ATLAS: A High-Cadence All-Sky Survey System

Abstract

Technology has advanced to the point that it is possible to image the entire sky every night and process the data in real time. The sky is hardly static: many interesting phenomena occur, including variable stationary objects such as stars or QSOs, transient stationary objects such as supernovae or M dwarf flares, and moving objects such as asteroids and the stars themselves. Funded by NASA, we have designed and built a sky survey system for the purpose of finding dangerous near-Earth asteroids (NEAs). This system, the "Asteroid Terrestrial-impact Last Alert System" (ATLAS), has been optimized to produce the best survey capability per unit cost, and therefore is an efficient and competitive system for finding potentially hazardous asteroids (PHAs) but also for tracking variables and finding transients. While carrying out its NASA mission, ATLAS now discovers more bright ($m<19$) supernovae candidates than any ground based survey, frequently detecting very young explosions due to its 2 day cadence. ATLAS discovered the afterglow of a gamma-ray burst independent of the high energy trigger and has released a variable star catalogue of 5$\times 10^6$ sources. This, the first of a series of articles describing ATLAS, is devoted to the design and performance of the ATLAS system. Subsequent articles will describe in more detail the software, the survey strategy, ATLAS-derived NEA population statistics, transient detections, and the first data release of variable stars and transient lightcurves.

arXiv comment26 pages, 12 figures, submitted to PASP

References in corpus (49)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Gaia mission
• Multi-messenger Observations of a Binary Neutron Star Merger
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• First Results from the Catalina Real-time Transient Survey
• Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
• The Palomar Transient Factory: System Overview, Performance and First Results
• Astrometry.net: Blind astrometric calibration of arbitrary astronomical images
• The Dark Energy Survey: more than dark energy - an overview
• A kilonova as the electromagnetic counterpart to a gravitational-wave source
• Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
• The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
• The Pan-STARRS1 Surveys
• Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
• Hydrogen-poor superluminous stellar explosions
• SkyMapper and the Southern Sky Survey
• The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
• PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects
• Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey
• Localization and broadband follow-up of the gravitational-wave transient GW150914
• Pan-STARRS Photometric and Astrometric Calibration
• MASTER optical detection of the first LIGO/Virgo neutron stars merging GW170817
• Sagittarius II, Draco II and Laevens 3: three new Milky Way satellites discovered in the Pan-STARRS 1 3pi Survey
• The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets
• Spectrophotometric Libraries, Revised Photonic Passbands and Zero-points for UBVRI, Hipparcos and Tycho Photometry
• ASASSN-15lh: A Highly Super-Luminous Supernova
• The Pan-STARRS Moving Object Processing System
• An Early Warning System for Asteroid Impact
• The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
• Super-luminous supernovae from PESSTO
• Discovery of eight z ~ 6 quasars from Pan-STARRS1
• Uncloaking globular clusters in the inner Galaxy
• LSQ14bdq: A Type Ic super-luminous supernova with a double-peaked light curve
• Real-Time Detection and Rapid Multiwavelength Follow-up Observations of a Highly Subluminous Type II-P Supernova from the Palomar Transient Factory Survey
• Discovery of a Cosmological, Relativistic Outburst via its Rapidly Fading Optical Emission
• SkyMapper Filter Set: Design and Fabrication of Large Scale Optical Filters
• Constraints on the Progenitor of SN 2016gkg From Its Shock-Cooling Light Curve
• How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?
• The ASAS-SN Bright Supernova Catalog $-$ I. 2013$-$2014
• iPTF14yb: The First Discovery of a GRB Afterglow Independent of a High-Energy Trigger
• First Results from Pan-STARRS1: Faint, High Proper Motion White Dwarfs in the Medium-Deep Fields
• Discovery of Main-Belt Comet P/2006 VW139 by Pan-STARRS1
• Observations of the GRB afterglow ATLAS17aeu and its possible association with GW170104
• Volumetric Survey Speed: A Figure of Merit for Transient Surveys
• First release of high-redshift superluminous supernovae from the Subaru HIgh-Z sUpernova CAmpaign (SHIZUCA). II. Spectroscopic properties
• Testing Accuracy and Precision of Existing Photometry Algorithms on Moving Targets
• Asiago Supernova classification program: blowing out the first two hundred candles
• On the capabilities of survey telescopes of moderate size

Cited by in corpus (645)

• The Zwicky Transient Facility: System Overview, Performance, and First Results
• The Zwicky Transient Facility: Science Objectives
• Tidal Disruption Events
• The Zwicky Transient Facility: Surveys and Scheduler
• Design and operation of the ATLAS Transient Science Server
• A First Catalog of Variable Stars Measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS)
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• The ATLAS All-Sky Stellar Reference Catalog
• The Zwicky Transient Facility Bright Transient Survey. II. A Public Statistical Sample for Exploring Supernova Demographics
• The Cow: discovery of a luminous, hot and rapidly evolving transient
• The Fast, Luminous Ultraviolet Transient AT2018cow: Extreme Supernova, or Disruption of a Star by an Intermediate-Mass Black Hole?
• The Final Season Reimagined: 30 Tidal Disruption Events from the ZTF-I Survey
• TESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26
• Optical-Ultraviolet Tidal Disruption Events
• The Automatic Learning for the Rapid Classification of Events (ALeRCE) Alert Broker
• 1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months
• POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae
• The ASAS-SN Catalog of Variable Stars III: Variables in the Southern TESS Continuous Viewing Zone
• The delay of shock breakout due to circumstellar material seen in most Type II Supernovae
• The destruction and recreation of the X-ray corona in a changing-look Active Galactic Nucleus
• The GROWTH Marshal: A Dynamic Science Portal for Time-Domain Astronomy
• Observational Properties of Thermonuclear Supernovae
• SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances
• Type Ia Supernova Explosions in Binary Systems: A Review
• RAPID: Early Classification of Explosive Transients using Deep Learning
• A Fully Automated Integral Field Spectrograph Pipeline for the SEDMachine: pysedm
• AT2018cow: a luminous millimeter transient
• Investigating the properties of stripped-envelope supernovae, what are the implications for their progenitors?
