papers

Publications (87)

astro-ph1996

The Las Campanas Redshift Survey

Stephen A. Shectman, Stephen D. Landy, Augustus Oemler +4

The Las Campanas Redshift Survey (LCRS) consists of 26418 redshifts of galaxies selected from a CCD-based catalog obtained in the band. The survey covers over 700 square degree…

astro-ph2007

Exploring the Variable Sky with the Sloan Digital Sky Survey

Branimir Sesar, Zeljko Ivezic, Robert H. Lupton +29

We quantify the variability of faint unresolved optical sources using a catalog based on multiple SDSS imaging observations. The catalog covers SDSS Stripe 82, and contains 58 mill…

cs.CL2020

Dynamic Context-guided Capsule Network for Multimodal Machine Translation

Huan Lin, Fandong Meng, Jinsong Su +5

Multimodal machine translation (MMT), which mainly focuses on enhancing text-only translation with visual features, has attracted considerable attention from both computer vision a…

astro-ph.GA2017

Models of the strongly lensed quasar DES J0408-5354

Adriano Agnello, Huan Lin, L. Buckley-Geer +82

We present gravitational lens models of the multiply imaged quasar DES J0408-5354, recently discovered in the Dark Energy Survey (DES) footprint, with the aim of interpreting its r…

astro-ph2007

A Survey of z~6 Quasars in the SDSS Deep Stripe: I. a Flux-Limited Sample at z_{AB}<21

Linhua Jiang, Xiaohui Fan, James Annis +9

We present the discovery of five quasars at z~6 selected from 260 deg^2 of the Sloan Digital Sky Survey (SDSS) southern survey, a deep imaging survey obtained by repeatedly scannin…

astro-ph.IM2012

The Dark Energy Survey Data Processing and Calibration System

Joseph J. Mohr, Robert Armstrong, Emmanuel Bertin +15

The Dark Energy Survey (DES) is a 5000 deg2 grizY survey reaching characteristic photometric depths of 24th magnitude (10 sigma) and enabling accurate photometry and morphology of…

astro-ph2008

Estimating the Redshift Distribution of Faint Galaxy Samples

Marcos Lima, Carlos E. Cunha, Hiroaki Oyaizu +3

We present an empirical method for estimating the underlying redshift distribution N(z) of galaxy photometric samples from photometric observables. The method does not rely on phot…

cs.DC2026

EPD-Serve: A Flexible Multimodal EPD Disaggregation Inference Serving System On Ascend

Fan Bai, Pai Peng, Zhengzhi Tang +8

With the widespread adoption of large multimodal models, efficient inference across text, image, audio, and video modalities has become critical. However, existing multimodal infer…

cs.CL2025

Qwen3 Embedding: Advancing Text Embedding and Reranking Through Foundation Models

Yanzhao Zhang, Mingxin Li, Dingkun Long +9

In this work, we introduce the Qwen3 Embedding series, a significant advancement over its predecessor, the GTE-Qwen series, in text embedding and reranking capabilities, built upon…

cs.CL2024

Qwen2 Technical Report

An Yang, Baosong Yang, Binyuan Hui +59

This report introduces the Qwen2 series, the latest addition to our large language models and large multimodal models. We release a comprehensive suite of foundational and instruct…

astro-ph2007

Photometric Redshift Error Estimators

Hiroaki Oyaizu, Marcos Lima, Carlos E. Cunha +2

Photometric redshift (photo-z) estimates are playing an increasingly important role in extragalactic astronomy and cosmology. Crucial to many photo-z applications is the accurate q…

cs.CL2023

Bridging the Domain Gaps in Context Representations for k-Nearest Neighbor Neural Machine Translation

