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And Ecclesiastical Cosmology
12 Strong Gravitational Lenses
The Assembly of the First Massive Black Holes Arxiv:1911.05791V1
Near Infrared Observations of Quasars with Extended Ionized Envelopes
The AIMSS Project – I. Bridging the Star Cluster–Galaxy Divide †‡§¶
The Structure & Stellar Populations of Nuclear Star Clusters in Late-Type
The Seyfert Galaxy Population
1. Introduction
Interpreting the Spitzer/IRAC Colours of 7 ≤ Z ≤ 9 Galaxies: Distinguishing Between Line Emission and Starlight Using ALMA
Viewing the 21 Cm Sky : a Slice of the Neutral Hydrogen Universe
SDSS DR7 Superclusters the Catalogues
Arxiv:1404.1378V1 [Astro-Ph.GA] 4 Apr 2014 .M C M
Linking Galaxy Formation with Cosmic Reionization
Investigation of the Orientation of Galaxies in Clusters: the Importance, Methods and Results of Research
2019 Workshop
Yale University Astronomy Department Newsletter Yale
Dwarfs After Mergers? the Case of NGC 520, NGC 772, Arp 141, NGC 3226/7, NGC 3656 and Arp 299
An Exploration of Astronomical Techniques of Visualization
Top View
Lecture Notes (Pdf)
Galactic Dust Map
New Constraints on Dust Emission and UV Attenuation of Z = 6.5–7.5 Galaxies from Millimeter Observations
Dust and Gas in Luminous Proto-Cluster Galaxies at Z = 4.05: the Case for Different Cosmic Dust Evolution in Normal and Starburst Galaxies
“Exotica” Catalog As the Centerpiece of Our Efforts to Expand the Diversity of Targets Surveyed in the Search for Extraterrestrial Intelligence (SETI)
Model Simulation of Jet Precession in Quasar PG 1302-102 S
Dusty Star Forming Galaxies at High Redshift
Space Math V
Testing the Tidal Stripping Origin of Ultra-Compact Dwarf Galaxies
Cycle 23 Abstract Catalog (Based on Phase I Submissions)
Milky Way Globular Clusters in Γ-Rays: Analyzing the Dynamical Formation of Millisecond Pulsars
Galaxies Through Space and Time Contents INTRODUCTION 4
Star Formation Rates in Nearby Markarian Galaxies
A Merger in the Dusty, Z=7.5 Galaxy A1689-Zd1?
Universe: the Light Speed Redshift Pavle Premovic
Arxiv:1511.03264V2 [Astro-Ph.GA] 4 Dec 2015 We find That the Csss Are Predominantly More Metal Rich Than Typical Galaxies at the Same Stellar Mass
Atoms to Astronomy
Arxiv:1511.03264V2 [Astro-Ph.GA] 4 Dec 2015 We find That the Csss Are Predominantly More Metal Rich Than Typical Galaxies at the Same Stellar Mass