output
19952026
most citedThe Apache Point Observatory Galactic Evolution Experiment (APOGEE)

1.8k citations

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29 papers · 1 filter

astro-ph.SR2024★ 34 cited

Sun-like stars produce superflares roughly once per century

Valeriy Vasilyev, Timo Reinhold, Alexander I. Shapiro +7

Stellar superflares are energetic outbursts of electromagnetic radiation, similar to solar flares but releasing more energy, up to erg on main sequence stars. It is unkno…

astro-ph.EP2024★ 15 cited

Two Distinct Populations of Dark Comets Delineated by Orbits and Sizes

Darryl Z. Seligman, Davide Farnocchia, Marco Micheli +7

Small bodies are capable of delivering essential prerequisites for the development of life, such as volatiles and organics, to the terrestrial planets. For example, empirical evide…

astro-ph.IM2024★ 2 cited

Pointing Accuracy Improvements for the South Pole Telescope with Machine Learning

P. M. Chichura, A. Rahlin, A. J. Anderson +93

We present improvements to the pointing accuracy of the South Pole Telescope (SPT) using machine learning. The ability of the SPT to point accurately at the sky is limited by its s…

physics.space-ph2024★ 6 cited

Suppression of the collisionless tearing mode by flow shear: implications for reconnection onset in the Alfvénic solar wind

A. Mallet, S. Eriksson, M. Swisdak +1

We analyse the collisionless tearing mode instability of a current sheet with a strong shear flow across the layer. The growth rate decreases with increasing shear flow, and is com…

astro-ph.EP2024★ 34 cited

A giant planet transiting a 3-Myr protostar with a misaligned disk

Madyson G. Barber, Andrew W. Mann, Andrew Vanderburg +35

Astronomers have found more than a dozen planets transiting 10-40 million year old stars, but even younger transiting planets have remained elusive. A possible reason for the lack…

astro-ph.SR2024★ 1 cited

Rising Near-Ultraviolet Spectra in Stellar Megaflares

Adam F. Kowalski, Rachel A. Osten, Yuta Notsu +5

Flares from M-dwarf stars can attain energies up to times larger than solar flares but are generally thought to result from similar processes of magnetic energy release and…

astro-ph.IM2024★ 1 cited

MAUVE: An Ultraviolet Astrophysics Probe Mission Concept

Mayura Balakrishnan, Rory Bowens, Fernando Cruz Aguirre +18

We present the mission concept "Mission to Analyze the UltraViolet universE" (MAUVE), a wide-field spectrometer and imager conceived during the inaugural NASA Astrophysics Mission…

physics.space-ph2024★ 3 cited

Extent of the Magnetotail of Venus From the Solar Orbiter, Parker Solar Probe and BepiColombo Flybys

Niklas J. T. Edberg, David J. Andrews, J. Jordi Boldú +20

We analyze data from multiple flybys by the Solar Orbiter, BepiColombo, and Parker Solar Probe (PSP) missions to study the interaction between Venus' plasma environment and the sol…

astro-ph.IM2024★ 2 cited

The assembly, characterization, and performance of SISTINE

Nicholas Nell, Kevin France, Nicholas Kruczek +6

The Suborbital Imaging Spectrograph for Transition region Irradiance from Nearby Exoplanet host stars (SISTINE) is a rocket-borne ultraviolet (UV) imaging spectrograph designed to…

astro-ph.SR2024★ 3 cited

A solar rotation signature in cosmic dust: frequency analysis of dust particle impacts on the Wind spacecraft

Lennart R. Baalmann, Silvan Hunziker, Arthur Péronne +7

Dust particle impacts on the Wind spacecraft were detected with its plasma wave instrument Wind/WAVES. Frequency analysis on this dust impact time series revealed spectral peaks in…

astro-ph.EP2024★ 15 cited

High-energy spectra of LTT 1445A and GJ 486 reveal flares and activity

H. Diamond-Lowe, G. W. King, A. Youngblood +19

The high-energy radiative output, from the X-ray to the ultraviolet, of exoplanet host stars drives photochemical reactions and mass loss in the upper regions of planetary atmosphe…

astro-ph.EP2024★ 62 cited

A Benchmark JWST Near-Infrared Spectrum for the Exoplanet WASP-39b

A. L. Carter, E. M. May, N. Espinoza +77

Observing exoplanets through transmission spectroscopy supplies detailed information on their atmospheric composition, physics, and chemistry. Prior to JWST, these observations wer…

astro-ph.EP2024★ 96 cited

Sulphur dioxide in the mid-infrared transmission spectrum of WASP-39b

Diana Powell, Adina D. Feinstein, Elspeth K. H. Lee +70

The recent inference of sulphur dioxide (SO) in the atmosphere of the hot (1100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations suggests that phot…

astro-ph.EP2024★ 5 cited

Energetic proton losses reveal Io's extended and longitudinally asymmetrical atmosphere