Zhiwei Cao, Baosong Yang, Huan Lin +6

-Nearest neighbor machine translation (NN-MT) has attracted increasing attention due to its ability to non-parametrically adapt to new translation domains. By using an upstre…

astro-ph.IM2016

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…

astro-ph.GA2015

Discovery of two gravitationally lensed quasars in the Dark Energy Survey

Adriano Agnello, Tommaso Treu, Fernanda Ostrovski +77

We present spectroscopic confirmation of two new lensed quasars via data obtained at the 6.5m Magellan/Baade Telescope. The lens candidates have been selected from the Dark Energy…

astro-ph2007

The Mass Of The Coma Cluster From Weak Lensing In The Sloan Digital Sky Survey

Jeffrey M. Kubo, Albert Stebbins, James Annis +4

We present a weak lensing analysis of the Coma Cluster using the Sloan Digital Sky Survey (SDSS) Data Release Five. Complete imaging of a ~ 200 square degree region is used to meas…

cs.LG2026

Zero-Shot Scalable Resilience in UAV Swarms: A Decentralized Imitation Learning Framework with Physics-Informed Graph Interactions

Huan Lin, Lianghui Ding

Large-scale Unmanned Aerial Vehicle (UAV) failures can split an unmanned aerial vehicle swarm network into disconnected sub-networks, making decentralized recovery both urgent and…

astro-ph.CO2020

Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing

DES Collaboration, Tim Abbott, Michel Aguena +129

We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected from the Dark Energy Survey (DES) Year 1 dataset. Our analysis uses the same shear…

cs.CL2026

Qwen-Scope: Turning Sparse Features into Development Tools for Large Language Models

Boyi Deng, Xu Wang, Yaoning Wang +15

Large language models have achieved remarkable capabilities across diverse tasks, yet their internal decision-making processes remain largely opaque, limiting our ability to inspec…

stat.AP2017

Estimating global species richness using symbolic data meta-analysis

Huan Lin, M. J. Caley, Scott A. Sisson

Global species richness is a key biodiversity metric. Despite recent efforts to estimate global species richness, the resulting estimates have been highly uncertain and often logic…

astro-ph.CO2017

Core or cusps: The central dark matter profile of a redshift one strong lensing cluster with a bright central image

Thomas E. Collett, Elizabeth Buckley-Geer, Huan Lin +58

We report on SPT-CLJ2011-5228, a giant system of arcs created by a cluster at . The arc system is notable for the presence of a bright central image. The source is a Lyman…

astro-ph.CO2012

The Sloan Bright Arcs Survey: Ten Strong Gravitational Lensing Clusters and Evidence of Overconcentration

Matthew P. Wiesner, Huan Lin, Sahar S. Allam +6

We describe ten strong lensing galaxy clusters of redshift 0.26-0.56 that were found in the Sloan Digital Sky Survey. We present measurements of richness, mass and velocity dispers…

astro-ph2008

Discovery of A Very Bright, Strongly-Lensed z=2 Galaxy in the SDSS DR5

Huan Lin, Elizabeth Buckley-Geer, Sahar S. Allam +8

We report on the discovery of a very bright z = 2.00 star-forming galaxy that is strongly lensed by a foreground z=0.422 luminous red galaxy (LRG). This system was found in a syste…

astro-ph.CO2014

Spectroscopic failures in photometric redshift calibration: cosmological biases and survey requirements

Carlos E. Cunha, Dragan Huterer, Huan Lin +2

We use N-body-spectro-photometric simulations to investigate the impact of incompleteness and incorrect redshifts in spectroscopic surveys to photometric redshift training and cali…

astro-ph2005

The Dependence of Galaxy Colors on Luminosity and Environment at z~0.4

H. K. C. Yee, B. C. Hsieh, Huan Lin +1

We analyse the B-R_c colors of galaxies as functions of luminosity and local galaxy density using a large photometric redshift catalog based on the Red-Sequence Cluster Survey. We…

cs.CL2025

Enhancing LLM Language Adaption through Cross-lingual In-Context Pre-training

Linjuan Wu, Haoran Wei, Huan Lin +4

Large language models (LLMs) exhibit remarkable multilingual capabilities despite English-dominated pre-training, attributed to cross-lingual mechanisms during pre-training. Existi…

eess.IV2022

WSSS4LUAD: Grand Challenge on Weakly-supervised Tissue Semantic Segmentation for Lung Adenocarcinoma

