Paris workshop on Bayesian Deep Learning for Cosmology and Time Domain Astrophysics
Buffon Amphitheater
APC laboratory, Université Paris Cité
Machine learning attracts a lot of interest in the fields of cosmology and time-domain astronomy and may potentially lead to major breakthroughs. Its adoption by the scientific community has been increasing dramatically in the past few years. Current progress in the machine learning community can simultaneously bring a lot to ours and must be monitored closely.
Among developments of interest for the astronomy community, probabilistic machine learning models, especially Bayesian neural networks, bring an estimation of uncertainty and combine deep neural networks architecture with Bayesian inference.
Cosmologists also rely a lot on forward modelling and often face intractable likelihoods. Modern techniques like simulation-based inference and differentiable programming can be very valuable for model selection and model parameters inference.
Time series analyses have relied for some time on the use of recurrent neural networks, more recently on transformers. Some other analyses have been using convolutional neural networks, or graph neural networks. The workshop will explore if new architectures like graph transformers could be relevant in some fields, and how such networks can be made probabilistic.
This workshop will give the participants the opportunity to learn more about these emerging methods and how to use and exploit them in their research. The program includes invited lectures and tutorials from major computer science experts and invited and contributed talk, and poster sessions aimed at sharing experience between physicists on the practical applications of machine learning. It is intended for researchers and students that are familiar with machine learning, use this type of algorithms for their own work, and want to learn about the advanced techniques related to Bayesian deep learning.
This workshop is part of the LSSTC Enabling Science effort and will give opportunity to younger scientists to apply for a grant covering lodging and part of the conference fees. Application can be made through a dedicated page on the menu on the left 👈.
Workshop program
- Mon 20 – "School day" with 4 x 90 min interactive sessions
- Tue 21–Fri 24 June – Workshop with keynote speakers, contributed talks, tutorials, round tables and lightning talks.
Workshop topics
- Cosmology and time-domain astro applications of Bayesian deep networks
- Methods for quantifying models uncertainty
- Anomaly and outlier detection
- Simulation-based and likelihood-free inference
- Probabilistic ML frameworks
- Use of Bayesian deep learning outside of academia
- Ethics of large-scale machine learning
Important dates
- April 19th 2022 – pre-registration, registration and call for contributions start
- May 18th 2022 – contributions & grant application deadline for pre-registered young scientists
- June 6th 2022 – end of registration
Confirmed speakers
- Anja Butter, ITP Heidelberg, Germany
- Colin Caroll, Google, USA
- Jean-Gabriel Ganascia, LIP6, Paris, France
- Stephen Green, MPI, Potsdam, Germany
- Alan Heavens, Imperial College, London, UK
- Tomasz Kacprzak, ETH Zurich / PSI, Switzerland
- Junpeng Lao, Google, Switzerland
- Ashley Villar, Penn State University, USA
- Ben Wandelt, IAP, Paris, France
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08:30
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09:00
Break: Discussions around coffee & tea - Registration¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
09:00
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09:10
Organisers: Welcome address - BDL School¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésidents de session: Alexandre Boucaud (APC / IN2P3), Eric Aubourg (APC) -
09:10
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10:40
Tutorials: BDL school¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésident de session: Alan Heavens ( Imperial College London)-
09:10
Orateur: Alan Heavens ( Imperial College London)
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09:10
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10:40
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11:10
Break: Coffee break¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
11:10
→
12:40
Tutorials: BDL School¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésident de session: Junpeng Lao (Google Zurich)-
11:10
Orateur: Junpeng Lao (Google Zurich)
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11:10
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12:40
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14:10
Break: Lunch (on your own)¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris - 14:10 → 15:40
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15:40
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16:10
Break: Coffee break¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
16:10
→
17:40
Tutorials: BDL school¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésident de session: Benjamin Wandelt (IAP)- 16:10
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08:30
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09:00
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08:30
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09:00
Discussions around coffee & tea - Registration 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
09:00
→
09:15
Organisers: Welcome address – Workshop¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésidents de session: Alexandre Boucaud (APC / IN2P3), Cécile Roucelle (APC), Eric Aubourg (APC) -
09:15
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10:35
Uncertainties¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
09:15
Orateur: Anja Butter (LAL Orsay)
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10:15
Orateur: Benjamin Remy (CEA Paris-Saclay)
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09:15
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10:35
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10:45
Lightning talks: lighting talks session 1¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPhD or postdocs present quickly their work
