We present analysis of 12,227 type-ab RR Lyraes (RRLs) found among the 200 million public light curves in Catalina Surveys Data Release 1. These stars span the largest volume of the Milky Way ever surveyed with RRLs, covering ~20,000 deg2 of the sky (0° 1500 of the RRLs. Using the accurate distances derived for the RRLs, we show the paths of the Sagittarius tidal streams crossing the sky at heliocentric distances from 20 to 60 kpc. By selecting samples of Galactic halo RRLs, we compare their velocity, metallicity, and distance with predictions from a recent detailed N-body model of the Sagittarius system. We find that there are some significant differences between the distances and structures predicted and our observations
A survey of RR Lyrae stars has been conducted in selected regions of the Galactic halo, using the 48...
We identify substructures of the Galactic halo using 3,003 type $ab$ RR Lyraes (RRab) with 6D positi...
We present a sample of 148 candidate RR Lyrae stars selected from Sloan Digital Sky Survey (SDSS) co...
We present analysis of 12,227 type-ab RR Lyraes (RRLs) found among the 200 million public light curv...
We present the analysis of 1207 RR Lyrae found in photometry taken by the Catalina Survey's Mount Le...
We present the results of a deep, wide-area variability survey in the Southern hemisphere, the first...
We apply the GC3 stream-finding method to RR Lyrae stars (RRLSs) in the Catalina survey. We find 2 R...
We present a sample of ~5000 RR Lyrae stars selected from the recalibrated LINEAR data set and detec...
RR Lyrae stars are ideal massless tracers that can be used to study the total mass and dark matter c...
We present an analysis of Galactic halo structure, substructure, and metallicity traced by mainseque...
We present ~47,000 periodic variables found during the analysis of 5.4 million variable star candida...
To explore the complex halo substructure that has been reported in the direction of the Vi...
We have measured the periods and light curves of 148 RR Lyrae variables from V = 13.5 to 19.7 from t...
Currently, only a small number of Milky Way (MW) stars are known to exist beyond 100 kpc from the Ga...
RR Lyrae stars may be the best practical tracers of Galactic halo (sub-)structure and kinematics. Th...
A survey of RR Lyrae stars has been conducted in selected regions of the Galactic halo, using the 48...
We identify substructures of the Galactic halo using 3,003 type $ab$ RR Lyraes (RRab) with 6D positi...
We present a sample of 148 candidate RR Lyrae stars selected from Sloan Digital Sky Survey (SDSS) co...
We present analysis of 12,227 type-ab RR Lyraes (RRLs) found among the 200 million public light curv...
We present the analysis of 1207 RR Lyrae found in photometry taken by the Catalina Survey's Mount Le...
We present the results of a deep, wide-area variability survey in the Southern hemisphere, the first...
We apply the GC3 stream-finding method to RR Lyrae stars (RRLSs) in the Catalina survey. We find 2 R...
We present a sample of ~5000 RR Lyrae stars selected from the recalibrated LINEAR data set and detec...
RR Lyrae stars are ideal massless tracers that can be used to study the total mass and dark matter c...
We present an analysis of Galactic halo structure, substructure, and metallicity traced by mainseque...
We present ~47,000 periodic variables found during the analysis of 5.4 million variable star candida...
To explore the complex halo substructure that has been reported in the direction of the Vi...
We have measured the periods and light curves of 148 RR Lyrae variables from V = 13.5 to 19.7 from t...
Currently, only a small number of Milky Way (MW) stars are known to exist beyond 100 kpc from the Ga...
RR Lyrae stars may be the best practical tracers of Galactic halo (sub-)structure and kinematics. Th...
A survey of RR Lyrae stars has been conducted in selected regions of the Galactic halo, using the 48...
We identify substructures of the Galactic halo using 3,003 type $ab$ RR Lyraes (RRab) with 6D positi...
We present a sample of 148 candidate RR Lyrae stars selected from Sloan Digital Sky Survey (SDSS) co...