Chu Han, Xipeng Pan, Lixu Yan +40

Lung cancer is the leading cause of cancer death worldwide, and adenocarcinoma (LUAD) is the most common subtype. Exploiting the potential value of the histopathology images can pr…

astro-ph2006

The 8 o'clock Arc: A Serendipitous Discovery of a Strongly Lensed Lyman Break Galaxy in the SDSS DR4 Imaging Data

Sahar S. Allam, Douglas L. Tucker, Huan Lin +4

We report on the serendipitous discovery of the brightest Lyman Break Galaxy (LBG) currently known, a galaxy at z=2.73 that is being strongly lensed by the z=0.38 Luminous Red Gala…

astro-ph1996

The Power Spectrum of Galaxy Clustering in the Las Campanas Redshift Survey

Huan Lin, Robert P. Kirshner, Stephen A. Shectman +4

The Las Campanas Redshift Survey (LCRS) contains 23697 galaxies, with an average redshift , distributed over six $1.5\arcdeg$ by $80\arcdeg$ slices in the North and South…

astro-ph.CO2013

The SOAR Gravitational Arc Survey - I: Survey overview and photometric catalogs

Cristina Furlanetto, Basilio X. Santiago, Martin Makler +10

We present the first results of the SOAR (Southern Astrophysical Research) Gravitational Arc Survey (SOGRAS). The survey imaged 47 clusters in two redshift intervals centered at $z…

astro-ph1998

Density-Dependent Luminosity Functions for Galaxies in the Las Campanas Redshift Survey

Benjamin C. Bromley, William H. Press, Huan Lin +1

Galaxies in the Las Campanas Redshift Survey are classified according to their spectra, and the resulting spectral types are analyzed to determine if local environment affects thei…

astro-ph.CO2011

The SDSS Coadd: 275 deg^2 of Deep SDSS Imaging on Stripe 82

James Annis, Marcelle Soares-Santos, Michael A. Strauss +17

We present details of the construction and characterization of the coaddition of the Sloan Digital Sky Survey Stripe 82 \ugriz\ imaging data. This survey consists of 275 deg of…

astro-ph.CO2024

TDCOSMO. XVI. Measurement of the Hubble Constant from the Lensed Quasar WGD20384008

Kenneth C. Wong, Frédéric Dux, Anowar J. Shajib +17

Time-delay cosmography is a powerful technique to constrain cosmological parameters, particularly the Hubble constant (). The TDCOSMO collaboration is performing an ongoing…

astro-ph2008

The Dark Energy Survey Data Management System

Joseph J. Mohr, Wayne Barkhouse, Cristina Beldica +17

The Dark Energy Survey collaboration will study cosmic acceleration with a 5000 deg2 griZY survey in the southern sky over 525 nights from 2011-2016. The DES data management (DESDM…

astro-ph.IM2010

Measuring the flatness of focal plane for very large mosaic CCD camera

Jiangang Hao, Juan Estrada, Herman Cease +10

Large mosaic multiCCD camera is the key instrument for modern digital sky survey. DECam is an extremely red sensitive 520 Megapixel camera designed for the incoming Dark Energy Sur…

astro-ph.IM2009

The Dark Energy Survey Data Management System: The Processing Framework

Michelle Gower, Joseph J. Mohr, Darren Adams +16

The Dark Energy Survey Data Management (DESDM) system will process and archive the data from the Dark Energy Survey (DES) over the five year period of operation. This paper focuses…

astro-ph2004

A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey III: Discovery of Five Additional Quasars

Xiaohui Fan, Joseph F. Hennawi, Gordon T. Richards +11

We present the discovery of five new quasars at z>5.7, selected from the multicolor imaging data of the Sloan Digital Sky Survey (SDSS). Three of them, at redshifts 5.93, 6.07, and…

astro-ph2005

Constraining Dark Energy with the Dark Energy Survey: Theoretical Challenges

James Annis, Sarah Bridle, Francisco J. Castander +14

The Dark Energy Survey (DES) will use a new imaging camera on the Blanco 4-m telescope at CTIO to image 5000 square degrees of sky in the South Galactic Cap in four optical bands,…

astro-ph.CO2010

The Sloan Bright Arcs Survey : Discovery of Seven New Strongly Lensed Galaxies from z=0.66-2.94