• Final Moments I: Precursor Emission, Envelope Inflation, and Enhanced Mass loss Preceding the Luminous Type II Supernova 2020tlf
• Machine Learning for the Zwicky Transient Facility
• GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR
• A very luminous jet from the disruption of a star by a massive black hole
• An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• ASASSN-14ko is a Periodic Nuclear Transient in ESO 253-G003
• A consistent estimate for Gravitational Wave and Electromagnetic transient rates
• The first tidal disruption flare in ZTF: from photometric selection to multi-wavelength characterization
• Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)
• The Zwicky Transient Facility Census of the Local Universe I: Systematic search for Calcium rich gap transients reveal three related spectroscopic sub-classes
• A New Class of Changing-Look LINERs
• A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
• Discovery and Follow-up of ASASSN-19dj: An X-ray and UV Luminous TDE in an Extreme Post-Starburst Galaxy
• PS18kh: A New Tidal Disruption Event with a Non-Axisymmetric Accretion Disk
• Searching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)
• Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS
• The Young Supernova Experiment: Survey Goals, Overview, and Operations
• Kilonova Luminosity Function Constraints based on Zwicky Transient Facility Searches for 13 Neutron Star Mergers
• A Search for Extragalactic Fast Blue Optical Transients in ZTF and the Rate of AT2018cow-like Transients
• The Prospects of Observing Tidal Disruption Events with the LSST
• ASASSN-18ey: The Rise of a New Black-Hole X-ray Binary
• The Science of the Einstein Telescope
• The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
• From Discovery to the First Month of the Type II Supernova 2023ixf: High and Variable Mass Loss in the Final Year before Explosion
• A data science platform to enable time-domain astronomy
• Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv
• Fast-transient Searches in Real Time with ZTFReST: Identification of Three Optically-discovered Gamma-ray Burst Afterglows and New Constraints on the Kilonova Rate
• Seeing Double: ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve
• The ASAS-SN Catalog of Variable Stars V: Variables in the Southern Hemisphere
• The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
• Evidence for Late-stage Eruptive Mass-loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient
• Mid-InfraRed Outburst in Nearby Galaxies (MIRONG) I: Sample Selection and Characterization
• Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science
• Palomar Gattini-IR: Survey overview, data processing system, on-sky performance and first results
• A Global Fireball Observatory
• Deciphering the extreme X-ray variability of the nuclear transient eRASSt J045650.3-203750: A likely repeating partial tidal disruption event
• The tidal disruption event AT2017eqx: spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow
• The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient
• SN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral Features
• ZTF 18aaqeasu (SN 2018byg): A Massive Helium-shell Double Detonation on a Sub-Chandrasekhar Mass White Dwarf
• Core-collapse, superluminous, and gamma-ray burst supernova host galaxy populations at low redshift: the importance of dwarf and starbursting galaxies
• The ASAS-SN Catalog of Variable Stars IX: The Spectroscopic Properties of Galactic Variable Stars
• Searches After Gravitational-waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo's Third Observing Run
• The volumetric rate of normal type Ia supernovae in the local universe discovered by the Palomar Transient Factory
• The 450 days X-ray monitoring of the changing-look AGN 1ES 1927+654
• Asteroid phase curves from ATLAS dual-band photometry
• SN 2017ens: The Metamorphosis of a Luminous Broad-lined Type Ic Supernova into an SN IIn
• The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
• New Modules for the SEDMachine to Remove Contaminations from Cosmic Rays and Non-target Light: BYECR and CONTSEP
• The Tidal Disruption Event AT2021ehb: Evidence of Relativistic Disk Reflection, and Rapid Evolution of the Disk-Corona System
• The ASAS-SN Catalog of Variable Stars X: Discovery of 116,000 New Variable Stars Using g-band Photometry
• Alert Classification for the ALeRCE Broker System: The Real-time Stamp Classifier
• Wind-reprocessed Transients
• The ASAS-SN Bright Supernova Catalog $-$ II. 2015
• SN2020bvc: a Broad-lined Type Ic Supernova with a Double-peaked Optical Light Curve and a Luminous X-ray and Radio Counterpart
• The Hydrogen-Poor Superluminous Supernovae from the Zwicky Transient Facility Phase-I Survey: I. Light Curves and Measurements
• Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae
• Circumstellar Interaction Powers the Light Curves of Luminous Rapidly Evolving Optical Transients
• Early Time Light Curves of Type Ia Supernovae Observed with TESS
• Evidence for a Compact Object in the Aftermath of the Extra-Galactic Transient AT2018cow
• Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory
• Transients from ONe White-Dwarf - Neutron-Star/Black-Hole Mergers
• The EREBOS project -- Investigating the effect of substellar and low-mass stellar companions on late stellar evolution
• The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels
• Teamwork Makes the Dream Work: Optimizing Multi-Telescope Observations of Gravitational-Wave Counterparts
• A JWST Survey of the Supernova Remnant Cassiopeia A
• YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-Loop
• No Stripped Companion Material in the Nebular Spectrum of the "Two-Component" Type Ia Supernova ASASSN-18bt
• Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results
• A nearby superluminous supernova with a long pre-maximum 'plateau' and strong CII features
• TOI-5205 b: A Short-period Jovian Planet Transiting a Mid-M Dwarf
• The Host Galaxy and Rapidly Evolving Broad-line Region in the Changing-look Active Galactic Nucleus 1ES 1927+654
• Discovery of the Fastest Early Optical Emission from Overluminous SN Ia 2020hvf: A Thermonuclear Explosion within a Dense Circumstellar Environment
• Scientific CMOS sensors in Astronomy: IMX455 and IMX411
• The rebrightening of a ROSAT-selected tidal disruption event: repeated weak partial disruption flares from a quiescent galaxy?
• The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae
• Second Data Release of the All-sky NOIRLab Source Catalog
• The ASAS-SN Bright Supernova Catalog -- IV. 2017
• Interstellar comet 3I/ATLAS: discovery and physical description
• Rapid "Turn-on" of type 1 AGN in a quiescent early type galaxy SDSS1115+0544
• On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion
• Year 1 of the ZTF high-cadence Galactic Plane Survey: Strategy, goals, and early results on new single-mode hot subdwarf B-star pulsators
• Discovery and characterization of five new eclipsing AM CVn systems
• Superluminous supernovae: an explosive decade
• Luminous Supernovae: Unveiling a Population Between Superluminous and Normal Core-collapse Supernovae
• Limits on the Electromagnetic Counterpart to S190814bv
• Identifying LISA verification binaries among the Galactic population of double white dwarfs
• The Zwicky Transient Facility Type Ia supernova survey: first data release and results
• Observations of SN 2017ein Reveal Shock Breakout Emission and A Massive Progenitor Star for a Type Ic Supernova
• Six New Compact Triply Eclipsing Triples Found With TESS
• Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters
• Evolution of a Relativistic Outflow and X-ray Corona in the Extreme Changing-Look AGN 1ES 1927+654
• SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements
• Asteroid models reconstructed from ATLAS photometry
• $\text{simsurvey}$: Estimating Transient Discovery Rates for the Zwicky Transient Facility
• Peculiar-velocity cosmology with Types Ia and II supernovae
• The Spectroscopic Classification of Astronomical Transients (SCAT) Survey: Overview, Pipeline Description, Initial Results, and Future Plans
• The Sporadic Activity of (6478) Gault: A YORP-driven event?
