Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
In order to understand the formation and subsequent evolution of galaxies one must first distinguish between the two main morphological classes of massive systems: spirals and early-type systems. This paper introduces a project, Galaxy Zoo, which provides visual morphological classifications for nea...
| Main Authors: | , , , , , , , , , , , |
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| Format: | Journal article |
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2008
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| _version_ | 1797077345526349824 |
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| author | Lintott, C Schawinski, K Slosar, A Land, K Bamford, S Thomas, D Raddick, M Nichol, R Szalay, A Andreescu, D Murray, P Berg, J |
| author_facet | Lintott, C Schawinski, K Slosar, A Land, K Bamford, S Thomas, D Raddick, M Nichol, R Szalay, A Andreescu, D Murray, P Berg, J |
| author_sort | Lintott, C |
| collection | OXFORD |
| description | In order to understand the formation and subsequent evolution of galaxies one must first distinguish between the two main morphological classes of massive systems: spirals and early-type systems. This paper introduces a project, Galaxy Zoo, which provides visual morphological classifications for nearly one million galaxies, extracted from the Sloan Digital Sky Survey (SDSS). This achievement was made possible by inviting the general public to visually inspect and classify these galaxies via the internet. The project has obtained more than 40,000,000 individual classifications made by ~100,000 participants. We discuss the motivation and strategy for this project, and detail how the classifications were performed and processed. We find that Galaxy Zoo results are consistent with those for subsets of SDSS galaxies classified by professional astronomers, thus demonstrating that our data provides a robust morphological catalogue. Obtaining morphologies by direct visual inspection avoids introducing biases associated with proxies for morphology such as colour, concentration or structual parameters. In addition, this catalogue can be used to directly compare SDSS morphologies with older data sets. The colour--magnitude diagrams for each morphological class are shown, and we illustrate how these distributions differ from those inferred using colour alone as a proxy for morphology. |
| first_indexed | 2024-03-07T00:16:35Z |
| format | Journal article |
| id | oxford-uuid:7b0b4986-b420-4bbf-947e-ca5c89dc574e |
| institution | University of Oxford |
| last_indexed | 2024-03-07T00:16:35Z |
| publishDate | 2008 |
| record_format | dspace |
| spelling | oxford-uuid:7b0b4986-b420-4bbf-947e-ca5c89dc574e2022-03-26T20:48:10ZGalaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky SurveyJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7b0b4986-b420-4bbf-947e-ca5c89dc574eSymplectic Elements at Oxford2008Lintott, CSchawinski, KSlosar, ALand, KBamford, SThomas, DRaddick, MNichol, RSzalay, AAndreescu, DMurray, PBerg, JIn order to understand the formation and subsequent evolution of galaxies one must first distinguish between the two main morphological classes of massive systems: spirals and early-type systems. This paper introduces a project, Galaxy Zoo, which provides visual morphological classifications for nearly one million galaxies, extracted from the Sloan Digital Sky Survey (SDSS). This achievement was made possible by inviting the general public to visually inspect and classify these galaxies via the internet. The project has obtained more than 40,000,000 individual classifications made by ~100,000 participants. We discuss the motivation and strategy for this project, and detail how the classifications were performed and processed. We find that Galaxy Zoo results are consistent with those for subsets of SDSS galaxies classified by professional astronomers, thus demonstrating that our data provides a robust morphological catalogue. Obtaining morphologies by direct visual inspection avoids introducing biases associated with proxies for morphology such as colour, concentration or structual parameters. In addition, this catalogue can be used to directly compare SDSS morphologies with older data sets. The colour--magnitude diagrams for each morphological class are shown, and we illustrate how these distributions differ from those inferred using colour alone as a proxy for morphology. |
| spellingShingle | Lintott, C Schawinski, K Slosar, A Land, K Bamford, S Thomas, D Raddick, M Nichol, R Szalay, A Andreescu, D Murray, P Berg, J Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey |
| title | Galaxy Zoo : Morphologies derived from visual inspection of galaxies
from the Sloan Digital Sky Survey |
| title_full | Galaxy Zoo : Morphologies derived from visual inspection of galaxies
from the Sloan Digital Sky Survey |
| title_fullStr | Galaxy Zoo : Morphologies derived from visual inspection of galaxies
from the Sloan Digital Sky Survey |
| title_full_unstemmed | Galaxy Zoo : Morphologies derived from visual inspection of galaxies
from the Sloan Digital Sky Survey |
| title_short | Galaxy Zoo : Morphologies derived from visual inspection of galaxies
from the Sloan Digital Sky Survey |
| title_sort | galaxy zoo morphologies derived from visual inspection of galaxies from the sloan digital sky survey |
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