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Doug Geisler

Researcher at University of La Serena

Publications -  287
Citations -  16158

Doug Geisler is an academic researcher from University of La Serena. The author has contributed to research in topics: Globular cluster & Galaxy. The author has an hindex of 66, co-authored 271 publications receiving 14489 citations. Previous affiliations of Doug Geisler include University of Concepción & University of Florida.

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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies and the Distant Universe

Michael R. Blanton, +415 more
- 29 Jun 2017 - 
TL;DR: SDSS-IV as mentioned in this paper is a project encompassing three major spectroscopic programs: the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA), the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and the Time Domain Spectroscopy Survey (TDSS).
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VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way

Dante Minniti, +72 more
- 01 Jul 2010 - 
TL;DR: In this article, the authors proposed a method to solve the problem of single-input single-output (SISO) communication in the context of artificial neural networks (ANNs).
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The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

Romina Ahumada, +345 more
- 25 Jun 2020 - 
TL;DR: The most recent data release from the Sloan Digital Sky Surveys (SDSS-IV) is DR16 as mentioned in this paper, which is the fourth and penultimate from the fourth phase of the survey.
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Vvv dr1: the first data release of the milky way bulge and southern plane from the near-infrared eso public survey vista variables in the via lactea

R. K. Saito, +121 more
- 01 Jan 2012 - 
TL;DR: The ESO VISTA public survey VISTA variables in the V�a L�ctea (VVV) started in 2010 and is expected to run for about five years.
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The M 81 group of galaxies: New distances, kinematics and structure ?;??

I. D. Karachentsev, +10 more
- 01 Feb 2002 - 
TL;DR: In the M 81 complex, the true distance moduli, derived from the brightness of the tip of the red giant branch, lie in the range of 27: 52 (NGC 2366) to 28: 30 (DDO 165) as discussed by the authors.