Staff Scientist at NASA HEASARC
- NASA Archival Data in The Cloud: Service & Discovery
I am a software engineer working at RHEA Group for the European Space Agency (ESA), specializing in heliophysics archives. My educational background includes a mathematics degree from Complutense University of Madrid (UCM) and a master's degree from the Autonomous University of Madrid (UAM).
My responsibilities involve delivering data collected from ESA missions to the scientific community using software applications. This involves a multi-step process: data ingestion, subsequent transformation, and delivery through web applications for the scientific community's utilization.
Linkedin profile: https://www.linkedin.com/in/adrián-trejo-gil-886725142/
- ESA Heliophysics archives interoperability and data access enhancements
- Binaural stellar spectra sonification based on variational autoencoders
- XMM-Newton Science Analysis System (SAS) on the cloud
- Decades of Transformation: Evolution of the NASA Astrophysics Data System's Infrastructure
- Building a production ML pipeline for gravitational wave detection
- The INAF radio data archive: from data publication to interoperability of time-domain data
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
I am a graduate student in Artificial Intelligence at the University of Bologna, Italy. This project was carried out as part of my master's thesis in the context of the AGILE space mission, working as an intern at the National Institute for Astrophysics (Istituto Nazionale di Astrofisica, INAF).
- Quantum Convolutional Neural Networks for the detection of Gamma-Ray Bursts in the AGILE space mission data.
- Using The NEOfixer API for NEO Follow-Up and NEO Queries
- Editor, Astrophysics Source Code Library (ASCL, ascl.net)
- Astronomy Department, University of Maryland College Park (US)
- Improving the visibility and citability of exoplanet research software
Research Software Engineer with a focus on data reduction pipelines.
PhD in Astrophysics with a focus on Low Surface Brightness structures.
- Bright Star Subtraction Pipeline for LSST: A Review of Progress
- From AI to L2 and beyond: A software engineer career turned into a journey through fascinating territories, landscapes and, of course, languages.
- The Supervisory Control and Data Acquisition Software System for the ASTRI Mini-Array Project
Graduated in 1993 from Novosibirsk State University, Russia. Master Degree in Computer Science with advancement in Physics and Mathematics.
1993 - 2000 - Budker Institute of Nuclear Physics. Automatization of physical processes (electron-positron collider, Novosibirsk, Russia; polarized electron source, Amsterdam, Netherlands).
2001 - 2018 - NASA Cassini mission, CIRS (Composite Infra-Red Spectrometer). Data processing. Software engineering.
2018 - present - University of Maryland, Small Bodies Node. Software engineering. Data processing. Database maintenance and distribution.
- The Small Bodies Node's MPC Annex and MPC Database Distribution System
- The Starchive
- Metrics are a kind of telemetry too: Time-series capture and curation with Sasquatch
Postdoctoral Researcher at Lawrence Berkeley National Laboratory.
- Open Source Software for Processing and Using Dark Energy Spectroscopic Instrument Data
- Improving CI/CD workflow efficiency with Kubernetes and an automated bot system
A software developer and researcher for the Radio Astronomy Research Group at the South African Radio Astronomy Observatory.
- RFInder: Radio Frequency Interference data evaluation and reduction
'm a Posdoctoral researcher at the Center for Astrophysics in Cambridge, MA. I develop new statistical methods and scientific open source software for the analysis of astronomical low counts data. I apply those methods to better understand the Galactic X-Ray and Gamma-Ray source populations.
I'm also interested in developing new methods and open data formats to combine data from multiple instruments, such as the Cherenkov Telescope Array Observatory (CTAO), H.E.S.S., HAWC and Fermi-LAT but also X-ray observatories such as Chandra. By advocating openess I hope to facilitate collaboration between astronomical observatories for better, more open and reproducible science.
I'm the lead developer of the open source software package Gammapy, sub-package maintainer of Astropy and a member of the CHASC astro-statistics collaboration. I'm also editor for the Astronomy and Astrophysics track of the Journal of Open Source Software JOSS.
- Joint Likelihood Deconvolution of Astronomical Images in the Presence of Poisson Noise
Baptiste Cecconi is a radio astronomer working at Observatoire de Paris. He contributed to many low frequency space radio instrument (Cassini, STEREO, JUICE, etc.)
- FAIR approach for Low Frequency Radio Astronomy
- Taking TESScut to the Cloud: Architecting for Availability, Performance and Cost
I'm a software developer and researcher at the South African Radio Astronomy Observatory. I work in radio polarimetry, galaxy cluster science, radio imaging and calibration algorithms and tooling for the MeerKAT radio observatory. I hold a BSc. (Hons.) and MSc. in Computer Science from the University of Cape Town and studying towards a Ph.D. in Radio Astronomy techniques at Rhodes University, South Africa.
- ALBUS: Modelling the Ionosphere with GNSS Interchange Data from the South African TrigNET
Staff scientist, MMT/Steward Observatory
- Why does every observatory, survey, project, and PI have to build their own incompatible archive from scratch? And can something be done about it?
- Ready-to-Use Astronomy Containers from CADC
I am an Assistant Scientist at the National Radio Astronomy Observatory (NRAO) in Socorro, New Mexico. I support Very Large Array (VLA) operations and conduct research in star formation, spectroscopic model fitting, and novel methods in radio astronomy. Prior to my appointment at the NRAO, I was a Jansky Postdoctoral Fellow at the NRAO, and earned my Ph.D. in astronomy at the University of Arizona.
- Bayesian non-LTE gas temperature estimation of cores in the CMZ using Julia
Senior in Mechanical Engineering with a minor in computer science at Columbia University School of Engineering and Applied Science.
- Using a convolutional neural network with all sky infrared images to classify sky regions as clear or cloudy
Bruce is the head of the Keck Observatory Archive, and the NASA/NAVO representative on the IVOA Executive Committee. His interests include in image processing, and investigating the application of cloud platforms in astronomy.
