papers

Publications (36)

astro-ph.EP2025

SO2, silicate clouds, but no CH4 detected in a warm Neptune

Achrene Dyrek, Michiel Min, Leen Decin +44

WASP-107b is a warm (~740 K) transiting planet with a Neptune-like mass of ~30.5 Earth masses and Jupiter-like radius of ~0.94 Jupiter radius, whose extended atmosphere is eroding.…

astro-ph.EP2023

15NH3 in the atmosphere of a cool brown dwarf

David Barrado, Paul Mollière, Polychronis Patapis +40

Brown dwarfs serve as ideal laboratories for studying the atmospheres of giant exoplanets on wide orbits as the governing physical and chemical processes in them are nearly identic…

astro-ph.IM2020

The nature of point source fringes in mid-infrared spectra acquired with the James Webb Space Telescope

Ioannis Argyriou, Martyn Wells, Alistair Glasse +10

The constructive and destructive interference in different layers of the James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) detector arrays modulate the detected sign…

astro-ph.EP2012

Surface Properties of Asteroids from Mid-Infrared Observations and Thermophysical Modeling

Michael Mueller

The subject of this work is the physical characterization of asteroids, focusing on the thermal inertia of near-Earth asteroids (NEAs). Thermal inertia governs the Yarkovsky effect…

astro-ph.EP2022

Exogenous delivery of water to Mercury

Kateryna Frantseva, David Nesvorný, Michael Mueller +3

Radar and spacecraft observations show the permanently shadowed regions around Mercury's North Pole to contain water ice and complex organic material. One possible source of this m…

astro-ph.EP2009

Eclipsing Binary Trojan Asteroid Patroclus: Thermal Inertia from Spitzer Observations

Michael Mueller, Franck Marchis, Joshua P. Emery +5

We present mid-infrared (8-33 micron) observations of the binary L5-Trojan system (617) Patroclus-Menoetius before, during, and after two shadowing events, using the Infrared Spect…

astro-ph.IM2016

The Astropy Problem

Demitri Muna, Michael Alexander, Alice Allen +151

The Astropy Project (http://astropy.org) is, in its own words, "a community effort to develop a single core package for Astronomy in Python and foster interoperability between Pyth…

astro-ph.EP2020

Spitzer's Solar System studies of asteroids, planets and the zodiacal cloud

David Trilling, Carey Lisse, Dale P. Cruikshank +13

In its 16 years of scientific measurements, the Spitzer Space Telescope performed a number of ground-breaking infrared measurements of Solar System objects. In this second of two p…

astro-ph.EP2016

NEOSurvey 1: Initial results from the Warm Spitzer Exploration Science Survey of Near Earth Object Properties

David E. Trilling, Michael Mommert, Joseph Hora +6

Near Earth Objects (NEOs) are small Solar System bodies whose orbits bring them close to the Earth's orbit. We are carrying out a Warm Spitzer Cycle 11 Exploration Science program…

math.AG2025

Reverse Hurwitz counts of genus 1 curves

Michael Mueller

In this paper, we study a problem that is in a sense a reversal of the Hurwitz counting problem. The Hurwitz problem asks: for a generic target -- with a list of

astro-ph.IM2023

The Science Performance of JWST as Characterized in Commissioning

Jane Rigby, Marshall Perrin, Michael McElwain +623

This paper characterizes the actual science performance of the James Webb Space Telescope (JWST), as determined from the six month commissioning period. We summarize the performanc…

astro-ph.EP2012

Physical characterization and origin of binary near-Earth asteroid (175706) 1996 FG3

