Lista de obras - Samantha Lawler - Dominio Público Uruguay

ALMA imaging of the M-dwarf Fomalhaut C’s debris disc

artículo científico publicado en 2021

ALMA observations of the debris disk of solar analog {tau} Ceti ⬇️

artículo científico publicado en 2016

Additional Keplerian Signals in the HARPS data for Gliese 667C: Further Analysis

artículo científico publicado en 2013

Bright satellites are disrupting astronomy research worldwide

artículo científico publicado en 2023

Consequences of a distant massive planet on the large semimajor axis trans-Neptunian objects ⬇️

artículo científico publicado en 2017

Details of Resonant Structures within a Nice Model Kuiper Belt: Predictions for High-perihelion TNO Detections

artículo científico publicado en 2017

Direct imaging of an asymmetric debris disk in the HD 106906 planetary system ⬇️

artículo científico publicado en 2015

Explorations beyond the snow line: Spitzer/IRS spectra of debris disks around solar-type stars ⬇️

artículo científico publicado en 2009

FOSSIL. I. The Spin Rate Limit of Jupiter Trojans

artículo científico

FOSSIL. II. The Rotation Periods of Small-sized Hilda Asteroids

artículo científico publicado en 2022

Frequency of Debris Disks around Solar‐Type Stars: First Results from aSpitzerMIPS Survey ⬇️

artículo científico publicado en 2006

Gas absorption in the KH 15D system: further evidence for dust settling in the circumbinary disk ⬇️

scientific article published in the Astrophysical Journal

Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems

scholarly article

IRS Spectra of Solar-Type Stars: A Search for Asteroid Belt Analogs ⬇️

artículo científico publicado en 2006

Locating planetesimal belts in the multiple-planet systems HD 128311, HD 202206, HD 82943, and HR 8799 ⬇️

scientific article published in the Astrophysical Journal

OSSOS III - Resonant trans-Neptunian populations: constraints from the first quarter of the outer solar system origins survey ⬇️

artículo científico publicado en 2017

OSSOS XXV: Large Populations and Scattering–Sticking in the Distant Trans-Neptunian Resonances

artículo científico publicado en 2022

OSSOS. IV. Discovery of a dwarf planet candidate in the 9:2 resonance with Neptune ⬇️

artículo científico publicado en 2016

OSSOS. IX. Two Objects in Neptune's 9:1 Resonance—Implications for Resonance Sticking in the Scattering Population

artículo científico publicado en 2018

OSSOS. VI. Striking Biases in the Detection of Large Semimajor Axis Trans-Neptunian Objects

artículo científico publicado en 2017

OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release

artículo científico publicado en 2018

OSSOS. VIII. The Transition between Two Size Distribution Slopes in the Scattering Disk

artículo científico publicado en 2018

OSSOS. XV. Probing the Distant Solar System with Observed Scattering TNOs

scientific article published on 02 July 2019

OSSOS. XVIII. Constraining Migration Models with the 2:1 Resonance Using the Outer Solar System Origins Survey

OSSOS. XXI. Collision Probabilities in the Edgeworth–Kuiper Belt

artículo científico publicado en 2021

OSSOS: The eccentricity and inclination distributions of the stable neptunian Trojans

artículo científico publicado en 2021

OSSOS: X. How to Use a Survey Simulator: Statistical Testing of Dynamical Models Against the Real Kuiper Belt

artículo científico publicado en 2018

Observational signatures of a massive distant planet on the scattering disk ⬇️

artículo científico publicado en 2016

Planets and debris disks: results from a Spitzer/MIPS search for infrared excess ⬇️

scientific article published in the Astrophysical Journal

Plaskett 1.8 m Observations of Starlink Satellites

artículo científico publicado en 2022

SATCON2 Observations Working Group Report ⬇️

report published in 2021

SONS: The JCMT legacy survey of debris discs in the submillimetre ⬇️

artículo científico publicado en 2017

Survey of nearby FGK stars at 160 {mu}m with Spitzer

artículo científico publicado en 2009

The Case for Space Environmentalism ⬇️

artículo científico publicado en 2022

The Debiased Kuiper Belt: Our Solar System as a Debris Disk

artículo científico publicado en 2013

The Structure of the Distant Kuiper Belt in a Nice Model Scenario ⬇️

artículo científico publicado en 2017

The debris disc of solar analogue τ Ceti: Herschel observations and dynamical simulations of the proposed multiplanet system ⬇️