- Processing All- Sky Images At Scale On The Amazon Cloud: A HiPS Example
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
- Revealing the Unknown Unknowns: Citizen Science as a Tool for Exploring Large Data Sets
- Planetary World Coordinate System in Astropy
Chi-kwan "CK" Chan is an Associate Astronomer/Research Professor at the University of Arizona. He leads both the Software and Data Compatibility and the Gravitational Physics Working Groups of the Event Horizon Telescope (EHT). CK created the collaboration's computational and data processing infrastructures and continues to manage them to this day. In addition to pioneering the use of Graphics Processing Units (GPUs) to accelerate the modeling of black holes, CK also developed many new algorithms to improve and accelerate modern research, built cloud computing infrastructures for large observational data, and applied machine learning algorithms to speed up and automate data processing.
- Cloud Data Processing for the Event Horizon Telescope
Chris is a software developer at the Lunar and Planetary Lab's Planetary Image Research Laboratory at the University of Arizona. He has been developing science-driven mission planning tools for around 20 years, largely in Java, Perl, C, and Python.
- Building a Science-Driven Mission Planning Tool with JMARS
- from 2023: "CCAT Data Center Manager" at University of Cologne
- 2014-today: PostDoc at University of Cologne, Germany
- Projects: GREAT/SOFIA, NANTEN-2, HIFI-ICC, CCAT
- 2009-2013: PhD Student /Astronomer on Duty at IRAM 30m, Granada, Spain
- Thesis: "The cold and dense interstellar medium of M 33"
- 2008-2009: Diplom-Thesis at Max-Planck Institut for Radioastronomy, Bonn, Germany
- Thesis: "An In-depth Study of the Interstellar Medium in the Barred Spiral Galaxy NGC3627"
- 2003-2009: Study of Physics at University of Bonn, Germany
- The CCAT Data Center
- The International Virtual Observatory Alliance in 2023
Chris Jeschke is an Assistant Group Supervisor and Research Software Engineer within the Space Exploration Sector at Johns Hopkins Applied Physics lab, where he enjoys applying the latest in cloud technologies and software engineering tools to develop novel solutions that enable space science and exploration.
- HelioCloud: A cloud-native platform for accelerating heliophysics research
I earned my Ph.D. at the Università Statale di Milano, working in the field of Ultra-high energy cosmic ray physics focusing on scientific software development and data analysis for the Pierre Auger Observatory.
I am currently a post-doctoral researcher at the Observatoire de Paris, where I work mainly as a developer and maintainer of Gammapy, an open-source Python package for very-high-energy astronomy.
- Open developments towards VHE multi-messenger astrophysics: the open library Gammapy with the Very-high-energy Open Data Format
I am a software engineer with a decade of experience in industry development, and I am relatively new to development in astrophysics.
I have experience with:
* Python
* postgres
* mysql
* javascript
* react
* typescript
* php
* ruby/rails
* mongoDB
* AWS
* Kubernetes
* Kafka
* Docker
* git
My past experience includes working at:
* RoundingWell
* Emma/Campaign Monitor
* Lonely Planet
* Dutchie
- General Coordinates Network
- VESPA Portal
Dr Darg is a member of the PDS Small Bodies Node at the University of Maryland, where he mostly writes software and dev-ops operations in support of the group's research. He has a DPhil in Astrophysics from Oxford University, and has held postgraduate positions at Oxford and Johns Hopkins University.
- CATCH: Finding celestial objects with Google's Spatial Indexing Library 'S2'
Daniel Wright was born in Wakefield, United Kingdom in 1982. He received the M.Eng degree in electronic engineering from the University of York, York, United Kingdom, in 2013. He then received the Ph.D degree in electronic engineering from the University of Sheffield, Sheffield, United Kingdom in 2021. From 2014 to 2015 he was with the RAL Space division of Rutherford Appleton Laboratory, Didcot, United Kingdom, focusing on the electronic design of spacecraft instrumentation. He is currently with the Oxford e-Research Center, University of Oxford, Oxford, United Kingdom, working on the deign of software for the Science Data Processor of the Square Kilometer Array. His research interests include radio astronomy algorithms and GPU acceleration.
- CLEAN algorithm implementation comparisons between popular software packages
Team Lead, Radio Software Group at the National Research Council of Canada - Dominion Radio Astrophysical Observatory
- The DRAO Solar Flux Monitoring Programme: Nearly 80 Years of Staring Directly at the Sun
Contributing to the development of IVOA standards since 2003.
- Evaluating IVOA ExecutionPlanner for CIRASA tools
- Improving Legacy Systems at the Minor Planet Center
- Best practices for developing high quality scientific pipelines in the framework of the ESA PLATO mission
- AstroDB Toolkit: A Collaborative Data Management Tool
- Annotated Coadds: Concise Metrics for Characterizing Survey Cadence and for Discovering Variable and Transient Sources
- ESASky: Unveiling the Universe through Multi-Wavelength and Time-Domain Exploration
Demitri Muna is a support scientist at the Chief Science Data Office at NASA Headquarters. He has a long background in developing astronomical software on projects like the Sloan Digital Sky Survey and Starchive, and has several open source packages available on GitHub. Demitri created and has taught the SciCoder workshop for early career astronomers since 2010. He will always ask you about the user interface for your code before the nuts and bolts behind it.
- NASA SMD Information Policy: Let's All Be FAIR
- Predicting the Radiation Field of Molecular Clouds using Denoising Diffusion Probabilistic Models
Dustin Lagoy is a researcher at the Dominion Radio Astronomy Observatory in Penticton, British Columbia. He focuses on software development for processing and distributing high-volume radio telescope data, as well as telescope control and digital systems. Before working in radio astronomy he developed hardware and algorithms for airborne and space-based remote-sensing radar systems at the NASA Jet Propulsion Lab and the University of Massachusetts.
- ML and next steps in the DRAO data handling pipelines
Dustin Swarm is a postdoctoral research scholar at University of Iowa. His research is in machine learning applications in high-energy astrophysics and cataclysmic variable systems. He also conducts ray tracing simulations for X-ray instrumentation.
- Outlier Identification in the Chandra Source Catalog
PhD student in Astrophysics at Università di Bologna (Unibo, Italy) and Istituto di Radioastronomia (INAF-IRA, Italy).