Jeffrey M. Kubo, Sahar S. Allam, Emily Drabek +11

We report the discovery of seven new, very bright gravitational lens systems from our ongoing gravitational lens search, the Sloan Bright Arcs Survey (SBAS). Two of the systems are…

astro-ph.CO2011

The SDSS Coadd: A Galaxy Photometric Redshift Catalog

Ribamar R. R. Reis, Marcelle Soares-Santos, James Annis +7

We present and describe a catalog of galaxy photometric redshifts (photo-z's) for the Sloan Digital Sky Survey (SDSS) Coadd Data. We use the Artificial Neural Network (ANN) techniq…

astro-ph.CO2018

Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82

Maria E. S. Pereira, Marcelle Soares-Santos, Martin Makler +9

We present the first weak lensing calibration of , a new galaxy cluster mass proxy corresponding to the total stellar mass of red and blue members, in two cluster sampl…

astro-ph.CO2011

The SDSS Coadd: Cosmic Shear Measurement

Huan Lin, Scott Dodelson, Hee-Jong Seo +7

Stripe 82 in the Sloan Digital Sky Survey was observed multiple times, allowing deeper images to be constructed by coadding the data. Here we analyze the ellipticities of backgroun…

astro-ph.CO2011

Intrinsic Alignment of Cluster Galaxies: the Redshift Evolution

Jiangang Hao, Jeffrey M. Kubo, Robert Feldmann +4

We present measurements of two types of cluster galaxy alignments based on a volume limited and highly pure ( 90%) sample of clusters from the GMBCG catalog derived from SDSS…

astro-ph2008

Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure

Manda Banerji, Filipe B. Abdalla, Ofer Lahav +1

We conduct a detailed analysis of the photometric redshift requirements for the proposed Dark Energy Survey (DES) using two sets of mock galaxy simulations and an artificial neural…

astro-ph2010

Estimating the Redshift Distribution of Photometric Galaxy Samples II. Applications and Tests of a New Method

Carlos E. Cunha, Marcos Lima, Hiroaki Oyaizu +2

In Lima et al. 2008 we presented a new method for estimating the redshift distribution, N(z), of a photometric galaxy sample, using photometric observables and weighted sampling fr…

cs.CL2023

From Statistical Methods to Deep Learning, Automatic Keyphrase Prediction: A Survey

Binbin Xie, Jia Song, Liangying Shao +6

Keyphrase prediction aims to generate phrases (keyphrases) that highly summarizes a given document. Recently, researchers have conducted in-depth studies on this task from various…

astro-ph2006

A New Survey for Giant Arcs

Joseph F. Hennawi, Michael D. Gladders, Masamune Oguri +11

We report on the first results of an imaging survey to detect strong gravitational lensing targeting the richest clusters selected from the photometric data of the Sloan Digital Sk…

astro-ph.GA2016

VDES J2325-5229 a z=2.7 gravitationally lensed quasar discovered using morphology independent supervised machine learning

Fernanda Ostrovski, Richard G. McMahon, Andrew J. Connolly +56

We present the discovery and preliminary characterization of a gravitationally lensed quasar with a source redshift and image separation of lensed by a foregrou…

astro-ph2005

Dark Energy Studies: Challenges to Computational Cosmology

James Annis, Francisco J. Castander, August E. Evrard +12

The ability to test the nature of dark mass-energy components in the universe through large-scale structure studies hinges on accurate predictions of sky survey expectations within…

astro-ph.HE2022

SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814

Douglas Tucker, Matthew Wiesner, Sahar Allam +140

On 2019 August 14 at 21:10:39 UTC, the LIGO/Virgo Collaboration (LVC) detected a possible neutron star-black hole merger (NSBH), the first ever identified. An extensive search for…

astro-ph2001

Very Red and Extremely Red Galaxies in the Fields of z ~ 1.5 Radio-Loud Quasars

Patrick B. Hall, Marcin Sawicki, Paul Martini +7

We previously identified an excess of mostly red galaxies around 31 RLQs at z=1-2. These fields have an ERO (extremely red object, R-K>6) density 2.7 times higher than the field. A…

astro-ph2007

A Galaxy Photometric Redshift Catalog for the Sloan Digital Sky Survey Data Release 6

