papers

Publications (216)

astro-ph.HE2017

Hydrogen-poor Superluminous Supernovae With Late-time H-alpha Emission: Three Events From the Intermediate Palomar Transient Factory

Lin Yan, R. Lunnan, D. Perley +20

We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H-alpha emission with line luminosities of (1-3)e+41…

cs.LG2025

Exploring Data Scaling Trends and Effects in Reinforcement Learning from Human Feedback

Wei Shen, Guanlin Liu, Zheng Wu +5

Reinforcement Learning from Human Feedback (RLHF) is crucial for aligning large language models with human preferences. While recent research has focused on algorithmic improvement…

astro-ph.GA2019

Panchromatic Study of the First Galaxies with Large ALMA Programs

Andreas Faisst, Matthieu Bethermin, Peter Capak +5

Thanks to deep optical to near-IR imaging and spectroscopy, significant progress is made in characterizing the rest-frame UV to optical properties of galaxies in the early universe…

astro-ph.HE2022

The prevalence and influence of circumstellar material around hydrogen-rich supernova progenitors

Rachel J. Bruch, Avishay Gal-Yam, Ofer Yaron +44

Narrow transient emission lines (flash-ionization features) in early supernova (SN) spectra trace the presence of circumstellar material (CSM) around the massive progenitor stars o…

astro-ph.HE2022

The Final Season Reimagined: 30 Tidal Disruption Events from the ZTF-I Survey

Erica Hammerstein, Sjoert van Velzen, Suvi Gezari +30

Tidal disruption events (TDEs) offer a unique way to study dormant black holes. While the number of observed TDEs has grown thanks to the emergence of wide-field surveys in the pas…

astro-ph.HE2022

The Zwicky Transient Facility phase I sample of hydrogen-rich superluminous supernovae without strong narrow emission lines

Tuomas Kangas, Lin Yan, Steve Schulze +19

We present a sample of 14 hydrogen-rich superluminous supernovae (SLSNe II) from the Zwicky Transient Facility (ZTF) between 2018 and 2020. We include all classified SLSNe with pea…

astro-ph.HE2018

A UV Resonance Line Echo from a Shell Around a Hydrogen-Poor Superluminous Supernova

R. Lunnan, C. Fransson, P. M. Vreeswijk +21

Hydrogen-poor superluminous supernovae (SLSN-I) are a class of rare and energetic explosions discovered in untargeted transient surveys in the past decade. The progenitor stars and…

astro-ph.HE2025

SN 2023uqf: An Interacting Supernova Coincident with a High-Energy Neutrino

Robert Stein, Anna Y. Q. Ho, Anjasha Gangopadhyay +30

Astrophysical high-energy (TeV-PeV) neutrinos were first discovered in 2013, but their origin remains largely unknown. Here we present SN 2023uqf, a supernova found in coincidence…

cs.AI2025

VAPO: Efficient and Reliable Reinforcement Learning for Advanced Reasoning Tasks

Yu Yue, Yufeng Yuan, Qiying Yu +24

We present VAPO, Value-based Augmented Proximal Policy Optimization framework for reasoning models., a novel framework tailored for reasoning models within the value-based paradigm…

astro-ph2007

Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 II: Diagnostics

Anna Sajina, Lin Yan, Lee Armus +4

We present mid-IR spectral decomposition of a sample of 48 Spitzer-selected ULIRGs spanning z~1-3 and likely L_IR~10^12-10^13Lsun. Our study aims at quantifying the star-formation…

astro-ph.HE2017

Spatially resolved analysis of Superluminous Supernovae PTF~11hrq and PTF~12dam host galaxies

Aleksandar Cikota, Annalisa De Cia, Steve Schulze +12

Superluminous supernovae (SLSNe) are the most luminous supernovae in the universe. They are found in extreme star-forming galaxies and are probably connected with the death of mass…

astro-ph2007

Discovery of Radio Jets in z~2 ULIRGs with Deep 9.7um Silicate Absorption

Anna Sajina, Lin Yan, Mark Lacy +1

Recent Spitzer observations have revealed a substantial population of z~2 ULIRGs with deep silicate absorption (τ_{9.7}>1). This paper reports a 20cm radio study of such a sample…

astro-ph.HE2026

AT2024wpp: An Extremely Luminous Fast Ultraviolet Transient Powered by Accretion onto a Black Hole