My main fields of interest are radio galaxies and galaxy clusters at low frequency and development of software for radio astronomy.
- GPU implementation in radio astronomy: a “giant leap” into the SKA era
Emmanuel Joliet has over 20 years of experience in the space and aeronautical industries, working on software development, data visualization, and data processing. His background is space engineering and astronomy.
He joined Gaia Science Operations team at ESAC in 2006 and contributed to key aspects of the mission.
In 2015, he moved to California to become the UI team lead for the NASA/IPAC Infrared Science Archive at Caltech.
Since 2020, he took the role of leading the Roman SSC pipeline development team and configuration management.
He is the project lead of Firefly (https://github.com/Caltech-IPAC/firefly), an open-source web-based UI library for astronomical data archive access and visualization.
He is a Cloudera Certified Developer for Apache Hadoop and HBase Specialist, and has a certificate in Machine Learning and data analytics from Caltech. He is also a HEALPix developer.
He's trained as Cloud Architect and developer using AWS, Azure and Google Cloud platform tools.
Publications: https://orcid.org/0000-0003-4824-0102
- Running Roman pipelines in NASA cloud with Airflow and Kubernetes
SE is a specialist of solid phase spectroscopy and surface studies. Currently a coI of several instruments on BepiColombo, formerly French team leader of VIRTIS on Rosetta. Coordinator of the VESPA activity in Europlanet programmes.
- Planetary World Coordinate System in Astropy
- Study of a spectral analysis system for planetary surfaces
Eva Sciacca (Ph.D. in Mathematics for Technology) is a Computer Scientist and Information Technology researcher with over a decade of experience, working at the Istituto Nazionale di Astrofisica (INAF) since 2012. She has been extensively involved in cutting-edge research activities in the field of big-data, visual analytics, and machine learning. She has been instrumental in facilitating astrophysical data processing on distributed computing infrastructures, with a special focus on High-Performance Computing (HPC) and Cloud Computing. Over the past five years, Eva has played a pivotal role in several European-funded projects, including VIALACTEA, INDIGO-DataCloud, AENEAS, EOSC-Pilot, NEANIAS, and SPACE. She has been at the forefront of harnessing the potential of the European Open Science Cloud (EOSC) and the European High-Performance Computing Joint Undertaking (EuroHPC JU) to advance scientific research, and she is actively involved in the IT activities of the Square Kilometre Array (SKA) Regional Centres.
- High performance visualization for Astronomy & Cosmology: the VisIVO’s pathway toward Exascale systems
Mr. Fabio Hernandez has been working in the field of computing for high energy physics research for more than 25 years. Affiliated to IN2P3/CNRS, the French national institute for nuclear physics and particle physics, he is currently the technical leader of the French component of the data processing infrastructure for performing the Legacy Survey of Space and Time (LSST) of the Vera C. Rubin Observatory.
Prior to that position, he spent several years as a senior international scientist visiting the Institute of High Energy Physics in Beijing (China) and served as an expert in the Office for science and technology of the Embassy of France in China. As the deputy director of France’s IN2P3 computing center and technical leader of the French contribution to the Worldwide LHC Computing Grid (WLCG), he was deeply involved in planning, prototyping, deploying and operating the global computing platform designed for processing the data produced by CERN’s Large Hadron Collider (LHC).
During his career, he has been very active in several projects sponsored by the European Commission in the field of distributed computing for science in Europe and in Latin America. He has held positions leading engineering teams in charge of software development for massive data storage, data center operations and distributed computing for international science projects.
Mr. Hernandez received his BSc. in computer science from University of Los Andes (Bogota, Colombia) and his MSc. in computer science from University Lyon 1 (Lyon, France).
- Preparing a scientific data processing facility for Rubin Observatory’s LSST: the case of France’s CC-IN2P3
- High performance visualization for Astronomy & Cosmology: the VisIVO’s pathway toward Exascale systems
- A new architecture of Convolutional Neural Networks for astronomical data
- Revealing Predictive Maintenance Strategies from Comprehensive Data Analysis of ASTRI Horn Historical Data
- Non-negative matrix factorization approach to sky subtraction for optical spectroscopy
- High throughput VLA Imaging with multiple GPUs
- "You might also like these images": unsupervised affine-transformation-independent representation learning for the ALMA Science Archive
I'm working at CDS since 1987 as a software engineer. I'm working in the Aladin team and contributes to IVOA since 2002. I am involved in the SKA SRC network since spring 2022.
- Mapping VOTable Data on Data Models: Implementation Status and Progress
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
Rubin Data Services Lead, Rubin Observatory
- Rubin Science Platform: on cloud, on-prem, all of the above
- Mapping VOTable Data on Data Models: Implementation Status and Progress
- Presentation of the Astronomical Table Serialisation System Query tool (QATSS) and its ecosystem.
- Preparing a scientific data processing facility for Rubin Observatory’s LSST: the case of France’s CC-IN2P3
Genie Hsieh received her Ph.D in Computer Engineering at the University of New Mexico. She has 10+ years of experiences in numerical methods development for simulation and modeling and scientific software development in the field of high performance computing, electrical systems, biology and image processing. She is a Software Engineer at NRAO now applying her expertise in HPC and medical image analysis to radio astronomical imaging techniques.
- An Adaptive-Scale Multi-Frequency CLEAN Deconvolution in CASA for Radio Interferometric Images
- An original way to manage huge astronomical table
- Mapping VOTable Data on Data Models: Implementation Status and Progress
- TSRS-Heritage Archive: Digitisation, Standardisation, and Future Perspectives
- Science Platform in the multi messenger and exascale era.
Technologist and software developer @ INAF - Osservatorio Astronomico di Cagliari
- Remote observations with DISCOS and the Sardinia Radio Telescope
- VisIVO Visual Analytics: An Interactive Visualization Tool for Astrophysical Data Analysis
Dr Gordon WH German is a CSIRO Senior Engineer for the Australian SKA Regional Centre, located in Perth Western Australia. He specialises in data reduction pipelines for ASKAP science projects, and is involved in the global SRCNet effort to provide data handing and reduction for the upcoming Square Kilometre Array Observatory.