• Extragalactic FXT Candidates Discovered by Chandra (2014-2022)
• Variable H$\alpha$ Emission in the Nebular Spectra of the Low-Luminosity Type Ia SN2018cqj/ATLAS18qtd
• The ASAS-SN Catalog of Variable Stars VII: Contact Binaries are Different Above and Below the Kraft Break
• A radio-detected Type Ia supernova with helium-rich circumstellar material
• A Blast from the Pasture: Studying the environment of AT 2018cow with MUSE
• Discovery of a Fast Iron Low-ionization Outflow in the Early Evolution of the Nearby Tidal Disruption Event AT2019qiz
• Low-Cost Access to the Deep, High-Cadence Sky: the Argus Optical Array
• Cosmological Fast Optical Transients with the Zwicky Transient Facility: A Search for Dirty Fireballs
• Transient-optimised real-bogus classification with Bayesian Convolutional Neural Networks -- sifting the GOTO candidate stream
• Assessing interstellar comet 3I/ATLAS with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope
• uGMRT observations of a Fast and Blue Optical Transient -- AT 2018cow
• 2900 square degree search for the optical counterpart of short gamma-ray burst GRB 180523B with the Zwicky Transient Facility
• Luminous Red Nova AT 2019zhd, a new merger in M 31
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• ASTROMER: A transformer-based embedding for the representation of light curves
• High-Cadence, Early-Time Observations of Core-Collapse Supernovae From the TESS Prime Mission
• A Systematic Study of Ia-CSM Supernovae from the ZTF Bright Transient Survey
• Ca hnk: Calcium-rich Transient SN 2016hnk from the Helium Shell Detonation of a Sub-Chandrasekhar White Dwarf
• SN2018kzr: a rapidly declining transient from the destruction of a white dwarf
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• Triply eclipsing triple stars in the northern TESS fields: TICs 193993801, 388459317 and 52041148
• The nuclear transient AT 2017gge: a tidal disruption event in a dusty and gas-rich environment and the awakening of a dormant SMBH
• A Bright Ultraviolet Excess in the Transitional 02es-like Type Ia Supernova 2019yvq
• The ASAS-SN Catalog of Variable Stars IV: Periodic Variables in the APOGEE Survey
• SN 2018bsz: a Type I superluminous supernova with aspherical circumstellar material
• The Tsinghua University-Ma Huateng Telescopes for Survey: Overview and Performance of the System
• Progenitor candidate for the type II-P supernova SN 2018aoq in NGC 4151
• A Swift Fix for Nuclear Outbursts
• Orbital Foregrounds for Ultra-Short Duration Transients
• Three Core-Collapse Supernovae with Nebular Hydrogen Emission
• The rise and fall of the iron-strong nuclear transient PS16dtm
• Detectability of kilonovae in optical surveys: $post$-$mortem$ examination of the LVC O3 run follow-up
• The unluckiest star: A spectroscopically confirmed repeated partial tidal disruption event AT 2022dbl
• The Circumstellar Environments of Double-Peaked, Calcium-strong Supernovae 2021gno and 2021inl
• AT 2020wey and the class of faint and fast Tidal Disruption Events
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• A Speed Bump: SN 2021aefx Shows that Doppler Shift Alone can Explain Early-Excess Blue Flux in Some Type Ia Supernovae
• Dynamical confirmation of a black hole in the X-ray transient Swift J1727.8-1613
• The Evolution of Luminous Red Nova AT 2017jfs in NGC 4470
• The Luminosity Function of Tidal Disruption Flares for the ZTF-I Survey
• Examining a Peak-Luminosity/Decline-Rate Relationship for Tidal Disruption Events
• The ZTF Source Classification Project: I. Methods and Infrastructure
• The BlackGEM telescope array I: Overview
• The Hyper Suprime-Cam SSP Transient Survey in COSMOS: Overview
• Four (Super)luminous Supernovae from the First Months of the ZTF Survey
• The lowest of the low: discovery of SN 2019gsc and the nature of faint Iax supernovae
• SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event
• Low luminosity Type II supernovae -- IV. SN 2020cxd and SN 2021aai, at the edges of the sub-luminous supernovae class
• Rapidly Evolving Transients from the Hyper Suprime-Cam SSP Transient Survey
• Discovery of an intermediate-luminosity red transient in M51 and its likely dust-obscured, infrared-variable progenitor
• Volumetric rates of Luminous Red Novae and Intermediate Luminosity Red Transients with the Zwicky Transient Facility
• The double-peaked type Ic Supernova 2019cad: another SN 2005bf-like object
• The luminous red nova variety: AT 2020hat and AT 2020kog
• The luminous type Ia supernova 2022ilv and its early excess emission
• From a Different Star: 3I/ATLAS in the context of the Ōtautahi-Oxford interstellar object population model
• A Hydrogen-Poor Superluminous Supernova with Enhanced Iron-Group Absorption: A New Link Between SLSNe and Broad-Lined Type Ic SNe
• Discovery of ATLAS17jrp as an Optical, X-ray and Infrared Bright TDE in a Star-forming Galaxy
• The ZTF Source Classification Project: II. Periodicity and variability processing metrics
• SN 2019muj -- a well-observed Type Iax supernova that bridges the luminosity gap of the class
• SN 2018gjx reveals that some SNe Ibn are SNe IIb exploding in dense circumstellar material
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• SN 2020kyg and the rates of faint Iax Supernovae from ATLAS
• Less than 1% of Core-Collapse Supernovae in the local universe occur in elliptical galaxies
• ZTF J1901+5309: A 40.6-Minute Orbital Period Eclipsing Double White Dwarf System
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• A systematic search for outbursting AM CVn systems with the Zwicky Transient Facility
• Investigating the Nature of the Luminous Ambiguous Nuclear Transient ASASSN-17jz
• The Most Rapidly Declining Type I Supernova 2019bkc/ATLAS19dqr
• A Mid-infrared Study of Superluminous Supernovae
• A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
• The New EXor Outburst of ESO-H-alpha~99 observed by Gaia ATLAS and TESS
• The population of tidal disruption events discovered with eROSITA
• Is the high-energy neutrino event IceCube-200530A associated with a hydrogen-rich superluminous supernova?
• SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environment
• Novel constraints on fifth forces and ultralight dark sector with asteroidal data
• The first Hubble diagram and cosmological constraints using superluminous supernova
• AT 2021loi: A Bowen Fluorescence Flare with a Rebrightening Episode, Occurring in a Previously-Known AGN
• Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs
• Discovery of the most ultra-luminous QSO using Gaia, SkyMapper and WISE
• Observations of the luminous red nova AT 2021biy in the nearby galaxy NGC 4631
• Minutes-duration Optical Flares with Supernova Luminosities
• The rise and fall of an extraordinary Ca-rich transient -- The discovery of ATLAS19dqr/SN 2019bkc
• Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods
• Discovery of the luminous X-ray ignition eRASSt J234402.9$-$352640; I. Tidal disruption event or a rapid increase in accretion in an active galactic nucleus?
