arxiv.org/abs/2101.08641v3
A dark-energy which behaves as the cosmological constant until a sudden phantom transition at very-low redshift ($z<0.1$) seems to solve the >4$σ$ disagreement between the local and high-redshift determinations of the Hubble constant, while maintain...
www.revenuecat.com/blog/replicating-a-postgresql-cluster-to-redshift
Points: 6 | Comments: 0 | Author: alfon
arxiv.org/abs/astro-ph/9408050v1
The weak distortions of high-redshift galaxies caused by gravitational light deflection near clusters of galaxies can be used to reconstruct the projected (two-dimensional) surface mass density of intermediate redshift clusters. This technique, pio...
en.wikipedia.org/wiki/2011_Louisiana%E2%80%93Lafayette_Ragin%27_Cajuns_softball_team
- Redshirt Freshman Utility Players 8 Megan Waterman - Sophomore 10 Tori Cummings - Redshirt Freshman 12 Christi Orgeron - Junior 17 Callie Philen - Sophomore
arxiv.org/abs/0711.0743v2
Gravitational wave standard sirens have been considered as precision distance indicators to high redshift; however, at high redshift standard sirens or standard candles such as supernovae suffer from lensing noise. We investigate lensing noise as a...
arxiv.org/abs/2503.00120v2
We present the COSMOS Spectroscopic Redshift Compilation encompassing ~ 20 years of spectroscopic redshifts within a 10 deg$^2$ area centered on the 2 deg$^2$ COSMOS legacy field. This compilation contains 487,666 redshifts of 266,284 unique objects...
www.bing.com/ck/a?!&&p=e1211c1581e039a675acac2a836694e8708dbd7e11355f69e842d02efc658748JmltdHM9MTc3MjQwOTYwMA&ptn=3&ver=2&hsh=4&fclid=38ae4a36-e9b9-6fe6-3a0b-5d26e8036e01&u=a1aHR0cHM6Ly93d3cucmVkZGl0LmNvbS9yL21vZGVyYXRlcG9saXRpY3MvY29tbWVudHMvaTFoZTN1L3Zpb2xlbnRfZXh0cmVtaXNtX29uX3JlZHN0YXRlLw&ntb=1
Jul 31, 2020 · Redstate is known for being extremely far right and having questionable accuracy, so it doesn't surprise me to see that kind of vitriol there. You'll find similar vitriol on Vox, Salon, Shareblue, â¦
arxiv.org/abs/astro-ph/0305077v1
We present unequivocal evidence for a huge (~80 x 100 x 100 Mpc^3) super-structure at redshift z=0.27 in the 3-D distribution of radio galaxies from the TONS08 sample, confirming tentative evidence for such a structure from the 7C redshift survey (...
arxiv.org/abs/1711.01693v1
English and Spanish translations are provided for Fritz Zwicky's seminal article on "The Redshift of Extragalactic Nebulae", published in German in Helvetica Physica Acta in 1933 <https://www.e-periodica.ch/digbib/view?pid=hpa-001:1933:6#112>. This p...
arxiv.org/abs/1410.4498v1
This white paper summarizes those conclusions of the Snowmass White Paper "Spectroscopic Needs for Imaging Dark Energy Experiments" (arXiv:1309.5384) which are relevant to the training of LSST photometric redshifts; i.e., the use of spectroscopic red...
arxiv.org/abs/1410.4506v1
This white paper summarizes the conclusions of the Snowmass White Paper "Spectroscopic Needs for Imaging Dark Energy Experiments" (arXiv:1309.5384) which are relevant to the calibration of LSST photometric redshifts; i.e., the accurate characterizati...
arxiv.org/abs/astro-ph/0702340v1
In this paper we derive the mass function of seed black holes that result from the central mass concentrated via disc accretion in collapsed haloes at redshift $z\approx 15$. Using standard arguments including stability, we show that these pre-gala...
arxiv.org/abs/astro-ph/0309081v1
Best, Rottgering and Lehnert (1999, 2000a) defined a new sample of powerful radio sources from the Molonglo Reference Catalogue, for which redshifts were compiled or measured for 177 of the 178 objects. For the final object, MRC1059-010 (3C249), th...
arxiv.org/abs/astro-ph/0309390v2
Some years ago (Jackson and Dodgson 1997) analysis of the angular-size/redshift relationship for ultra-compact radio sources indicted that for spatially flat universes the best choice of cosmological parameters was Omega_m=0.2 and Omega_Lambda=0.8....
arxiv.org/abs/1610.08362v1
I investigate the consistency of the VIMOS Public Extragalactic Redshift Survey v7 galaxy sample with the expansion history and linear growth rate predicted by General Relativity (GR) and a Planck (2015) cosmology. To do so, I measure the redshift-sp...
arxiv.org/abs/0708.1761v1
We review our attempts to discover lost baryons at low redshift with ``X-ray forest'' of absorption lines from the warm-hot intergalactic medium. We discuss the best evidence to date along the Mrk 421 sightline. We then discuss the missing baryons...
arxiv.org/abs/astro-ph/9608017v2
We investigate a distortion in redshift-space which causes galaxies to appear to lie in walls concentric about the observer, forming a rough bull's-eye pattern. We simulate what an observer would see in a thin slice of redshift-space, including a m...
arxiv.org/abs/1611.03866v2
We present an HST/ACS weak gravitational lensing analysis of 13 massive high-redshift (z_median=0.88) galaxy clusters discovered in the South Pole Telescope (SPT) Sunyaev-Zel'dovich Survey. This study is part of a larger campaign that aims to robustl...
arxiv.org/abs/0711.1754v1
This is the written account of the second of two panel discussions, on "Reconciling observations and modeling of star formation at high redshifts". The chair of the panel was Pavel Kroupa, and panel members were Marc Balcells, John Beckman, Christo...
arxiv.org/abs/1110.5626v1
In this paper we use H II starburst galaxy apparent magnitude versus redshift data from Siegel et al. (2005) to constrain dark energy cosmological model parameters. These constraints are generally consistent with those derived using other data sets,...