Man

Domenico Sapone

Associate professor

Universidad de Chile

Santiago, Chile

Líneas de Investigación


Cosmology and large scale structures. Data scientist and software developer. Bayesian Statistics. Full member of Euclid Consortium in galaxy clustering and likelihood groups. Member of Dark Energy Science Collaboration LSST.

Educación

  •  Physics, UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA. Italia, 2004
  •  Cosmology, UNIVERSITE DE GENEVE. Suiza, 2009

Experiencia Académica

  •   Lecturer Full Time

    UNIVERSITE DE GENEVE

    Sciences

    Geneve, Suiza

    2009 - 2009

  •   Postdoctoral Full Time

    Consejo Superior de Investigación Científica (CSIC)

    Madrid, España

    2009 - 2012

  •   Assistant professor Full Time

    UNIVERSIDAD DE CHILE

    FCFM

    Santiago, Chile

    2014 - A la fecha

Experiencia Profesional

  •   Junior Consultant Full Time

    GOALSYSTEM

    Madrid, España

    2012 - 2013

Formación de Capital Humano


I have had under my supervision 6 master students and 10 undergraduates students who worked with me in their thesis and in the "Introduction to research course". All of my students have been trained in data analysis for cosmological observables, building a clear vision of Bayesian Statistic and likelihood analysis.
I always encouraged my students to take parallel courses in statistical methods and lately in Machine learning process in order to create an entire group at the department of physics devoted to such aspect of science. The main idea is to develop an entire likelihood code for the galaxy clustering observable for matter power spectrum to be used to analyze the data coming from future experiments, such as Euclid and LSST, in which I am member in both consortia.
The students manifested a great enthusiasm in data analysis and sophisticated statistical methods, probably motivated by the increasing interest in both science and enterprises. In fact, my main idea is to give all the possible knowledge needed in order to help them choose their proper careers, and, not to mention, to be prepared to the new upcoming era of cosmology in which we are in need of more sophisticated, and faster, methods to analyze the future catalogs.


Difusión y Transferencia


The department of physics of the Universidad de Chile and the Conicyt itself encourage the outreach program.
I have been dedicating time to the transfer of knowledge, participating to public seminars and appearing directly to medias (radio, television, blogs...) in order to make Cosmology understandable and hence attractive to the audience. I have myself forced to give a minimum of at least four outreach seminars per year.
I will continue dedicating my time on reaching people, creating short videos and demonstrations of the physical phenomena. At the moment, we are discussing with the Social media and Data Lab group, here at the Faculty of Sciences of the University of Chile, in order to make demonstrations of the physical phenomena that drive the Universe. The main idea is to prepare ourselves to explain with classical experiment the acceleration of the universe and formation of structures.


Premios y Distinciones

  •   Adisu Fellowship

    UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA

    Italia, 2000

    Public institution that funds fellowships to bright students each year.

  •   Adisu Fellowship

    UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA

    Italia, 2003

    Public institution that funds fellowships to bright students each year.

  •   Adisu Fellowship

    UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA

    Italia, 2004

    Public institution that funds fellowships to bright students each year.

  •   Universidad de Messina

    UNIVERSITA DEGLI STUDI DI MESSINA

    Italia, 1999

    Public institution that funds fellowships to bright students each year.

  •   Fellowship assistant to laboratories

    UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA

    Italia, 2002

    Public institution that funds fellowships to bright students each year.

  •   Marc Birkigt fellowship

    UNIVERSITE DE GENEVE

    Suiza, 2007

    Private institution that funds fellowships to bright students each year.

  •   Euclid Star Prize 2019

    EUROPEAN SPACE AGENCE-NETHERLANDS

    Francia, 2019

    For creating the official pipeline of Euclid satellite for forecasting the cosmological parameters using the galaxy clustering observable.