Daniel A. Perley, Anna Y. Q. Ho, Zoë McGrath +69

We present the discovery of AT 2024wpp ("Whippet"), a fast and luminous 18cow-like transient. At a redshift of z=0.0868, revealed by Keck Cosmic Web Imager spectroscopy of its fain…

cs.CL2025

Seed1.5-Thinking: Advancing Superb Reasoning Models with Reinforcement Learning

ByteDance Seed, :, Jiaze Chen +267

We introduce Seed1.5-Thinking, capable of reasoning through thinking before responding, resulting in improved performance on a wide range of benchmarks. Seed1.5-Thinking achieves 8…

astro-ph2001

Probing the evolution of galaxies using redshifted H-alpha emission

Paul P. van der Werf, Alan F. M. Moorwood, Lin Yan

In this paper we review the present status and implications of H-alpha surveys at various redshifts. With the advent of sensitive wide-format near-infrared detectors on large teles…

astro-ph.HE2016

Host-Galaxy Properties of 32 Low-Redshift Superluminous Supernovae from the Palomar Transient Factory

Daniel A. Perley, Robert Quimby, Lin Yan +9

We present ultraviolet through near-infrared photometry and spectroscopy of the host galaxies of all superluminous supernovae (SLSNe) discovered by the Palomar Transient Factory pr…

astro-ph.HE2014

A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies

Iair Arcavi, Avishay Gal-Yam, Mark Sullivan +23

We present the results of a Palomar Transient Factory (PTF) archival search for blue transients which lie in the magnitude range between "normal" core-collapse and superluminous su…

astro-ph.CO2012

Characterizing the Mid-IR Extragalactic Sky with WISE and SDSS

Lin Yan, E. Donoso, C. -W. Tsai +10

The Wide-field Infrared Survey Explorer (WISE) has completed its all-sky survey at 3.4-22 micron. We merge the WISE data with optical SDSS data and provide a phenomenological chara…

cs.DC2025

A General Framework for Augmenting Lossy Compressors with Topological Guarantees

Nathaniel Gorski, Xin Liang, Hanqi Guo +2

Topological descriptors such as contour trees are widely utilized in scientific data analysis and visualization, with applications from materials science to climate simulations. It…

astro-ph.CO2024

ZTF SN Ia DR2: Overview

Mickael Rigault, Mathew Smith, Ariel Goobar +53

We present the first homogeneous release of several thousand Type Ia supernovae (SNe Ia), all having spectroscopic classification, and spectroscopic redshifts for half the sample.…

astro-ph.CO2012

Origin of the 12um Emission Across Galaxy Populations from WISE and SDSS Surveys

E. Donoso, Lin Yan, C. Tsai +6

We cross-matched Wide-field Infrared Survey Explorer (WISE) sources brighter than 1 mJy at 12um with the Sloan Digital Sky Survey (SDSS) galaxy spectroscopic catalog to produce a s…

astro-ph.HE2022

Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine

Samaporn Tinyanont, Stan E. Woosley, Kirsty Taggart +34

We present observations of a peculiar hydrogen- and helium-poor stripped-envelope (SE) supernova (SN) 2020wnt, primarily in the optical and near-infrared (near-IR). Its peak absolu…

astro-ph.CO2013

Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts

Gregory F. Snyder, Christopher C. Hayward, Anna Sajina +5

We analyze the link between active galactic nuclei (AGN) and mid-infrared flux using dust radiative transfer calculations of starbursts realized in hydrodynamical simulations. Focu…

cs.CV2025

Seed1.5-VL Technical Report

Dong Guo, Faming Wu, Feida Zhu +194

We present Seed1.5-VL, a vision-language foundation model designed to advance general-purpose multimodal understanding and reasoning. Seed1.5-VL is composed with a 532M-parameter v…

astro-ph.GA2021

AGN on the move: A search for off-nuclear AGN from recoiling SMBHs and ongoing galaxy mergers with the Zwicky Transient Facility

Charlotte Ward, Suvi Gezari, Sara Frederick +16

A supermassive black hole (SMBH) ejected from the potential well of its host galaxy via gravitational wave recoil carries important information about the mass ratio and spin alignm…

astro-ph.CO2011

Probing Very Bright End of Galaxy Luminosity Function at z >~ 7 Using Hubble Space Telescope Pure Parallel Observations

