output
19922026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

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64 papers · 1 filter

astro-ph.CO2021★ 32 cited

The DESI -body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey

Cameron Grove, Chia-Hsun Chuang, Ningombam Chandrachani Devi +19

Analysis of large galaxy surveys requires confidence in the robustness of numerical simulation methods. The simulations are used to construct mock galaxy catalogs to validate data…

astro-ph.CO2021★ 267 cited

Improved limits on the tensor-to-scalar ratio using BICEP and Planck

M. Tristram, A. J. Banday, K. M. Górski +14

We present constraints on the tensor-to-scalar ratio r using a combination of BICEP/Keck 2018 and Planck PR4 data allowing us to fit for r consistently with the six parameters of t…

astro-ph.HE2021★ 3 cited

Exploring the MeV Sky with a Combined Coded Mask and Compton Telescope: The Galactic Explorer with a Coded Aperture Mask Compton Telescope (GECCO)

Elena Orlando, Eugenio Bottacini, Alexander Moiseev +33

The sky at MeV energies is currently poorly explored. Here we present an innovative mission concept that builds on and improves past and currently proposed missions at such energie…

astro-ph.HE2021★ 32 cited

Orbital decay in M82 X-2

Matteo Bachetti, Marianne Heida, Thomas Maccarone +21

M82 X-2 is the first pulsating ultraluminous X-ray source (PULX) discovered. The luminosity of these extreme pulsars, if isotropic, implies an extreme mass transfer rate. An altern…

astro-ph.IM2021

Panoramic SETI: overall mechanical system design

Aaron M. Brown, Michael L Aronson, Shelley A. Wright +8

PANOSETI (Pulsed All-Sky Near-infrared Optical Search for Extra Terrestrial Intelligence) is a dedicated SETI (Search for Extraterrestrial Intelligence) observatory that is being d…

astro-ph.IM2021★ 3 cited

Panoramic SETI: Overall focal plane electronics and timing and network protocols

Wei Liu, Dan Werthimer, Ryan Lee +11

The PANOSETI experiment is an all-sky, all-the-time visible search for nanosecond to millisecond time-scale transients. The experiment will deploy observatory domes at several site…

astro-ph.IM2021★ 34 cited

Faint objects in motion: the new frontier of high precision astrometry

Fabien Malbet, Céline Boehm, Alberto Krone-Martins +83

Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint ob…

astro-ph.SR2021★ 27 cited

Toward Improved Understanding of Magnetic Fields Participating in Solar Flares: Statistical Analysis of Magnetic Field within Flare Ribbons

Maria D. Kazachenko, Benjamin J. Lynch, Antonia Savcheva +2

Violent solar flares and coronal mass ejections (CMEs) are magnetic phenomena. However, how magnetic fields reconnecting in the flare differ from non-flaring magnetic fields remain…

astro-ph.GA2021★ 30 cited

The Simons Observatory: Galactic Science Goals and Forecasts

Brandon S. Hensley, Susan E. Clark, Valentina Fanfani +31

Observing in six frequency bands from 27 to 280 GHz over a large sky area, the Simons Observatory (SO) is poised to address many questions in Galactic astrophysics in addition to i…

astro-ph.HE2021★ 13 cited

Unveiling the Fermi Bubbles origin with MeV photon telescopes

Michela Negro, Henrike Fleischhack, Andreas Zoglauer +2

The Fermi Bubbles (FB) are a pair of large-scale ellipsoidal structures extending above and below the Galactic plane almost symmetrically aligned with the Galactic Center. After mo…

physics.space-ph2021★ 8 cited

A Systematic Look at the Temperature Gradient Contribution to the Dayside Magnetopause Current

Jason M. H. Beedle, David J. Gershman, Vadim M. Uritsky +2

Magnetopause diamagnetic currents arise from density and temperature driven pressure gradients across the boundary layer. While theoretically recognized, the temperature contributi…

astro-ph.SR2021★ 68 cited

The In Situ Signature of Cyclotron Resonant Heating

Trevor A. Bowen, Benjmin D. G. Chandran, Jonathan Squire +9

The dissipation of magnetized turbulence is an important paradigm for describing heating and energy transfer in astrophysical environments such as the solar corona and wind; howeve…

astro-ph.SR2021★ 22 cited

Suprathermal Ion Energy spectra and Anisotropies near the Heliospheric Current Sheet crossing observed by the Parker Solar Probe during Encounter 7

