Susan M. Lederer
YOU?
Author Swipe
View article: An Ultra-hot Low-mass Brown Dwarf Eclipsing the Puffy White Dwarf J0404+1112
An Ultra-hot Low-mass Brown Dwarf Eclipsing the Puffy White Dwarf J0404+1112 Open
Most exoplanets known orbit stars that will evolve into red giants, then white dwarfs (WDs). Understanding the population of substellar WD companions informs the common-envelope evolution process (E. Villaver & M. Livio 2009), thereby shed…
View article: Hubble's Multi-Year Search for Exospheres in the TRAPPIST-1 System Reveals Frequent Microflares
Hubble's Multi-Year Search for Exospheres in the TRAPPIST-1 System Reveals Frequent Microflares Open
Ly-$α$ observations provide a powerful probe of stellar activity and atmospheric escape in exoplanetary systems. We present here an analysis of 104 HST/STIS orbits monitoring the TRAPPIST-1 system between 2017 and 2022, covering 3--5 trans…
View article: Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3
Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3 Open
View article: An Earth-sized exoplanet ripe for emission spectroscopy with JWST in orbit around a nearby ultracool dwarf star
An Earth-sized exoplanet ripe for emission spectroscopy with JWST in orbit around a nearby ultracool dwarf star Open
The JWST space telescope has the potential to measure the emission spectrum of a highly irradiated exoplanet as small as the Earth, especially if it transits a very nearby and cold star similar in size to Jupiter. Such ‘ultracool dwarf sta…
View article: Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides
Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides Open
We have collected transit times for the TRAPPIST-1 system with the Spitzer Space Telescope over four years. We add to these ground-based, HST, and K2 transit-time measurements, and revisit an N -body dynamical analysis of the seven-planet …
View article: Refining the transit timing and photometric analysis of TRAPPIST-1: Masses, radii, densities, dynamics, and ephemerides
Refining the transit timing and photometric analysis of TRAPPIST-1: Masses, radii, densities, dynamics, and ephemerides Open
We have collected transit times for the TRAPPIST-1 system with the Spitzer Space Telescope over four years. We add to these ground-based, HST and K2 transit time measurements, and revisit an N-body dynamical analysis of the seven-planet sy…
View article: data/ directory associated with https://github.com/ericagol/TRAPPIST1_Spitzer
data/ directory associated with https://github.com/ericagol/TRAPPIST1_Spitzer Open
Data directory for the repository associated with the paper "Refining the transit timing and photometric analysis of TRAPPIST-1: Masses, radii, densities, dynamics, and ephemerides."
View article: data/ directory associated with https://github.com/ericagol/TRAPPIST1_Spitzer
data/ directory associated with https://github.com/ericagol/TRAPPIST1_Spitzer Open
Data directory for the repository associated with the paper "Refining the transit timing and photometric analysis of TRAPPIST-1: Masses, radii, densities, dynamics, and ephemerides."
View article: TRAPPIST-1: Global results of the Spitzer Exploration Science Program Red Worlds★
TRAPPIST-1: Global results of the Spitzer Exploration Science Program Red Worlds★ Open
Context. With more than 1000 h of observation from Feb. 2016 to Oct. 2019, the Spitzer Exploration Program Red Worlds (ID: 13067, 13175 and 14223) exclusively targeted TRAPPIST-1, a nearby (12 pc) ultracool dwarf star, finding that it is o…
View article: NASA's Orbital Debris JAO/ES-MCAT Optical Telescope Facility on Ascension Island
NASA's Orbital Debris JAO/ES-MCAT Optical Telescope Facility on Ascension Island Open
The NASA Orbital Debris Program Office has a long-standing optical program begun over three and a half decades ago in 1984, designed to observe the Earth-orbiting environment with optical telescopes. Photometrically calibrated optical data…
View article: Ground-based follow-up observations of TRAPPIST-1 transits in the near-infrared
Ground-based follow-up observations of TRAPPIST-1 transits in the near-infrared Open
The TRAPPIST-1 planetary system is a favourable target for the atmospheric characterization of temperate earth-sized exoplanets by means of transmission spectroscopy with the forthcoming James Webb Space Telescope (JWST). A possible obstac…
View article: Disentangling the Planet from the Star in Late-Type M Dwarfs: A Case Study of TRAPPIST-1g
Disentangling the Planet from the Star in Late-Type M Dwarfs: A Case Study of TRAPPIST-1g Open
The atmospheres of late M stars represent a significant challenge in the characterization of any transiting exoplanets because of the presence of strong molecular features in the stellar atmosphere. TRAPPIST-1 is an ultracool dwarf, host t…
View article: Vis-NIR disk-integrated photometry of asteroid 25143 Itokawa around opposition by AMICA/Hayabusa
Vis-NIR disk-integrated photometry of asteroid 25143 Itokawa around opposition by AMICA/Hayabusa Open
View article: The nature of the TRAPPIST-1 exoplanets
The nature of the TRAPPIST-1 exoplanets Open
Context. The TRAPPIST-1 system hosts seven Earth-sized, temperate exoplanets orbiting an ultra-cool dwarf star. As such, it represents a remarkable setting to study the formation and evolution of terrestrial planets that formed in the same…
View article: Atmospheric reconnaissance of the habitable-zone Earth-sized planets orbiting TRAPPIST-1
Atmospheric reconnaissance of the habitable-zone Earth-sized planets orbiting TRAPPIST-1 Open
View article: Early 2017 observations of TRAPPIST-1 with Spitzer
Early 2017 observations of TRAPPIST-1 with Spitzer Open
The recently detected TRAPPIST-1 planetary system, with its seven planets transiting a nearby ultracool dwarf star, offers the first opportunity to perform comparative exoplanetology of temperate Earth-sized worlds. To further advance our …
View article: The UKIRT Hemisphere Survey: definition and J-band data release
The UKIRT Hemisphere Survey: definition and J-band data release Open
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
View article: Characterizing Non-Resolved Debris Through Spectral and Photometric Ground-Based Telescopic Data: What Can Laboratory Ground-truth Data Do for You?