- Processing large Radio Astronomy data cubes within an Objectstore
- The Rubin Science Platform: powered by IVOA standards and contemporary software deployment methodologies
- Mapping VOTable Data on Data Models: Implementation Status and Progress
- PEG-ify ADQL
I am a student at the Complutense University of Madrid in Spain, currently getting my Master's degree in Astrophysics. I am currently learning and working with different implementations of Machine Learning and Deep Learning in both regression and classification using datasets of galactic properties and images from deep survey missions.
At the moment I am working on my Master's Thesis with the European Space Agency (ESA) and the spanish Astrobiology Center.
- Using Open Science Studio platform to study structural relationships of remote galaxies from the CANDELS catalogs
- Accelerated Briggs Weighting Function on NVIDIA GPUs with CUDA
Ph.D. in radio astronomy
Dutch National Weather Institute
Dutch National Cancer Institute
Efficient computing
GPU programming
From 2015 - present at The Netherlands eScience Center
- From LOFAR to SKA: towards a GPU-based source extractor
- Discover your astronomical data from python – simply!
- Multi-wavelength archival research: where are the obstacles and how to tackle them?
- 3D visualisation of radio data in scientific archive
As an Operations Data Scientist at SKAO, I'm part of the team tasked with developing and prototyping the software for the globally distributed network of SKA Regional Centres.
- The Road to Science Verification for the SKA Regional Centre Network
- Comet Statistics - A graphical representation of international comet discovery and observation statistics from the NASA PDS Small Bodies Node and the Minor Planet Center
- hypothesis - property-based testing for Python
- The continuing evolution of the Data Central web service
- Creating Spectral Cubes from NIRSpec MSA slitlet stepped observation
- What’s new on ESA Datalabs?
- Navigating ESA HST and JWST Science Archives through Automated Jupyter Notebooks
- SPOT: A collaborative framework for Planetary Science Operations Planning
Postdoctoral Researcher
MIT Kavli Institute for Astrophysics and Space Research
Massachusetts Institute of Technology
- Developing an efficient large-scale machine learning pipeline to classify the millions of NASA TESS light curves in search for variable stars
- Lessons Learned from a Multi-wavelength Time Domain Use Case on a Science Platform
As an astronomical software developer at the Smithsonian Astrophysical Observatory, I have worked on data pipelines for instruments which produce spectra and scan the sky. At MIT, Cornell, and MIT again, worked on spectra of solar system objects, positions of stars and planets and modelled planetary rings and multiple stars from occultation data, all of which I wrote pipelines to reduce. Over the past I also have worked on inclusion, diversity, and equity issues in astronomy, locally, nationally, and internationally.
- Writing Software Which Will Continue to Work
- The Future of FITS and Other Standardized Astronomical Data Formats.
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
- SKA Regional Centres Architecture: One data lake, multiples nodes
- User Experience and its role in astronomy
John Romein is researcher at ASTRON (the Netherlands Institute for Radio Astronomy) since 2004, and is Principal Investigator of several projects on High-Performance Computing for radio astronomy. His primary focus is the use of accelerator hardware, such as GPUs and FPGAs. John Romein received his Ph.D. in Computer Science at the Vrije Universiteit, Amsterdam in 2001, on distributed game-tree search. As a postdoctoral researcher, he solved the game of Awari using a large computer cluster and did research on parallel algorithms for bioinformatics. His research interests include high-performance computing, parallel algorithms, networks, programming languages, and compiler construction.
- Streaming Signal Processing on GPUs
- Automated anomaly detection at scale with the cloud-based Roman Data Monitoring Tool
Jonathan is a senior DevOps engineer at Rubin Observatory, and now contributes as a contractor through J.Sick Codes Inc. from Canada. Jonathan's main contributions are to Rubin's documentation platform, science platform, and internal developer service infrastructure, Jonathan's go-to technologies are Python and FastAPI for web applications, React/Next.js for front-end applications, Kafka for event streaming, and Kubernetes with Argo CD for application deployment. Previously Jonathan received a PhD in astronomy from Queen's University for a near-UV to near-IR study of the Andromeda Galaxy's integrated and resolved stellar populations with CFHT.
- UX for Docs: Documentation Engineering at Rubin
- HelioCloud: A cloud-native platform for accelerating heliophysics research
- A Generic Interface for Serving Time Series Data: HAPI Explained
I am an astronomer interested in time-domain astronomy, photometry extraction methods, data-driven solutions, machine-learning applications for astronomy, and software development for data analysis.
I got my Ph.D. in Astronomy in 2018 at Universidad de Chile. I am currently a research scientist at Bay Area Environmental Research Institute at NASA Ames.
- PSFMachine: a Python library for rapid PSF photometry on Kepler/TESS data
- Europe's revolutionary sky surveyors: Gaia and Euclid
- New Generation of Proposal Handling System (PHS) for ESA Missions: Evolution of XMM-Newton Software
- XMM-Newton Science Analysis System building evolution over the years.
- BurstCube Ground Software and Data Analysis Pipeline
- SOFIA/GREAT: post-ops and quality measures for heterodyne data
Julie is a Professional Research Assistant at the Laboratory for Atmospheric and Space Physics (LASP), partnered with the University of Colorado Boulder. She is passionate about leading and facilitating technical work and group efforts across organizational and cultural boundaries, and building relationships within communities in the process. Her interdisciplinary background is fitting for this kind of work; she comes with a B.S. in applied physics (2015), an M.S. in atmospheric science (2018), and experience working with several space mission software and community projects—in particular, including being the principal investigator for the Python in Heliophysics Community (PyHC).
- The Python in Heliophysics Community: an overview and call to connect with the wider ADASS Python community
- Using unsupervised learning for explorative discovery in astrophysical simulations
Karel Adamek is a departmental lecturer at the University of Oxford and currently contributes to the Square Kilometre Array with an interest in many-core architectures and data processing in astronomy in general.