Hiroaki Oyaizu, Marcos Lima, Carlos E. Cunha +3

We present and describe a catalog of galaxy photometric redshifts (photo-z's) for the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6). We use the Artificial Neural Network (AN…

astro-ph1998

Spectral Classification and Luminosity Function of Galaxies in the Las Campanas Redshift Survey

Benjamin C. Bromley, William H. Press, Huan Lin +1

We construct a spectral classification scheme for the galaxies of the Las Campanas Redshift Survey (LCRS) based on a principal component analysis of the measured galaxy spectra. We…

astro-ph2007

SDSS Standard Star Catalog for Stripe 82: the Dawn of Industrial 1% Optical Photometry

Zeljko Ivezic, J. Allyn Smith, Gajus Miknaitis +2

We describe a standard star catalog constructed using multiple SDSS photometric observations (at least four per band, with a median of ten) in the system. The catalog inclu…

cs.CL2023

WR-ONE2SET: Towards Well-Calibrated Keyphrase Generation

Binbin Xie, Xiangpeng Wei, Baosong Yang +5

Keyphrase generation aims to automatically generate short phrases summarizing an input document. The recently emerged ONE2SET paradigm (Ye et al., 2021) generates keyphrases as a s…

astro-ph2008

The Sloan Bright Arcs Survey : Six Strongly Lensed Galaxies at z=0.4-1.4

Jeffrey M. Kubo, Sahar S. Allam, James Annis +5

We present new results of our program to systematically search for strongly lensed galaxies in the Sloan Digital Sky Survey (SDSS) imaging data. In this study six strong lens syste…

astro-ph2008

Cross-correlation Weak Lensing of SDSS Galaxy Clusters I: Measurements

Erin S. Sheldon, David E. Johnston, Ryan Scranton +12

This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in Sloan Digital Sky Survey. The photometrically selected cluster sample, known as…

astro-ph.IM2016

The DESI Experiment Part II: Instrument Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…

eess.IV2021

Multi-Layer Pseudo-Supervision for Histopathology Tissue Semantic Segmentation using Patch-level Classification Labels

Chu Han, Jiatai Lin, Jinhai Mai +15

Tissue-level semantic segmentation is a vital step in computational pathology. Fully-supervised models have already achieved outstanding performance with dense pixel-level annotati…

astro-ph.CO2009

The Sloan Nearby Cluster Weak Lensing Survey

Jeffrey M. Kubo, James Annis, Frances Mei Hardin +10

We describe and present initial results of a weak lensing survey of nearby () galaxy clusters in the Sloan Digital Sky Survey (SDSS). In this first study, galaxy…

astro-ph.GA2018

DES Science Portal: Computing Photometric Redshifts

Julia Gschwend, Aurelio Carnero Rosell, Ricardo Ogando +68

A significant challenge facing photometric surveys for cosmological purposes is the need to produce reliable redshift estimates. The estimation of photometric redshifts (photo-zs)…

astro-ph.CO2010

Mid-Infrared Spectroscopy of Two Lensed Star-forming Galaxies

Ross Fadely, Sahar S. Allam, Andrew J. Baker +7

We present low-resolution, rest-frame ~ 5 - 12 micron Spitzer/IRS spectra of two lensed z ~ 2 UV-bright star-forming galaxies, SDSS J120602.09+514229.5 and SDSS J090122.37+181432.3…

astro-ph1999

Star Formation in Las Campanas Compact Groups

Sahar S. Allam, Douglas L. Tucker, Huan Lin +1

Compact groups (CGs) of galaxies offer an exceptional laboratory for the study of dense galaxian environments --- where interactions, tidally induced activity, and mergers are expe…

eess.IV2022

CKD-TransBTS: Clinical Knowledge-Driven Hybrid Transformer with Modality-Correlated Cross-Attention for Brain Tumor Segmentation