• Optimizing Serendipitous Detections of Kilonovae: Cadence and Filter Selection
• Vetting the optical transient candidates detected by the GWAC network using convolutional neural networks
• Newly identified compact hierarchical triple system candidates using Gaia DR3
• SN 2022acko: the First Early Far-Ultraviolet Spectra of a Type IIP Supernova
• Early-Time Ultraviolet Spectroscopy and Optical Follow-up Observations of the Type IIP Supernova 2021yja
• Supernova Rates and Luminosity Functions from ASAS-SN I: 2014--2017 Type Ia SNe and Their Subtypes
• SNIascore: Deep Learning Classification of Low-Resolution Supernova Spectra
• Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)
• Classifying Image Sequences of Astronomical Transients with Deep Neural Networks
• SN 2017ivv: two years of evolution of a transitional Type II supernova
• The First Release of the AST3-1 Point Source Catalogue from Dome A, Antarctica
• A new study on a type Iax stellar remnant and its probable association with SN 1181
• Inferencing Progenitor and Explosion Properties of Evolving Core-collapse Supernovae from Zwicky Transient Facility Light Curves
• Polarimetry of Hydrogen-Poor Superluminous Supernovae
• A Study of Nine Triply Eclipsing Triples
• LSQ13ddu: A rapidly-evolving stripped-envelope supernova with early circumstellar interaction signatures
• Broad-emission-line dominated hydrogen-rich luminous supernovae
• Recurring tidal disruption events a decade apart in IRAS F01004-2237
• Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
• Identification of RR Lyrae stars in multiband, sparsely-sampled data from the Dark Energy Survey using template fitting and Random Forest classification
• From Out of the Blue: Swift Links 2002es-like, 2003fg-like, and Early-Time Bump Type Ia Supernovae
• Early emission lines in SN 2024ggi revealed by high-resolution spectroscopy
• Gaia18aen: First symbiotic star discovered by Gaia
• Real-Time Value-Driven Data Augmentation in the Era of LSST
• The Foundation Supernova Survey: Photospheric Velocity Correlations in Type Ia Supernovae
• The far side of the Galactic bar/bulge revealed through semi-regular variables
• Long-term follow-up observations of extreme coronal line emitting galaxies
• The accretion of a solar mass per day by a 17-billion solar mass black hole
• The Kitt Peak Electron Multiplying CCD demonstrator
• Follow-up Studies of Five Cataclysmic Variable Candidates Discovered by LAMOST
• An in-depth reanalysis of the alleged type Ia supernova progenitor Henize 2-428
• A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
• SN 2020bqj: a Type Ibn supernova with a long lasting peak plateau
• PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae
• TACOS: TESS AM~CVn Outbursts Survey
• Gap Transients Interacting with Circumstellar Medium
• The "Giraffe": Discovery of a stripped red giant in an interacting binary with a $\sim 2M_{\odot }$ lower giant
• Compact white-dwarf binaries in the combined SRG/eROSITA/SDSS eFEDS survey
• Universality in the Random Walk Structure Function of Luminous Quasi-Stellar Objects
• Symbiotic stars in the era of modern ground- and space-based surveys
• A luminous stellar outburst during a long-lasting eruptive phase first, and then SN IIn 2018cnf
• A search for compact object companions to high mass function single-lined spectroscopic binaries in Gaia DR3
• Late-time H/He-poor circumstellar interaction in the type-Ic supernova SN 2021ocs: an exposed oxygen-magnesium layer and extreme stripping of the progenitor
• Observations of the low-luminosity Type Iax supernova 2019gsc: a fainter clone of SN 2008ha?
• SN 2018hti: a nearby superluminous supernova discovered in a metal-poor galaxy
• Investigating Taxonomic Diversity within Asteroid Families through ATLAS Dual-Band Photometry
• Physical Characterization of Main-Belt Comet (248370) 2005 QN173
• A WISE view on extreme AGB stars
• SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
• Multiple Peaks and a Long Precursor in the Type IIn Supernova 2021qqp: An Energetic Explosion in a Complex Circumstellar Environment
• The Large Array Survey Telescope -- Science Goals
• Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernova
• Multiwavelength observations of the extraordinary accretion event AT2021lwx
• SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1
• On the nature of the unusual transient AT 2018cow from HI observations of its host galaxy
• (6478) Gault: Physical characterization of an active main-belt asteroid
• An 18.9-minute Blue Large-Amplitude Pulsator Crossing the 'Hertzsprung Gap' of Hot Subdwarfs
• SN 2016gsd: An unusually luminous and linear type II supernova with high velocities
• Limits on Simultaneous and Delayed Optical Emission from Well-localized Fast Radio Bursts
• The Gaia alerted fading of the FUor-type star Gaia21elv
• The VVV Infrared Variability Catalog (VIVA-I)
• The ASAS-SN Bright Supernova Catalog -- V. 2018-2020
• SRGA J181414.6-225604: A new Galactic symbiotic X-ray binary outburst triggered by an intense mass loss episode of a heavily obscured Mira variable
• The Whisper of a Whimper of a Bang: 2400 Days of the Type Ia SN 2011fe Reveals the Decay of ${}^{55}$Fe
• Mysterious, Variable, and Extremely Hot: White Dwarfs Showing Ultra-High Excitation Lines I. Photometric Variability
• A Two-Stage Deep Learning Detection Classifier for the ATLAS Asteroid Survey
• $V$-band photometry of asteroids from ASAS-SN: Finding asteroids with slow spin
• SN 2021foa, a transitional event between a Type IIn (SN 2009ip-like) and a Type Ibn supernova
• Machine Learning for Transient Recognition in Difference Imaging With Minimum Sampling Effort
• Very Large Telescope Observations of Interstellar Comet 3I/ATLAS. II. From Quiescence to Glow: Dramatic Rise of Ni i Emission and Incipient CN Outgassing at Large Heliocentric Distances*
• Predicting electromagnetic counterparts using low-latency, gravitational-wave data products
• GRANDMA Observations of ZTF/Fink Transients during Summer 2021
• Pan-chromatic photometric classification of supernovae from multiple surveys and transfer learning for future surveys
• SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction
• Photometry and spectroscopy of the Type Icn supernova 2021ckj: The diverse properties of the ejecta and circumstellar matter of Type Icn SNe
• Active asteroid (6478) Gault: a blue Q-type surface below the dust?