H. L. F. Huybrighs, C. P. A. van Buchem, A. Blöcker +3

Along the I24, I27 and I31 flybys of Io (1999-2001), the Energetic Particle Detector (EPD) onboard the Galileo spacecraft observed localised regions of energetic protons losses (15…

astro-ph.SR2024★ 4 cited

Simultaneous spectropolarimetric observations in the H and Ca II 8662 Å lines of an active region

Harsh Mathur, K. Nagaraju, Rahul Yadav +1

We present spectropolarimetric observations of an active region recorded simultaneously in the H Ca II 8662 Å lines. The sunspot exhibits multiple structures, including a lightb…

astro-ph.GA2024★ 4 cited

The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM

Samantha L. Garza, Jessica K. Werk, Benjamin D. Oppenheimer +9

We present an analysis of \textit{HST}/COS/G160M observations of CIV in the inner circumgalactic medium (CGM) of a novel sample of eight z0, LL galaxies, p…

astro-ph.EP2024★ 2 cited

Interpolation and synthesis of sparse samples in exoplanet atmospheric modeling

Jacob Haqq-Misra, Eric T. Wolf, Thomas J. Fauchez +1

This paper highlights methods from geostatistics that are relevant to the interpretation, intercomparison, and synthesis of atmospheric model data, with a specific application to e…

physics.space-ph2024★ 10 cited

First direct observations of interplanetary shock impact angle effects on actual geomagnetically induced currents: The case of the Finnish natural gas pipeline system

Denny M. Oliveira, Eftyhia Zesta, Sergio Vidal-Luengo

The impact of interplanetary (IP) shocks on the Earth's magnetosphere can greatly disturb the geomagnetic field and electric currents in the magnetosphere-ionosphere system. At hig…

physics.space-ph2024★ 7 cited

Impacting the dayside Martian ionosphere from above and below: Effects of the impact of CIRs and ICMEs close to aphelion (April 2021) and during dust storms (June-July 2022) seen with MAVEN ROSE

Marianna Felici, Jennifer Segale, Paul Withers +6

We use 62 electron density profiles collected by the Radio Occultation Science Experiment (ROSE), on MAVEN, when Mars was hit by CIRs and ICMEs close to aphelion (April 2021) and d…

astro-ph.GA2024★ 2 cited

Carbon- and Oxygen-rich stars in MaStar: identification and classification

Lewis Hill, Claudia Maraston, Daniel Thomas +5

Carbon- and Oxygen-rich stars populating the Thermally-Pulsing Asymptotic Giant Branch (TP-AGB) phase of stellar evolution are relevant contributors to the spectra of ~1 Gyr old po…

astro-ph.SR2024★ 2 cited

Observations of Locally Excited Waves in the Low Solar Atmosphere Using the Daniel K. Inouye Solar Telescope (DKIST)

Shah Mohammad Bahauddin, Catherine E. Fischer, Mark P. Rast +5

We present an interpretation of the recent Daniel K. Inouye Solar Telescope (DKIST) observations of propagating wavefronts in the lower solar atmosphere. Using MPS/University of Ch…

astro-ph.SR2024★ 23 cited

Nature vs. Nurture: Distinguishing Effects from Stellar Processing and Chemical Evolution on Carbon and Nitrogen in Red Giant Stars

John D. Roberts, Marc H. Pinsonneault, Jennifer A. Johnson +16

The surface [C/N] ratios of evolved giants are strongly affected by the first dredge-up (FDU) of nuclear-processed material from stellar cores. C and N also have distinct nucleosyn…

astro-ph.SR2024★ 7 cited

Reconstruction of Polarization Properties of Whistler Waves From Two Magnetic and Two Electric Field Components: Application to Parker Solar Probe Measurements

L. Colomban, O. V. Agapitov, V. Krasnoselskikh +8

The search-coil magnetometer (SCM) aboard Parker Solar Probe (PSP) measures the 3 Hz to 1 MHz magnetic field fluctuations. During Encounter 1, the SCM operated as expected; however…

astro-ph.SR2024★ 2 cited

Stellar flares

Adam F. Kowalski

Magnetic storms on stars manifest as remarkable, randomly occurring changes of the luminosity over durations that are tiny in comparison to the normal evolution of stars. These ste…