Jianwei Lin, Jiatai Lin, Cheng Lu +12

Brain tumor segmentation (BTS) in magnetic resonance image (MRI) is crucial for brain tumor diagnosis, cancer management and research purposes. With the great success of the ten-ye…

astro-ph.CO2025

TDCOSMO 2025: Cosmological constraints from strong lensing time delays

TDCOSMO Collaboration, Simon Birrer, Elizabeth J. Buckley-Geer +30

We present cosmological constraints from 8 strongly lensed quasars (hereafter, the TDCOSMO-2025 sample). Building on previous work, our analysis incorporated new deflector stellar…

astro-ph1996

The Luminosity Function of Galaxies in the Las Campanas Redshift Survey

Huan Lin, Robert P. Kirshner, Stephen A. Shectman +4

We present the -band luminosity function for a sample of 18678 galaxies, with average redshift , from the Las Campanas Redshift Survey. The luminosity function may be f…

cs.CL2024

mGTE: Generalized Long-Context Text Representation and Reranking Models for Multilingual Text Retrieval

Xin Zhang, Yanzhao Zhang, Dingkun Long +10

We present systematic efforts in building long-context multilingual text representation model (TRM) and reranker from scratch for text retrieval. We first introduce a text encoder…

astro-ph2000

Spectroscopic Gravitational Lens Candidates in the CNOC2 Field Galaxy Redshift Survey

Patrick B. Hall, H. K. C. Yee, Huan Lin +7

We present five candidate gravitational lenses discovered spectroscopically in the Canadian Network for Observational Cosmology Field Galaxy Redshift Survey (CNOC2), along with one…

cs.NI2025

Multi-Level Damage-Aware Graph Learning for Resilient UAV Swarm Networks

Huan Lin, Chenguang Zhu, Lianghui Ding +2

Unmanned aerial vehicle (UAV) swarm networks leverage resilient algorithms to restore connectivity from communication network split issues. However, existing graph learning-based a…

cs.CL2025

Qwen3 Technical Report

An Yang, Anfeng Li, Baosong Yang +57

In this work, we present Qwen3, the latest version of the Qwen model family. Qwen3 comprises a series of large language models (LLMs) designed to advance performance, efficiency, a…

astro-ph2000

The Distribution of [OII] Equivalent Widths of LCRS Galaxies

Michael Blanton, Huan Lin

We present a simple functional form for the joint distribution of R-band luminosity and [OII] 3727 emission-line equivalent widths of galaxies, and show that this form is a good fi…

astro-ph.IM2026

The Vera C. Rubin Observatory Data Preview 1

Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325

We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…

astro-ph1998

A blind test of photometric redshift prediction

David W. Hogg, Judith G. Cohen, Roger Blandford +16

Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts obtained in the Hubble Deep Field with the Keck Telescope are presented. The best…

stat.CO2020

New models for symbolic data analysis

Boris Beranger, Huan Lin, Scott A. Sisson

Symbolic data analysis (SDA) is an emerging area of statistics concerned with understanding and modelling data that takes distributional form (i.e. symbols), such as random lists,…

cs.CL2025

Qwen2.5 Technical Report

Qwen, :, An Yang +41

In this report, we introduce Qwen2.5, a comprehensive series of large language models (LLMs) designed to meet diverse needs. Compared to previous iterations, Qwen 2.5 has been sign…

astro-ph2000

Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey

Patrick B. Hall, H. K. C. Yee, Huan Lin +7

We present a sample of 47 confirmed and 14 candidate Active Galactic Nuclei (AGN) discovered in the Canadian Network for Observational Cosmology field galaxy redshift survey (CNOC2…

astro-ph.CO2015

Mass Calibration of Galaxy Clusters at Redshift 0.1-1.0 using Weak Lensing in the Sloan Digital Sky Survey Stripe 82 Co-add