Haojing Yan, Lin Yan, Michel A. Zamojski +8

We report the first results from the Hubble Infrared Pure Parallel Imaging Extragalactic Survey, which utilizes the pure parallel orbits of the Hubble Space Telescope to do deep im…

astro-ph.GA2013

The LAMOST Survey of Background Quasars in the Vicinity of the Andromeda and Triangulum Galaxies -- II. Results from the Commissioning Observations and the Pilot Surveys

Zhi-Ying Huo, Xiao-Wei Liu, Mao-Sheng Xiang +68

We present new quasars discovered in the vicinity of the Andromeda and Triangulum galaxies with the LAMOST during the 2010 and 2011 observational seasons. Quasar candidates are sel…

astro-ph.HE2022

Radio observations of the tidal disruption event AT2020opy: a luminous non-relativistic outflow encountering a dense circumnuclear medium

Adelle J. Goodwin, James Miller-Jones, Sjoert van Velzen +9

Tidal disruption events (TDEs) occur when a star passes too close to a supermassive black hole and is destroyed by tidal gravitational forces. Radio observations of TDEs trace sync…

astro-ph.CO2010

Mid-infrared spectroscopy of Spitzer-selected ultra-luminous starbursts at z~2

Nicolas Fiolet, Alain Omont, Guilaine Lagache +13

We want to study the mid-infrared properties and the starburst and AGN contributions, of 24um sources at z~2, through analysis of mid-infrared spectra combined with millimeter, rad…

astro-ph.HE2020

The Zwicky Transient Facility Census of the Local Universe I: Systematic search for Calcium rich gap transients reveal three related spectroscopic sub-classes

Kishalay De, Mansi M. Kasliwal, Anastasios Tzanidakis +47

(Abridged) Using the Zwicky Transient Facility alert stream, we are conducting a large campaign to spectroscopically classify all transients occurring in galaxies in the Census of…

astro-ph.GA2015

Detection of Broad H Emission Lines in the Late-time Spectra of a Hydrogen-poor Superluminous Supernova

Lin Yan, R. Quimby, E. Ofek +14

iPTF13ehe is a hydrogen-poor superluminous supernova (SLSN) at z=0.3434, with a slow-evolving light curve and spectral features similar to SN2007bi. It rises within (83-148)days (r…

astro-ph.CO2011

The Nature of Double-Peaked [O III] Active Galactic Nuclei

Hai Fu, Lin Yan, Adam D. Myers +4

Active galactic nuclei (AGNs) with double-peaked [O III] lines are suspected to be sub-kpc or kpc-scale binary AGNs. However, pure gas kinematics can produce the same double-peaked…

astro-ph.CO2012

Mid-Infrared Selection of AGN with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-Selected AGN in COSMOS

Daniel Stern, Roberto J. Assef, Dominic J. Benford +15

The Wide-field Infrared Survey Explorer (WISE) is an extremely capable and efficient black hole finder. We present a simple mid-infrared color criterion, W1-W2 \geq 0.8 (i.e., [3.4…

cs.LG2026

Dual-Scale Temporal Fusion Reveals Structured Predictability in Subseasonal-to-Seasonal Temperature Prediction

Elnaz Bashir, Jiali Wang, Lin Yan

Subseasonal-to-seasonal (S2S) temperature forecasts, spanning several weeks to a few months, are critically needed in agriculture practice, energy planning, and extreme-weather ind…

astro-ph.HE2019

Supernova 2017eaw: molecule and dust formation from infrared observations

Samaporn Tinyanont, Mansi M Kasliwal, Kelsie Krafton +15

We present infrared (IR) photometry and spectroscopy of the Type II-P SN 2017eaw and its progenitor in the nearby galaxy NGC 6946. Progenitor observations in the Ks band in 4 epoch…

astro-ph.CO2009

Massive Galaxies in COSMOS: Evolution of Black hole versus bulge mass but not versus total stellar mass over the last 9 Gyrs?

