Workflows

Resolving coordinates from a source names ... (2)

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Snippet showing how to use AstroTaverna tool for coordinates resolving. The input is a list of source names and the output is a VOTable with three columns: SourceName, RAJ2000, DECJ2000.

Created: 2013-04-12 | Last updated: 2013-04-22

Table format coversion: ASCII to VOTable (2)

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Snippet showing how to use AstroTaverna tool for table format conversion

Created: 2013-04-12 | Last updated: 2013-04-12

Retrieving information from HST ConeSearch... (1)

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This workflow retieves information from Hubble Space Telescope VO Services in the form of VOTables. The input of the workflow is an ASCII file with a list of source names. This file is converted to a VOTable, and coordinates added with an extra-column needed to query SIAP Image service. The final result are two different VOTables issued as the response of both VO Services, Images VOTable has been previously filtered.

Created: 2013-04-12

Crossmatching VOTables (2)

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Snippet showing how to use AstroTaverna tool for crossmatching two VOTables VOTable samples may be downloaded from MyExperiment http://www.myexperiment.org/files/911/versions/1/download/SDSS7.vot http://www.myexperiment.org/files/910/versions/1/download/2MASS.vot

Created: 2013-04-12 | Last updated: 2013-04-22

Credits: Jose Enrique Ruiz

Discovery of Brown Dwarfs mining the 2MASS... (1)

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Brown dwarfs are objects occupying the gap between the least massive stars and the most massive planets. They are intrinsically faint objects so their detection is not straighforward and, in fact, was almost impossible until the advent of global surveys at deep optical and near-infrared bands like SDSS, 2MASS or DENIS among others. Here we propose to mine the SDSS and 2MASS databases to identify T-type brown dwarfs through an appropriate combination of colours in the optical and the infra-red...

Created: 2013-04-12

Credits: Jose Enrique Ruiz

Venus: Compare VEX data with HYB model (1)

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It compares data from VEX from a certain date range with what HYB has modeled in the coordinates where VEX spacecraft is at that moment.

Created: 2013-04-07

Credits: David PS Natasha

jpylyzer: Extract width and height (1)

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No description

Created: 2013-04-04

ImageMagick: Convert JPG to TIFF (3)

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Converts a JPG image to a TIFF image

Created: 2013-04-04 | Last updated: 2013-04-04

EB-eye getAllResultIds and WSDbfetch fetch... (1)

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Get database entries for a query using EB-eye to perform the initial query against the database to get entry identifiers and using the identifiers with WSDbfetch to retrieve the entry data in the desired format. Note: this particular implementation is not suitable for queries which return large numbers of results.

Created: 2013-03-28

Credits: Hamish McWilliam

Comparison of Peptide and Protein Fraction... (1)

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This workflow was used to analyze the data in a manuscript by Mostovenko et al. (2013, submitted), comparing peptide and protein fractionation methods. The workflow identifies proteins by X!Tandem database search and validates the results using PeptideProphet. Additional information such as pI and fraction number is extracted and plotted for IEF and SCX data. For each protein identified in SDS-PAGE derived data sequences are downloaded from UniProt and plotted against the fraction number. Rs...

Created: 2013-03-27

Credits: Kate Mostovenko Yassene Magnus Palmblad

Attributions: Plasma Precipitation Analysis

When do the Fastest type II CME should be ... (1)

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The fastest CME is found from an interval of time, and propagated to Earth, in two steps, first to obtain the Solar wind speed at Earth and then propagated again with a more reasonable CME speed. The output produces Min-Max ETAs for each object in the heliosphere and the plots of the final propagation model. This Workflow was produced as one of the challenges in the HELIO CDAW-IV hosted at TCD

Created: 2013-03-21

Credits: Gab Anja Le Blanc David PS

Attributions: When did the fastest type II CME happened?

Monthly counts for event occurences betwee... (1)

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This workflow provides monthly counts of events in HEC between the beginning of year_start and the end of year_end. Returns the result as comma separated file (csv) and as list of lists.

Created: 2013-03-21

Credits: Nadia Cerezo Anja Le Blanc David PS

Attributions: Monthly counts for event occurences between beginning of year_start and end of year_end

Find data from a list of instruments and a... (1)

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For a certain time range, it looks for flares between a energy range (GOES x-ray flare class), and it provides the observations for such time range for the list of instruments asked. It also provides the table of flares with its properties. Note: This workflow does not look whether the instrument was not looking to the right field of view (eg., CDS)

Created: 2013-03-20

Credits: David PS Anja Le Blanc Nadia Cerezo Gab

Attributions: find events in xray and radio

Untitled (1)

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v2

Created: 2013-03-15

Untitled (1)

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2

Created: 2013-03-15

Untitled (1)

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Initial version

Created: 2013-03-15