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10:35
Orateur: Vincenzo Mariani (Observatoire de la Côte d'Azur, GeoAzur)
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10:37
Orateur: Federico Stachurski (University of Glasgow)
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10:39
Orateur: Kristen Lackeos (Max Planck Institute for Radio Astronomy)
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10:41
Deep Learning Techniques for Time Series Analysis in the context of Gravitational Waves Detection¶ 2mOrateur: Vlad-Andrei Basceanu (Institute of Space Science, Romania)
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10:35
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10:45
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11:15
Coffee break 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
11:15
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11:25
Lightning talks: lighting talks session 2¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPhD or postdocs present quickly their work
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11:15
There's no difference: Convolutional Neural Networks for transient detection without template subtraction¶ 1mOrateur: Tatiana Acero Cuellar (University of Delaware)
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11:16
We report the automatic detection of 11 transients (7 possible supernovae and 4 active galactic nuclei candidates) within the Zwicky Transient Facility fourth data release (ZTF DR4), all of them observed in 2018 and absent from public catalogs. Among these, three were not part of the ZTF alert stream. Our transient mining strategy employs 41 physically motivated features extracted from both real light curves and four simulated light curve models (SN Ia, SN II, TDE, SLSN-I). These features are input to a k-D tree algorithm, from which we calculate the 15 nearest neighbors. After pre-processing and selection cuts, our dataset contained approximately a million objects among which we visually inspected the 105 closest neighbors from seven of our brightest, most well-sampled simulations, comprising 89 unique ZTF DR4 sources. Our result illustrates the potential of coherently incorporating domain knowledge and automatic learning algorithms, which is one of the guiding principles directing the SNAD team. It also demonstrates that the ZTF DR is a suitable testing ground for data mining algorithms aiming to prepare for the next generation of astronomical data.
Orateur: Konstantin Malanchev (University of Illinois at Urbana-Champaign)
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11:15
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11:25
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12:05
Time Domain Astrophysics¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
11:25
Orateur: Konstantin Malanchev (University of Illinois at Urbana-Champaign)
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11:45
Orateur: Helen Qu (University of Pennsylvania)
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11:25
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12:05
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13:45
Lunch on your own : see booklet infos for advice & suggestions 1h 40m
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13:45
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14:15
Discussions around coffee & tea + poster discussions 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
14:15
→
15:55
Time Domain Astrophysics¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
14:15
Orateur: Prof. Victoria Ashley Villar (Penn State university)
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15:15
Orateur: Paula Sanchez Saez (European Southern Observatory (ESO))
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15:35
Orateur: Emille Ishida (Universit ́e Clermont Auvergne, CNRS/IN2P3, LPC)
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14:15
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15:55
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16:25
Coffee break 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
16:25
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17:55
Round table: Inference & uncertainties¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésident de session: Francois Lanusse ({CNRS}UMR7158)-
16:25
Chair : François Lanusse - AIM/CEA/CNRS/Paris-Saclay University/Paris Cite University
Panel :
Yvonne Becherini - Université de Paris, APC, diiP
Emille Ishida - CNRS/LPC-Clermont
Colin Carroll - Google
Benjamin Wandelt - Institut d'Astrophysique de Paris
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16:25
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08:30
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09:00
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08:30
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09:00
Discussions around coffee & tea + poster discussions 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
09:00
→
10:40
ML Methodology: Simulation based Inference, tools and methods¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris- 09:00
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10:00
Fast Inference of Star Formation Histories of Galaxies with Spectra and Simulation-Based Inference (SBI)¶ 20mOrateur: Gourav Khullar (Dept of Astronomy and Astrophysics, Kavli Institute for Cosmological Physics (KICP), University of Chicago)
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10:20
Orateur: Matthew Docherty (UCL)
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10:40
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11:10
Coffee break 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
11:10
→
11:20
Lightning talks: lighting talks session 3¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPhD or postdocs present quickly their work
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11:10
The aim of this work is to provide a data-driven approach to estimate a background model for the Gamma-Ray Burst Monitor (GBM) of Fermi satellite. We employ a Neural Network (NN) to estimate each detector background signal given the information of the satellite: position, velocity, direction of the detectors, etc.