• RINGO3 polarimetry of very young ZTF supernovae
• Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys
• A candidate relativistic tidal disruption event at 340 Mpc
• Discovery of Super-Slow Rotating Asteroids with ATLAS and ZTF photometry
• Orbital decay in an accreting and eclipsing 13.7 minute orbital period binary with a luminous donor
• Nebular Halpha emission in SN Ia 2016jae
• NEOExchange -- An online portal for NEO and Solar System science
• Searching for precursor activity of Type IIn Supernovae
• AT 2023clx: the Faintest and Closest Optical Tidal Disruption Event Discovered in Nearby Star-forming Galaxy NGC 3799
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
• Scary Barbie: An Extremely Energetic, Long-Duration Tidal Disruption Event Candidate Without a Detected Host Galaxy at z = 0.995
• Beyond Gaia: Asteroseismic Distances of M giants using Ground-Based Transient Surveys
• Outbursting Young Stellar Object PGIR 20dci in the Perseus Arm
• The fast transient AT 2023clx in the nearby LINER galaxy NGC 3799 as a tidal disruption of a very low-mass star
• Supernova Siblings and their Parent Galaxies in the Zwicky Transient Facility Bright Transient Surve
• Refinement of the convex shape model and tumbling spin state of (99942) Apophis using the 2020-2021 apparition data
• Citizen ASAS-SN Data Release I: Variable Star Classification Using Citizen Science
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• SN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases
• Searching for Dark Clumps with Gravitational-Wave Detectors
• Panchromatic evolution of three luminous red novae: Forbidden hugs in pandemic times -- IV
• Sample of hydrogen-rich superluminous supernovae from the Zwicky Transient Facility
• A Spectral Classification System for Hydrogen-deficient Carbon Stars
• SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environment
• Probing the Soft X-ray Properties and Multi-Wavelength Variability of SN2023ixf and its Progenitor
• Light-Curve Structure and Halpha Line Formation in the Tidal Disruption Event AT 2019azh
• Repeating periodic eruptions of the supernova impostor SN 2000ch
• The DEHVILS Survey Overview and Initial Data Release: High-Quality Near-Infrared Type Ia Supernova Light Curves at Low Redshift
• Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine
• Identification of SRGt 062340.2-265715 as a bright, strongly variable, novalike cataclysmic variable
• Six Outbursts of Comet 46P/Wirtanen
• The detection efficiency of type Ia supernovae from the Zwicky Transient Facility: Limits on the intrinsic rate of early flux excesses
• Early and Extensive Ultraviolet Through Near Infrared Observations of the Intermediate-Luminosity Type Iax Supernovae 2024pxl
• Probing pre-supernova mass loss in double-peaked Type Ibc supernovae from the Zwicky Transient Facility
• Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date
• Automated Detection of Satellite Trails in Ground-Based Observations Using U-Net and Hough Transform
• Association of the IceCube neutrinos with blazars in the CGRaBS sample
• Asymmetries and Circumstellar Interaction in the Type II SN 2024bch
• Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
• Tails: Chasing Comets with the Zwicky Transient Facility and Deep Learning
• Characterization of low-significance gravitational-wave compact binary sources
• Minute-Cadence Observations of the LAMOST Fields with the TMTS: II. Catalogues of Short-Period Variable Stars from the First Two-Year Surveys
• Environmental Dependence of Type Ia Supernovae in Low-Redshift Galaxy Clusters
• The Type Ibn Supernova 2019kbj -- Indications for Diversity in Type Ibn Supernova Progenitors
• Multi-wavelength detection of an ongoing FUOr-type outburst on a low-mass YSO
• Rapid bursts of magnetically gated accretion in the intermediate polar V1025 Cen
• SN 2024abfo: a partially stripped SN II from a yellow supergiant
• Video Observations of Tiny Near-Earth Objects with Tomo-e Gozen
• The fall of CSS100217: a tidal disruption-induced low state in an apparently hostless active galactic nucleus
• Optical polarization and spectral properties of the H-poor superluminous supernovae SN 2021bnw and SN 2021fpl
• O'TRAIN: a robust and flexible Real/Bogus classifier for the study of the optical transient sky
• Probing the Progenitors of Type Ia Supernovae using Circumstellar Material Interaction Signatures
• Asteroids seen by JWST-MIRI: Radiometric Size, Distance and Orbit Constraints
• Discovery and physical characterization as the first response to a potential asteroid collision: The case of 2023 DZ2
• Simulating the tidal disruption of stars by stellar-mass black holes using moving-mesh hydrodynamics
• Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• The Flux Distribution and Sky Density of 25th Magnitude Main Belt Asteroids
• Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources
• Measuring White Dwarf Variability from Sparsely Sampled Gaia DR3 Multi-Epoch Photometry
• A Precursor Plateau and Pre-Maximum [O II] Emission in the Superluminous SN2019szu: A Pulsational Pair-Instability Candidate
• DELIGHT: Deep Learning Identification of Galaxy Hosts of Transients using Multi-resolution Images
• Searching for the Next Galactic Luminous Red Nova
• Optical Rebrightening of Extragalactic Transients from the Zwicky Transient Facility
• The GRBSN webtool: An open-source repository for gamma-ray burst-supernova associations
• Pre-discovery TESS Observations of Interstellar Object 3I/ATLAS
• The dynamics of debris streams from tidal disruption events: exact solutions, critical stream density, and hydrogen recombination
• An extremely hot white dwarf with a rapidly rotating K-type subgiant companion: UCAC2 46706450
• Interstellar Comet 3I/ATLAS: Evidence for Galactic Cosmic Ray Processing
• Still alive and kicking: A significant outburst in changing-look AGN Mrk 1018
• Type Ia Supernova Progenitor Properties and Their Host Galaxies
• Simultaneous visible spectrophotometry of interstellar object 3I/ATLAS with Seimei/TriCCS
• On the diversity of strongly-interacting Type IIn supernovae
• DW Cnc: a micronova with a negative superhump and a flickering spin
• IXPE Observation of the Low-Synchrotron Peaked Blazar S4 0954+65 During An Optical-X-ray Flare
• Discovery of the most luminous quasar of the last 9 Gyr
• TESS Shines Light on the Origin of the Ambiguous Nuclear Transient ASASSN-18el
• SN 2024ggi: another year, another striking Type II supernova
• Understanding of the properties of neural network approaches for transient light curve approximations
• Episodic mass loss in the very luminous red supergiant [W60] B90 in the Large Magellanic Cloud
• The Extremely Metal-Poor SN 2023ufx: A Local Analog to High-Redshift Type II Supernovae
• Multiwavelength monitoring of the nucleus in PBC J2333.9-2343: the giant radio galaxy with a blazar-like core
• Long-lasting activity of asteroid (248370) 2005 QN 173
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• SN 2020pvb: a Type IIn-P supernova with a precursor outburst
• Highly Variable Active Galactic Nuclei in the SRG/eROSITA All-Sky Survey: I. Constructing Sample and Catalog of Sources Detected in Low State
• Shape models and spin states of Jupiter Trojans: Testing the streaming instability formation scenario
• SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy
• The Evryscope Fast Transient Engine: Real-Time Detection for Rapidly Evolving Transients
• VERITAS discovery of very high energy gamma-ray emission from S3 1227+25 and multiwavelength observations
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• Photometric and dynamic characterisation of active asteroid (248370) 2005 QN173
• Main-belt and Trojan Asteroid Phase Curves from the ATLAS Survey
• Asteroid Discovery and Light Curve Extraction Using the Hough Transform -- A Rotation Period Study for Sub-Kilometer Main-Belt Asteroids
• SN 2020cpg: an energetic link between type IIb and Ib supernovae
• Asteroid spin-states of a 4 Gyr collisional family
• New magnetic chemically peculiar stars and candidates in the ATLAS First Catalog of Variable Stars
• Shock-cooling Constraints via Early-time Observations of the Type IIb SN 2022hnt
• Searching for late-time interaction signatures in Type Ia supernovae from the Zwicky Transient Facility
• Massive stars exploding in a He-rich circumstellar medium. XI. Diverse evolution of five Ibn SNe 2020nxt, 2020taz, 2021bbv, 2023utc and 2024aej
• SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• Possible Circumstellar Interaction Origin of the Early Excess Emission in Thermonuclear Supernovae
• Constraints on the rate of supernovae lasting for more than a year from Subaru/Hyper Suprime-Cam
• SN 2020uem: A Possible Thermonuclear Explosion within A Dense Circumstellar Medium (II) The Properties of The CSM from Polarimetry and Light Curve Modeling
• SN 2020uem: A Possible Thermonuclear Explosion within A Dense Circumstellar Medium (I) The Nature of Type IIn/Ia-CSM SNe from Photometry and Spectroscopy
• Results from the Pan-STARRS Search for Kilonovae: Contamination by Massive Stellar Outbursts
• SN 2024bfu, SN 2025qe, and the early light curves of type Iax supernovae
• Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems
• Cyclotron emitting magnetic white dwarfs in post common envelope binaries discovered with the Zwicky Transient Facility
• Spectral dataset of young type Ib supernovae and their time evolution
• A study in scarlet -- I. Photometric properties of a sample of Intermediate Luminosity Red Transients
• New Candidates for AM Canum Venaticorum Stars among ASAS-SN Transients
• SN 2016hil-- a Type II supernova in the remote outskirts of an elliptical host and its origin
• A Targeted Search for Main Belt Comets
• SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion
• Perfecting our set of spectrophotometric standard DA white dwarfs
• JWST Imaging of the Cartwheel Galaxy Reveals Dust Associated with SN 2021afdx
• Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasiperiodic Eruptions
• SNGuess: A method for the selection of young extragalactic transients
• Swift J0503.7-2819: A Short-Period Asynchronous Polar or Stream-Fed Intermediate Polar
• The Fast Evolving, Tremendous and Blue Superoutburst in ASASSN-21au Reveals a Dichotomy in the Outbursts of Long-period AM CVns
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• The Discovery and Evolution of a Possible New Epoch of Cometary Activity by the Centaur (2060) Chiron
• An Asymmetric Eclipse Seen Towards the Pre-Main Sequence Binary System V928 Tau
• SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon lines
• A diverse, overlooked population of Type Ia supernovae exhibiting mid-infrared signatures of delayed circumstellar interaction
• Mechanisms for high spin in black-hole neutron-star binaries and kilonova emission: inheritance and accretion
• Mining archival data from wide-field astronomical surveys in search of near-Earth objects
• Sudden extreme obscuration of a Sun-like main-sequence star: evolution of the circumstellar dust around ASASSN-21qj
• K2: Background Survey -- the search for undiscovered transients in Kepler/K2 data
• Metallicity beats sSFR: The connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
• LISA double white dwarf binaries as Galactic accelerometers
• Galactic Positrons from Thermonuclear Supernovae
• Using LSST late-time photometry to constrain Type Ibc supernovae and their progenitors
• The Next Generation of Cosmological Measurements with Type Ia Supernovae
• Astreaks: Astrometry of NEOs with trailed background stars
• AT 2018dyk: tidal disruption event or active galactic nucleus? Follow-up observations of an extreme coronal line emitter with the Dark Energy Spectroscopic Instrument
• Automated classification of eclipsing binary systems in the VVV Survey
• Hidden shock powering the peak of SN 2020faa
• The bright long-lived Type II SN 2021irp powered by aspherical circumstellar material interaction (I): Revealing the energy source with photometry and spectroscopy
• A catalog to unite them all: REGALADE, a revised galaxy compilation for the advanced detector era
• Diagnosing The Ejecta Properties of Engine-Driven Supernovae from Observables in Their Initial Phase
• ZTF SN Ia DR2: High-velocity components in the Si II $\lambda$6355
• Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve
• A long-lasting eruption heralds SN 2023ldh, a clone of SN 2009ip
• Near-Discovery SOAR Photometry of the Third Interstellar Object: 3I/ATLAS
• Observational properties of a bright type Iax SN 2018cni and a faint type Iax SN 2020kyg
• SN 2023zaw: an ultra-stripped, nickel-poor supernova from a low-mass progenitor
• Massive stars exploding in a He-rich circumstellar medium $-$ X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt
• Spin states of X-complex asteroids in the inner main belt -- I. Investigating the Athor and Zita collisional families
• AT2021acak: a candidate tidal disruption event found in the Zwicky Transient Facility survey
• Detection of disk-jet co-precession in a tidal disruption event
• Monitoring near-Earth-object discoveries for imminent impactors
• OGLE-BLAP-001 and ZGP-BLAP-08: two possible magnetic blue large-amplitude pulsators
• Fast and Not-so-Furious: Case Study of the Fast and Faint Type IIb SN 2021bxu
• Searching for stellar cycles on low mass stars using TESS data
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• Optical polarization of stellar-fed active and quiescent supermassive black holes
• Gaia23ckh: Symbiotic outburst of the assumed Mira variable V390 Sco
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• An X-ray View of the Ambiguous Nuclear Transient AT2019pev
• A survey for variable young stars with small telescopes: VI -- Analysis of the outbursting Be stars NSW284, Gaia19eyy, and VES263
• AT 2020iko: a WZ Sge-type DN candidate with an anomalous precursor event
• Hard X-ray Observations of the Hydrogen-poor Superluminous Supernova SN 2018hti with NuSTAR
• Investigating episodic mass loss in evolved massive stars: III. Spectroscopy of dusty massive stars in three northern galaxies
• SN 2019hcc: A Type II Supernova Displaying Early O II Lines
• The nebular phase of SN 2024ggi: a low-mass progenitor with no signs of interaction
• Hawai'i Supernova Flows: A Peculiar Velocity Survey Using Over a Thousand Supernovae in the Near-Infrared
• A thermonuclear supernova interacting with hydrogen- and helium-deficient circumstellar material. SN 2020aeuh as a SN Ia-CSM-C/O?