Kevin J. Walsh, Marco Delbo, Michael Mueller +2

The near-Earth asteroid (NEA) (175706) 1996 FG3 is a particularly interesting spacecraft target: a binary asteroid with a low-DeltaV heliocentric orbit. The orbit of its satellite…

astro-ph2007

Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect

Marco Delbo, Aldo Dell'oro, Alan W. Harris +2

Thermal inertia determines the temperature distribution over the surface of an asteroid and therefore governs the magnitude the Yarkovsky effect. The latter causes gradual drifting…

astro-ph.EP2015

Physical Characterization of TNOs with JWST

Alex Parker, Noemi Pinilla-Alonso, Pablo Santos-Sanz +14

Studies of the physical properties of Trans-Neptunian Objects (TNOs) are a powerful probe into the processes of planetesimal formation and solar system evolution. JWST will provide…

astro-ph.EP2015

Observing Near-Earth Objects with the James Webb Space Telescope

Cristina A. Thomas, Paul Abell, Julie Castillo-Rogez +6

The James Webb Space Telescope (JWST) has the potential to enhance our understanding of near-Earth objects (NEOs). We present results of investigations into the observability of NE…

physics.optics2022

Gas-plasma based generation of broadband THz radiation with 640 mW average power

Joachim Buldt, Henning Stark, Michael Mueller +3

We present a high-power source of broadband terahertz radiation covering the whole THz spectral region (0.1-30 THz). The two-color gas plasma generation process is driven by a stat…

astro-ph.IM2023

JWST MIRI flight performance: The Medium-Resolution Spectrometer

Ioannis Argyriou, Alistair Glasse, David R. Law +22

The Medium-Resolution Spectrometer (MRS) provides one of the four operating modes of the Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope (JWST). The MRS is a…

astro-ph.IM2021

BayesicFitting, a PYTHON Toolbox for Bayesian Fitting and Evidence Calculation

Do Kester, Michael Mueller

BayesicFitting is a comprehensive, general-purpose toolbox for simple and standardized model fitting. Its fitting options range from simple least-squares methods, via maximum likel…

astro-ph.EP2013

The Discovery of Cometary Activity in Near-Earth Asteroid (3552) Don Quixote

Michael Mommert, Joseph L. Hora, Alan W. Harris +8

The near-Earth object (NEO) population, which mainly consists of fragments from collisions between asteroids in the main asteroid belt, is thought to include contributions from sho…

astro-ph.IM2023

Observations of the Planetary Nebula SMP LMC 058 with the JWST MIRI Medium Resolution Spectrometer

O. C. Jones, J. Álvarez-Márquez, G. C. Sloan +21

During the commissioning of {\em JWST}, the Medium-Resolution Spectrometer (MRS) on the Mid-Infrared Instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magell…

astro-ph.EP2018

Infrared Lightcurves of Near Earth Objects

Joseph L. Hora, Amir Siraj, Michael Mommert +9

We present lightcurves and derive periods and amplitudes for a subset of 38 near earth objects (NEOs) observed at 4.5 microns with the IRAC camera on the the Spitzer Space Telescop…

quant-ph1998

Product rule for gauge invariant Weyl symbols and its application to the semiclassical description of guiding center motion

Michael Mueller

We derive a product rule for gauge invariant Weyl symbols which provides a generalization of the well-known Moyal formula to the case of non-vanishing electromagnetic fields. Apply…

astro-ph.IM2026

ngVLTI: Cost and Feasibility of a Four-Telescope VLTI Expansion for Milliarcsecond-Scale Imaging

Sylvestre Lacour, Johan Kosmalski, Michael Mueller +8

The paper evaluates the technical design and cost feasibility of adding four 8 m-class unit telescopes to the VLTI, presenting a compact segmented‑mirror concept and a rough €80 M…

#optical interferometry#telescope design#segmented mirrors#cost analysis
astro-ph.EP2015

