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Full-Text Articles in Stars, Interstellar Medium and the Galaxy
Most Observations Of Our Nearest Neighbor: Flares On Proxima Centauri, James R. A. Davenport, David M. Kipping, Dimitar Sasselov, Jaymie M. Matthews, Chris Cameron
Most Observations Of Our Nearest Neighbor: Flares On Proxima Centauri, James R. A. Davenport, David M. Kipping, Dimitar Sasselov, Jaymie M. Matthews, Chris Cameron
Physics & Astronomy
We present a study of white-light flares from the active M5.5 dwarf Proxima Centauri using the Canadian microsatellite Microvariability and Oscillations of STars. Using 37.6 days of monitoring data from 2014 to 2015, we have detected 66 individual flare events, the largest number of white-light flares observed to date on Proxima Cen. Flare energies in our sample range from 1029 to 1031.5erg. The flare rate is lower than that of other classic flare stars of a similar spectral type, such as UV Ceti, which may indicate Proxima Cen had a higher flare rate in its youth. …
The Kepler Catalog Of Stellar Flares, James R. A. Davenport
The Kepler Catalog Of Stellar Flares, James R. A. Davenport
Physics & Astronomy
A homogeneous search for stellar flares has been performed using every available Kepler light curve. An iterative light curve de-trending approach was used to filter out both astrophysical and systematic variability to detect flares. The flare recovery completeness has also been computed throughout each light curve using artificial flare injection tests, and the tools for this work have been made publicly available. The final sample contains 851,168 candidate flare events recovered above the 68% completeness threshold, which were detected from 4041 stars, or 1.9% of the stars in the Kepler database. The average flare energy detected is ~1035 erg. …
Hectomap And Horizon Run 4: Dense Structures And Voids In The Real And Simulated Universe, Ho Seong Hwang, Margaret J. Geller, Changbom Park, Daniel G. Fabricant, Michael J. Kurtz, Kenneth J. Rines, Juhan Kim, Antonaldo Diaferio, J. Jabran Zahid, Perry Berland, Michael Calkins, Susan Tokarz, Sean Moran
Hectomap And Horizon Run 4: Dense Structures And Voids In The Real And Simulated Universe, Ho Seong Hwang, Margaret J. Geller, Changbom Park, Daniel G. Fabricant, Michael J. Kurtz, Kenneth J. Rines, Juhan Kim, Antonaldo Diaferio, J. Jabran Zahid, Perry Berland, Michael Calkins, Susan Tokarz, Sean Moran
Physics & Astronomy
HectoMAP is a dense redshift survey of red galaxies covering a 53 deg2 strip of the northern sky. HectoMAP is 97% complete for galaxies with r < 20.5, (g− r) > 1.0, and (r − i) > 0.5. The survey enables tests of the physical properties of large-scale structure at intermediate redshift against cosmological models. We use the Horizon Run 4, one of the densest and largest cosmological simulations based on the standard Λ Cold Dark Matter (ΛCDM) model, to compare the physical properties of observed large-scale structures with simulated ones in a volume-limited sample covering 8 × 106 …
Hydrostatic And Caustic Mass Profiles Of Galaxy Clusters, Ben J. Maughan, Paul A. Giles, Kenneth J. Rines, Antonaldo Diaferio, Margaret J. Geller, Nina Van Der Pyl, Massimiliano Bonamente
Hydrostatic And Caustic Mass Profiles Of Galaxy Clusters, Ben J. Maughan, Paul A. Giles, Kenneth J. Rines, Antonaldo Diaferio, Margaret J. Geller, Nina Van Der Pyl, Massimiliano Bonamente
Physics & Astronomy
We compare X-ray and caustic mass profiles for a sample of 16 massive galaxy clusters. We assume hydrostatic equilibrium in interpreting the X-ray data, and use large samples of cluster members with redshifts as a basis for applying the caustic technique. The hydrostatic and caustic masses agree to better than ≈20 per cent on average across the radial range covered by both techniques (∼[0.2–1.25]R500). The mass profiles were measured independently and do not assume a common functional form. Previous studies suggest that, at R500 , the hydrostatic and caustic masses are biased low and high, respectively. …