activity
20152023
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 348 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.CO2023

A Strong Blend in the Morning: Studying the Circumgalactic Medium Before Cosmic Noon with Strong, Blended Lyman- Forest Systems

Sean Morrison, Debopam Som, Matthew M. Pieri +2

We study of the properties of a new class of circumgalactic medium absorbers identified in the Lyman- forest: "Strong, Blended Lyman-" (or SBLA) absorption systems. We study…

astro-ph.SR2023★ 1 cited

Cataclysmic Variables from Sloan Digital Sky Survey V -- the search for period bouncers continues

K. Inight, Boris T. Gänsicke, A. Schwope +25

SDSS-V is carrying out a dedicated survey for white dwarfs, single and in binaries, and we report the analysis of the spectroscopy of cataclysmic variables (CVs) and CV candidates…

astro-ph.GA2023★ 11 cited

The miniJPAS survey quasar selection III: Classification with artificial neural networks and hybridisation

G. Martínez-Solaeche, Carolina Queiroz, R. M. González Delgado +28

This paper is part of large effort within the J-PAS collaboration that aims to classify point-like sources in miniJPAS, which were observed in 60 optical bands over 1 deg$^2…

astro-ph.GA2023★ 12 cited

The miniJPAS survey quasar selection II: Machine learning classification with photometric measurements and uncertainties

Natália V. N. Rodrigues, L. Raul Abramo, Carolina Queiroz +23

Astrophysical surveys rely heavily on the classification of sources as stars, galaxies or quasars from multi-band photometry. Surveys in narrow-band filters allow for greater discr…

astro-ph.GA2023★ 13 cited

The SDSS-V Black Hole Mapper Reverberation Mapping Project: Unusual Broad-Line Variability in a Luminous Quasar

Logan B. Fries, Jonathan R. Trump, Megan C. Davis +30

We present a high-cadence multi-epoch analysis of dramatic variability of three broad emission lines (MgII, H, and H) in the spectra of the luminous quasar ((5100Å) = $…

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…

astro-ph.CO2022★ 13 cited

The cross-correlation of galaxies in absorption with the Lyman forest

Ignasi Pérez-Ràfols, Matthew M. Pieri, Michael Blomqvist +3

We present the first clustering measurement of Strong Blended Lyman (SBLA) absorption systems by measuring their cross-correlation with the Lyman forest. SBLAs are a new po…

astro-ph.GA2022

The miniJPAS survey quasar selection I: Mock catalogues for classification

Carolina Queiroz, L. Raul Abramo, Natália V. N. Rodrigues +27

In this series of papers, we employ several machine learning (ML) methods to classify the point-like sources from the miniJPAS catalogue, and identify quasar candidates. Since no r…

astro-ph.CO2022

Forecasts for WEAVE-QSO: 3D clustering and connectivity of critical points with Lyman- tomography

Katarina Kraljic, Clotilde Laigle, Christophe Pichon +12

The upcoming WEAVE-QSO survey will target a high density of quasars over a large area, enabling the reconstruction of the 3D density field through Lyman- tomography over unprece…

astro-ph.CO2020★ 7 cited

Probing Large-scale UV Background Inhomogeneity Associated with Quasars using Metal Absorption

Sean Morrison, Matthew M. Pieri, Debopam Som +1

We study large-scale UV background inhomogeneity in three-dimensions associated with the observed quasar populations at high redshift. We do this by measuring metal absorption thro…

astro-ph.CO2019★ 7 cited

Probing Inhomogeneity in the Helium Ionizing UV Background

Sean Morrison, Matthew M. Pieri, David Syphers +1

We present an analysis combining the simultaneous measurement of intergalactic absorption by hydrogen (H I), helium (He II) and oxygen (O VI) in UV and optical quasar spectra. The…

astro-ph.GA2019★ 13 cited

Spectroscopic QUasar Extractor and redshift (z) EstimatorSQUEzE I: Methodology

Ignasi Pérez-Ràfols, Matthew M. Pieri, Michael Blomqvist +2

We present SQUEzE, a software package to classify quasar spectra and estimate their redshifts. SQUEzE is a random forest classifier operating on the parameters of candidate emissio…

astro-ph.GA2017★ 23 cited

Early metal enrichment of gas-rich galaxies at z~5

Suraj Poudel, Varsha P. Kulkarni, Sean Morrison +4

We present abundance measurements of elements O, C, Si and Fe for three gas-rich galaxies at z~5 using observations from the Very Large Telescope (VLT) and the Keck telescope in or…

astro-ph.GA2016★ 17 cited

Element Abundances in a Gas-rich Galaxy at z = 5: Clues to the Early Chemical Enrichment of Galaxies

Sean Morrison, Varsha P. Kulkarni, Debopam Som +3

Element abundances in high-redshift quasar absorbers offer excellent probes of the chemical enrichment of distant galaxies, and can constrain models for population III and early po…

astro-ph.GA2015★ 20 cited

Keck and VLT Observations of Super-damped Lyman-alpha Absorbers at z=2=2.5: Constraints on Chemical Compositions and Physical Conditions

Varsha P. Kulkarni, Debopam Som, Sean Morrison +3

We report Keck/ESI and VLT/UVES observations of three super-damped Lyman-alpha quasar absorbers with H I column densities log N(HI) >= 21.7 at redshifts z=2-2.5. All three absorber…