On Fridays we'll allow posts that don't normally fit in the usual data-hoarding theme, including posts that would usually be removed by rule 4: “No memes or 'look at this '”
#Vvv disk catalog free
No memes or 'look at this old storage medium/ connection speed/purchase' (except on Free Post Fridays).Search the Internet, this subreddit and our wiki before posting.And we're trying really hard not to forget.ģ.3v Pin Reset Directions :D / Alt Imgur link Along the way we have sought out like-minded individuals to exchange strategies, war stories, and cautionary tales of failures. Everyone has their reasons for curating the data they have decided to keep (either forever or For A Damn Long Timetm). government or corporate espionage), cultural and familial archivists, internet collapse preppers, and people who do it themselves so they're sure it's done right. Among us are represented the various reasons to keep data - legal requirements, competitive requirements, uncertainty of permanence of cloud services, distaste for transmitting your data externally (e.g. The VVV NIR Galaxy Catalogue is a new data set providing information for extragalactic studies in the Galactic plane. We aim at producing a deep, point spread function (PSF) photometric catalog for the VVV survey J-,H-, and K s-band data. High-delity photometric catalogs are needed to utilize the data.
The survey was designed for mapping 562deg2 in the Galactic bulge and the southern disk in five near-infrared broadband filters -Z(effWe conclude that interstellar extinction and stellar density are the main limitations for the detection of background galaxies in the Zone of Avoidance. The VISTA Variables in the Via Lactea (VVV) survey is an ESO Infrared Large Public survey (Minniti+ 2010NewA.15.433M & Saito+ 2012A& A.537A.107S) that uses the 4m VISTA telescope located at Cerro Paranal Observatory, Chile. We also present a description of the 185 2MASS extended sources observed in the region, of which 16% of these objects had no previous description, which we have now classified. The survey was designed for mapping 562deg 2 in the Galactic bulge and the southern disk in five near-infrared broadband filters -Z(eff0.8um), Y (#Vvv disk catalog archive
Zip, StuffIt, RAR, 7-Zip, tar, gzip, bzip2, CompactPro and LHA archive formats support. We used SExtractor + PSFEx to identify extended objects and to measure their sizes, the light concentration index, magnitudes, and colours. Trusted catalog database format for scalability and storage of huge data. Our aim is to map the galaxy distribution across the Southern Galactic plane using the VISTA Variables in the V\’ia L\’actea Survey (VVV), which reach 2 to 4 magnitudes deeper than 2MASS. Past near-infrared (NIR) surveys, such as the Two Micron All Sky Survey (2MASS), have shown the power of probing large-scale structure at these latitudes. Knowledge about the large-scale distribution of galaxies is far from complete in the Zone of Avoidance, which is mostly due to high interstellar extinction and to source confusion at lower Galactic latitudes.
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