Knud Jahnke, Angela Bongiorno, Marcella Brusa +22

We constrain the ratio of black hole (BH) mass to total stellar mass of type-1 AGN in the COSMOS survey at 1<z<2. For 10 AGN at mean redshift z~1.4 with both HST/ACS and HST/NICMOS…

cs.SE2022

spotFuzzer: Static Instrument and Fuzzing Windows COTs

Yeming Gu, Hui Shu, Rongkuan Ma +2

The security research on Windows has received little attention in the academic circle. Most of the new methods are usually designed for Linux system, and are difficult to transplan…

astro-ph.GA2014

Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies

Suzy F. Jones, Andrew W. Blain, Daniel Stern +9

We present SCUBA-2 850um submillimetre (submm) observations of the fields of 10 dusty, luminous galaxies at z ~ 1.7 - 4.6, detected at 12um and/or 22um by the WISE all-sky survey,…

astro-ph2002

Star Formation in Emission-Line Galaxies Between Redshifts of 0.8 and 1.6

Erin K. S. Hicks, Matthew A. Malkan, Harry I. Teplitz +2

Optical spectra of 14 emission-line galaxies representative of the 1999 NICMOS parallel grism Ha survey of McCarthy et al. are presented. Of the 14, 9 have emission lines confirmin…

astro-ph.GA2020

A Mid-infrared Flare in the Active Galaxy MCG-02-04-026: Dust Echo of a Nuclear Transient Event

Luming Sun, Ning Jiang, Tinggui Wang +8

We report the discovery of a mid-infrared (MIR) flare using WISE data in the center of the nearby Seyfert 1.9 galaxy MCG-02-04-026. The MIR flare began in the first half of 2014, p…

astro-ph.HE2019

ZTF18aalrxas: A Type IIb Supernova from a very extended low-mass progenitor

C. Fremling, H. Ko, A. Dugas +31

We investigate ZTF18aalrxas, a double-peaked Type IIb core-collapse supernova (SN) discovered during science validation of the Zwicky Transient Facility (ZTF). ZTF18aalrxas was dis…

astro-ph1998

Deep H-band Galaxy Counts and Half-light Radii from HST/NICMOS Parallel Observations

Lin Yan, Patrick McCarthy, Lisa Storrie-Lombardi +1

We present deep galaxy counts and half-light radii from F160W () images obtained with NICMOS on HST. Nearly 9 arcmin have been imaged with camera 3, with dept…

cs.LG2025

Virtual Width Networks

Seed, Baisheng Li, Banggu Wu +115

We introduce Virtual Width Networks (VWN), a framework that delivers the benefits of wider representations without incurring the quadratic cost of increasing the hidden size. VWN d…

astro-ph.HE2021

Reverberation in tidal disruption events: dust echoes, coronal emission lines, multi-wavelength cross-correlations, and QPOs

Sjoert van Velzen, Dheeraj R. Pasham, Stefanie Komossa +2

Stellar tidal disruption events (TDEs) are typically discovered by transient emission due to accretion or shocks of the stellar debris. Yet this luminous flare can be reprocessed b…

astro-ph.CO2011

Extended Schmidt Law: Role Of Existing Stars In Current Star Formation

Yong Shi, George Helou, Lin Yan +4

We propose an "extended Schmidt law" with explicit dependence of the star formation efficiency (SFE=SFR/Mgas) on the stellar mass surface density. This relation has a power-law ind…

astro-ph.CO2011

A Kiloparsec-Scale Binary Active Galactic Nucleus Confirmed by the Expanded Very Large Array

Hai Fu, Zhi-Yu Zhang, Roberto J. Assef +6

We report the confirmation of a kpc-scale binary active galactic nucleus (AGN) with high-resolution radio images from the Expanded Very Large Array (EVLA). SDSS J150243.1+111557 is…

astro-ph.IM2016

The IPAC Image Subtraction and Discovery Pipeline for the intermediate Palomar Transient Factory

Frank Masci, Russ Laher, Umaa Rebbapragada +17

We describe the near real-time transient-source discovery engine for the intermediate Palomar Transient Factory (iPTF), currently in operations at the Infrared Processing and Analy…

astro-ph.CO2014

The Angular Clustering of WISE-Selected AGN: Different Haloes for Obscured and Unobscured AGN

E. Donoso, Lin Yan, D. Stern +1

We calculate the angular correlation function for a sample of 170,000 AGN extracted from the Wide-field Infrared Survey Explorer (WISE) catalog, selected to have red mid-IR colors…

astro-ph.SR2012

Spitzer Photometry of WISE-Selected Brown Dwarf and Hyper-Luminous Infrared Galaxy Candidates