- Towards using GANs in astrophysical Monte-Carlo simulations
- AstroDB Toolkit: A Collaborative Data Management Tool
- Galaxy cluster detection on SDSS images using deep machine learning
- Cartographic Mapping using High-Resolution Shape Models
ATLAS Co-PI and senior software engineer Larry Denneau was the chief software architect of the Pan-STARRS moving object processing system (MOPS) and adapted it to ATLAS. MOPS is a software package that automatically identifies solar system objects (in particular hazardous asteroids) in the ATLAS and Pan-STARRS data streams.
Larry has been poking at computer keyboards since the early 80s and received his B.S.E.E. from the University of Arizona, whereupon he quickly escaped academia. His software career has spanned projects ranging from surface metrology for the semiconductor industry, medical scheduling, geophysical instrumentation, and a dot-com Internet startup that actually turned a profit. Now back in academia, Larry received a Ph.D. in astrophysics from Queen's University Belfast and has enthusiastically joined the effort to protect the earth from dangerous asteroids.
- Software and Shared Workflows for the Planetary Defense Community
I work on the Subaru Prime Focus Spectrograph Galactic Archeology project.
- Simulating stellar color-magnitude diagrams on the GPU
- Project Manger for the XMM-Newton SSC activities in Strasbourg
- Project manager for ground segment software of the MXT camera of the SVOM spacecraft
- Former data model working group chair in the IVOA
- Mapping VOTable Data on Data Models: Implementation Status and Progress
Head Oh the IT department of Observatoire de Paris
Technical manager of Paris Astronomical Data Centre
Chair of the IVOA applications working group
- Planetary science discovery portals with spatial selection
Automation Engineer working at the Astrophysics and Space Science Observatory of Bologna (OAS), a branch of Italian National Institute for Astrophysics (INAF).
- A new Deep Learning Model for Gamma-ray bursts’ light curves simulation
- The Online Observation Quality System Implementation for the ASTRI Mini-Array Project
- O-type Stars' Stellar Parameter Estimation with ANN
- AI in Astronomy
- Collaborative and Guided Visual Analytics Methods for Space and Planetary Science Applications
Manuel Parra Royón is a postdoctoral researcher at the Instituto de Astrofísica de Andalucía (IAA-CSIC) in Spain. His research interests include data mining, machine learning, and big data analytics. He is currently working on the development of the SKA Regional Centres Network for the Square Kilometre Array Observatory (SKAO).
Manuel received his Ph.D. in computer science from the University of Granada in 2019. His dissertation focused on the use of machine learning for data mining in cloud computing. He also holds a Master's degree in Data Science and Intelligent Systems and a degree in Computer Science.
Before joining the IAA-CSIC, Parra Royón worked as researcher at the University of Granada, where he was involved in several projects on big data analytics, Machine Learning, IA and Science platforms. He also worked as a data engineer at the European Organization for Nuclear Research (CERN) in Geneva, Switzerland.
Parra Royón is passionate about using data science to solve real-world problems. He is particularly interested in using data mining to improve the efficiency and effectiveness of large-scale scientific experiments.
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
- Empowering SKA Data Challenges: A homogeneous platform for enhanced collaboration and scalability fully aligned with Open Science.
- SKA Observatory software
- The INAF radio data archive: from data publication to interoperability of time-domain data
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
- TSRS-Heritage Archive: Digitisation, Standardisation, and Future Perspectives
- ViaLactea Knowledge Base: status and perspectives
- Navigating ESA HST and JWST Science Archives through Automated Jupyter Notebooks
- EXPLORING THE DARK SIDE OF THE UNIVERSE: THE EUCLID SCIENTIFIC ARCHIVE SYSTEM
- Navigating ESA HST and JWST Science Archives through Automated Jupyter Notebooks
- Exploring the journey towards scientific knowledge through one year of public data at the European JWST Archive
SW Engineer at Aurora Technology. Since 2013, working as external personal for the ESAC Science Data Center (ESDC) of the European Space Agency (ESA)
MSc in Computing Engineering
MSc in Astronomy
Interests: ML, IA
- DOIs at the ESDC and the new ESDC DOI TAP Service.
2022-Present - PhD at Heidelberg University & Max Planck Institute for Astronomy & Heidelberg Institute for Theoretical Studies;
2020-2022 - MSc in Computer Science at Moscow Institute of Physics and Technology;
2016-2020 - BSc in theoretical astrophysics at Moscow Institute of Physics and Technology
- Point-spread-function interpolation as a key to precise scientific outcome
- HelioLinC3D: Software for Discovery of Solar System Objects in LSST-scale Datasets
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
Mark Kettenis is a Software Project Scientist at the Join Institute for VLBI in Europe. He is involved in the various software projects for processing of VLBI data, from data acquisition all the way though data processing software in the end-user domain.
- VLBI data processing in CASA
- The VLA Sky Survey
Software engineer working on data manipulation tools and the Virtual Observatory.
- TOPCAT Corner Plot
- Discover your astronomical data from python – simply!
- PEG-ify ADQL
- All your shapes in ADQL: MOCs in the TAP ecosystem
- The INAF radio data archive: from data publication to interoperability of time-domain data
Martin Beroiz is a strong Python and C programmer with skills in web development and the design of libraries and applications. He is currently employed by the California Institute of Technology (Caltech) in a scientific staff position for the LIGO Laboratory. His interests include API Design, UI/UX, Astronomy Software and Automation.
- Distributing Public Data with the Gravitational Wave Open Science Center
Working at the CDS from 2018, I did develop expertise in software development and visualisation for astronomy. Since then I did contribute to the maintenance of open source astronomy python libraries such as Astroquery, MOCpy and Aladin Lite. My main work is related to the development of the web viewer Aladin Lite. I am also part of SKA where I am involved in the SRC Network as a member of the team specialized in the visualisation of large radio data cubes.
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
- Lessons learned from building LOFAR data pipelines
Max Brodheim is a Scientific Software Engineer and Data Reduction Pipeline Lead at the W. M. Keck Observatory.