• Rotation state, colors, and albedo of the mission-accessible tiny near-Earth asteroid 2001 QJ${}_{142}$
• GOTO065054+593624: a 8.5 mag amplitude dwarf nova identified in real time via Kilonova Seekers
• ELEPHANT: ExtragaLactic alErt Pipeline for Hostless AstroNomical Transients
• A search for intermediate-mass black holes in compact stellar systems through optical emissions from tidal disruption events
• A method of photometric data extraction for asteroids from time-domain surveys
• Debiasing astro-Photometric Observations with Corrections Using Statistics (DePhOCUS)
• The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor
• TUVOpipe: a pipeline to search for UV transients with Swift-UVOT
• Comet 240P/NEAT is Stirring
• Propagating Uncertainties in the SALT3 Model Training Process to Cosmological Constraints
• Diversity of dust properties in external galaxies confirmed by polarization signals from Type II supernovae
• Limiting the accretion disk light in two mass transferring hot subdwarf binaries
• Eclipsing Binaries Found by the EREBOS Project: Gaia DR2 6097540197980557440 -- A Deeply Eclipsing sdB+dM System
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• A detailed study of the barium central star of the planetary nebula Abell 70
• An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi
• Examining the Properties of Low-Luminosity Hosts of Type Ia Supernovae from ASAS-SN
• eROSITA-RU Tidal Disruption Events with Keck-I/LRIS: Sample Selection, Optical Properties, and Host Galaxy Demographics
• The fast rise of the unusual Type IIL/IIb SN 2018ivc
• Searching for Radio Transients with Inverted Spectra in Epoch 1 of VLASS and VCSS, and Identification of a Sample of Candidate Relativistic Nuclear Transients
• Astrometric follow-up of near-Earth asteroid 2024 YR4 during a Torino scale level 3 alert
• Modeling the fast optical transient SN 2019bkc/ATLAS19dqr with a central engine and implication for its origin
• The luminosity function of TDEs from fallback-powered emission: implications for the black hole mass function
• Low-mass and sub-stellar eclipsing binaries in stellar clusters
• The role of triple evolution in the formation of LISA double white dwarfs
• VERITAS and multiwavelength observations of the Blazar B3 2247+381 in response to an IceCube neutrino alert
• A Physical Model of Delayed Rebrightenings in Shock-interacting Supernovae without Narrow Line Emission
• TCP J07222683$+$6220548: a new AM CVn type system with infrequent outbursts
• The ATLAS Virtual Research Assistant
• An Accretion Flare Interpretation for the Ultra-High-Energy Neutrino Event KM3-230213A
• Luminous, rapidly declining supernovae as stripped transitional objects in low metallicity environments: the case of SN 2022lxg
• GRB 241105A: A test case for GRB classification and rapid r-process nucleosynthesis channels
• Basaltic quasi-mini-moon: Characterizing 2024 PT5 with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope
• Exploring the Solar System with the NOIRLab Source Catalog I: Detecting Objects with CANFind
• Multi-scale stamps for real-time classification of alert streams
• ZTFJ0038+2030: a long period eclipsing white dwarf and a substellar companion
• K2 Discovery of a Circumsecondary Disk Transiting EPIC 220208795
• Textual interpretation of transient image classifications from large language models
• Site Selection for the Second Flyeye Telescope: A Simulation Study for Optimizing Near-Earth Object Discovery
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• Improving the discovery of near-Earth objects with machine-learning methods
• Unveiling the Cosmic Dance of Repeated Nuclear Transient ASASSN-14ko: Insights from Multiwavelength Observations
• Photometric calibration in u-band using blue halo stars
• The bright long-lived Type II SN 2021irp powered by aspherical circumstellar material interaction (II): Estimating the CSM mass and geometry with polarimetry and light curve modeling
• Gaia20bdk -- a new FUor in Sh 2-301 Star Forming Region
• What to expect: kilonova light curve predictions via equation of state marginalization
• PNV J00444033+4113068: early superhumps with 0.7 mag amplitude and non-red color
• SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope
• The automation of optical transient discovery and classification in Rubin-era time-domain astronomy
• Real-bogus scores for active anomaly detection
• Improving the Determination of Supernova Cosmological Redshifts by Using Galaxy Groups
• ZTF J185259.31+124955.2: A new evolved disc-eclipsing binary system
• Activity of the Jupiter co-orbital comet P/2019~LD${}_2$ (ATLAS) observed with OSIRIS at the 10.4 m GTC
• Discovery of the magnetic cataclysmic variable XMM J152737.4-205305.9 with a deep eclipse-like feature
• A Broker Integrated Algorithm for Gravitational Wave - Electromagnetic Counterpart Searches in O4a and O4b Runs
• AT 2017fvz: a nova in the dwarf irregular galaxy NGC 6822
• Discovery of periodic variables in the hot subdwarf catalogue through a systematic search in Zwicky Transient Facility data
• The DEHVILS in the Details: Type Ia Supernova Hubble Residual Comparisons and Mass Step Analysis in the Near-Infrared
• ZTF-observed late-time signals of pre-ZTF transients
• Observational diversity of bright long-lived Type II supernovae
• Rapid-response characterization of near-Earth asteroid 2024 YR4 during a Torino Scale 3 alert
• Investigating Possible Correlations between Gamma-Ray and Optical Lightcurves for TeV-Detected Northern Blazars over 8 Years of Observations
• High-velocity CP2 stars in the Galactic halo
• Improved models for near-Earth asteroids (2100) Ra-Shalom, (3103) Eger, (12711) Tukmit & (161989) Cacus
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• Searching for supermassive black holes binaries within SRG/eROSITA-De I: Properties of the X-ray selected candidates
• SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope
• The Type Ia Supernova 2021hem: A 2003fg-like Event in an Apparently Hostless Environment
• SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material
• Revisiting the unification of tidal disruption events with polarimetry
• SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction
• Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
• MUSE IFU observations of galaxies hosting Tidal Disruption Events
• CGCS 6306, another X-ray-emitting asymptotic giant branch star confirmed to be a symbiotic binary
• A Morphological Model to Separate Resolved-Unresolved Sources in the DESI Legacy Surveys: Application in the LS4 Alert Stream
• Survey-Wide Asteroid Discovery with a High-Performance Computing Enabled Non-Linear Digital Tracking Framework
• Ejected from home: C/1980 E1 (Bowell) and C/2024 L5 (ATLAS)
• Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors
• AT2020ohl: its nature and probable implications
• Accretion Flares from Stellar Collisions in Galactic Nuclei
• Machine Learning applications for Cataclysmic Variable discovery in the ZTF alert stream
• Machine-directed gravitational-wave counterpart discovery
• Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine
• Predictions of Imminent Earth Impactors Discovered by LSST
• Antarctic Survey Telescope 3-3: Overview, System Performance and Preliminary Observations at Yaoan, Yunnan
• A real-time search for Type Ia Supernovae with late-time CSM interaction in ZTF
• The X-ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-Driven Massive Star Explosions
• RedDots: Planetary masses in the GJ1061 system from planet-planet interaction
• Multiband analysis of the O'Connell effect in 14 eclipsing binaries
• A long-lived compact jet in the black hole X-ray binary candidate AT2019wey
• The story of SN 2021aatd -- a peculiar 1987A-like supernova with an early-phase luminosity excess
• Climate Change in Hell: Long-Term Variation in Transits of the Evaporating Planet K2-22b
• Light-curve analysis and shape models of NEAs 7335, 7822, 154244 and 159402
• (208) Lacrimosa: A case that missed the Slivan state?
