no code implementations • 4 Nov 2020 • Johannes U. Lange, Alexie Leauthaud, Sukhdeep Singh, Hong Guo, Rongpu Zhou, Tristan L. Smith, Francis-Yan Cyr-Racine
It has been shown that the lensing amplitude of galaxies in the Baryon Oscillation Spectroscopic Survey (BOSS) is lower than expected given their clustering properties.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
2 code implementations • 13 Sep 2017 • Johnny P. Greco, Jenny E. Greene, Michael A. Strauss, Lauren A. MacArthur, Xzavier Flowers, Andy D. Goulding, Song Huang, Ji Hoon Kim, Yutaka Komiyama, Alexie Leauthaud, Lukas Leisman, Robert H. Lupton, Cristóbal Sifón, Shiang-Yu Wang
We define LSBGs to have mean surface brightnesses $\bar{\mu}_\mathrm{eff}(g)>24. 3$ mag arcsec$^{-2}$, which allows nucleated galaxies into our sample.
Astrophysics of Galaxies
2 code implementations • 13 Jun 2016 • Andrew Hearin, Duncan Campbell, Erik Tollerud, Peter Behroozi, Benedikt Diemer, Nathan J. Goldbaum, Elise Jennings, Alexie Leauthaud, Yao-Yuan Mao, Surhud More, John Parejko, Manodeep Sinha, Brigitta Sipocz, Andrew Zentner
We present the first stable release of Halotools (v0. 2), a community-driven Python package designed to build and test models of the galaxy-halo connection.
Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
no code implementations • 22 Sep 2015 • Beth Reid, Shirley Ho, Nikhil Padmanabhan, Will J. Percival, Jeremy Tinker, Rita Tojeiro, Martin White, Daniel J. Eisenstein, Claudia Maraston, Ashley J. Ross, Ariel G. Sanchez, David Schlegel, Erin Sheldon, Michael A. Strauss, Daniel Thomas, David Wake, Florian Beutler, Dmitry Bizyaev, Adam S. Bolton, Joel R. Brownstein, Chia-Hsun Chuang, Kyle Dawson, Paul Harding, Francisco-Shu Kitaura, Alexie Leauthaud, Karen Masters, Cameron K. McBride, Surhud More, Matthew D. Olmstead, Daniel Oravetz, Sebastian E. Nuza, Kaike Pan, John Parejko, Janine Pforr, Francisco Prada, Sergio Rodriguez-Torres, Salvador Salazar-Albornoz, Lado Samushia, Donald P. Schneider, Claudia G. Scoccola, Audrey Simmons, Mariana Vargas-Magana
We also present the algorithms used to create large scale structure catalogues for the final Data Release (DR12) samples and the associated random catalogues that quantify the survey mask.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
1 code implementation • 3 Dec 2014 • Kevin Bundy, Matthew A. Bershady, David R. Law, Renbin Yan, Niv Drory, Nicholas MacDonald, David A. Wake, Brian Cherinka, José R. Sánchez-Gallego, Anne-Marie Weijmans, Daniel Thomas, Christy Tremonti, Karen Masters, Lodovico Coccato, Aleksandar M. Diamond-Stanic, Alfonso Aragón-Salamanca, Vladimir Avila-Reese, Carles Badenes, Jésus Falcón-Barroso, Francesco Belfiore, Dmitry Bizyaev, Guillermo A. Blanc, Joss Bland-Hawthorn, Michael R. Blanton, Joel R. Brownstein, Nell Byler, Michele Cappellari, Charlie Conroy, Aaron A. Dutton, Eric Emsellem, James Etherington, Peter M. Frinchaboy, Hai Fu, James E. Gunn, Paul Harding, Evelyn J. Johnston, Guinevere Kauffmann, Karen Kinemuchi, Mark A. Klaene, Johan H. Knapen, Alexie Leauthaud, Cheng Li, Lihwai Lin, Roberto Maiolino, Viktor Malanushenko, Elena Malanushenko, Shude Mao, Claudia Maraston, Richard M. McDermid, Michael R. Merrifield, Robert C. Nichol, Daniel Oravetz, Kaike Pan, John K. Parejko, Sebastian F. Sanchez, David Schlegel, Audrey Simmons, Oliver Steele, Matthias Steinmetz, Karun Thanjavur, Benjamin A. Thompson, Jeremy L. Tinker, Remco C. E. van den Bosch, Kyle B. Westfall, David Wilkinson, Shelley Wright, Ting Xiao, Kai Zhang
MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10, 000 nearby galaxies.
no code implementations • 6 Feb 2007 • Jason D. Rhodes, Richard Massey, Justin Albert, Nicholas Collins, Richard S. Ellis, Catherine Heymans, Jonathan P. Gardner, Jean-Paul Kneib, Anton Koekemoer, Alexie Leauthaud, Yannick Mellier, Alexandre Refregier, James E. Taylor, Ludovic van Waerbeke
We derive a parametric correction for the effect of CTE on the shapes of objects in the COSMOS field as a function of observation date, position within the ACS WFC field, and object flux.