Electrons in the Young Solar Wind: First Results from the Parker Solar Probe. (arXiv:1912.02216v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Halekas_J/0/1/0/all/0/1">J. S. Halekas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Whittlesey_P/0/1/0/all/0/1">P. Whittlesey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Larson_D/0/1/0/all/0/1">D. E. Larson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+McGinnis_D/0/1/0/all/0/1">D. McGinnis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Maksimovic_M/0/1/0/all/0/1">M. Maksimovic</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Berthomier_M/0/1/0/all/0/1">M. Berthomier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kasper_J/0/1/0/all/0/1">J. C. Kasper</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Case_A/0/1/0/all/0/1">A. W. Case</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Korreck_K/0/1/0/all/0/1">K. E. Korreck</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stevens_M/0/1/0/all/0/1">M. L. Stevens</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Klein_K/0/1/0/all/0/1">K. G. Klein</a>, […]

Simulated Direct Imaging Detection of Water Vapor For Exo-Earths. (arXiv:1912.02228v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Ross_A/0/1/0/all/0/1">Anna Sage Ross</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Robinson_T/0/1/0/all/0/1">Tyler D. Robinson</a> Habitable planets are often defined as terrestrial worlds capable of maintaining surface liquid water. As a result, atmospheric water vapor can be a critical indicator of habitability. Thus, habitability-themed exoplanet investigations emphasize detection of water vapor […]

The East Asian Observatory SCUBA–2 survey of the COSMOS field: unveiling 1147 bright sub-millimeter sources across 2.6 square degrees. (arXiv:1912.02229v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Simpson_J/0/1/0/all/0/1">J. M. Simpson</a> (EACOA: ASIAA), <a href="http://arxiv.org/find/astro-ph/1/au:+Smail_I/0/1/0/all/0/1">Ian Smail</a> (Durham University), <a href="http://arxiv.org/find/astro-ph/1/au:+Swinbank_A/0/1/0/all/0/1">A. M. Swinbank</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chapman_S/0/1/0/all/0/1">S. C. Chapman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_C/0/1/0/all/0/1">Chian-Chou Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Geach_J/0/1/0/all/0/1">J. E. Geach</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Matsuda_Y/0/1/0/all/0/1">Y. Matsuda</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_R/0/1/0/all/0/1">R. Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_W/0/1/0/all/0/1">Wei-Hao […]

Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A. (arXiv:1912.02234v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Ono_M/0/1/0/all/0/1">Masaomi Ono</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nagataki_S/0/1/0/all/0/1">Shigehiro Nagataki</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ferrand_G/0/1/0/all/0/1">Gilles Ferrand</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Takahashi_K/0/1/0/all/0/1">Koh Takahashi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Umeda_H/0/1/0/all/0/1">Hideyuki Umeda</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yoshida_T/0/1/0/all/0/1">Takashi Yoshida</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Orlando_S/0/1/0/all/0/1">Salvatore Orlando</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Miceli_M/0/1/0/all/0/1">Marco Miceli</a> We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing […]

Streaming Classification of Variable Stars. (arXiv:1912.02235v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Zorich_L/0/1/0/all/0/1">Lukas Zorich</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pichara_K/0/1/0/all/0/1">Karim Pichara</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Protopapas_P/0/1/0/all/0/1">Pavlos Protopapas</a> In the last years, automatic classification of variable stars has received substantial attention. Using machine learning techniques for this task has proven to be quite useful. Typically, machine learning classifiers used for this task require to have a fixed […]

The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates. (arXiv:1912.02238v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Krefting_N/0/1/0/all/0/1">Nick Krefting</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sajina_A/0/1/0/all/0/1">Anna Sajina</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lacy_M/0/1/0/all/0/1">Mark Lacy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nyland_K/0/1/0/all/0/1">Kristina Nyland</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Farrah_D/0/1/0/all/0/1">Duncan Farrah</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Darvish_B/0/1/0/all/0/1">Behnam Darvish</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Duivenvoorden_S/0/1/0/all/0/1">Steven Duivenvoorden</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Duncan_K/0/1/0/all/0/1">Ken Duncan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gonzalez_Perez_V/0/1/0/all/0/1">Violeta Gonzalez-Perez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lagos_C/0/1/0/all/0/1">Claudia del P. Lagos</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Oliver_S/0/1/0/all/0/1">Seb Oliver</a>, <a […]

Magnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter. (arXiv:1912.02244v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Badman_S/0/1/0/all/0/1">Samuel T. Badman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bale_S/0/1/0/all/0/1">Stuart D. Bale</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Oliveros_J/0/1/0/all/0/1">Juan C. Martinez Oliveros</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Panasenco_O/0/1/0/all/0/1">Olga Panasenco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Velli_M/0/1/0/all/0/1">Marco Velli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stansby_D/0/1/0/all/0/1">David Stansby</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Buitrago_Casas_J/0/1/0/all/0/1">Juan C. Buitrago-Casas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Reville_V/0/1/0/all/0/1">Victor Reville</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bonnell_J/0/1/0/all/0/1">John W. Bonnell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Case_A/0/1/0/all/0/1">Anthony W. […]

Microlensing and Photon Bunching: The impact of decoherence. (arXiv:1912.02246v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Lewis_G/0/1/0/all/0/1">Geraint F. Lewis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tuthill_P/0/1/0/all/0/1">Peter Tuthill</a> Gravitational microlensing within the Galaxy offers the prospect of probing the details of distant stellar sources, as well as revealing the distribution of compact (and potentially non-luminous) masses along the line-of-sight. Recently, it has been suggested that additional […]

WISPR Imaging of a Pristine CME. (arXiv:1912.02255v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Hess_P/0/1/0/all/0/1">Phillip Hess</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rouillard_A/0/1/0/all/0/1">Alexis Rouillard</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kouloumvakos_A/0/1/0/all/0/1">Athanasios Kouloumvakos</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liewer_P/0/1/0/all/0/1">Paulett C. Liewer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_J/0/1/0/all/0/1">Jie Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dhakal_S/0/1/0/all/0/1">Suman Dhakal</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stenborg_G/0/1/0/all/0/1">Guillermo Stenborg</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Colaninno_R/0/1/0/all/0/1">Robin C. Colaninno</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Howard_R/0/1/0/all/0/1">Russell A. Howard</a> The Wide-field Imager for Solar Probe (WISPR) on board the Parker Solar Probe (PSP) observed a CME […]

A Catalog of Emission-Line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation. (arXiv:1912.02261v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Pharo_J/0/1/0/all/0/1">John Pharo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Malhotra_S/0/1/0/all/0/1">Sangeeta Malhotra</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rhoads_J/0/1/0/all/0/1">James E. Rhoads</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pirzkal_N/0/1/0/all/0/1">Norbert Pirzkal</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Finkelstein_S/0/1/0/all/0/1">Steven L. Finkelstein</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ryan_R/0/1/0/all/0/1">Russell Ryan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cimatti_A/0/1/0/all/0/1">Andrea Cimatti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Christensen_L/0/1/0/all/0/1">Lise Christensen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hathi_N/0/1/0/all/0/1">Nimish Hathi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Koekemoer_A/0/1/0/all/0/1">Anton Koekemoer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Harish_S/0/1/0/all/0/1">Santosh Harish</a>, <a […]

A New Likely Redback Millisecond Pulsar Binary with a Massive Neutron Star: 4FGL J2333.1–5527. (arXiv:1912.02264v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Swihart_S/0/1/0/all/0/1">Samuel J. Swihart</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Strader_J/0/1/0/all/0/1">Jay Strader</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Urquhart_R/0/1/0/all/0/1">Ryan Urquhart</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Orosz_J/0/1/0/all/0/1">Jerome A. Orosz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shishkovsky_L/0/1/0/all/0/1">Laura Shishkovsky</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chomiuk_L/0/1/0/all/0/1">Laura Chomiuk</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Salinas_R/0/1/0/all/0/1">Ricardo Salinas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aydi_E/0/1/0/all/0/1">Elias Aydi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dage_K/0/1/0/all/0/1">Kristen C. Dage</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kawash_A/0/1/0/all/0/1">Adam M. Kawash</a> We present the discovery of […]