Roger L. Griffith, J. Davy Kirkpatrick, Peter R. M. Eisenhardt +23

We present Spitzer 3.6 and 4.5 m photometry and positions for a sample of 1510 brown dwarf candidates identified by the WISE all-sky survey. Of these, 166 have been spectroscop…

astro-ph.CO2009

Global Star Formation Rate Density over 0.7<z<1.9

Hyunjin Shim, James Colbert, Harry Teplitz +4

We determine the global star formation rate density at 0.7<z<1.9 using emission-line selected galaxies identified in Hubble Space Telescope Near Infrared Camera and Multi-Object Sp…

cs.AI2025

Process Supervision-Guided Policy Optimization for Code Generation

Ning Dai, Zheng Wu, Renjie Zheng +7

Reinforcement learning (RL) with unit test feedback has enhanced large language models' (LLMs) code generation, but relies on sparse rewards provided only after complete code evalu…

astro-ph.GA2020

Mid-InfraRed Outburst in Nearby Galaxies (MIRONG) I: Sample Selection and Characterization

Ning Jiang, Tinggui Wang, Liming Dou +9

The optical time-domain astronomy has grown rapidly in the past decade but the dynamic infrared sky is rarely explored. Aiming to construct a sample of mid-infrared outburst in nea…

astro-ph.GA2026

Halfway to the Peak: Kinematic Signatures of Stable Rotating Disks in Luminous Infrared Galaxies at z=0.5-0.6

Miriam Eleazer, Alexandra Pope, Anna Sajina +13

We present a kinematic study of six infrared-luminous galaxies observed with the Mid-InfraRed Instrument Medium-Resolution Spectrometer (MIRI/MRS) onboard JWST. These galaxies lie…

astro-ph.CO2023

Uncovering a population of gravitational lens galaxies with magnified standard candle SN Zwicky

Ariel Goobar, Joel Johansson, Steve Schulze +35

Detecting gravitationally lensed supernovae is among the biggest challenges in astronomy. It involves a combination of two very rare phenomena: catching the transient signal of a s…

astro-ph.HE2019

Rapid "Turn-on" of type 1 AGN in a quiescent early type galaxy SDSS1115+0544

Lin Yan, Tinggui Wang, Jiang Ning +8

We present a detailed study of a transient in the center of SDSS1115+0544 based on the extensive UV, optical, mid-IR light curves (LC) and spectra over 1200 days. The host galaxy i…

astro-ph.HE2023

A Superluminous Supernova Lightened by Collisions with Pulsational Pair-instability Shells

Weili Lin, Xiaofeng Wang, Lin Yan +23

Superluminous supernovae are among the most energetic stellar explosions in the Universe, but their energy sources remain an open question. Here we present long-term observations o…

astro-ph.HE2025

SN 2021aaev: a Hydrogen-Rich Superluminous Supernova with Early Flash and Long-Lived Circumstellar Interaction in an Unusual Host Environment

Yang Hu, Ragnhild Lunnan, Priscila J. Pessi +25

We present photometric and spectroscopic observations of SN\,2021aaev, a hydrogen-rich, superluminous supernova with persistent (at least days) narrow Balmer lines (SLSN-…

astro-ph.GA2020

The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr

D. Schaerer, M. Ginolfi, M. Bethermin +34

The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \si…

astro-ph.CO2011

A massive proto-cluster of galaxies at a redshift of z {\approx} 5.3

Peter L. Capak, Dominik Riechers, Nick Z. Scoville +14

Massive clusters of galaxies have been found as early as 3.9 Billion years (z=1.62) after the Big Bang containing stars that formed at even earlier epochs. Cosmological simulations…

astro-ph.HE2023

Tidal Disruption Event Demographics with the Zwicky Transient Facility: Volumetric Rates, Luminosity Function, and Implications for the Local Black Hole Mass Function

Yuhan Yao, Vikram Ravi, Suvi Gezari +26

We conduct a systematic tidal disruption event (TDE) demographics analysis using the largest sample of optically selected TDEs. A flux-limited, spectroscopically complete sample of…

astro-ph.HE2024

A cosmic formation site of silicon and sulphur revealed by a new type of supernova explosion

Steve Schulze, Avishay Gal-Yam, Luc Dessart +47

The cores of stars are the cosmic furnaces where light elements are fused into heavier nuclei. The fusion of hydrogen to helium initially powers all stars. The ashes of the fusion…

astro-ph.GA2015

Binary Active Galactic Nuclei in Stripe 82: Constraints on Synchronized Black Hole Accretion in Major Mergers

Hai Fu, J. M. Wrobel, A. D. Myers +2

Representing simultaneous black hole accretion during a merger, binary active galactic nuclei (AGNs) could provide valuable observational constraints to models of galaxy mergers an…

astro-ph.GA2024

Halfway to the Peak: The JWST MIRI 5.6 micron number counts and source population

