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Solar Orbiter Radio and Plasma Waves - Time Domain Sampler: In-flight performance and first results
DOI: 10.1051/0004-6361/202140948 Bibcode: 2021A&A...656A..26S

Maksimovic, M.; Bale, S. D.; Chust, T. +20 more

Context. The Radio and Plasma Waves (RPW) instrument on board Solar Orbiter has been operating nearly continuously since the launch in February 2020. The Time Domain Sampler (TDS) receiver of the RPW instrument is dedicated to waveform measurements of plasma waves and dust impact signatures in an intermediate frequency range from 0.2 to 200 kHz. <…

2021 Astronomy and Astrophysics
SolarOrbiter 10
Hubble Frontier Field Clusters and Their Parallel Fields: Photometric and Photometric Redshift Catalogs
DOI: 10.3847/1538-4365/abea9d Bibcode: 2021ApJS..256...27P

Mobasher, Bahram; Davidzon, I.; Sánchez, F. J. +1 more

We present a multiband analysis of the six Hubble Frontier Field clusters and their parallel fields, producing catalogs with measurements of source photometry and photometric redshifts. We release these catalogs to the public along with maps of intracluster light and models for the brightest galaxies in each field. This rich data set covers a wave…

2021 The Astrophysical Journal Supplement Series
eHST 10
Low star formation efficiency due to turbulent adiabatic compression in the Taffy bridge
DOI: 10.1051/0004-6361/202037887 Bibcode: 2021A&A...647A.138V

Braine, J.; Schneider, B.; Vollmer, B. +1 more

The Taffy system (UGC 12914/15) consists of two massive spiral galaxies that had a head-on collision about 20 Myr ago. It represents an ideal laboratory for studying the reaction of the interstellar medium (ISM) to a high-speed (∼1000 km s−1) gas-gas collision. New sensitive, high-resolution (2.7″ or ∼800 pc) CO(1−0) observations of the…

2021 Astronomy and Astrophysics
eHST 10
The Eris/Dysnomia system I: The orbit of Dysnomia
DOI: 10.1016/j.icarus.2020.114130 Bibcode: 2021Icar..35514130H

Buie, M. W.; Grundy, W. M.; Holler, B. J. +1 more

We present new results on the Eris/Dysnomia system including analysis of new images from the WFC3 instrument on the Hubble Space Telescope (HST). Seven HST orbits were awarded to program 15171 in January and February 2018, with the intervals between observations selected to sample Dysnomia over a full orbital period. Using relative astrometry of E…

2021 Icarus
eHST 10
Peeking Between the Pulses: The Far-UV Spectrum of the Previously Unseen White Dwarf in AR Scorpii
DOI: 10.3847/1538-4357/abd4db Bibcode: 2021ApJ...908..195G

Garnavich, Peter; Littlefield, Colin; Lyutikov, Maxim +1 more

The compact object in the interacting binary AR Sco has widely been presumed to be a rapidly rotating, magnetized white dwarf (WD), but it has never been detected directly. Isolating its spectrum has proven difficult because the spin-down of the WD generates pulsed synchrotron radiation that far outshines the WD's photosphere. As a result, a previ…

2021 The Astrophysical Journal
eHST 10
An XMM-Newton study of active-inactive galaxy pairs
DOI: 10.1093/mnras/stab808 Bibcode: 2021MNRAS.504..393G

Guainazzi, Matteo; Paragi, Zsolt; Bianchi, Stefano +8 more

While theory and simulations indicate that galaxy mergers play an important role in the cosmological evolution of accreting black holes and their host galaxies, samples of active galactic nuclei (AGNs) in galaxies at close separations are still small. In order to increase the sample of AGN pairs, we undertook an archival project to investigate the…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 10
A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event
DOI: 10.3847/1538-4357/abde34 Bibcode: 2021ApJ...909..102B

Riddle, Reed; Stern, Daniel; Gezari, Suvi +9 more

We present the discovery of a luminous X-ray transient, serendipitously detected by Swift's X-ray Telescope on 2020 February 5, located in the nucleus of the galaxy SDSS J143359.16+400636.0 at z = 0.099 (luminosity distance DL = 456 Mpc). The transient was observed to reach a peak luminosity of ∼1044 erg s-1 in the…

2021 The Astrophysical Journal
Gaia 10
Magnetic Field Reconstruction for a Realistic Multi-Point, Multi-Scale Spacecraft Observatory
DOI: 10.3389/fspas.2021.727076 Bibcode: 2021FrASS...8..144B

Klein, K. G.; Verscharen, D.; Roberts, O. W. +3 more

Future in situ space plasma investigations will likely involve spatially distributed observatories comprised of multiple spacecraft, beyond the four and five spacecraft configurations currently in operation. Inferring the magnetic field structure across the observatory, and not simply at the observation points, is a necessary step towards characte…

2021 Frontiers in Astronomy and Space Sciences
Cluster 10
Spectrophotometric properties of materials observed by Pancam on the Mars Exploration Rovers: 4. Final mission observations
DOI: 10.1016/j.icarus.2020.114261 Bibcode: 2021Icar..35714261J

Johnson, Jeffrey R.; Grundy, William M.; Lemmon, Mark T. +4 more

The last sets of Panoramic Camera (Pancam) visible/near-infrared (432-1009 nm) multispectral observations made under varying viewing and illumination geometries by the Mars Exploration Rovers Spirit and Opportunity were examined using radiative transfer models to study the surface scattering and microphysical nature of rock and soil units at both …

2021 Icarus
MEx 10
FORCAST Imaging of Two Small Nearby Clusters: The Coronet and B 59
DOI: 10.3847/1538-4357/ac133d Bibcode: 2021ApJ...920....7S

Vacca, William D.; Reipurth, Bo; Sandell, Göran +1 more

We present mid-infrared imaging of two young clusters, the Coronet in the CrA cloud core and B 59 in the Pipe Nebula, using the FORCAST camera on the Stratospheric Observatory for Infrared Astronomy. We also analyze Herschel Space Observatory4 PACS and SPIRE images of the associated clouds. The two clusters are at similar, and very clos…

2021 The Astrophysical Journal
Herschel 10