The estimated background can be employed into a triggering algorithm to discover significant long/weak events that are not previously detected by other approaches.
We show the potential of the model by estimating the background on GBM data for Gamma-Ray Bursts (GRBs) present in GBM cataloge, the long GRB 190320 and ultra-long GRB 091024.
The proposed approach is straightforwardly generalizable to estimate the background model of other satellites.Orateur: Dr Riccardo Crupi (Università di Udine) -
11:12
Orateur: Claire Theobald (LORIA)
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11:14
Improvement of the statistical model of a photoz bayesian estimator hybridizing a SED template fitting and a gaussian process¶ 2mOrateur: Joseph Chevalier (IJCLab)
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11:16
Orateur: Ivan Martin Vilchez (Institute of Space Science (ICE, CSIC and IEEC))
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11:18
When merging, two black holes spiral each other before coalescing into a bigger compact object, distorting the fabric of space-time and emitting gravitational waves. These can be detected and analyzed. Most of the analysis techniques rely on computationally-expensive Bayesian inference software. Recently, machine-learning-based techniques have emerged. These have the advantage that the computational burden is moved upstream; the model needs to be trained once in a more expensive step but is then able to produce samples very rapidly. That way, the analysis of gravitational wave data can be done faster during the observation periods. Since the detection rate increases each time the detectors are upgraded, it means that it will be more and more complicated to keep up the pace to analyze the data. Therefore, fast techniques such as machine-learning-based ones are very interesting. In addition, it is desirable to extract as much information as possible out of the observed events. This requires accounting for the lower mass binary black holes but also probing the higher-order mode content present in the signal. To analyze the entire possible spectrum of binary black hole signals and to extract as much information as possible, we present a deep-learning-based algorithm able to analyze merging compact objects down to a chirp mass of 3 solar masses. Using this method would facilitate the analysis of the increasing amount of gravitational wave events to analyze.
Orateur: Alex Kolmus
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11:10
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11:20
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12:40
ML Methodology: Simulation based Inference, tools and methods¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
11:20
Orateur: Matthew Mould (University of Birmingham)
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11:40
Orateur: Justine Zeghal (APC)
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12:00
Orateur: Alexis Sánchez (Universidad de Concepción)
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12:20
Orateur: Alice Desmons (UNSW Sydney)
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11:20
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12:40
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14:00
Lunch on your own : see booklet infos for advice & suggestions 1h 20m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
14:00
→
14:30
Discussions around coffee & tea + poster discussions 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
14:30
→
15:50
Gravitational Waves¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
14:30
Orateur: Stephen Green (Albert Einstein Institute Potsdam)
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15:30
Orateur: Natalia Korsakova (APC)
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14:30
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15:50
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17:30
Poster session: posters and a cup of tea¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
19:00
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21:00
Cocktail - La Barge 2h Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris
-
08:30
→
09:00
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08:30
→
09:00
Discussions around coffee & tea + poster discussions 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
09:00
→
10:40
Cosmology¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
09:00
In large scale structure cosmology, the information about the cosmological parameters governing the evolution of the universe is contained in the complex and rich structure of dark matter density field.
To date, this information was probed using simple human-designed statistics, such as the 2-pt functions, which are not guaranteed or expected to capture the full information content of the LSS maps.
Recently, multiple AI-based methods have been proposed to work with this highly complex data: both for parameter inference and to aid the generation of simulations.
In this talk I will review the progress of practical appliacations of AI to the LSS inference and modelling and highlight with the focus on areas in which AI can be a "game-changer".
I will discuss the recent applications of AI to weak lensing analysis, probe combination, mass map emulators and the creation multi-field simulations.