Leonid Sajkov, Anna Sajina, Alexandra Pope +9

We present an analysis of eight JWST Mid-Infrared Instrument (MIRI) 5.6 micron images with depths of ~0.1 uJy. We detect 2854 sources within our combined area of 18.4 squar…

astro-ph.EP2021

Initial Characterization of Active Transitioning Centaur, P/2019 LD2 (ATLAS), using Hubble, Spitzer, ZTF, Keck, APO and GROWTH Visible & Infrared Imaging and Spectroscopy

Bryce T. Bolin, Yanga R. Fernandez, Carey M. Lisse +43

We present visible and mid-infrared imagery and photometry of temporary Jovian co-orbital comet P/2019 LD taken with HST/WFC3, Spitzer/IRAC, the GROWTH telescope network, visib…

quant-ph2023

Multi-parameter quantum metrology with stabilized multi-mode squeezed state

Yue Li, Xu Cheng, Lingna Wang +11

Squeezing a quantum state along a specific direction has long been recognized as a crucial technique for enhancing the precision of quantum metrology by reducing parameter uncertai…

astro-ph1998

Studying the Evolution of Field Galaxies Using NICMOS/HST Parallel Imaging and Grism Data

Lin Yan, Patrick J. McCarthy, Lisa J. Storrie-Lombardi +1

We present results from our analysis of F160W NICMOS Parallel images. These data cover ~9~sq. arcminutes and reach 3 depths of H 24.3 25.5 in a diameter ap…

astro-ph.GA2025

The ALPINE-CRISTAL-JWST Survey: Revealing Less Massive Black Holes in High-Redshift Galaxies

Wenke Ren, John D. Silverman, Andreas L. Faisst +25

We present a systematic search for broad-line active galactic nuclei (AGNs) in the ALPINE-CRISTAL-JWST sample of 18 star-forming galaxies () at redshift…

astro-ph.HE2024

WTP19aalnxx: Discovery of a bright mid-infrared transient in the emerging class of low luminosity supernovae revealed by delayed circumstellar interaction

Charlotte Myers, Kishalay De, Lin Yan +11

While core-collapse supernovae (SNe) often show early and consistent signs of circumstellar (CSM) interaction, some exhibit delayed signatures due to interaction with distant mater…

astro-ph.CO2012

Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies

Jingwen Wu, Chao-Wei Tsai, Jack Sayers +20

We have used the Caltech Submillimeter Observatory (CSO) to follow-up a sample of WISE-selected, hyperluminous galaxies, so called W1W2-dropout galaxies. This is a rare (~ 1000 all…

astro-ph2003

The CORALS Survey: A Review and Progress Report on The Search for Dust Obscured Quasar Absorption Line Systems

Sara L. Ellison, Max Pettini, Chris W. Churchill +6

We present a brief overview of the ongoing Complete Optical and Radio Absorption Line System (CORALS) survey. We review the results of our survey for z>2.2 damped Lyman alpha syste…

astro-ph.HE2018

Light curves of hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory

Annalisa De Cia, A. Gal-Yam, A. Rubin +24

We investigate the light-curve properties of a sample of 26 spectroscopically confirmed hydrogen-poor superluminous supernovae (SLSNe-I) in the Palomar Transient Factory (PTF) surv…

astro-ph.GA2020

The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at

Federica Loiacono, Roberto Decarli, Carlotta Gruppioni +32

We present the first [CII] 158 m luminosity function (LF) at from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [CII] at Early tim…

astro-ph.GA2016

The Role of Star-Formation and AGN in Dust Heating of z=0.3-2.8 Galaxies - II. Informing IR AGN fraction estimates through simulations

Eric Roebuck, Anna Sajina, Christopher C. Hayward +4

A key question in extragalactic studies is the determination of the relative roles of stars and AGN in powering dusty galaxies at 1-3 where the bulk of star-formation and AG…

cs.HC2021

Geometry-Aware Merge Tree Comparisons for Time-Varying Data with Interleaving Distances

Lin Yan, Talha Bin Masood, Farhan Rasheed +2

Merge trees, a type of topological descriptor, serve to identify and summarize the topological characteristics associated with scalar fields. They present a great potential for the…

astro-ph2008

Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 III: Far-IR to Radio Properties and Optical Spectral Diagnostics

