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1 to 10 of 2,468 Results
2012-2013 SPT-GMOS - Redshift Catalogs, 1D+2D Spectra, and Imaging
Aug 4, 2025 - SPT Galaxy Cluster Followup Dataverse
Matthew B Bayliss, 2014, "2012-2013 SPT-GMOS - Redshift Catalogs, 1D+2D Spectra, and Imaging", https://doi.org/10.7910/DVN/27079, Harvard Dataverse, V2
This is the release of Gemini-South/GMOS spectroscopic observations of South Pole Telescope clusters that were conducted between mid 2012 through late 2013. These data have all been processed through a first-pass reduction script. Subsequent data releases will include improved iterations of the data processing (e.g., including a more careful treatm...
Best fit model of the Radcliffe Wave
Mar 8, 2024 - The Radcliffe Wave Is Oscillating
Konietzka, Ralf, 2024, "Best fit model of the Radcliffe Wave", https://doi.org/10.7910/DVN/F98QHY, Harvard Dataverse, V1, UNF:6:4zUAYP70tqXnxjQB/Crw4g== [fileUNF]
Tab-separated ASCII machine readable table of the best fit model in Konietzka et al. 2024. The best fit model was derived by applying the model described in Konietzka et al. 2024 to the spatial and kinematic molecular cloud and stellar cluster observations. Data columns are as follows: (1) x: Heliocentric Galactic Cartesian x position (pc) (2) y: H...
Radcliffe_Wave_best_fit_model_Konietzka2024.tab
Mar 8, 2024 - Best fit model of the Radcliffe Wave
Tabular Data - 46.1 KB - 4 Variables, 1500 Observations - UNF:6:4zUAYP70tqXnxjQB/Crw4g==
12CO radial velocities along the Radcliffe Wave
Feb 20, 2024 - The Radcliffe Wave Is Oscillating
Konietzka, Ralf, 2024, "12CO radial velocities along the Radcliffe Wave", https://doi.org/10.7910/DVN/Q7F4PC, Harvard Dataverse, V1, UNF:6:wCNWnEds9k2/RmYNjfjREw== [fileUNF]
Tab-separated ASCII machine readable table of the 12CO data presented in Konietzka et al. 2024. Data columns are as follows: (1) name: name of the molecular cloud or tenuous connection (2) x: Heliocentric Galactic Cartesian x position (pc) (3) y: Heliocentric Galactic Cartesian y position (pc) (4) z: Heliocentric Galactic Cartesian z position (pc)...
Radcliffe_Wave_CO_analysis_Konietzka2024.tab
Feb 20, 2024 - 12CO radial velocities along the Radcliffe Wave
Tabular Data - 5.2 KB - 13 Variables, 79 Observations - UNF:6:wCNWnEds9k2/RmYNjfjREw==
Stellar cluster catalog along the Radcliffe Wave
Feb 20, 2024 - The Radcliffe Wave Is Oscillating
Konietzka, Ralf, 2024, "Stellar cluster catalog along the Radcliffe Wave", https://doi.org/10.7910/DVN/XSCB9N, Harvard Dataverse, V1, UNF:6:uqaOQfhvfwAvUTaC2mZ2CA== [fileUNF]
Tab-separated ASCII machine readable table of the stellar clusters used in Konietzka et al. 2024. Data columns are as follows: (1) name: name of the stellar cluster (2) reference: reference in which the cluster was originally characterized (3) x: Heliocentric Galactic Cartesian x position (pc) (4) sigmax: Error of the mean Heliocentric Galactic Car...
Radcliffe_Wave_stellar_clusters_Konietzka2024.tab
Feb 20, 2024 - Stellar cluster catalog along the Radcliffe Wave
Tabular Data - 10.6 KB - 16 Variables, 125 Observations - UNF:6:uqaOQfhvfwAvUTaC2mZ2CA==
Replication Data for: Breaking Waves on the Surface of the Heartbeat Star MACHO 80.7443.1718
May 30, 2023 - Morgan MacLeod Dataverse
MacLeod, Morgan, 2023, "Replication Data for: Breaking Waves on the Surface of the Heartbeat Star MACHO 80.7443.1718", https://doi.org/10.7910/DVN/47WXLT, Harvard Dataverse, V1
Replication data from simulations with Athena++, MESA, and GYRE for paper studying tidal wave breaking on the surface of the heartbeat star MACHO 80.7443.1718.
machoHBdata.zip
May 30, 2023 - Replication Data for: Breaking Waves on the Surface of the Heartbeat Star MACHO 80.7443.1718
ZIP Archive - 89.1 GB - MD5: 7462509bae3f81c369c8f7b7de882111
Fitting 25 years of GONG data - Tables
Jan 5, 2023 - Sylvain Korzennik Dataverse
Korzennik, Sylvain, 2023, "Fitting 25 years of GONG data - Tables", https://doi.org/10.7910/DVN/8VCH91, Harvard Dataverse, V2
You can find here the tables resulting from fitting a 25 year long time series of GONG observations, using different leakage matrices and using or not an asymmetric mode profile, and presented in "Precision and systematic errors in global helioseismology mode fitting and inversions: Leveraging some 25 years of nearly uninterrupted observations", S.G...
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