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Á. Bongiovanni

Universite Paris Saclay
H指数:26
被引数:4,412

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GASTON-GP: Source catalogue and millimetre variability of massive protostellar objects

GASTON-GP:原恒星物体源目录及其毫米波变异性

2026-03-090
OA
Resolved ISM properties and scaling relations in the barred galaxy NGC 3627: constraints from NIKA2 observations

棒旋星系NGC 3627中分辨的ISM特性与尺度关系:NIKA2观测的约束

2026-03-011
PRE
Blind detection of galaxy clusters in the COSMOS field via the SZ effect

通过SZ效应在COSMOS视场中对星系团进行盲检测

2026-01-010
OA
N2CLS: the NIKA2 view of the distant Universe

N2CLS:NIKA2对遥远宇宙的观测

2026-01-010
OAAI
The SZ-Mass scaling relation with the NIKA2 SZ Large Program

SZ质量关系与NIKA2 SZ大型计划

2026-01-010
OA
NIKA2 maps tracing dust grain evolution in cores of TMC1

NIKA2望远镜绘制TMC1核心中尘埃颗粒演化的追踪图谱

2026-01-010
OAAI
Overview of final results from the NIKA2 Sunyaev-Zeldovich Large Program

NIKA2日yaev-Zeldovich大型计划最终结果概述

2026-01-010
OA
A panchromatic view of N2CLS GOODS-N: The evolution of the dust cosmic density since z ∼ 7

N2CLS GOODS-N区域的泛光视图:自红移z ∼ 7以来宇宙尘埃密度的演化

2025-04-180
PRE
CO-CAVITY project: Molecular gas and star formation in void galaxies
2024-12-050
PRE
CAVITY, Calar Alto Void Integral-field Treasury surveY and project extension
2024-09-130
OA
The Lockman-SpReSO project: Main properties of infrared-selected star-forming galaxies

Lockman-spreso项目: 红外选择的恒星形成星系的主要特性

2024-06-250
OA
GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652II. The mass-metallicity relationship and the effect of the environment
2024-05-300
OA
The Lockman-SpReSO project: Galactic flows in a sample of far-infrared galaxies
2024-03-290
OA
The Lockman-SpReSO project Description, target selection, observations, and catalogue preparation
2023-01-173
OA
Nonsequential neural network for simultaneous, consistent classification, and photometric redshifts of OTELO galaxies
2021-11-191
OA
The OTELO survey Revealing a population of low-luminosity active star-forming galaxies at z ∼ 0.9
2021-09-031
OA
The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution The mass-size relation up to z=2

作为形态学探针的OTELO调查。银河系演化的最后十个Gyr直到z = 2的质量大小关系

2021-03-129
OA