Asteroid thermophysical modeling

Marco Delbo, Michael Mueller, Joshua P. Emery +2

The field of asteroid thermophysical modeling has experienced an extraordinary growth in the last ten years, as new thermal infrared data became available for hundreds of thousands…

astro-ph.EP2013

Physical Characterization of Warm Spitzer-observed Near-Earth Objects

Cristina A. Thomas, Joshua P. Emery, David E. Trilling +3

Near-infrared spectroscopy of Near-Earth Objects (NEOs) connects diagnostic spectral features to specific surface mineralogies. The combination of spectroscopy with albedos and dia…

astro-ph.EP2011

ExploreNEOs III: Physical characterization of 65 low-deltaV NEOs

Michael Mueller, M. Delbo', J. L. Hora +14

Space missions to NEOs are being planned at all major space agencies, and recently a manned mission to an NEO was announced as a NASA goal. Efforts to find and select suitable targ…

astro-ph.SR2023

MINDS. The detection of CO with JWST-MIRI indicates abundant CO in a protoplanetary disk

Sierra L. Grant, Ewine F. van Dishoeck, Benoît Tabone +43

We present JWST-MIRI MRS spectra of the protoplanetary disk around the low-mass T Tauri star GW Lup from the MIRI mid-INfrared Disk Survey (MINDS) GTO program. Emission from $^{12}…

physics.optics2022

The scaling potential of beam-splitter-based coherent beam combination

Michael Mueller, Christopher Aleshire, Joachim Buldt +4

The impact of nonlinear refraction and residual absorption on the achievable peak and average power in beam-splitter-based coherent beam combination is analyzed theoretically. Whil…

physics.optics2021

Temporal contrast enhancement of energeticlaser pulses by filtered self-phase-modulation broadened spectra

Joachim Buldt, Michael Mueller, Robert Klas +3

We present a novel approach for temporal contrast enhancement of energetic laserpulses by filtered SPM broadened spectra. A measured temporal contrast enhancement by at least 7 ord…

physics.optics2022

Multipass cell for high-power few-cycle compression

Michael Mueller, Joachim Buldt, Henning Stark +2

A multipass cell for nonlinear compression to few-cycle pulse duration is introduced comprising dielectrically enhanced silver mirrors on silicon substrates. Spectral broadening wi…

astro-ph.EP2010

The Dust Trail of Comet 67P/Churyumov-Gerasimenko between 2004 and 2006

Jessica Agarwal, Michael Mueller, William T. Reach +3

We report on observations of the dust trail of comet 67P/Churyumov-Gerasimenko (CG) in visible light with the Wide Field Imager at the ESO/MPG 2.2m telescope at 4.7 AU before aphel…

astro-ph.EP2023

MINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRI

Danny Gasman, Ewine F. van Dishoeck, Sierra L. Grant +41

MIRI/MRS on board the JWST allows us to probe the inner regions of protoplanetary disks. Here we examine the disk around the classical T Tauri star Sz 98, which has an unusually la…

astro-ph.IM2023

Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST

Jeroen Bouwman, Sarah Kendrew, Thomas P. Greene +21

We present here the first ever mid-infrared spectroscopic time series observation of the transiting exoplanet \object{L 168-9 b} with the Mid-Infrared Instrument (MIRI) on the Jame…

astro-ph.EP2010

Dust Environment Modelling of Comet 67P/Churyumov-Gerasimenko

Jessica Agarwal, Michael Mueller, Eberhard Gruen

Dust is an important constituent in cometary comae; its analysis is one of the major objectives of ESA's Rosetta mission to comet 67P/Churyumov-Gerasimenko (C-G). Several instrumen…

astro-ph.EP2023

The Chemical Inventory of the Inner Regions of Planet-forming Disks -- The JWST/MINDS Program

Inga Kamp, Thomas Henning, Aditya M. Arabhavi +40

The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-formi…

astro-ph.EP2018

Delivery of organics to Mars through asteroid and comet impacts

Kateryna Frantseva, Michael Mueller, Inge Loes ten Kate +2

Given rapid photodissociation and photodegradation, the recently discovered organics in the Martian subsurface and atmosphere were probably delivered in geologically recent times.…