Gergö Popping
0000-0003-1151-4659
25 papers found
Refreshing results…
Semi-analytic forecasts for JWST – III. Intrinsic production efficiency of Lyman-continuum radiation
The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral Atomic Carbon [C i]
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6
The ALMA Spectroscopic Survey in the HUDF: Constraining Cumulative CO Emission at 1 ≲ z ≲ 4 with Power Spectrum Analysis of ASPECS LP Data from 84 to 115 GHz
Semi-analytic forecasts for JWST – II. Physical properties and scaling relations for galaxies at z = 4–10
ALMACAL – VI. Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
The ALMA Spectroscopic Survey in the HUDF: the Molecular Gas Content of Galaxies and Tensions with IllustrisTNG and the Santa Cruz SAM
The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies
The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in theHubbleUltra Deep Field: CO Emission Lines and 3 mm Continuum Sources
The Molecular Gas Reservoirs of z ∼ 2 Galaxies: A Comparison of CO(1−0) and Dust-based Molecular Gas Masses
IQ-Collaboratory 1.1: The Star-forming Sequence of Simulated Central Galaxies
A Theory for the Variation of Dust Attenuation Laws in Galaxies
Semi-analytic forecasts forJWST– I. UV luminosity functions atz = 4–10
The art of modelling CO, [C i], and [C ii] in cosmological galaxy formation models
ALMACAL V: absorption-selected galaxies with evidence for excited ISMs
ALMACAL – III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H i-absorption-selected system
Hierarchical Bayesian inference of the initial mass function in composite stellar populations
Dissecting the IRX–β dust attenuation relation: exploring the physical origin of observed variations in galaxies
Missing publications? Search for publications with a matching author name.