Bruno Moraes

About Bruno Moraes

Bruno Moraes, With an exceptional h-index of 22 and a recent h-index of 19 (since 2020), a distinguished researcher at Universidade Federal do Rio de Janeiro, specializes in the field of Cosmology, Particle Physics, Extragalactic Astrophysics.

His recent articles reflect a diverse array of research interests and contributions to the field:

Mapeamentos de galáxias

The 6× 2pt method: supernova velocities meet multiple tracers

Lensing without borders–I. A blind comparison of the amplitude of galaxy–galaxy lensing between independent imaging surveys

Constraining AGN feedback model with SZ profile

On the weak-lensing masses of a new sample of galaxy groups

Probing hot gas around luminous red galaxies through the Sunyaev–Zel’dovich effect

Bruno Moraes Information

University

Position

Instituto de Física

Citations(all)

1698

Citations(since 2020)

1006

Cited By

1162

hIndex(all)

22

hIndex(since 2020)

19

i10Index(all)

28

i10Index(since 2020)

24

Email

University Profile Page

Google Scholar

Bruno Moraes Skills & Research Interests

Cosmology

Particle Physics

Extragalactic Astrophysics

Top articles of Bruno Moraes

Mapeamentos de galáxias

Cadernos de Astronomia

2024/3/15

The 6× 2pt method: supernova velocities meet multiple tracers

Monthly Notices of the Royal Astronomical Society

2022/5

Constraining AGN feedback model with SZ profile

EPJ Web of Conferences

2022

Yin-Zhe Ma
Yin-Zhe Ma

H-Index: 36

Bruno Moraes
Bruno Moraes

H-Index: 18

On the weak-lensing masses of a new sample of galaxy groups

Monthly Notices of the Royal Astronomical Society

2021/7

Facundo Rodriguez
Facundo Rodriguez

H-Index: 0

Bruno Moraes
Bruno Moraes

H-Index: 18

Probing hot gas around luminous red galaxies through the Sunyaev–Zel’dovich effect

Monthly Notices of the Royal Astronomical Society

2020/1

Yin-Zhe Ma
Yin-Zhe Ma

H-Index: 36

Bruno Moraes
Bruno Moraes

H-Index: 18

See List of Professors in Bruno Moraes University(Universidade Federal do Rio de Janeiro)

Co-Authors

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