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D5.3v2 Calculation of Luminosity Profiles for a Samp...

Created: 2013-01-05 16:45:48 | Last updated: 2013-01-05 16:48:45

Credits: Jose Enrique Ruiz

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: Adobe PDF

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Extraction of Properties from a Sample of Galaxies

Created: 2013-01-05 16:54:48 | Last updated: 2013-01-05 16:57:46

Credits: Jose Enrique Ruiz

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: Adobe PDF

Comments: 0 | Viewed: 60 times | Downloaded: 37 times

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Calculation of Luminosity Profiles for a Sample of G...

Created: 2013-01-05 16:57:08

Credits: Jose Enrique Ruiz

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: Adobe PDF

Comments: 0 | Viewed: 60 times | Downloaded: 110 times

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AstroGrid and the VO

Unique name: astrogrid.org
Created: Tuesday 05 February 2008 19:44:08 (UTC)

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AMIGA

Unique name: AMIGA
Created: Wednesday 25 January 2012 17:06:37 (UTC)

44 shared items   |   0 announcements

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ICS Use Case Solutions

Created: 2010-07-12 13:54:16 | Last updated: 2010-07-13 10:57:46

1 item in this pack

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Luminosity Profiles Research Object

Created: 2013-01-05 16:34:46 | Last updated: 2013-01-05 16:58:18

7 items in this pack

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Galaxies Sample Selection Research Object

Created: 2013-01-05 16:51:56 | Last updated: 2013-01-05 16:59:16

4 items in this pack

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retrieving solar monitor urls for votable ... (1)

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No description

Created: 2009-11-12 | Last updated: 2009-11-12

Credits: Anja Le Blanc

find events in xray and radio (7)

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instruments: hessiEC, phoenix2 attention: hessi name has changed!

Created: 2010-03-16 | Last updated: 2010-03-16

Credits: Anja Le Blanc

retrieve data for all instruments for even... (1)

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This workflow uses the HEC to retrieve events for a time spane given by the user from a HEC table given by the user as well. It uses all instruments available in the DPAS to retrieve data for the events Output: XML as returned by the DPASThis workflow uses the HEC to retrieve events for a time spane given by the user from a HEC table given by the user as well. It uses all instruments available in the DPAS to retrieve data for the events; empty results are filtered out, the data is combind wi...

Created: 2010-04-21

Credits: Anja Le Blanc

Attributions: DPAS general query HEC standard query Retrieve all data for all instruments for a given periode of time

Call VSO web service with HELIO input data (1)

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  date transformation from 2000-10-02T23:00:00 to 20001002230000 HELIO instrument names as in http://helio-dev.i4ds.ch/xsd/instruments.xsd spitt into source and instrument names; if these pair don't exist only first part (source) is tried.

Created: 2010-08-04 | Last updated: 2010-08-04

Credits: Anja Le Blanc

retrive dpas data for all ics instruments ... (1)

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This workflow demonstrates the standard query there events for a period of time are requested from the HEC service, available instruments for this time come from the ICS and data only for the times of the events are requested from the DPAS.

Created: 2010-09-14 | Last updated: 2010-09-14

Credits: Anja Le Blanc

Attributions: Extracting data from VOTable format by using XPath query Retrieve all data for all instruments for a given periode of time

retrive dpas data for all ics instruments ... (1)

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This workflow demonstrates the standard query where events for a period of time are requested from the HEC service, available instruments for this time come from the ICS and data only for the times of the events are requested from the DPAS. In this version data from only 3 random events (out of the HEC list) will be requested from the DPAS.

Created: 2010-09-14 | Last updated: 2010-09-14

Credits: Anja Le Blanc

Attributions: retrive dpas data for all ics instruments for HEC event data

Associate hessi flares with active regions (3)

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This workflow is querying the HFC ActiveRegions list and HEC hessi_flare list. It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: HFCout is a modified VOTable where a field is added with the number of associated hessi flares. combined_output is a 2 dimensional list with an VOTable for each Active region and one with an VOTable for all associated flares for that Active Region.

Created: 2011-02-11 | Last updated: 2011-10-24

Credits: Anja Le Blanc

Calculate Sun data from date (2)

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caluculates B0 (radians), position angle and sun radius (arcsec) B0 - heliographic latitude of the centre of disk position angle - of the north end of the axis of rotation, measured +ve if east of the north point of the disk radius - the apparent radus of the Sun in arcsec This is created using the calculations from the IDL routine get_sun.pro

Created: 2011-02-15 | Last updated: 2011-03-02

Credits: Anja Le Blanc

Converting from heliocentric coordinate sy... (1)

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Converting from heliocentric coordinate system with coordinates in arcsec to coordinates in longitude latitude Based on the IDL script xy2lonlat.pro http://hesperia.gsfc.nasa.gov/ssw/gen/idl/solar/xy2lonlat.pro Stonyhurst Heliographic Coordinate System to Helioprojective-Cartesian Coordinate System

Created: 2011-02-18 | Last updated: 2011-02-18

Credits: Anja Le Blanc

Associate goes X ray flares with active r... (1)

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This workflow is querying the HFC ActiveRegions list and HEC goes_xray_flare list. It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: HFCout is a modified VOTable where a field is added with the number of associated hessi flares. combined_output is a 2 dimensional list with an VOTable for each Active region and one with an VOTable for all associated flares for that Active Region.

