Tootfinder

The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars
I. McDonald, S. Srinivasan, P. Scicluna, O. C. Jones, A. A. Zijlstra, S. H. J. Wallstr\"om, T. Danilovich, J. H. He, J. P. Marshall, J. Th. van Loon, R. Wesson, F. Kemper, A. Trejo-Cruz, J. Greaves, T. Dharmawardena, J. Cami, H. Kim, K. E. Kraemer, C. J. R. Clark, H. Shinnaga, C. Haswell, H. Imai, J. G. A. Wouterloot, A. J. P\'erez Vidal, G. Rau, the NESS collaboration

The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars
We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved Stars Survey (NESS), and (2) a partially overlapping set of 507 evolved stars within 300 pc. We also investigate distance determinations to these stars, their luminosity functions and their spatial distribution. Gaia APSIS GSP-Phot AENEAS temperatures of bright giant stars often appear to be underestimated. Existing l…

Heute vor 15 Jahren: Am 26. Mai 2019 gab #Großbritannien bekannt, dass es 225 #Atomwaffen besitzt, von denen 160 einsatzbereit sind.

The Stellar Populations and Rest-Frame Colors of Star-Forming Galaxies at $z \approx 8$: Exploring the Impact of Filter Choice and Star Formation History Assumption with JADES
Jakob M. Helton, Stacey Alberts, George H. Rieke, Kevin N. Hainline, Zhiyuan Ji, Marcia J. Rieke, Benjamin D. Johnson, Brant Robertson, Sandro Tacchella, Lily Whitler, William M. Baker, Rachana Bhatawdekar, Kristan Boyett, Andrew J. Bunker, Phillip A. Cargile, Stefano Carniani, Stephane Charlot, Jacopo Chevallard…

The Stellar Populations and Rest-Frame Colors of Star-Forming Galaxies at $z \approx 8$: Exploring the Impact of Filter Choice and Star Formation History Assumption with JADES
Our understanding of the physical properties of star-forming galaxies during the Epoch of Reionization (EoR, at $z > 6$) suffers from degeneracies among the apparent properties of the stars, the nebular gas, and the dust. These degeneracies are most prominent with photometry, which has insufficient (1) spectral resolution and (2) rest-frame spectral coverage. We explore ways to break these degeneracies with a sample of $N = 22$ high-redshift star-forming galaxies at $7 < z_{\mathrm{phot}} \leq …