Anna Sajina, Lin Yan, Dieter Lutz +7

We present the far-IR, millimeter, and radio photometry as well as optical and near-IR spectroscopy of a sample of 48 z~1-3 Spitzer-selected ULIRGs with IRS mid-IR spectra. Our goa…

astro-ph.CO2010

A Massive Molecular Gas Reservoir in the z=5.3 Submillimeter Galaxy AzTEC-3

Dominik A. Riechers, Peter L. Capak, Christopher L. Carilli +6

We report the detection of CO 2-1, 5-4, and 6-5 emission in the highest-redshift submillimeter galaxy (SMG) AzTEC-3 at z=5.298, using the Expanded Very Large Array and the Plateau…

astro-ph.HE2019

Discovery of Highly Blueshifted Broad Balmer and Metastable Helium Absorption Lines in a Tidal Disruption Event

T. Hung, S. B. Cenko, Nathaniel Roth +25

We report the discovery of non-stellar hydrogen Balmer and metastable helium absorption lines accompanying a transient, high-velocity (0.05) broad absorption line (BAL) system i…

astro-ph.GA2016

The Local [CII] 158 um Emission Line Luminosity Function

Shoubaneh Hemmati, Lin Yan, Tanio Diaz-Santos +4

We present, for the first time, the local [CII] 158 um emission line luminosity function measured using a sample of more than 500 galaxies from the Revised Bright Galaxy Sample (RB…

astro-ph.HE2019

GROWTH on S190426c. II. Real-Time Search for a Counterpart to the Probable Neutron Star-Black Hole Merger using an Automated Difference Imaging Pipeline for DECam

Daniel A. Goldstein, Igor Andreoni, Peter E. Nugent +17

The discovery of a transient kilonova following the gravitational-wave event GW170817 highlighted the critical need for coordinated rapid and wide-field observations, inference, an…

astro-ph.EP2020

Characterization of the Nucleus, Morphology and Activity of Interstellar Comet 2I/Borisov by Optical and Near-Infrared GROWTH, Apache Point, IRTF, ZTF and Keck Observations

Bryce T. Bolin, Carey M. Lisse, Mansi M. Kasliwal +52

We present visible and near-infrared photometric and spectroscopic observations of interstellar object 2I/Borisov taken from 2019 September 10 to 2019 November 29 using the GROWTH,…

astro-ph.HE2019

A New Class of Changing-Look LINERs

Sara Frederick, Suvi Gezari, Matthew J. Graham +28

We report the discovery of six active galactic nuclei (AGN) caught "turning on" during the first nine months of the Zwicky Transient Facility (ZTF) survey. The host galaxies were c…

cs.CG2018

Homology-Preserving Dimensionality Reduction via Manifold Landmarking and Tearing

Lin Yan, Yaodong Zhao, Paul Rosen +2

Dimensionality reduction is an integral part of data visualization. It is a process that obtains a structure preserving low-dimensional representation of the high-dimensional data.…

cs.LG2025

Enhancing Multi-Step Reasoning Abilities of Language Models through Direct Q-Function Optimization

Kaixuan Ji, Guanlin Liu, Ning Dai +6

Reinforcement Learning (RL) plays a crucial role in aligning large language models (LLMs) with human preferences and improving their ability to perform complex tasks. However, curr…

cs.CV2022

Multilevel Robustness for 2D Vector Field Feature Tracking, Selection, and Comparison

Lin Yan, Paul Aaron Ullrich, Luke P. Van Roekel +2

Critical point tracking is a core topic in scientific visualization for understanding the dynamic behavior of time-varying vector field data. The topological notion of robustness h…

astro-ph.GA2020

The ALPINE-ALMA [C II] Survey: [C II]158micron Emission Line Luminosity Functions at

Lin Yan, A. Sajina, F. Loiacono +28

We present the [CII]158m line luminosity functions (LFs) at using the ALMA observations of 118 sources, which are selected to have UV luminosity an…

astro-ph.EP2020

Characterization of Temporarily-Captured Minimoon 2020 CD by Keck Time-resolved Spectrophotometry

Bryce T. Bolin, Christoffer Fremling, Timothy R. Holt +42

We present time-resolved visible spectrophotometry of minimoon 2020 CD, the second asteroid known to become temporarily captured by the Earth-Moon system's gravitational field.…

astro-ph2004

The First Measurements of Galaxy Clustering from IRAC Data of the Spitzer First Look Survey

