The Einstein On-Line System

Bibcode
1992ASPC...25...44K
Karakashian, T.; Harris, D. E.; Garcia, M.; Fabbiano, G.; Flanagan, J. M.; Stern, C. P.
Bibliographical reference

Astronomical Data Analysis Software and Systems I, A.S.P. Conference Series, Vol. 25, 1992, Diana M. Worrall, Chris Biemesderfer, and Jeannette Barnes, eds., p. 44.

Advertised on:
0
1992
Number of authors
6
IAC number of authors
0
Citations
3
Refereed citations
0
Description
The Einstein On-Line System (EOLS) is a collection of data, software, and documentation from the Einstein Observatory project and is located on a computer at the Smithsonian Astrophysical Observatory. The interface is menu-driven, terminal-independent, and is available via the Internet, SPAN, or telephone dial-up. Using EOLS, astronomers have access to 4 Gigabytes of Einstein processed data and documentation. Products may be retrieved via VMS copy (over SPAN), ftp (over Internet), or electronic mail. In addition, all numerical databases are available via NASA's Astrophysics Data System (ADS). The EOLS project is actively evolving in response to users' comments. Over the next two years, more than 30 Gigabytes of additional Einstein data will be made available in the EOLS.
Type
Non-refereed

It may interest you

  • Non-refereed
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    New Robotic Telescope system progress towards critical design review
    The 4m class New Robotic Telescope (NRT) is an optical facility designed to revolutionize the rapid follow-up and classification of variable and transient objects. The project is at the stage where key systems are progressing through their detailed design phases, which presents a major engineering challenge for all project partners to manage design
    Copley, David et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..3WC
    Citations
    0
  • Non-refereed
    Phase diversity application on the EST MCAO testbench
    Phase Diversity (PD) is a technique widely used to measure and compensate for Non-Common Path Aberrations (NCPA) in optical systems. Beyond its traditional applications, PD has found further uses in solar astrophysics, where it enhances image quality by processing multiple images to correct residual aberrations. In this work, we introduce a
    Rodriguez-Linares, Nicolas et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13097E..5OR
    Citations
    0