- FITS Data Displays for Observatory Operations
Meredith Rawls is a research scientist in the Department of Astronomy at the University of Washington. She writes software and data pipelines to handle terabytes of nightly images from Vera C. Rubin Observatory's Legacy Survey of Space and Time, which will produce the highest resolution movie of the night sky ever made. Her background is in stellar astrophysics, and she earned her PhD from New Mexico State University. Lately she studies the plethora of newly-launched commercial satellites in the hopes observers worldwide don't lose the sky, and she co-chairs SatHub at the new International Astronomical Union Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference (IAU CPS).
- Quantifying and Mitigating Satellite Constellation Interference with SatHub
- Deep Learning and IACT: bridging the gap between Monte-Carlo simulations and LST-1 data using domain adaptation
- Modernizing IRAF to Support Gemini Data Reduction
I have always loved research in galaxies and larger-scale objects. I pursued stargazing and astrophotography in my early life. I received an Associate of Science from Dixie State University (2009), where I worked under a NASA undergraduate grant to relate solar cycles to satellite observations of oxygen and temperature variations within the ionosphere. I received a Bachelor in Physics Astronomy from Northern Arizona University (2012), where I worked under a NASA undergraduate grant to map ancient Mars environments inferred from 10,000 crater morphologies I cataloged. I received a Ph.D. and Master in Physics from the University of Utah (2021 ), where I spectroscopically detected -1,600 strong galaxy-scale gravitational lens candidates in preparation to study how galaxies form and evolve.
- Improving Stellar Dynamic Modeling of Single-Fiber Kinematics
- IAU CPS SatHub and Tools to Mitigate Satellite Constellation Interference
Miguel Flores R. is a Ph.D. student at the University of Guadalajara working on the applications of ANN for processing and fitting models of stellar spectra. He is also a Sr. Data Science Globant developing models for systems that go from optimization in the energy and natural resources sector, to gaming live operations. Flores holds a BSc and MSc degrees in physics from the University of Guadalajara. During his former years, his research interests were in the areas of quantum information theory and complex systems focused on discrete systems dynamics. In 2018 has the opportunity of working in the Global IA and Data Science team at HP Inc. in Palo Alto, CA, working on human behavior models and web interactions. His current research project explores the multidisciplinary application of IA structures to process, analyze and model big dimensional systems.
- Fundamental Parameter Estimations of O-type Stars Binary Systems Using Recurrent Neural Networks
I am an assistant professor at Strasbourg University and a collaborator of the Centre de Données Astronomiques de Strasbourg (CDS).
- Mapping VOTable Data on Data Models: Implementation Status and Progress
Postdoctoral researcher at the University of Arizona
- A data processing pipeline for the Aspera SmallSat Mission
- PyCPL: The ESO Common Pipeline Library in Python v1.0
Nicholas is a Telescope Computer Engineer at the National Research Council's Dominion Radio Astrophysical Observatory up in Canada. He builds control systems for a number of on-site radio telescopes. He is also a PhD candidate at the University of Victoria working on Radio Frequency Interference monitoring.
- To monorepo or not to monorepo: a multi-lingual, telescope-agnostic steering control system
- EXPLORE science platform and scientific data applications for space sciences
- High performance visualization for Astronomy & Cosmology: the VisIVO’s pathway toward Exascale systems
HiRISE Science Operations and Software Engineer
Lunar and Planetary Laboratory
The University of Arizona
Tucson, Arizona
- Updating science operations planning software for a sudden loss of capacity in the HiRISE CCD array
I am a Technologist at the Italian Institute for Astrophysics. I am involved in the development of real-time analysis pipelines for high-energy projects such as AGILE, CTA, and ASTRI Mini Array. My research is focused on the implementation of Deep Learning models to analyze high-energy astrophysical data.
- Preliminary results of a new Deep Learning model to predict from the orbital parameters the background count rates of the AGILE Anticoincidence System.
- Learning from the Machines
- A brightening future for research software engineering
- Automated anomaly detection at scale with the cloud-based Roman Data Monitoring Tool
Distinguished Professor Oleg Smirnov holds the SARAO Research Chair in Radio Astronomy Techniques & Technologies (RATT) at Rhodes University, and also heads the Radio Astronomy Research Group at the South African Radio Astronomy Observatory (SARAO). He is an expert in observational radio interferometry, calibration and imaging algorithms, data processing and software infrastructure for the new generation of radio telescopes, including South Africa’s MeerKAT telescope, a precursor for the Square Kilometre Array. His RATT group has produced some of the most spectacular MeerKAT images published to date.
- Stimela 2, kubernauts, and dask-ms: radio interferometry data reduction in the cloud
- New software tools provided by the Minor Planet Center
I am a research professor at The George Washington University. My research area is multi-wavelength observations of magnetic cataclysmic variables with a current focus on radio observations. I have been developing scientific software for over 40 years. My first project was developing a data acquisition program for an optical polarimeter at the South African Astronomical Observatory. The program was written in the C programming language for an IBM AT personal computer. In the mid-90s, a colleague and I advocated for Python to be the primary data analysis language for astronomy. As a result, I spent a number of years at the Space Telescope Science Institute developing core Python packages for scientific computing and astronomy, e.g., numerical python/numpy, PyFITS, and matplotlib. In the last five years, I have migrated from Python to the Julia programming language, because I believe it is the future of scientific programming. I am currently developing various core Julia modules and applications for astronomy. Two such modules are the Astrometry module for precise time and position calculations, and Visfit for analyzing radio interferometric data.
- The current state of Julia software libraries for astronomy
- Comet Statistics - A graphical representation of international comet discovery and observation statistics from the NASA PDS Small Bodies Node and the Minor Planet Center
I don't have a life.
- A Dynamic GUI to Supercharge your Scripts
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
- Profiling and Optimizing the High Performance Gridder
- MPEC Watch, a novel community reference resource based on the Minor Planet Center live data
Ramon Ramirez-Linan is CTO and Co-founder of Navteca, a small business that focus on helping scientific organizations like NASA, NOAA and USGS to accelerate new technology adoption to increase research and discovery pace.
Ramon works primarily on the NASA Science Cloud at GSFC , his team deploys and managed Open Science Studio, a Jupyterhub + HPC based platform
- Using Open Science Studio platform to study structural relationships of remote galaxies from the CANDELS catalogs
- SAMP ImageJ Plugin
- Discover your astronomical data from python – simply!
