New in DR14 is the first public release of data from the extended Baryon Oscillation Spectroscopic Survey (eBOSS); the first data from the second phase of the Apache Point Observatory (APO) Galactic Evolution Experiment (APOGEE - 2), including stellar parameter estimates from an innovative data driven machine learning algorithm known as «The Cannon»; and almost twice as many data cubes from
the Mapping Nearby Galaxies at APO (MaNGA) survey as were in the previous release (N = 2812 in total).
The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS - IV Survey
MApping Nearby Galaxies at Apache Point Observatory
Not exact matches
Astronomers working with the Sloan Digital Sky Survey have used a 2.5 - meter telescope at the Apache Point Observatory in Sunspot, New Mexico, to
map the location of more than 930,000
nearby galaxies, determining the distance to each by how much the expansion of the universe has stretched, or «redshifted,» the wavelength of the
galaxy's light.
Remarkably, the distribution of star - forming
galaxies around a cluster of
galaxies in the more distant universe (5 billion years ago) corresponds much more closely with the weak lensing
map than a slice of the more
nearby universe (3 billion years ago).
They are the locations of bright stars and other
nearby objects that get in the way of the observations of more distant
galaxies and are hence masked out in these
maps as no weak - lensing signal can be measured in these areas.
The scientists from the USA, Australia, and Europe used the powerful DEIMOS spectrograph installed on the world's largest optical telescope at Keck Observatory to conduct a major survey of
nearby galaxies called SLUGGS, which
mapped out the speeds of their stars.
The Local Volume Mapper will create the first complete spectroscopic
maps of several important
nearby galaxies.