July 2, 2019
11:30AM - 12:30PM
PRB 4138
Add to Calendar
2019-07-02 11:30:00
2019-07-02 12:30:00
Summer Seminar Series: Upcoming Large Scale Structure Results from the Dark Energy Survey- Jack Elvin-Poole
Upcoming large scale structure results from the Dark Energy Survey
The Dark Energy Survey (DES) has provided world leading measurements in multiple probesof the late time universe. Using probes of weak gravitational lensing, galaxy clustering, cluster cosmology and supernovae from the first year of observations, DES is able test the Lambda CDM model with greater constraining power than any other individual galaxy survey. I will present the latest updates from the upcoming DES Year 3 large scale structure cosmologyanalysis, which use an observed area three times that of Year 1. I will discuss galaxy clustering analyses to both detect baryon acoustic oscillations (BAO) in the DES data, and to combine with with weak lensing.
PRB 4138
OSU ASC Drupal 8
ascwebservices@osu.edu
America/New_York
public
Date Range
Add to Calendar
2019-07-02 11:30:00
2019-07-02 12:30:00
Summer Seminar Series: Upcoming Large Scale Structure Results from the Dark Energy Survey- Jack Elvin-Poole
Upcoming large scale structure results from the Dark Energy Survey
The Dark Energy Survey (DES) has provided world leading measurements in multiple probesof the late time universe. Using probes of weak gravitational lensing, galaxy clustering, cluster cosmology and supernovae from the first year of observations, DES is able test the Lambda CDM model with greater constraining power than any other individual galaxy survey. I will present the latest updates from the upcoming DES Year 3 large scale structure cosmologyanalysis, which use an observed area three times that of Year 1. I will discuss galaxy clustering analyses to both detect baryon acoustic oscillations (BAO) in the DES data, and to combine with with weak lensing.
PRB 4138
Center for Cosmology and AstroParticle Physics (CCAPP)
ccapp@osu.edu
America/New_York
public
Upcoming large scale structure results from the Dark Energy Survey
The Dark Energy Survey (DES) has provided world leading measurements in multiple probesof the late time universe. Using probes of weak gravitational lensing, galaxy clustering, cluster cosmology and supernovae from the first year of observations, DES is able test the Lambda CDM model with greater constraining power than any other individual galaxy survey. I will present the latest updates from the upcoming DES Year 3 large scale structure cosmologyanalysis, which use an observed area three times that of Year 1. I will discuss galaxy clustering analyses to both detect baryon acoustic oscillations (BAO) in the DES data, and to combine with with weak lensing.