scholarly article

The debris disk around {gamma} Doradus resolved with Herschel ⬇️

artículo científico publicado en 2012

The outer solar system origins survey. I. Design and first-quarter discoveries ⬇️

artículo científico publicado en 2016

Visibility Predictions for Near-future Satellite Megaconstellations: Latitudes near 50° Will Experience the Worst Light Pollution

scientific article published on 17 December 2021

Lista de obras de Samantha Lawler

ALMA imaging of the M-dwarf Fomalhaut C’s debris disc

ALMA observations of the debris disk of solar analog {tau} Ceti ⬇️

Additional Keplerian Signals in the HARPS data for Gliese 667C: Further Analysis

Bright satellites are disrupting astronomy research worldwide

Consequences of a distant massive planet on the large semimajor axis trans-Neptunian objects ⬇️

Details of Resonant Structures within a Nice Model Kuiper Belt: Predictions for High-perihelion TNO Detections

Direct imaging of an asymmetric debris disk in the HD 106906 planetary system ⬇️

Explorations beyond the snow line: Spitzer/IRS spectra of debris disks around solar-type stars ⬇️

FOSSIL. I. The Spin Rate Limit of Jupiter Trojans

FOSSIL. II. The Rotation Periods of Small-sized Hilda Asteroids

Frequency of Debris Disks around Solar‐Type Stars: First Results from aSpitzerMIPS Survey ⬇️

Gas absorption in the KH 15D system: further evidence for dust settling in the circumbinary disk ⬇️

Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems

IRS Spectra of Solar-Type Stars: A Search for Asteroid Belt Analogs ⬇️

Locating planetesimal belts in the multiple-planet systems HD 128311, HD 202206, HD 82943, and HR 8799 ⬇️

OSSOS III - Resonant trans-Neptunian populations: constraints from the first quarter of the outer solar system origins survey ⬇️

OSSOS XXV: Large Populations and Scattering–Sticking in the Distant Trans-Neptunian Resonances

OSSOS. IV. Discovery of a dwarf planet candidate in the 9:2 resonance with Neptune ⬇️

OSSOS. IX. Two Objects in Neptune's 9:1 Resonance—Implications for Resonance Sticking in the Scattering Population

OSSOS. VI. Striking Biases in the Detection of Large Semimajor Axis Trans-Neptunian Objects

OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release

OSSOS. VIII. The Transition between Two Size Distribution Slopes in the Scattering Disk

OSSOS. XV. Probing the Distant Solar System with Observed Scattering TNOs

OSSOS. XVIII. Constraining Migration Models with the 2:1 Resonance Using the Outer Solar System Origins Survey

OSSOS. XXI. Collision Probabilities in the Edgeworth–Kuiper Belt

OSSOS: The eccentricity and inclination distributions of the stable neptunian Trojans

OSSOS: X. How to Use a Survey Simulator: Statistical Testing of Dynamical Models Against the Real Kuiper Belt

Observational signatures of a massive distant planet on the scattering disk ⬇️

Planets and debris disks: results from a Spitzer/MIPS search for infrared excess ⬇️

Plaskett 1.8 m Observations of Starlink Satellites

SATCON2 Observations Working Group Report ⬇️

SONS: The JCMT legacy survey of debris discs in the submillimetre ⬇️

Survey of nearby FGK stars at 160 {mu}m with Spitzer

The Case for Space Environmentalism ⬇️

The Debiased Kuiper Belt: Our Solar System as a Debris Disk

The Structure of the Distant Kuiper Belt in a Nice Model Scenario ⬇️

The debris disc of solar analogue τ Ceti: Herschel observations and dynamical simulations of the proposed multiplanet system ⬇️

The debris disk around {gamma} Doradus resolved with Herschel ⬇️

The outer solar system origins survey. I. Design and first-quarter discoveries ⬇️

Visibility Predictions for Near-future Satellite Megaconstellations: Latitudes near 50° Will Experience the Worst Light Pollution