MSc student in Artificial Intelligence at the University of Bologna. Bachelor's degree in Computer Science at the University of Pisa. Intern at the National Institute of Astrophysics (INAF).
- A new Deep Learning Model for Gamma-ray bursts’ light curves simulation
- Towards Machine-Interpretable Coordinate Transform Metadata in Heliophysics
Rob Seaman is the Data Engineer and a Co-investigator for the Catalina Sky Survey (CSS) of the Lunar and Planetary Laboratory at the University of Arizona. Using multiple survey and follow-up telescopes in Arizona and Australia, CSS has discovered nearly half of all near-Earth asteroids, including four impactors and two mini-moons. Rob serves as chair of the IAU Time Domain working group and co-chairs the SPIE Observatory Operations conference. His diverse interests include archiving, rapid transient response, data compression (FPACK), and timekeeping in astronomy.
- Welcome to ADASS
- The Future of FITS and Other Standardized Astronomical Data Formats.
Dr. Ronan Higgins is a postdoctoral researcher at the University of Cologne. He is currently working as the deputy project engineer for the CCAT observatory. He did his PhD at Maynooth university on the HIFI instrument flown on board the Herschel space observatory. After his PhD he started a postdoctoral position at the University of Cologne where he worked as the support astronomer for the NANTEN2 telescope in norther Chile with particular focus on the SMART heterodyne array receiver. As SOFIA (Stratospheric Observatory for Infrared Astronomy) operations ramped up in 2015 he joined the upGREAT team and worked as an instrument scientist with a focus on the calibration software and housekeeping system. Since 2021 he works on the CCAT observatory which is currently under trial assembly in Germany with shipment to Chile planned for 2024.
- SOFIA/GREAT: inflight operations of a heterodyne receiver
- Radio celestial source fringe signals detection based on Transformer self-attention mechanism
- The Future of LOFAR Data Services
Sara de la Fuente is an Aerospace Engineer with more than two decades of experience working in the design and execution of space operations for the European Space Agency (ESA). Her experience in ESA missions is very extensive, working in the Flight Dynamics Interplanetary Team for missions like Mars Express and Rosetta, in the Galileo Constellation Ground Control Segment Team, and in the Planetary Science Ground Segment Team for BepiColombo and JUICE missions.
She has also extensive experience in team coordination and technical leadership in Space Operations and Development, working as Flight Dynamics Engineering Team Coordinator for the European satellite navigation constellation Galileo, and as Science Operations Development Team Coordinator for the BepiColombo probe to Mercury.
She is currently the Science Operations and Software Development Manager of the RHEA Group Service Team at the European Space Astronomy Centre (ESAC) for the following Planetary missions: Mars Express, ExoMars TGO, BepiColombo, JUICE & EnVision.
- SPOT: A collaborative framework for Planetary Science Operations Planning
- Towards automated structural analysis of galaxies in large imaging surveys
- EXPLORING THE DARK SIDE OF THE UNIVERSE: THE EUCLID SCIENTIFIC ARCHIVE SYSTEM
- Experimenting with Large Language Models and vector embeddings in NASA SciX
M.C in Physics by Universidad Nacional Autónoma de México.
PhD in Astrophysics by Universidad de la Laguna, Tenerife, Spain.
Researcher at Universidad de Guadalajara, México.
Main research topics: evolution of low-mass stars and applications of AI in Astronomy.
- Automatic classification of evolved objects from the Gaia’s DR2 and DR3 databases using Deep Learning Tools
Researcher at the Institute of Astronomy and Meteorology of CUCEI, University of Guadalajara, México.
Research areas: Application of Artificial Intelligence techniques in Astronomy.
Kinematic and polarimetric analysis of Planetary Nebulae and symbiotic systems.
Determination of distances to Planetary Nebulae.
- Automatic classification of evolved objects from the Gaia’s DR2 and DR3 databases using Machine Learning Tools
Simone Riggi received the Ph.D. in Physics from the University of Catania (Italy) in 2010. He currently holds a permanent position as Research Technologist in the IT and Radioastronomy group of the INAF-Osservatorio Astrofisico Catania (Italy). Previously, he was a post-doctoral fellow at the Universidad de
Santiago de Compostela (Spain), Centro Siciliano di Fisica Nucleare e Struttura della Materia (Italy) and visiting student at the Forschungszentrum Karlsruhe (Germany).
His research activity mainly focuses on Radioastronomy, High-Energy Cosmic Rays, Muon Tomography, Computer Science. He was involved and contributed to several research and technological projects, among them the Square Kilometer Array (SKA) as member
of the Dish and Telescope Manager consortia, the Australian Square Kilometre
Array Pathfinder (ASKAP) as member of the EMU survey, the H2020 AENEAS
project for the design of SKA Regional Data Centers, the Pierre Auger Observatory and the Muon Portal project. Present technological activities include the development of monitoring and control systems for medium/large scientific facilities, simulation and modelling, design and development of data analysis software for astronomy and astroparticle physics, distributed computing and
scientific visualization. He is author/co-author of more than 100 scientific publications and conference communications in these research and technological fields.
- Detection and classification of radio sources with deep learning
Simon is the co-head of the Research Data & Software group at the AAO in Macquarie University, and leads a range of software and data projects, including the Data Central Science Platform. In a former life, he was a research astronomer, studying stellar oscillations and exoplanets.
- The International Virtual Observatory Alliance in 2023
Solai Jeyakumar
Departamento de Astronomia
Universidad de Guanajuato
Mexico
- Galaxy Classification using Topological Data Analysis
- Mapping VOTable Data on Data Models: Implementation Status and Progress
- A Good IDIA : Scientific Computing at Scale
Associate Astronomer at NSF's NOIRLab, Survey Data Scientist for the Astro Data Lab and Lead Scientist for the CSDC Spectroscopic Services
- SPARCL: SPectra Analysis and Retrievable Catalog Lab
- Open Source Science Initiative at NASA
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
I am a graduate student who is interested in how mathematical tools can be used to unravel the mysteries of the universe. My current areas of interest are mathematical modeling, data analysis, and space plasma physics. I am currently working with Dr. Kristopher Klein of the University of Arizona's Lunar & Planetary Laboratory. Together we are working on improving and quantifying data analysis techniques which will be applied to the multi-spacecraft NASA mission HelioSwarm.
