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Tag: galaxies

Workflow Curves Exploration (1)

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Exploration of curves of cubes that contain galaxy observations

Created: 2014-02-12

Credits: User Julian Garrido

Workflow Retrieve object properties from NED and VO... (4)

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From an initial list of galaxy names, retrieve some of their properties from Virtual Observatory archives and services (NASA Extragalactic Database NED), and calculate others like Distance, based on the ones previously obtained (e.g. recession velocity, equatorial and galactic coordinates). The sample is filtered in a later step with criteria related to the angular size of the object and its declination. The goal is to build a sample of objects and their properties with up-to-date physical in...

Created: 2013-04-25 | Last updated: 2013-06-27

Blob VOTable of AMIGA Galaxies

Created: 2013-04-23 16:12:52

Credits: User Jose Enrique Ruiz

License: Creative Commons Attribution-Share Alike 3.0 Unported License

This VOTable is provided by Vizier Service with ref: J_A+A_540_A47_table1 - AMIGA X: The AMIGA sample of isolated galaxies X. A First Look at Isolated Galaxy Colors. Fernandez Lorenzo et al. 2012

File type: Trident (Package)

Comments: 0 | Viewed: 52 times | Downloaded: 25 times

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

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

Credits: User Jose Enrique Ruiz

License: Creative Commons Attribution-Share Alike 3.0 Unported License

This document describes the "Luminosity Profiles" Research Object

File type: Adobe PDF

Comments: 0 | Viewed: 57 times | Downloaded: 108 times

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Blob Extraction of Properties from a Sample of Galaxies

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

Credits: User Jose Enrique Ruiz

License: Creative Commons Attribution-Share Alike 3.0 Unported License

This document describes the "Galaxies Sample Selection" Research Object

File type: Adobe PDF

Comments: 0 | Viewed: 57 times | Downloaded: 36 times

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Pack Galaxies Sample Selection Research Object


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

 In order to understand the evolution of galaxies, detailed analysis of images plays a key role. During the last years telescopes working at different wavelengths have been imaging the whole sky. One example of this is the Sloan Digital Sky Survey. The generated images provides a wealth of information, publicly available, and hence allowing them to be used by any interested group in the study of their own samples of objects or generation of new samples. The two main processing of the ima...

4 items in this pack

Comments: 0 | Viewed: 63 times | Downloaded: 22 times

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Pack Luminosity Profiles Research Object


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

In order to understand the evolution of galaxies, detailed analysis of images plays a key role. During the last years telescopes working at different wavelengths have been imaging the whole sky. One example of this is the Sloan Digital Sky Survey. The generated images provides a wealth of information, publicly available, and hence allowing them to be used by any interested group in the study of their own samples of objects or generation of new samples. The two main processing of the images ge...

7 items in this pack

Comments: 0 | Viewed: 57 times | Downloaded: 20 times

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Workflow 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: User Juandesant User Jsm

Workflow 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: User Juandesant User Jsm

Workflow Get completion function V / Vm using the a... (1)

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Get completion function V / Vm using the apparent magnitude list of a set of galaxies

Created: 2012-09-03 | Last updated: 2012-09-03

Credits: User Julian Garrido

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