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  2. Optical Gravitational Lensing Experiment - Wikipedia

    en.wikipedia.org/wiki/Optical_Gravitational...

    Most of the observations have been made at the Las Campanas Observatory in Chile. Cooperating institutions include Princeton University and the Carnegie Institution. The project is now in its fourth phase. The first phase, OGLE-I (1992–1995), used the 1.0-metre (3 ft 3 in) Swope telescope and a single-chip CCD sensor.

  3. SeaWiFS - Wikipedia

    en.wikipedia.org/wiki/SeaWiFS

    NASA offers free software designed specifically to work with SeaWiFS data through the ocean color website. This software, entitled SeaDAS (SeaWiFS Data Analysis System), is built for visualization and processing of satellite data and can work with Level 1, 2, and 3 data. Though it was originally designed for SeaWiFS data, its capabilities have ...

  4. SPICE (observation geometry system) - Wikipedia

    en.wikipedia.org/wiki/SPICE_(observation...

    It has become the de facto standard for handling much of the so-called observation geometry information on NASA's planetary missions, and it is now widely used in support of science data analysis on planetary missions of other space agencies as well. Some SPICE capabilities are also used on a variety of astrophysics, solar physics and earth ...

  5. Observation.org - Wikipedia

    en.wikipedia.org/wiki/Observation.org

    Observation.org is a worldwide platform of naturalists, citizen scientists, and biologists to collect, validate and share biodiversity observations. Observation.org may be accessed via its website or from its mobile applications like ObsIdentify. The Observation.org database holds 233 million nature observations and 79 million photos. [1]

  6. Data assimilation - Wikipedia

    en.wikipedia.org/wiki/Data_assimilation

    The measurements are usually made of a real-world system, rather than of the model's incomplete representation of that system, and so a special function called the observation operator (usually depicted by h() for a nonlinear operator or H for its linearization) is needed to map the modeled variable to a form that can be directly compared with ...

  7. Pulsar timing array - Wikipedia

    en.wikipedia.org/wiki/Pulsar_timing_array

    Following the discovery of the more stable millisecond pulsar in 1982, Foster and Backer [11] improved the sensitivity to GWs by applying in 1990 the Hellings-Downs analysis to an array of highly stable millisecond pulsars and initiated a ‘pulsar timing array program’ to observe three pulsars using the National Radio Astronomy Observatory ...

  8. List of cosmological computation software - Wikipedia

    en.wikipedia.org/wiki/List_of_cosmological...

    This List of Cosmological Computation Software catalogs the tools and programs used by scientists in cosmological research.. In the past few decades, the accelerating technological evolution has profoundly enhanced astronomical instrumentation, enabling more precise observations and expanding the breadth and depth of data collection by several orders of magnitude.

  9. Open scientific data - Wikipedia

    en.wikipedia.org/wiki/Open_scientific_data

    Early discourses and policy frameworks on open scientific data emerged immediately in the wake of the creation of the first large knowledge infrastructure. The World Data Center system (now the World Data System), aimed to make observation data more readily available in preparation for the International Geophysical Year of 1957–1958. [21]