• Light-curve Modelling for The Initial Rising Phase of Rapidly-evolving Transients Powered by Continuous Outflow
• Hubble Space Telescope Imaging of Luminous Extragalactic Infrared Transients and Variables from the SPIRITS Survey
• Intermediate-luminosity red transients: Spectrophotometric properties and connection to electron-capture supernova explosions
• The hydrogen-free circumstellar interaction in the Type Ib supernova 2021efd: A clue to the mechanism of the helium-layer stripping
• Insights on the Rotational State and Shape of Asteroid (203) Pompeja from TESS Photometry
• Early emission characterization of TDE 2025aarm
• Radio Variability in Recently-Quenched Galaxies: The Impact of TDE or AGN Driven Outflows
• A Tidal Disruption Event from an Intermediate-mass Black Hole Revealed by Comprehensive Multi-wavelength Observations
• Physical Characterization of Asteroid (16583) Oersted Combining Stellar Occultation and Photometric Data
• BeyonCE -- Light Curve Modelling Beyond Circular Eclipsers I. Shallot Explorer
• Circumstellar Medium Constraints on the Environment of Two Nearby Type Ia Supernovae: SN 2017cbv and SN 2020nlb
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• V4141 Sgr: Outflows and repeated outbursts
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• The ensemble broad-frequency power spectrum of Stripe-82 quasars from multiple surveys
• Matching seismic masses for RR Lyrae-type and oscillating red horizontal-branch stars in M4
• A persistent bow shock in a diskless magnetised accreting white dwarf
• Confirmation of Seven Faint ATLAS Variable Star Candidates
• A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow
• Normal or transitional? The evolution and properties of two type Ia supernovae in the Virgo cluster
• A Radio Changing-state Jet in the Narrow-line Seyfert 1 Galaxy J1105+1452
• On The Unusual Variability of 2MASS J06195260-2903592: A Long-Lived Disk around a Young Ultracool Dwarf
• Gaia20fnr: A binary-lens microlensing event with full orbital motion revealed by four space telescopes
• An X-ray and Optical Study of the Dwarf Nova Candidate OGLE-BLG-DN-0064
• Optimizing the hunt for extraterrestrial high-energy neutrino counterparts
• New Insights into Time Series Analysis IV: Panchromatic and Flux Independent Period Finding Methods
• NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists
• A MeerKAT survey of nearby dwarf novae: I. New detections
• SN 2024abvb: A Type Icn Supernova in the Outskirts of its Host Galaxy
• Constraining Lens Masses in Moderately to Highly Magnified Microlensing Events from Gaia
• Multivariate time series transformer embeddings for light curves of periodic variable stars
• Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja
• A low mass, binary-stripped envelope for the Type IIb SN 2024abfo
• Giant outbursts of clumpy material preceding Type II supernova 2024qiw
• The New Status Qvo? SN 2021qvo is Another 2003fg-like Type Ia Supernova with a Rising Light-Curve Bump
• Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility
• eROSITA-selection of new period-bounce Cataclysmic Variables: First follow-up confirmation using TESS and SDSS
• Physical properties of long-rising type II supernovae -- Bayesian analytic modeling and spectrophotometric correlations
• Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter
• IRAS 00450+7401 and the mid-infrared fade/burst cycle of R Coronae Borealis-type stars
• AT 2023prq: A Classical Nova in the Halo of the Andromeda Galaxy
• Optimizing Convolution Direction and Template Selection for Difference Image Analysis
• Discovery of a 310-day Period from the Enshrouded Massive System NaSt1 (WR 122)
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Spectroscopy of AT 2016blu's recurring supernova impostor outbursts
• Faintest of them all : ZTF 21aaoryiz/SN 2021fcg -- Discovery of an extremely low luminosity type Iax supernova
• Progenitor and Close-In Circumstellar Medium of Type II Supernova 2020fqv from High-Cadence Photometry and Ultra-Rapid UV Spectroscopy
• Smart obervation method with wide field small aperture telescopes for real time transient detection
• Early results in the search for extreme coronal line emitters with the Dark Energy Spectroscopic Instrument
• X-ray and Optical Analysis of the Prototype Polar AN UMa
• Rate of Repeating Tidal Disruption Events with 5--19 years interval
• SN 2024hpj: A perspective on SN 2009ip-like events
• SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host
• AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary
• The Solar System Notification Alert Processing System (SNAPS): Asteroid Population Outlier Detection
• Finding Fast Transients in Real Time Using Novel Light Curve Analysis Algorithm
• Spectral Analysis of New Black Hole Candidate AT2019wey Observed by NuSTAR
• A Dedicated Lunar Trojan Asteroid Survey with Small Ground-Based Telescopes
• First systematic high-precision survey of bright supernovae I. Methodology for identifying early bumps
• GPU-Enabled Searches for Periodic Signals of Unknown Shape
• Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
• The Recurrent Nova U Scorpii from the 2010.1 to 2022.4 Eruptions; the Missed Eruption of 2016.78 +- 0.10 and the Critical Complex Period Changes
• The Astronomy Commons Platform: A Deployable Cloud-Based Analysis Platform for Astronomy
• The Visual Survey Group: A Decade of Hunting Exoplanets and Unusual Stellar Events with Space-Based Telescopes
• A catalogue of Type 2 active galactic nuclei in the 6dF Galaxy Survey
• Science with a large field-of-view polarization survey: The Large Array Survey Telescope Polarization Node (LAST-P)
• Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653-1001
• Spin Parameters and Shape Models of Near-Earth Asteroids (4660) Nereus, (21088) Chelyabinsk, (66146) 1998 TU3, and (297418) 2000 SP43
• The Bochum Survey of the Southern Galactic Disk: III. Complete Data Release
• A long life of excess: The interacting transient SN 2017hcc
• WISE J005128.08+645651.7: An enigmatic R Coronae Borealis star
• Multimessenger Constraints on the Central Engine in SN 2023ixf: Neutron Star or Black Hole?
• AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission
• Refined rotational state and shape model of (98943) Torifune ahead of the Hayabusa2# flyby
• Late-time evolution of the interacting stripped-envelope supernova 2017dio
• Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves
• VarWISE: Infrared Variability via NEOWISE Single Exposure Photometry
• Multiwavelength Characterization of a New Magnetic Cataclysmic Variable 2CXO J050740.7-091337
• GRB 260310A / SN 2026fgk: A Multi-Wavelength Study of a Nearby Underluminous Long GRB and SN with a Complex Afterglow
• A Minute-Cadence Deep Bulge Survey: First Data Release of DREAMS
• Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
• VLTI-GRAVITY observations of blazars
• Probing Quasar Viewing Angle with the Variability Structure Function
• An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise
• Relative frequencies of core-collapse supernovae as a function of metallicity: observations vs theoretical predictions
• Zwicky Transient Facility and Globular Clusters: The RR Lyrae gri-Band Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity Relations
• SDSS J153231.80+420342.7: a triple black hole candidate with a close binary black hole
• SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve
• The extremely low-luminosity Type Iax SNe 2022ywf and 2023zgx
• AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events
• Variable Red Giants Exploration with MASTER Robotic Net: Main Algorithms and Study of Three Mira-type Targets
• The nearby He-rich superluminous supernova SN 2021bnw during photospheric phases
• An infrared echo from a circumstellar disk in the hydrogen- and helium-poor SN 2024aecx
• Nested, asymmetric H-He circumstellar shells in the Type Icn/Ibn SN 2024abvb