massive high-z Balmer break galaxies are less common than previously reported
Guillaume Desprez (Author), Nicholas S. Martis (Author), Yoshihisa Asada (Author), Marcin Sawicki (Author), Chris J. Willott (Author), Adam Muzzin (Author), Roberto Abraham (Author), Maruša Bradač (Author), Gabriel B. Brammer (Author), Vicente Estrada-Carpenter (Author), Kartheik G. Iyer (Author), Victoria Strait (Author), Gregor Rihtaršič (Author)

Abstract

No abstract data available

Keywords

galaxies evolution;high-redshift galaxies;dark ages;reionization;

Data

Language: English
Year of publishing:
Typology: 1.01 - Original Scientific Article
Organization: UL FMF - Faculty of Mathematics and Physics
UDC: 524.8
COBISS: 194804483 Link will open in a new window
ISSN: 1365-2966
Views: 15
Downloads: 2
Average score: 0 (0 votes)
Metadata: JSON JSON-RDF JSON-LD TURTLE N-TRIPLES XML RDFA MICRODATA DC-XML DC-RDF RDF

Other data

Secondary language: English
Type (COBISS): Article
Pages: str. 2935-2952
Volume: ǂVol. ǂ530
Issue: ǂissue ǂ3
Chronology: May 2024
DOI: 10.1093/mnras/stae1084
ID: 23636651
Recommended works:
, massive high-z Balmer break galaxies are less common than previously reported
, no subtitle data available
, building the first galaxies-chapter 1
, XVI. Discovering a bluer z ~ 4–7 universe through UV slopes
, ǂthe ǂages of stellar populations in MACS1149-JD1