- Multi-Spacecraft Observatory Data Analysis Techniques
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
Data Scientist at LAPP, CNRS, working on deep learning for Imaging Atmospheric Cherenkov Telescope and on open software in the astronomy and particle physics communities
- Deep Learning and IACT: bridging the gap between Monte-Carlo simulations and LST-1 data using domain adaptation
- Observers' Data Access Portal at KOA
- Perl Metaprogrammed TikZ Spectra for the AAOmega Spectrograph
Scientific Data Analyst at the National Radio Astronomy Observatory.
- Automation of VLASS Quick Look Image Quality Assurance
Trey Roby been a programmer in the industry for years and joined Caltech/IPAC back in the Spitzer days and now works at the IRSA archive doing web development.
Currently his focus is Firefly, used by many web applications and archives at IPAC and Rubin.
This development involves building reusable web applications using Java, JavaScript, and the many modern technologies such as React and Docker.
- Firefly: Using VO Protocols to Build Dynamic UIs
I am a Senior Staff Scientist at the Space Telescope Science Institute (STScI). Since 2020, I have been leading science support for the Roman Space Telescope data pipelines and the Roman archive.
- Automated anomaly detection at scale with the cloud-based Roman Data Monitoring Tool
• Leading Member of INAF contribution HPC, Big data and Quantum Computing for the Italian National Center (EU Recovery Plan)
• Member of the Board of Directors of the COMETA Consortium (http://www.consorzio-cometa.it/)
• Member of the INAF Committee for HPC
• President of the INAF National Science Group for the Technology (RSN5 2020-2023)
• INAF Leading Member for the formal agreement INAF-CINECA for HPC resources un to 2022
• INAF PI of the formal agreement CINECA - ESA GAIA DPCT for HPC resources for the Astrometric Verification Unit for the ESA Gaia Mission
• PI of the MoU signed between INAF-Catania Astrophysical Observatory and University of Malta on: "Scientific research cooperation Educational activities in subjects of common interest; Mobility of staff and researchers; Mobility of students including doctoral candidates; Exchange of information and sharing of know-how "
• co-PI of the MoU between IDIA and INAF for the iDaVIE Virtual Reality project(https://idavie.readthedocs.io/ en/latest/#) “ICT-VR-Lab & MeerKAT Fornax Survey teams";
• PI and co_PI of many project for the Visual Analytic tools (VisIVO and Vialactea visualization tools http:// palantir7.oats.inaf.it/visivoweb/, https://www.oact.inaf.it/2019/07/16/vialactea-visual-analytics-tool-for-star- formation-studies-of-the-galactic-plane/)
• PI for the system solver code on HPC and pre-Exascale systems (ESA GAIA-AVU)
- Astrophysics and Cosmos Observation. The Italian National Centre on HPC, Big Data and Quantum Computing
Valentina Cesare is an astrophysicist and a fixed-term researcher at the Osservatorio Astrofisico di Catania and she is currently working on the porting of scientific applications related to Gaia space mission (specifically, the Gaia AVU-GSR Parallel Solver) on HPC, HTC, and GPU environments, to the development of workflows for scientific visualization, and to other activities in the context of Centro Nazionale di Ricerca in High Performance Computing, Big Data and Quantum Computing–PNRR in Future Computing. She got the Ph.D. in Physics and Astrophysics at the University of Torino, with a thesis about modified gravity.
- The Gaia AVU–GSR Parallel Solver: CUDA solutions for linear systems solving and covariances calculation toward Exascale infrastructures
- High performance visualization for Astronomy & Cosmology: the VisIVO’s pathway toward Exascale systems
Victoria Catlett is a software engineer at the Green Bank Observatory.
- Dysh: Spectral-Line Calibration of SDFITS Files
I am a radioastronomer and data steward, currently working at INAF - Istituto di Radioastronomia (IRA) in Bologna (Italy), member of the Italian Centre for Astronomical Archives (IA2), the IVOA Radio Interest Group and the Italian Square Kilometre Array Regional Centre (ITA-SRC).
I work for development and maintenance of the Italian radio telescopes data archive, and in promoting Open Science practices, e.g. by supporting IVOA initiatives and developments of data centres for future facilities, like the Square Kilometre Array (SKA).
I am also active in the fields of radio polarimetry/magnetism (mainly in Active Galactive Nuclei) and cosmology with radio telescopes.
- The INAF radio data archive: from data publication to interoperability of time-domain data
- Prototyping access from visualisation tools to SKA science images and cubes stored in a rucio DataLake through IVOA discovery and access services
After completing my PhD in Astronomy in Padua (Italy) in 2022, I started in dec 2022 a 2-yr post-doctoral contract at the Observatory of Paris. My work deals with the search and characterization of giant planets and brown dwarfs around stars observed by imaging using state-of-the-art reduction algorithms, in order to compare their observed and theoretical properties.
I have also worked on a survey with the SPHERE instrument called BEAST, which has identified substellar companions around young B-type stars. My current efforts are part of the general quest to understand the mechanisms of substellar companion formation.
- MADYS: determining and comparing stellar and substellar parameters across isochronal models
- Gemini Data Reductions - Saving Legacy Software With The Cloud
- Deep learning in automatic detection of radio 21 cm neutral hydrogen absorption
NED task lead
- Best practices in data presentation
Yash Gondhalekar recently graduated with a bachelor's degree in Computer Science from the Birla Institute of Technology and Science, Pilani.
- Improving detection of small planets in upcoming transit surveys
- Application of a Simulation-Based Inference method to a galaxy cluster cosmology analysis
- Efficient Image Visualization and Analysis with CARTA - Cube Analysis and Rendering Tool for Astronomy
- Anomaly Detection in ASKAP’s Monitoring Data through Collaborative Intelligence