  •   Builder status Euclid Consortium

    European Space Agency (ESA)

    Francia, 2022

    Builder Status is conferred on those Euclideans who have made key, long-term contributions, especially to Euclid infrastructure


 

Article (50)

<i>Euclid</i> preparation - XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and <i>H</i>-band images
<i>Euclid</i> preparation XXII. Selection of quiescent galaxies from mock photometry using machine learning
<i>Euclid</i> preparation XXIV. Calibration of the halo mass function in ?(<i>ν</i>)CDM cosmologies
<i>Euclid</i> preparation XXIX. Water ice in spacecraft Part I: The physics of ice formation and contamination
<i>Euclid</i> preparation XXV. The <i>Euclid</i> Morphology Challenge: Towards model-fitting photometry for billions of galaxies
<i>Euclid</i> preparation XXVI. The <i>Euclid</i> Morphology Challenge: Towards structural parameters for billions of galaxies
<i>Euclid</i> preparation XXX. Performance assessment of the NISP red grism through spectroscopic simulations for the wide and deep surveys
<i>Euclid</i>: Calibrating photometric redshifts with spectroscopic cross-correlations
<i>Euclid</i>: Forecasts from the void-lensing cross-correlation
<i>Euclid</i>: Testing the Copernican principle with next-generation surveys
Euclid: Cosmology forecasts from the void-galaxy cross-correlation function with reconstruction
Can varying the gravitational constant alleviate the tensions?
<i>Euclid</i> preparation XVIII. The NISP photometric system
<i>Euclid</i> preparation XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data release
Euclid preparation XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey
Euclid: Forecast constraints on consistency tests of the ΛCDM model
Does jackknife scale really matter for accurate large-scale structure covariances?
Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography
Is there any measurable redshift dependence on the SN Ia absolute magnitude?
Euclid preparation VIII. The Complete Calibration of the Colour-Redshift Relation survey: VLT/KMOS observations and data release
Euclid preparation: VI. Verifying the performance of cosmic shear experiments
Euclid preparation: VII. Forecast validation for Euclid cosmological probes
Euclid preparation: X. The Euclid photometric-redshift challenge
Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey
Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments
Evaporating primordial black holes as varying dark energy
Relativistic effects in the large-scale structure with effective dark energy fluids
Validating the Fisher approach for stage IV spectroscopic surveys
Euclid preparation V. Predicted yield of redshift 7 < z < 9 quasars from the wide survey
Testing extended Jordan-Brans-Dicke theories with future cosmological observations
Constraints on inflation with LSS surveys: features in the primordial power spectrum
Internal robustness of growth rate data
Null tests of the standard model using the linear model formalism
Combined constraints on deviations of dark energy from an ideal fluid from Euclid and Planck
Accuracy of the growth index in the presence of dark energy perturbations
Novel null-test for the. cold dark matter model with growth-rate data
Reconstruction of the null-test for the matter density perturbations
Comparison of piecewise-constant methods for dark energy
Curvature versus distances: Testing the FLRW cosmology
Can dark energy viscosity be detected with the Euclid survey?
Fingerprinting dark energy. III. Distinctive marks of viscosity
A parametrization of the growth index of matter perturbations in various Dark Energy models and observational prospects using a Euclid-like survey
DARK ENERGY IN PRACTICE
Fingerprinting dark energy. II. Weak lensing and galaxy clustering tests
Constraints on early dark energy from CMB lensing and weak lensing tomography
Fingerprinting dark energy
Measuring the dark side (with weak lensing)
Dark energy versus modified gravity
Crossing the phantom divide

Proyecto (2)

SOAP-COSMO: STATISTICS FOR OBSERVED ANISOTROPIES AND PROBES IN COSMOLOGY
DARK ENERGY PERTURBATIONS AND TOOLS IN COSMOLOGY

Review (1)

Cosmology and fundamental physics with the Euclid satellite
52
Domenico Sapone

Associate professor

Physics

Universidad de Chile

Santiago, Chile

1
Gonzalo Palma

Associate Professor

Physics

FCFM, UNIVERSIDAD DE CHILE

Santiago, Chile