M. I. Desai, D. G. Mitchell, D. J. McComas +31

We present observations of >10-100 keV/nucleon suprathermal (ST) H, He, O, and Fe ions associated with crossings of the heliospheric current sheet (HCS) at radial distances <0.1 au…

astro-ph.SR2021★ 58 cited

Strong perpendicular velocity-space in proton beams observed by Parker Solar Probe

J. L. Verniero, B. D. G. Chandran, D. E. Larson +16

The SWEAP instrument suite on Parker Solar Probe (PSP) has detected numerous proton beams associated with coherent, circularly polarized, ion-scale waves observed by PSP's FIELDS i…

astro-ph.SR2021★ 35 cited

Whistler waves observed by Solar Orbiter / RPW between 0.5 AU and 1 AU

M. Kretzschmar, T. Chust, V. Krasnoselskikh +29

The goal of our study is to detect and characterize the electromagnetic waves that can modify the electron distribution functions, with a special attention to whistler waves. We an…

astro-ph.CO2021★ 16 cited

Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods

Giuseppe Puglisi, Gueorgui Mihaylov, Georgia V. Panopoulou +4

Characterizing the sub-mm Galactic emission has become increasingly critical especially in identifying and removing its polarized contribution from the one emitted by the Cosmic Mi…

astro-ph.HE2021★ 1 cited

Spectral and Timing Analysis of NuSTAR and Swift/XRT Observations of the X-Ray Transient MAXI J0637-430

Hadar Lazar, John A. Tomsick, Sean N. Pike +10

We present results for the first observed outburst from the transient X-ray binary source MAXI J0637-430. This study is based on eight observations from the Nuclear Spectroscopic T…

astro-ph.SR2021★ 29 cited

Simulations of radio-wave anisotropic scattering to interpret type III radio bursts measurements by Solar Orbiter, Parker Solar Probe, STEREO and Wind

S. Musset, M. Maksimovic, E. Kontar +9

We use multi-spacecraft observations of invididual type III radio bursts in order to calculate the directivity of the radio emission, to be compared to the results of ray-tracing s…

astro-ph.SR2021★ 10 cited

Multiple electron acceleration instances during a series of solar microflares observed simultaneously at X-rays and microwaves

Marina Battaglia, Rohit Sharma, Yingjie Luo +3

Even small solar flares can display a surprising level of complexity regarding their morphology and temporal evolution. Many of their properties, such as energy release and electro…

astro-ph.SR2021★ 19 cited

Magnetic reconnection as a mechanism to produce multiple protonpopulations and beams locally in the solar wind

B. Lavraud, R. Kieokaew, N. Fargette +37

Context. Spacecraft observations early revealed frequent multiple proton populations in the solar wind. Decades of research on their origin have focused on processes such as magnet…

astro-ph.HE2021★ 1 cited

Study of in the COSI 2016 superpressure balloon flight

Jacqueline Beechert

The Compton Spectrometer and Imager (COSI) is a balloon-borne compact Compton telescope designed to survey the -ray sky from 0.2 to 5 MeV. COSI's wide field-of-view (FOV) and ex…

astro-ph.SR2021★ 17 cited

Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations

A. Vecchio, M. Maksimovic, V. Krupar +18

In order to allow for a comparison with the measurements from other antenna systems, the voltage power spectral density measured by the Radio and Plasma waves receiver (RPW) on boa…

astro-ph.SR2021★ 117 cited

A solar source of Alfvénic magnetic field switchbacks: {\em in situ} remnants of magnetic funnels on supergranulation scales

S. D. Bale, T. S. Horbury, M. Velli +17

One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfvénic magnetic field reversals terme…

astro-ph.SR2021★ 52 cited

Multipoint interplanetary coronal mass ejections observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind and STEREO-A

C. Möstl, A. J. Weiss, M. A. Reiss +12

We report the result of the first search for multipoint in situ and imaging observations of interplanetary coronal mass ejections (ICMEs) starting with the first Solar Orbiter (Sol…