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Candidate Ly{alpha}-emitting galaxies spectra
Questions as to what drove the bulk reionization of the universe, how that reionization proceeded, and how the hard ionizing radiation reached the intergalactic medium remain... -
Survey for z< 0.04 CLAGNs
We have conducted a systematic survey for z<0.04 active Galactic nuclei (AGNs) that may have changed spectral class over the past decade. We use SkyMapper, Pan-STARRS and the... -
Boost recall in QSO selection
The identification of bright quasi-stellar objects (QSOs) is of fundamental importance to probe the intergalactic medium and address open questions in cosmology. Several... -
z-GAL. III. Physical properties
The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM Northern Extended Millimeter Array, with the aim to measure their redshift and study their... -
z-GAL.I. Overview
Using the IRAM NOrthern Extended Millimetre Array (NOEMA), we conducted a Large Programme (z-GAL) to measure redshifts for 126 bright galaxies detected in the Herschel... -
Galaxy Clusters from SCUSS
This paper presents the identification of galaxy clusters from the photometric redshift catalog based on three imaging surveys of SCUSS, Sloan Digital Sky Survey, and unWISE. By... -
Siena Galaxy Atlas 2020 (SGA-2020)
We present the 2020 version of the Siena Galaxy Atlas (SGA-2020), a multiwavelength optical and infrared imaging atlas of 383620 nearby galaxies. The SGA-2020 uses optical grz... -
DESI z>~5 quasar survey. I. New z~4.7-6.6 QSOs
We report the first results of a high-redshift (z>~5) quasar survey using the Dark Energy Spectroscopic Instrument (DESI). As a DESI secondary target program, this survey is... -
BASS. XXXIV. ALMA obs. of Swift/BAT AGNs
We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby (z<0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray... -
BASS. XXXIII. Blazars in the 14-195keV range
We derive the most up-to-date Swift-Burst Alert Telescope (BAT) blazar luminosity function in the 14-195keV range, making use of a clean sample of 118 blazars detected in the... -
Extreme emission line galaxies in COSMOS & NEP
We present a search for extreme emission line galaxies (EELGs) at z<1 in the COSMOS and North Ecliptic Pole (NEP) fields with imaging from Subaru/Hyper Suprime-Cam (HSC) and... -
Virial factor of SDSS DR5 QSOs
Under the hypothesis of gravitational redshift induced by a central supermassive black hole, and based on line widths and shifts of redward-shifted H{beta} and FeII broad... -
Black hole mergers with Obelisk simulation
Massive black hole (BH) mergers will be key targets of future gravitational wave and electromagnetic observational facilities. In order to constrain BH evolution with the... -
Classification of Markarian galaxies
Markarian (Mrk) galaxies, revealed due to their ultraviolet excess are very famous; they play a significant role in many astrophysical problems and come in a variety of types:... -
Properties of stellar clumps in stripped tails
In this work, we aim to characterize the stellar populations of star-forming regions detached from the stellar disks of galaxies undergoing ram-pressure stripping. Using images... -
DESI Peculiar Velocity survey
We describe the target selection and characteristics of the DESI Peculiar Velocity Survey, the largest survey of peculiar velocities (PVs) using both the fundamental plane (FP)... -
The Swift/UVOT+MaNGA (SwiM) v4.1 catalog
We present the the new Swift/UVOT+MaNGA (SwiM) catalog (SwiM_v4.1). SwiM_v4.1 is designed to study star formation and dust attenuation within nearby galaxies given the unique... -
SDSS Seyfert 1.9 galaxies with Ha emission line fit
The traditional classification for a subclass of the Seyfert galaxies is visual inspection or using a quantity defined as a flux ratio between the Balmer line and forbidden... -
DESI Legacy Imaging Surveys DR8
We present photometric redshift (photo-z) estimates for the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys, currently the most sensitive optical survey... -
Star formation rates in z~0.35 cluster galaxies
Ram-pressure stripping (RPS) is the mechanism most often invoked to explain the observed differences between cluster and field galaxies. In the local Universe, its effect on the...