scholarly journals THE NINTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST SPECTROSCOPIC DATA FROM THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY

2012 ◽  
Vol 203 (2) ◽  
pp. 21 ◽  
Author(s):  
Christopher P. Ahn ◽  
Rachael Alexandroff ◽  
Carlos Allende Prieto ◽  
Scott F. Anderson ◽  
Timothy Anderton ◽  
...  
2017 ◽  
Vol 233 (2) ◽  
pp. 25 ◽  
Author(s):  
Franco D. Albareti ◽  
Carlos Allende Prieto ◽  
Andres Almeida ◽  
Friedrich Anders ◽  
Scott Anderson ◽  
...  

2014 ◽  
Vol 211 (2) ◽  
pp. 17 ◽  
Author(s):  
Christopher P. Ahn ◽  
Rachael Alexandroff ◽  
Carlos Allende Prieto ◽  
Friedrich Anders ◽  
Scott F. Anderson ◽  
...  

2009 ◽  
Vol 5 (S267) ◽  
pp. 464-464
Author(s):  
J. A. Vázquez-Mata ◽  
H. M. Hernández-Toledo ◽  
Changbom Park ◽  
Yun-Young Choi

We present a new catalog of isolated galaxies (coined as UNAM–KIAS) obtained through an automated systematic search. The 1520 isolated galaxies were found in ~ 1.4 steradians of the sky in the Sloan Digital Sky Survey Data Release 5 (SDSS DR5) photometry. The selection algorithm was implemented from a variation of the criteria developed by Karachentseva (1973), with full redshift information. This new catalog is aimed to carry out comparative studies of environmental effects and constraining the currently competing scenarios of galaxy formation and evolution.


2011 ◽  
Vol 527 ◽  
pp. A126 ◽  
Author(s):  
F.-X. Pineau ◽  
C. Motch ◽  
F. Carrera ◽  
R. Della Ceca ◽  
S. Derrière ◽  
...  

2004 ◽  
Vol 128 (2) ◽  
pp. 561-568 ◽  
Author(s):  
Misty C. Bentz ◽  
Patrick B. Hall ◽  
Patrick S. Osmer

2017 ◽  
Vol 45 ◽  
pp. 1760023
Author(s):  
S. O. Kepler ◽  
Alejandra Daniela Romero ◽  
Ingrid Pelisoli ◽  
Gustavo Ourique

White dwarf stars are the final stage of most stars, born single or in multiple systems. We discuss the identification, magnetic fields, and mass distribution for white dwarfs detected from spectra obtained by the Sloan Digital Sky Survey up to Data Release 13 in 2016, which lead to the increase in the number of spectroscopically identified white dwarf stars from 5[Formula: see text]000 to 39[Formula: see text]000. This number includes only white dwarf stars with [Formula: see text], i.e., excluding the Extremely Low Mass white dwarfs, which are necessarily the byproduct of stellar interaction.


Author(s):  
Xin-Fa Deng ◽  
Guisheng Yu ◽  
Peng Jiang

AbstractUsing two volume-limited Main galaxy samples of the Sloan Digital Sky Survey Data Release 7 , we explore influences of galaxy interactions on AGN activity. It is found that in the faint volume-limited sample, paired galaxies have a slightly higher AGN fraction than isolated galaxies, whereas in the luminous volume-limited sample, an opposite trend can be observed. The significance is <1σ. Thus, we do not observe strong evidence that interactions or mergers likely trigger the AGN activity.


2005 ◽  
Vol 621 (2) ◽  
pp. 643-650 ◽  
Author(s):  
David M. Goldberg ◽  
Timothy D. Jones ◽  
Fiona Hoyle ◽  
Randall R. Rojas ◽  
Michael S. Vogeley ◽  
...  

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