFlow articles

transformers icon transformers

šŸ¤— Transformers: State-of-the-art Machine Learning for Pytorch, TensorFlow, and JAX.

ultralytics icon ultralytics

NEW - YOLOv8 šŸš€ in PyTorch > ONNX > OpenVINO > CoreML > TFLite

xspect icon xspect

Code to measure equivalent widths, derive stellar parameters, and determine elemental abundances from high-resolution spectra

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