I will present upcoming simulation sets available to the community that can be used to further advance these techniques.Orateur: Dr Tomasz Kacprzak (ETH Zurich) -
10:00
Orateur: Gautham Narayan (University of Illinois at Urbana-Champaign)
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10:20
Orateur: Denise Lanzieri (Cosmostat, CEA Paris-Saclay)
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09:00
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10:40
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11:10
Coffee break 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
11:10
→
12:30
Cosmology¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
11:10
Unraveling the role of cosmic velocity field in dark matter halo mass function using deep learning¶ 20mOrateurs: Erfan Abbasgholinezhad (Sharif Uniersity of Technology), Saba Etezad Razavi (Sharif University of Technology)
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11:30
Orateur: Farida Farsian (Bologna University)
- 11:50
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12:10
Interpreting non-Gaussian posterior distributions of cosmological parameters with normalizing flows¶ 20mOrateur: Cyrille Doux (Laboratoire de Physique Subatomique et de Cosmologie)
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11:10
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12:30
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14:00
Lunch on your own : see booklet infos for advice & suggestions 1h 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
14:00
→
14:30
Discussions around coffee & tea + poster discussions 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
14:30
→
15:50
Ethics of large scale machine learning¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
14:30
Orateur: Prof. Jean-Gabriel Ganascia (Sorbonne Université)
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15:30
Orateur: Arya Farahi (University of Texas at Austin)
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14:30
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15:50
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16:20
Coffee break 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
16:20
→
17:20
Cosmology: remote talks¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris-
16:20
Orateur: Shoubaneh Hemmati (shemmati@caltech.edu)
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16:40
Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment¶ 20mOrateur: Yesukhei Jagvaral
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17:00
COSMOPOWER: Deep Learning - accelerated Bayesian inference from next-generation cosmological surveys¶ 20m
Next-generation Large-Scale Structure (LSS) and Cosmic Microwave Background (CMB) surveys will provide us with unprecedented levels of precision in the final constraints on our cosmological model. However, the computational challenges posed by these enormous datasets dangerously hinder their analysis within a Bayesian framework for rigorous uncertainty propagation – a condition necessary to ensure correspondingly high levels of accuracy in the final constraints.
In my talk I will present COSMOPOWER, an open-source Python framework for Deep Learning accelerated Bayesian inference from next-generation CMB and LSS surveys. COSMOPOWER provides orders-of-magnitude acceleration to the inference pipeline by training Deep Learning emulators of matter and CMB power spectra. I will show how these emulators meet the accuracy requirements for application to both currently available cosmological data, such as from the Kilo-Degree Survey (KiDS), as well as to simulated, next-generation data from e.g. a Euclid-like survey. The emulators always recover the fiducial cosmological constraints, while providing a speed-up factor up to Ο(10^4) to the complete inference pipeline. Bayesian parameter contours can thus be recovered in just a few seconds on a common laptop, as opposed to the many hours, days or months of runtime on computer clusters required by standard methods. I will conclude with an outlook on extensions of this software that are currently being developed to extend COSMOPOWER into a fully differentiable library for cosmology.
Orateur: Alessio Spurio Mancini (University College London)
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16:20
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17:20
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17:30
break 10m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris -
17:30
→
19:00
Round table: ML in the next decades¶ Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 ParisPrésident de session: Eric Aubourg (APC)-
17:30
Jean-Gabriel Ganascia - Sorbonne Université
Laurent Daudet - LightOn
Anja Butter - IPT Heidelberg
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17:30
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08:30
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09:00
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08:30
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09:00
Discussions around coffee & tea 30m Amphitheater 3B (Halle aux farines - Université Paris Cité)
Amphitheater 3B
Halle aux farines - Université Paris Cité
10, 16 rue Françoise Dolto 75013 Paris 9, 15 esplanade Pierre Vidal-Naquet 75013 Paris -
09:00
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10:30
ML Tools: Effective scan and while_loop in TF and JAX¶ Amphitheater 3B (Halle aux farines - Université Paris Cité)
Amphitheater 3B
Halle aux farines - Université Paris Cité
10, 16 rue Françoise Dolto 75013 Paris 9, 15 esplanade Pierre Vidal-Naquet 75013 ParisPrésident de session: Junpeng Lao (Google Zurich) -
10:30
→
11:00
Coffee break 30m Amphitheater 3B (Halle aux farines - Université Paris Cité)
Amphitheater 3B
Halle aux farines - Université Paris Cité
10, 16 rue Françoise Dolto 75013 Paris 9, 15 esplanade Pierre Vidal-Naquet 75013 Paris - 11:00 → 12:00
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12:00
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12:30
Getting lunch to go : see booklet infos for advice & suggestions 30m
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12:30
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14:00
Breakout session over lunch¶ 1h 30m Buffon Amphitheater
Buffon Amphitheater
APC laboratory, Université Paris Cité
Amphitheater : 15 rue Hélène Brion 75013 Paris APC : 10 Rue Alice Domon et Léonie Duquet, 75013 Paris
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08:30
→
09:00