Characterizing Non-Resolved Debris Through Spectral and Photometric Ground-Based Telescopic Data: What Can Laboratory Ground-truth Data Do for You? Open
NASA's ODPO has recently collected data of unresolved objects at GEO with the 3.8m UKIRT infrared telescope on Mauna Kea and the 1.3m MCAT visible telescope on Ascension Island. Analyses of SWIR data of rocket bodies and HS-376 solar-panel…
View article: Temporal evolution of the high-energy irradiation and water content of TRAPPIST-1 exoplanets
Temporal evolution of the high-energy irradiation and water content of TRAPPIST-1 exoplanets Open
The ultracool dwarf star TRAPPIST-1 hosts seven Earth-size transiting planets, some of which could harbour liquid water on their surfaces. UV observations are essential to measure their high-energy irradiation, and to search for photodisso…
View article: United Kingdom Infrared Telescope's Spectrograph Observations of Human-Made Space Objects
United Kingdom Infrared Telescope's Spectrograph Observations of Human-Made Space Objects Open
Presented here are the results of the United Kingdom Infrared Telescope (UKIRT) spectral observations of human-made space objects taken from 2014 to 2015. The data collected using the UKIRT 1-5 micron Imager Spectrometer (UIST) cover the w…
View article: A terrestrial-sized exoplanet at the snow line of TRAPPIST-1
A terrestrial-sized exoplanet at the snow line of TRAPPIST-1 Open
The TRAPPIST-1 system is the first transiting planet system found orbiting an ultra-cool dwarf star. At least seven planets similar to Earth in radius and in mass were previously found to transit this host star. Subsequently, TRAPPIST-1 wa…
View article: Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1
Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1 Open
View article: Characterization of the High-Albedo NEA 3691 Bede
Characterization of the High-Albedo NEA 3691 Bede Open
Characterization of NEAs provides important inputs to models for atmospheric entry, risk assessment and mitigation. Diameter is a key parameter because diameter translates to kinetic energy in atmospheric entry. Diameters can be derived fr…
View article: A combined transmission spectrum of the Earth-sized exoplanets TRAPPIST-1 b and c
A combined transmission spectrum of the Earth-sized exoplanets TRAPPIST-1 b and c Open
View article: Development of the NASA MCAT Auxiliary Telescope for Orbital Debris Research
Development of the NASA MCAT Auxiliary Telescope for Orbital Debris Research Open
The National Aeronautical Space Administration has deployed the Meter Class Autonomous Telescope (MCAT) to Ascension Island with plans for it to become fully operational by summer 2016. This telescope will be providing data in support of r…
View article: Temperate Earth-sized planets transiting a nearby ultracool dwarf star
Temperate Earth-sized planets transiting a nearby ultracool dwarf star Open
View article: Phase-Angle Dependence of Determinations of Diameter, Albedo, and Taxonomy: A case study of NEO 3691 Bede
Phase-Angle Dependence of Determinations of Diameter, Albedo, and Taxonomy: A case study of NEO 3691 Bede Open
Parameters important for NEO risk assessment and mitigation include Near-Earth Object diameter and taxonomic classification, which translates to surface composition. Diameters of NEOs are derived from the thermal fluxes measured by WISE, N…
View article: Characterizing Debris in the Infrared with UKIRT
Characterizing Debris in the Infrared with UKIRT Open
The United Kingdom Infrared Telescope (UKIRT) has been a major asset for the NASA Orbital Debris Program Office (OPDO) since March, 2014. With the UKIRT current contract coming to an end at the finish of FY15, there is a golden opportunity…
View article: Observing Strategies for Focused, Faint Orbital Debris Surveys Using the Magellan Telescope
Observing Strategies for Focused, Faint Orbital Debris Surveys Using the Magellan Telescope Open
A breakup of the Titan 3C-17 Transtage rocket body was reported to have occurred on June 4th, 2014 at 02:38 UT by the Space Surveillance Network (SSN). Five objects were associated with this breakup and this is the fourth breakup known for…
View article: NEAs: Phase Angle Dependence of Asteroid Class and Diameter from Observational Studies
NEAs: Phase Angle Dependence of Asteroid Class and Diameter from Observational Studies Open
We will discuss the results of a planned observation campaign of Near Earth Asteroids (NEAs), 1999 CU3, 2002 GM2, 2002 FG7, and 3691 Bede with instruments on the United Kingdom Infrared Telescope (UKIRT) from 15-Mar-2015 to 28-April 2015 U…