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Maria Dainotti

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

Japan

Research Interests

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Articles (40)

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Collaborators (17)

Bing Zhang

The University of Hong Kong

HONG KONG

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Agnieszka Pollo

National Centre for Nuclear Research

POLAND

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Nozomu Tominaga

Professor

National Astronomical Observatory of Japan

JAPAN

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Gaetano Lambiase

Full Professor

Università degli Studi di Napoli Federico II

ITALY

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Apratim Dey

Assistant Professor

Washington University in St. Louis

UNITED STATES

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Tomoya Takiwaki

准教授/Associate Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Vahe' Petrosian

Professor

Stanford University

UNITED STATES

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Simone Dichiara

Assistant Research Professor

Pennsylvania State University

UNITED STATES

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Dieter Hartmann

Prof

Clemson University

UNITED STATES

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Gopal Bhatta

Professor

University of Zielona Góra

POLAND

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Salvatore Capozziello

Docenti di ruolo di Ia fascia

Università degli Studi di Napoli Federico II

ITALY

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Alessandro Melchiorri

Professore Ordinario

Sapienza University of Rome

ITALY

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Boris Betancourt Kamenetskaia

Senior Researcher

Institute for Basic Science

SOUTH KOREA

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Kazunori Kohri

Professor

University of Tokyo

JAPAN

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Kazunari Iwasaki

Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Shulei Cao

Southern Methodist University

UNITED STATES

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Bharat Ratra

University of Kansas

UNITED STATES

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Maria Dainotti

Research Interests

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Articles (40)

Creation of viscous dark energy by the Hubble flow: Comparison with SNe Ia Master sample binned data

Gamma-ray bursts as an independent high-redshift probe of dark energy

The effective running Hubble constant in SNe Ia as a marker for the dark energy nature

Synchrotron Self-Compton Reverse Shock in Energy-injection and Radiative Scenarios

GRB 250704B/EP250704a a short gamma-ray burst powered by a magnetar

Cosmological Evolution of Gamma-Ray Bursts

Parameterizations of the Hubble Constant from the Binned Type Ia Supernova Master Sample: Logarithmic versus Power-law Forms

Interpretation of the binned SNe Ia master sample data via a scalar quintessence component: Phantom transition?

Evaluating gamma-ray burst light curve reconstruction: A diverse machine learning approach

Multi-model framework for reconstructing gamma-Ray burst light curves

Model-independent calibration of Gamma-Ray Bursts with neural networks

Probing Evolution of Long Gamma-Ray Burst Properties through Their Cosmic Formation History

The multiwavelength correlations quest for central engines of GRB plateaus: Magnetar vs black hole spin-down

Variation of microphysical parameters in reverse-shock scenario

Late-Time Radio Diagnostics of Magnetar Magnetic Burial and Reemergence in GRB Afterglows

Gamma-Ray Burst Light-curve Reconstruction: A Comparative Machine and Deep Learning Analysis

Probing Evolution of Long GRB Properties through their Cosmic Formation History Aided by Machine Learning–predicted Redshifts

Exploring jet structure and dynamics in short gamma-ray bursts: A case study on GRB 090510

Two Dynamical Scenarios for Binned Master Sample Interpretation

A New Master Supernovae Ia sample and the investigation of the Hubble tension

The Density and Ionization Profiles of Optically Dark and High-Redshift GRBs Probed by X-ray Absorption

Revisiting the concordance ΛCDM model using Gamma-Ray Bursts together with supernovae Ia and Planck data

Gamma-Ray Bursts as Distance Indicators by a Statistical Learning Approach

A new binning method to choose a standard set of Quasars

Inferring the Redshift of More than 150 GRBs with a Machine-learning Ensemble Model

Progenitors of Low-redshift Gamma-Ray Bursts

On the statistical assumption on the distance moduli of Supernovae Ia and its impact on the determination of cosmological parameters

Parameter Inference of a State-of-the-Art Physical Afterglow Model for GRB 190114C

The Scavenger Hunt for Quasar Samples to Be Used as Cosmological Tools

Afterglow Polarization from Off-axis Gamma-Ray Burst Jets

Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts

A Stochastic Approach to Reconstruct Gamma-Ray-burst Light Curves

Quasars: Standard Candles up to z = 7.5 with the Precision of Supernovae Ia

The Closure Relations in High-Energy Gamma-ray Bursts Detected by Fermi-LAT

A Bias-free Cosmological Analysis with Quasars Alleviating H 0 Tension

Off-axis Afterglow Closure Relations and Fermi-LAT Detected Gamma-Ray Bursts

Modeling Gamma-Ray Burst Afterglow Observations with an Off-axis Jet Emission

The Quest for New Correlations in the Realm of the Gamma-Ray Burst—Supernova Connection

The Closure Relations in Optical Afterglow of Gamma-Ray Bursts

Gamma-ray burst data strongly favour the three-parameter fundamental plane (Dainotti) correlation over the two-parameter one

Collaborators (17)

Bing Zhang

Agnieszka Pollo

Nozomu Tominaga

Gaetano Lambiase

Apratim Dey

Tomoya Takiwaki

Vahe' Petrosian

Simone Dichiara

Dieter Hartmann

Gopal Bhatta

Salvatore Capozziello

Alessandro Melchiorri

Boris Betancourt Kamenetskaia

Kazunori Kohri

Kazunari Iwasaki

Shulei Cao

Bharat Ratra

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