Fan Fang, David L. Shupe, Gillian Wilson +19

We present the first results of the angular auto-correlation function of the galaxies detected by the Infrared Array Camera (IRAC) instrument in the First Look Survey (FLS) of the…

astro-ph.HE2026

Late-Time HST UV Detections Reveal Eruptive Mass Loss and Circumstellar Interaction in a Quarter of Stripped-Envelope Supernovae

C. Fremling, S. Covarrubias, J. Sollerman +19

We present HST WFC3/UVIS F275W near-UV imaging of 91stripped-envelope supernovae (SE SNe; Types IIb, Ib, Ic) from Snapshot program SNAP-16657, observed at phases of 270-1845 days (…

astro-ph2006

Star Formation and Extinction in Redshift z~2 Galaxies: Inferences from Spitzer MIPS Observations

Naveen A. Reddy, Charles C. Steidel, Dario Fadda +5

Using very deep Spitzer/MIPS 24 micron observations, we present an analysis of the bolometric luminosities (L[bol]) and UV extinction properties of more than 200 spectroscopically…

astro-ph1996

A Spectroscopic Survey for Binary Stars in the Globular Cluster NGC5053

Lin Yan, J. G. Cohen

We carried out a radial velocity survey for spectroscopic binaries in the low density globular cluster NGC5053. Our sample contains a total of 77 cluster member giant and subgiant…

astro-ph.HE2024

Probing pre-supernova mass loss in double-peaked Type Ibc supernovae from the Zwicky Transient Facility

Kaustav K. Das, Mansi M. Kasliwal, Jesper Sollerman +34

Eruptive mass loss of massive stars prior to supernova (SN) explosion is key to understanding their evolution and end fate. An observational signature of pre-SN mass loss is the de…

astro-ph.GA2020

The BUFFALO HST Survey

Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron +91

The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. B…

cs.CG2021

Sketching Merge Trees for Scientific Data Visualization

Mingzhe Li, Sourabh Palande, Lin Yan +1

Merge trees are a type of topological descriptors that record the connectivity among the sublevel sets of scalar fields. They are among the most widely used topological tools in vi…

cs.LG2025

What's Behind PPO's Collapse in Long-CoT? Value Optimization Holds the Secret

Yufeng Yuan, Yu Yue, Ruofei Zhu +2

Reinforcement learning (RL) is pivotal for enabling large language models (LLMs) to generate long chains of thought (CoT) for complex tasks like math and reasoning. However, Proxim…

astro-ph.HE2023

A 12.4 day periodicity in a close binary system after a supernova

Ping Chen, Avishay Gal-Yam, Jesper Sollerman +37

Neutron stars and stellar-mass black holes are the remnants of massive star explosions. Most massive stars reside in close binary systems, and the interplay between the companion s…

astro-ph2007

The infrared luminosity function of galaxies at redshifts z=1 and z~2 in the GOODS fields

K. I. Caputi, G. Lagache, Lin Yan +6

We present the rest-frame 8 micron luminosity function (LF) at redshifts z=1 and ~2, computed from Spitzer 24 micron-selected galaxies in the GOODS fields over an area of 291 sq. a…

astro-ph.HE2020

Early Ultra-Violet observations of type IIn supernovae constrain the asphericity of their circumstellar material

Maayane T. Soumagnac, Eran O. Ofek, Jingyi Liang +41

We present a survey of the early evolution of 12 Type IIn supernovae (SNe IIn) in the Ultra-Violet (UV) and visible light. We use this survey to constrain the geometry of the circu…

astro-ph.HE2023

A Systematic Study of Ia-CSM Supernovae from the ZTF Bright Transient Survey

Yashvi Sharma, Jesper Sollerman, Christoffer Fremling +35

Among the supernovae (SNe) that show strong interaction with the circumstellar medium, there is a rare subclass of Type Ia supernovae, SNe Ia-CSM, that show strong narrow hydrogen…

astro-ph.HE2018

Spectra of Hydrogen-Poor Superluminous Supernovae from the Palomar Transient Factory

Robert M. Quimby, Annalisa De Cia, Avishay Gal-Yam +20

Most Type I superluminous supernovae (SLSNe-I) reported to date have been identified by their high peak luminosities and spectra lacking obvious signs of hydrogen. We demonstrate t…

astro-ph.HE2016

On the early-time excess emission in hydrogen-poor superluminous supernovae

Paul M. Vreeswijk, Giorgos Leloudas, Avishay Gal-Yam +27

We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient Factory. Both show ex…