Matthew P. Wiesner, Huan Lin, Marcelle Soares-Santos

We present galaxy cluster mass-richness relations found in the Sloan Digital Sky Survey Stripe 82 co-add using clusters found using a Voronoi tessellation cluster finder. These rel…

astro-ph.CO2009

The Sloan Bright Arcs Survey: Four Strongly Lensed Galaxies with Redshift >2

H. Thomas Diehl, Sahar S. Allam, James Annis +7

We report the discovery of four very bright, strongly-lensed galaxies found via systematic searches for arcs in Sloan Digital Sky Survey Data Release 5 and 6. These were followed-u…

cs.CL2021

Towards User-Driven Neural Machine Translation

Huan Lin, Liang Yao, Baosong Yang +5

A good translation should not only translate the original content semantically, but also incarnate personal traits of the original text. For a real-world neural machine translation…

cs.NI2025

Bio-inspired Integrated Networking and Control for Large-Scale Swarm: A Hierarchical Co-design

Huan Lin, Dakai Liu, Lianghui Ding +2

Unmanned aerial vehicle (UAV) swarms encounter the challenge of high overhead due to both network management and formation control requirements. In this paper, we propose a Bio-ins…

astro-ph.CO2024

A Cohesive Deep Drilling Field Strategy for LSST Cosmology

Philippe Gris, Humna Awan, Matthew R. Becker +4

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will image billions of astronomical objects in the wide-fast-deep primary survey and in a set of minisurveys in…

astro-ph2006

Photometric Calibration of the DES

Douglas L. Tucker, James T. Annis, Huan Lin +15

The Dark Energy Survey (DES) is a 5000 sq deg griz imaging survey to be conducted using a proposed 3 sq deg (2.2deg-diameter) wide-field mosaic camera on the CTIO Blanco 4m telesco…

astro-ph1997

The Influence of Environment on the Star Formation Rates of Galaxies

Yasuhiro Hashimoto, Augustus Oemler, Huan Lin +1

We have used a sample of 15749 galaxies taken from the Las Campanas Redshift Survey to investigate the effects of environment on the rate of star formation (SFR) in galaxies. The s…

cs.NI2025

Multi-hop Differential Topology based Algorithms for Resilient Network of UAV Swarm

Huan Lin, Lianghui Ding

Unmanned aerial vehicle (UAV) swarm networks face severe challenges of communication network split (CNS) issues caused by massive damage in hostile environments. In this paper, we…

astro-ph1999

The Galaxy-Weighted Small-Scale Velocity Dispersion of the Las Campanas Redshift Survey

Jonathan E. Baker, Marc Davis, Huan Lin

The pair-weighted relative velocity dispersion of galaxies provides a measure of the thermal energy of fluctuations of the observed galaxy distribution, but the measure is difficul…

cs.CL2023

PolyLM: An Open Source Polyglot Large Language Model

Xiangpeng Wei, Haoran Wei, Huan Lin +15

Large language models (LLMs) demonstrate remarkable ability to comprehend, reason, and generate following nature language instructions. However, the development of LLMs has been pr…

astro-ph.CO2009

A Survey of z~6 Quasars in the SDSS Deep Stripe. II. Discovery of Six Quasars at z_{AB}>21

Linhua Jiang, Xiaohui Fan, Fuyan Bian +10

We present the discovery of six new quasars at z~6 selected from the Sloan Digital Sky Survey (SDSS) southern survey, a deep imaging survey obtained by repeatedly scanning a stripe…

astro-ph.CO2011

The SDSS Coadd: Cross-Correlation Weak Lensing and Tomography of Galaxy Clusters

Melanie Simet, Jeffrey M. Kubo, Scott Dodelson +7

The shapes of distant galaxies are sheared by intervening galaxy clusters. We examine this effect in Stripe 82, a 275 square degree region observed multiple times in the Sloan Digi…