Created: 2011-02-18 | Last updated: 2011-02-18

Credits: Anja Le Blanc

Associate flares with active regions (1)

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This workflow is querying the HFC ActiveRegions list and HEC flare lists (names retrieved from the ontlogoy) It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: HFCout is a modified VOTable where a field per flare list is added with the number of associated flares. combined_output is a 2 dimensional list with an VOTable for each Active region and each one with an VOTable for all associated flares for that Active Region.

Created: 2011-02-22 | Last updated: 2011-08-24

Credits: Anja Le Blanc

Attributions: Associate goes X ray flares with active regions Associate hessi flares with active regions

Extract content of columns from VOTables (3)

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Extracts all values from all columns which are passed from the input ColumnNames

Created: 2011-02-24 | Last updated: 2012-08-20

Credits: Anja Le Blanc

Converting from coordinates in longitude l... (1)

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Based on lonlat2xy.pro Converts from Helioprojective-Cartesian Coordinate System to Stonyhurst Heliographic Coordinate SystemBased on lonlat2xy.pro http://hesperia.gsfc.nasa.gov/ssw/gen/idl/solar/lonlat2xy.pro Converts from Helioprojective-Cartesian Coordinate System to Stonyhurst Heliographic Coordinate System

Created: 2011-03-02 | Last updated: 2011-03-02

Credits: Anja Le Blanc

MDES simple execution (2)

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workflow to query MDES, obtaining the DES results and from it extracting the VOTable and the PNG plot for the time range queried.

Created: 2011-03-02 | Last updated: 2014-03-12

Credits: Anja Le Blanc

Find instruments of a special type in a se... (1)

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This workflow takes a type of isnstrument as input and the minimum and maxium coordinates in HCI as input. Cadence for the location service is for defining the 'continues' presence. Output is a VOTable based on the ICS return where two columns are added for the time this instrument has entered and exited the Region of Interest.

Created: 2011-08-24 | Last updated: 2011-08-24

Credits: Anja Le Blanc

Find instruments of a special type in a se... (1)

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This workflow takes a type of isnstrument as input and the minimum and maxium coordinates in HCI as input. Cadence for the location service is for defining the 'continues' presence. Output is a VOTable based on the ICS return where two columns are added for the time this instrument has entered and exited the Region of Interest.

Created: 2011-08-24 | Last updated: 2011-08-24

Credits: Anja Le Blanc

Attributions: Find instruments of a special type in a section of space described in HCI coordinates

Basic Call of HELIO Coordinate Transformat... (1)

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Transforms an input VOTable Coordinate set to a specified output VOTable Coordinate set. This workflow performs some remote computation and may take some time to complete.

Created: 2011-11-08 | Last updated: 2011-11-08

Credits: Anja Le Blanc

Basic Call of HELIO Coordinate Transformat... (2)

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Transforms an input VOTable Coordinate set to a specified output VOTable Coordinate set. This workflow performs some remote computation and may take some time to complete.

Created: 2011-11-09 | Last updated: 2012-07-09

Credits: Anja Le Blanc

Attributions: Basic Call of HELIO Coordinate Transformation Service

Split VOTable into its values (1)

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This workflow takes a single VOTable and splits it up in a vector for the names of fields, a vector for the UCDs of the fields, a vector for the UTypes of the fields, and a two dimensional vector for the values.

Created: 2012-03-14 | Last updated: 2012-03-14

Credits: Anja Le Blanc

VOTable of NED Images from a List of Objects (1)

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Extraction of metadata using NED Image Virtual Observatory Service into a single VOTable, providing a list of objects and the width for each field in arcmin. Among the most relevant metadata are the URL link to the FITS images. This Wf makes use of a Tool developed as an internal pyhton script file.

Created: 2012-07-01 | Last updated: 2012-07-01

Credits: Jose Enrique Ruiz

Attributions: Astronomical object name to equatorial coordinates Resolver

Intialize Sample (2)

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This workflow saves a tabular *.pckl Python pickle dataset in the local file system, containing values calculated on physical parameters associated to potential companions of a sample of target galaxies. These original physical parameters are extracted from a postgreSQL database, containing information of all galaxies covered by the SDSS spectroscopic survey. The workflow first access the external database located in the AMIGA server and selects the target galaxies from the sample (those havi...

Created: 2013-01-04 | Last updated: 2013-01-05

Credits: Juandesant Jsm

Environment (2)

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From a previously selected cube of galaxies residing in a remote database, we provide extragalactic environment parameters for all galaxies sample. This workflow takes as input the path of the tabular *.pckl Python pickle dataset created in the previous workflow, as well as the database connection settings and several criteria on how to filter the potential companions of the target galaxies. It provides a file with the SDSS identifiers of each target galaxy of the sample, environmental estim...

Created: 2013-01-04 | Last updated: 2013-01-14

Credits: Juandesant Jsm