COSMOS field

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Section of the COSMOS Field, taken in infrared light, with a total effective exposure time of 55 hours. Up to 2 million galaxies are in the picture.

The COSMOS Field, or the Cosmic Evolution Survey Deep Field, is a mosaic of deep space, which was photographed with the Hubble Space Telescope's Advanced Camera for Surveys [1] in segments from 2003 to 2004. It was the capstone of the COSMOS project, which aimed to observe and study how galaxies are affected by celestial environments.

Description[edit]

The project and COSMOS field was a study of the way in which galaxies are influenced by physical properties and the environment that surrounds them. The COSMOS field was chosen to be the focal point of research due to its abundance of galaxies and other celestial bodies, and its scarcity of gas. The research from the project has be used to identify deep-space galaxies and astrophysics.[2]

The Cosmic Evolution Survey (COSMOS)[3][4] was a wide field observational astronomy project. It was aimed at observing the correlation between galaxies, star formations, active galactic nuclei and dark matter[5] and how they evolve, with large-scale structures of the universe. The survey included imaging in multiple wavelengths and spectroscopic analysis from X-rays to radio waves, in a region of two square degrees in the Constellation Sextans.[6]

COSMOS, when it was proposed in 2003 as an exploratory survey to be carried out with the Advanced Camera for Surveys of the Hubble, was the largest HST project ever approved. Combined with the fact that the area of sky proposed as a survey had never been the subject of observations,[7] the project has stimulated the main world astronomical structures to explore the sky in this direction, thus resulting in one of the most substantial, deepest and most uniform data sets in the entire electromagnetic spectrum.[8]

2 million galaxies have been identified in the COSMOS field.[9] [10] NASA and the ESO studied the COSMOS region, the region in which the mosaic was taken, and further research is ongoing. The mosaic itself covers a 2 square degree equatorial field. The age of the galaxies differ, spanning 75% of the age of the observable universe.[11] HubbleSite states that "the COSMOS field is the largest contiguous survey of the universe, that covers two square degrees of sky. By comparison, the Earth's Moon is one-half degree across. The field is being imaged by most major space-based and ground-based telescopes". To compare, the well-known Hubble Ultra-Deep Field is the farthest visible view into the universe."[12] The COSMOS field is the largest-ever contiguous survey of the Universe, and was the largest Hubble project ever approved before the CANDELS project[13] was carried out from 2010 to 2013.[14]

Gallery[edit]

  • COSMOS field imaged by the Canada France Hawaii Telescope (CFHT). Red crosses mark some of the active galaxies with supermassive black holes at their centers.
    COSMOS field imaged by the Canada France Hawaii Telescope (CFHT). Red crosses mark some of the active galaxies with supermassive black holes at their centers.
  • The full mosaic composed of 575 separate ACS images
    The full mosaic composed of 575 separate ACS images
  • Sample of non-star-forming galaxies from the COSMOS survey
    Sample of non-star-forming galaxies from the COSMOS survey

See also[edit]

References[edit]

  1. ^ "WebbTelescope.org".
  2. ^ "For the Public". COSMOS. Retrieved 2024-03-26.
  3. ^ "COSMOS Overview". irsa.ipac.caltech.edu. Retrieved 2024-03-25.
  4. ^ Casey, Caitlin M.; Kartaltepe, Jeyhan S.; Drakos, Nicole E.; Franco, Maximilien; Harish, Santosh; Paquereau, Louise; Ilbert, Olivier; Rose, Caitlin; Cox, Isabella G. (2023-03-08), "COSMOS-Web: An Overview of the JWST Cosmic Origins Survey", The Astrophysical Journal, 954 (1): 31, arXiv:2211.07865, Bibcode:2023ApJ...954...31C, doi:10.3847/1538-4357/acc2bc
  5. ^ Darvish, Behnam; Mobasher, Bahram; Martin, D. Christopher; Sobral, David; Scoville, Nick; Stroe, Andra; Hemmati, Shoubaneh; Kartaltepe, Jeyhan (2017-03-01). "Cosmic Web of Galaxies in the COSMOS Field: Public Catalog and Different Quenching for Centrals and Satellites". The Astrophysical Journal. 837 (1): 16. arXiv:1611.05451. Bibcode:2017ApJ...837...16D. doi:10.3847/1538-4357/837/1/16. ISSN 0004-637X.
  6. ^ Ata, Metin; Kitaura, Francisco-Shu; Lee, Khee-Gan; Lemaux, Brian C.; Kashino, Daichi; Cucciati, Olga; Hernández-Sánchez, Mónica; Le Fèvre, Oliver (2021). "BIRTH of the COSMOS field: Primordial and evolved density reconstructions during cosmic high noon". Monthly Notices of the Royal Astronomical Society. 500 (3): 3194–3212. arXiv:2004.11027. doi:10.1093/mnras/staa3318.
  7. ^ academic.oup.com https://academic.oup.com/mnras/article/501/4/6103/6108279. Retrieved 2024-04-15. {{cite web}}: Missing or empty |title= (help)
  8. ^ "SEDS COSMOS Field". lweb.cfa.harvard.edu. Retrieved 2024-04-15.
  9. ^ Darvish, Behnam; Mobasher, Bahram; Martin, D. Christopher; Sobral, David; Scoville, Nick; Stroe, Andra; Hemmati, Shoubaneh; Kartaltepe, Jeyhan (February 2017). "Cosmic Web of Galaxies in the COSMOS Field: Public Catalog and Different Quenching for Centrals and Satellites". The Astrophysical Journal. 837 (1): 16. arXiv:1611.05451. Bibcode:2017ApJ...837...16D. doi:10.3847/1538-4357/837/1/16. ISSN 0004-637X.
  10. ^ Zatloukal, M.; Röser, H.-J.; Wolf, C.; Hippelein, H.; Falter, S. (2007-10-01). "Distant galaxy clusters in the COSMOS field found by HIROCS". Astronomy & Astrophysics. 474 (1): L5–L8. arXiv:0709.0411. Bibcode:2007A&A...474L...5Z. doi:10.1051/0004-6361:20078063. ISSN 0004-6361.
  11. ^ "Home Page". COSMOS. Retrieved 2024-03-25.
  12. ^ "HubbleSite".
  13. ^ Kartaltepe, Jeyhan (2012-07-04). "CANDELS: COSMOS: The Cosmic Evolution Survey". CANDELS. Retrieved 2024-04-17.
  14. ^ "Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey". IPAC. Retrieved 2024-04-17.

External links[edit]

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