Signatures of Clouds in Hot Jupiter Atmospheres: Modeled High Resolution Emission Spectra from 3D General Circulation Models. (arXiv:1912.02268v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Harada_C/0/1/0/all/0/1">Caleb K. Harada</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kempton_E/0/1/0/all/0/1">Eliza M.-R. Kempton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rauscher_E/0/1/0/all/0/1">Emily Rauscher</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Roman_M/0/1/0/all/0/1">Michael Roman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brinjikji_M/0/1/0/all/0/1">Marah Brinjikji</a> Observations of scattered light and thermal emission from hot Jupiter exoplanets have suggested the presence of inhomogeneous aerosols in […]

Global-scale Observations and Modeling of Far-Ultraviolet Airglow During Twilight. (arXiv:1912.02271v1 [physics.space-ph]) <a href="http://arxiv.org/find/physics/1/au:+Solomon1_S/0/1/0/all/0/1">Stanley C. Solomon1</a>, <a href="http://arxiv.org/find/physics/1/au:+Andersson_L/0/1/0/all/0/1">Laila Andersson</a>, <a href="http://arxiv.org/find/physics/1/au:+Burns_A/0/1/0/all/0/1">Alan G. Burns</a>, <a href="http://arxiv.org/find/physics/1/au:+Eastes_R/0/1/0/all/0/1">Richard W. Eastes</a>, <a href="http://arxiv.org/find/physics/1/au:+Martinis_C/0/1/0/all/0/1">Carlos Martinis</a>, <a href="http://arxiv.org/find/physics/1/au:+McClintock_W/0/1/0/all/0/1">William E. McClintock</a>, <a href="http://arxiv.org/find/physics/1/au:+Richmond_A/0/1/0/all/0/1">Arthur D. Richmond</a> The NASA Global-scale Observations of the Limb and Disk (GOLD) ultraviolet imaging spectrograph performs observations of upper-atmosphere airglow […]

O2- and CO-Rich Atmospheres for Potentially Habitable Environments on TRAPPIST-1 Planets. (arXiv:1912.02313v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Hu_R/0/1/0/all/0/1">Renyu Hu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Peterson_L/0/1/0/all/0/1">Luke Peterson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wolf_E/0/1/0/all/0/1">Eric T. Wolf</a> Small exoplanets of nearby M dwarf stars present the possibility to find and characterize habitable worlds within the next decade. TRAPPIST-1, an ultracool M dwarf star, was recently found to have seven […]

Hi-C 2.1 Observations of Small-Scale Miniature-Filament-Eruption-Like Cool Ejections in Active Region Plage. (arXiv:1912.02319v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Sterling_A/0/1/0/all/0/1">Alphonse C. Sterling</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moore_R/0/1/0/all/0/1">Ronald L. Moore</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Panesar_N/0/1/0/all/0/1">Navdeep K. Panesar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Reardon_K/0/1/0/all/0/1">Kevin P. Reardon</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Molnar_M/0/1/0/all/0/1">Momchil Molnar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rachmeler_L/0/1/0/all/0/1">Laurel A. Rachmeler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Savage_S/0/1/0/all/0/1">Sabrina L. Savage</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Winebarger_A/0/1/0/all/0/1">Amy R. Winebarger</a> We examine 172 Ang ultra-high-resolution images of a solar plage […]

