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Signal Synchronization Strategies and Time Domain SETI with Gaia DR3
DOI: 10.3847/1538-3881/acde79 Bibcode: 2023AJ....166...79N

Davenport, James R. A.; Siemion, Andrew P. V.; Croft, Steve +1 more

Spatiotemporal techniques for signal coordination with actively transmitting extraterrestrial civilizations, without the need for prior communication, can constrain technosignature searches to a significantly smaller coordinate space. With the variable star catalog from Gaia Data Release 3, we explore two related signaling strategies: the SETI Ell…

2023 The Astronomical Journal
Gaia 3
A Geologic Map of Vesta Produced Using a Hybrid Method for Incorporating Spectroscopic and Morphologic Data
DOI: 10.3847/PSJ/acebe9 Bibcode: 2023PSJ.....4..157A

Williams, David A.; Aileen Yingst, R.; Berman, Daniel C. +3 more

We have constructed a global geologic map of the minor planet Vesta at 1:300,000-scale using Dawn spacecraft imaging, spectroscopic, topographic, and elemental data. In this effort, we used a mapping method that requires creating two maps independently: the first map uses morphology and topography to define map units, while the second map relies o…

2023 The Planetary Science Journal
eHST 3
The SSA22 H I Tomography Survey (SSA22-HIT). I. Data Set and Compiled Redshift Catalog
DOI: 10.3847/1538-3881/acb707 Bibcode: 2023AJ....165..208M

Ouchi, Masami; Hennawi, Joseph F.; Inoue, Akio K. +16 more

We conducted a deep spectroscopic survey, named SSA22-HIT, in the SSA22 field with the DEep Imaging MultiObject Spectrograph (DEIMOS) on the Keck telescope, designed to tomographically map high-z H I gas through analysis of Lyα absorption in background galaxies' spectra. In total, 198 galaxies were spectroscopically confirmed at 2.5 < z < 6 …

2023 The Astronomical Journal
eHST 3
Refining Orbits of Bright Binary Systems
DOI: 10.3390/galaxies11010008 Bibcode: 2023Galax..11....8M

Miroshnichenko, Anatoly S.; Danford, Stephen; Andronov, Ivan L. +3 more

We obtained spectra of several bright binary systems (ζ02 UMa, 2 Lac, and ϕ Aql), which were mostly observed with photographic plates and whose orbits were not determined very accurately. Each system was monitored for a few years with the 81-cm telescope equipped with an échelle spectrograph at the Three College Observatory in North Carolina. The …

2023 Galaxies
Gaia 3
Lower-ionosphere electron density and effective recombination coefficients from multi-instrument space observations and ground VLF measurements during solar flares
DOI: 10.1016/j.jastp.2023.106074 Bibcode: 2023JASTP.24706074Z

Dominique, Marie; Žigman, Vida; Grubor, Davorka +2 more

A new model to predict the electron density and effective recombination coefficient of the lower ionosphere under solar flare conditions is presented. This model relies on space-borne solar irradiance measurements in coincidence with ground recorded active transmissions of Very Low Frequency (VLF), (<30 kHz) signals. Use is made of the irradian…

2023 Journal of Atmospheric and Solar-Terrestrial Physics
PROBA-2 3
The rotation period distribution in the young open cluster NGC 6709
DOI: 10.1051/0004-6361/202245441 Bibcode: 2023A&A...673A.119C

Granzer, T.; Barnes, S. A.; Weingrill, J. +1 more

Open clusters serve as a useful tool for calibrating models of the relationship between mass, rotation, and age for stars with an outer convection zone due to the homogeneity of the stars within the cluster. Cluster-to-cluster comparisons are essential to determine whether the universality of spin-down relations holds. NGC 6709

2023 Astronomy and Astrophysics
Gaia 3
Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra
DOI: 10.3847/1538-4357/acc066 Bibcode: 2023ApJ...948...16K

Kim, Seung-Lee

A star's rotation rate is difficult to estimate without surface inhomogeneities such as dark or bright spots. This paper presents asteroseismic results to determine the rotation rates of δ Sct-type pulsating primary stars in two eclipsing binary systems, AB Cas and OO Dra. After removing the binarity-induced light variations from archival TESS dat…

2023 The Astrophysical Journal
Gaia 3
Photometric variable stars in the young open cluster NGC 6823
DOI: 10.1093/mnras/stad013 Bibcode: 2023MNRAS.520.1092L

Chen, W. P.; Bhatt, B. C.; Pandey, J. C. +8 more

We present stellar variability towards the young open cluster NGC 6823. Time series V- and I-band CCD photometry led to identification and characterization of 88 variable stars, of which only 14 have been previously recognized. We ascertain the membership of each variable with optical UBVI and infrared photometry, and with Gaia EDR3 parallax and p…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
The source of electrons at comet 67P
DOI: 10.1093/mnras/stad2168 Bibcode: 2023MNRAS.525.5041S

Nilsson, H.; Goetz, C.; Henri, P. +8 more

We examine the origin of electrons in a weakly outgassing comet, using Rosetta mission data and a 3D collisional model of electrons at a comet. We have calculated a new data set of electron-impact ionization (EII) frequency throughout the Rosetta escort phase, with measurements of the Rosetta Plasma Consortium's Ion and Electron Sensor (RPC/IES). …

2023 Monthly Notices of the Royal Astronomical Society
Rosetta 3
Solar active region magnetic parameters and their relationship with the properties of halo coronal mass ejections
DOI: 10.1016/j.jastp.2023.106106 Bibcode: 2023JASTP.24906106S

Moon, Y. -J.; Shanmugaraju, A.; Ebenezer, E. +2 more

The coronal mass ejections (CMEs) from the sun consist of the plasma and strong magnetic fields (∼4-5 G at 1.3 R) and generally, the fast CMEs are often associated with energetic particles of energy few hundreds of MeV. When the fast CMEs are ejected towards the Earth, they can disrupt the flow of solar wind in the heliosphere and impa…

2023 Journal of Atmospheric and Solar-Terrestrial Physics
SOHO 3