Distribution and Energy Balance of Pluto’s Nitrogen Ice, as seen by New Horizons in 2015. (arXiv:1912.02333v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Lewis_B/0/1/0/all/0/1">Briley Lewis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stansberry_J/0/1/0/all/0/1">John Stansberry</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Holler_B/0/1/0/all/0/1">Bryan Holler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Grundy_W/0/1/0/all/0/1">William Grundy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schmitt_B/0/1/0/all/0/1">Bernard Schmitt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Protopapa_S/0/1/0/all/0/1">Silvia Protopapa</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lisse_C/0/1/0/all/0/1">Carey Lisse</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stern_S/0/1/0/all/0/1">S. Alan Stern</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Young_L/0/1/0/all/0/1">Leslie Young</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Weaver_H/0/1/0/all/0/1">Harold Weaver</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Olkin_C/0/1/0/all/0/1">Catherine Olkin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ennico_K/0/1/0/all/0/1">Kimberly Ennico</a>, the […]

Cold giant planets evaporated by hot white dwarfs. (arXiv:1912.02345v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Schreiber_M/0/1/0/all/0/1">Matthias R. Schreiber</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gaensicke_B/0/1/0/all/0/1">Boris T. Gaensicke</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Toloza_O/0/1/0/all/0/1">Odette Toloza</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hernandez_M/0/1/0/all/0/1">Mercedes-S. Hernandez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lagos_F/0/1/0/all/0/1">Felipe Lagos</a> Atmospheric escape from close-in Neptunes and hot Jupiters around sun-like stars driven by extreme ultraviolet (EUV) irradiation plays an important role in the evolution of exo-planets and in […]

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere. (arXiv:1912.02348v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_C/0/1/0/all/0/1">C. H. K. Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bale_S/0/1/0/all/0/1">S. D. Bale</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bonnell_J/0/1/0/all/0/1">J. W. Bonnell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Borovikov_D/0/1/0/all/0/1">D. Borovikov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bowen_T/0/1/0/all/0/1">T. A. Bowen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burgess_D/0/1/0/all/0/1">D. Burgess</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Case_A/0/1/0/all/0/1">A. W. Case</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chandran_B/0/1/0/all/0/1">B. D. G. Chandran</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wit_T/0/1/0/all/0/1">T. Dudok de Wit</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Goetz_K/0/1/0/all/0/1">K. Goetz</a>, <a […]

Identification of Magnetic Flux Ropes from Parker Solar Probe Observations during the First Encounter. (arXiv:1912.02349v1 [physics.space-ph]) <a href="http://arxiv.org/find/physics/1/au:+Zhao_L/0/1/0/all/0/1">L.-L. Zhao</a>, <a href="http://arxiv.org/find/physics/1/au:+Zank_G/0/1/0/all/0/1">G. P. Zank</a>, <a href="http://arxiv.org/find/physics/1/au:+Adhikari_L/0/1/0/all/0/1">L. Adhikari</a>, <a href="http://arxiv.org/find/physics/1/au:+Hu_Q/0/1/0/all/0/1">Q. Hu</a>, <a href="http://arxiv.org/find/physics/1/au:+Kasper_J/0/1/0/all/0/1">J. C. Kasper</a>, <a href="http://arxiv.org/find/physics/1/au:+Bale_S/0/1/0/all/0/1">S. D. Bale</a>, <a href="http://arxiv.org/find/physics/1/au:+Korreck_K/0/1/0/all/0/1">K. E. Korreck</a>, <a href="http://arxiv.org/find/physics/1/au:+Case_A/0/1/0/all/0/1">A. W. Case</a>, <a href="http://arxiv.org/find/physics/1/au:+Stevens_M/0/1/0/all/0/1">M. Stevens</a>, <a href="http://arxiv.org/find/physics/1/au:+Bonnell_J/0/1/0/all/0/1">J. W. Bonnell</a>, <a href="http://arxiv.org/find/physics/1/au:+Wit_T/0/1/0/all/0/1">T. Dudok […]

A Linear Formation Flying Astronomical Interferometer in Low Earth Orbit. (arXiv:1912.02350v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Hansen_J/0/1/0/all/0/1">Jonah T. Hansen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ireland_M/0/1/0/all/0/1">Michael J. Ireland</a> Space interferometry is the inevitable endpoint of high angular resolution astrophysics, and a key technology that can be leveraged to analyse exoplanet formation and atmospheres with exceptional detail. However, the anticipated cost of large missions […]