Jun 4

Analyzing Cosmic Clusters

Striking image shows mass distribution of nearby galaxy cluster

Striking image shows mass distribution of nearby galaxy cluster 
Using the Dark Energy Camera at Cerro Tololo Inter-American Observatory, a Program of NSF’s NOIRLab, astronomers are measuring weak gravitational lensing to map the distribution of mass in nearby galaxy clusters. As well as producing remarkable images like this one, the information will shed light on the relationships between the constituent parts of nearby galaxy clusters, such as gas, stellar populations, and dark matter.

The galaxy cluster Abell 3827 is the subject of this striking image. In addition to featuring a field of galaxies and foreground stars, the image is overlaid with a map with hues of red, blue and purple. Though they are attractive, these colors aren’t for decoration — they represent the distribution of mass in the heart of Abell 3827 with red showing the largest mass concentration.

Credit: CTIO/NOIRLab/NSF/AURA

Release Images

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noirlab2012a – Striking image shows mass distribution of nearby galaxy cluster

Using the Dark Energy Camera at Cerro Tololo Inter-American Observatory, a Program of NSF’s NOIRLab, astronomers are measuring weak gravitational lensing to map the distribution of mass in nearby galaxy clusters. As well as producing remarkable images like this one, the information will shed light on the relationships between the constituent parts of nearby galaxy clusters, such as gas, stellar populations, and dark matter.

The galaxy cluster Abell 3827 is the subject of this striking image. In addition to featuring a field of galaxies and foreground stars, the image is overlaid with a map with hues of red, blue and purple. Though they are attractive, these colors aren’t for decoration — they represent the distribution of mass in the heart of Abell 3827 with red showing the largest mass concentration.

Credit: CTIO/NOIRLab/NSF/AURA

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noirlab2012b – Excerpt of main image with lensing map

Galaxy clusters are massive conglomerations of hundreds or even thousands of galaxies, bound together by their mutual gravitational attraction.

Credit: CTIO/NOIRLab/NSF/AURA

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noirlab2012c – Main image without lensing map

This image is a snapshot from the Local Volume Complete Cluster Survey (LoVoCCS), a survey program investigating 107 nearby galaxy clusters.

Credit: CTIO/NOIRLab/NSF/AURA

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noirlab2012d – Excerpt of main image without lensing map

LoVoCCS takes advantage of an astrophysical phenomenon called weak gravitational lensing to measure the mass and matter distributions of these clusters.

Credit: CTIO/NOIRLab/NSF/AURA

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noirlab2012e – Illustration of weak lensing

Weak lensing allows us to map the structure of the Universe, both the dark matter that comprises the cosmic web as well as the luminous matter that traces it. By measuring statistical changes to alignments of distant galaxies, the masses of astronomical objects can be measured.

Credit: NOIRLab/NSF/AURA

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Using the Dark Energy Camera at Cerro Tololo Inter-American Observatory, a Program of NSF’s NOIRLab, astronomers are measuring weak gravitational lensing to map the distribution of mass in nearby galaxy clusters. As well as producing remarkable images like this one, the information will shed light on the relationships between the constituent parts of nearby galaxy clusters, such as gas, stellar populations, and dark matter.

The galaxy cluster Abell 3827 is the subject of this striking image. In addition to featuring a field of galaxies and foreground stars, the image is overlaid with a map with hues of red, blue and purple. Though they are attractive, these colors aren’t for decoration — they represent the distribution of mass in the heart of Abell 3827 with red showing the largest mass concentration.

Galaxy clusters are massive conglomerations of hundreds or even thousands of galaxies, bound together by their mutual gravitational attraction. They are among the most massive astrophysical objects known, weighing thousands of times as much as the Milky Way, and they contain vast amounts of high-temperature intergalactic gas and dark matter.

This image is a snapshot from the Local Volume Complete Cluster Survey (LoVoCCS), a survey program investigating 107 nearby galaxy clusters. LoVoCCS takes advantage of an astrophysical phenomenon called weak gravitational lensing to measure the mass and matter distributions of these clusters.

Gravitational lensing occurs when a massive astronomical object such as Abell 3827 distorts light from a background object. This distortion is proportional to the mass of the foreground object, making gravitational lensing a powerful way for astronomers to determine the masses of distant objects. While strong gravitational lensing can appear to duplicate or warp distant galaxies, creating intricate rings and arcs, the subtle signs of weak gravitational lensing can only be measured statistically [1].

By averaging the tiny distortions of the many background galaxies visible in this image, the LoVoCCS team were able to create a detailed map of Abell 3827’s mass distributions. These measurements — and those from the other galaxy clusters in the LoVoCCS survey — will allow astronomers to shed light on the relation between the stellar populations, gas, and dark matter in nearby galaxy clusters.

To gather the information required for the survey, the LoVoCCS team are using the Dark Energy Camera (DECam), a high-performance instrument mounted on the Victor M. Blanco 4m telescope at Cerro Tololo Inter-American Observatory (CTIO). Originally built to undertake the Dark Energy Survey, DECam now supports a wide variety of astronomical programs, both large and small. Read more about LoVoCCS in the latest edition of NOIRLab’s newsletter, The NOIRLab Mirror.

Notes

[1] Strong gravitational lensing can produce conspicuous arcs, rings, and even celestial doppelgängers. The first gravitationally lensed object to be detected, the Twin Quasar, appears in duplicate as a result of the lensing effect of an intervening galaxy.

More information

The LoVoCCS collaboration consists of Ranga-Ram Chary (IPAC/Caltech), Doug Clowe (Ohio), MichaelCooper (UC Irvine), Ian Dell’Antonio (Brown, PI), Megan Donahue (Michigan State), Gus Evrard (Michigan), Shenming Fu (Brown), Mark Lacy (NRAO), Tod Lauer (NOIRLab), Binyang Liu (Brown), Jacqueline McCleary (NASA/JPL), Massimo Meneghetti (INAF/Bologna), Hironao Miyatake (Nagoya Univ.), Priyamvada Natarajan (Yale), Elena Pierpaoli (USC), Marc Postman (STScI), Jubee Sohn (SAO), Keiichi Umetsu (ASIAA), Yousuke Utsumi (SLAC/Stanford), and Gillian Wilson (UC Riverside).

NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab), the US center for ground-based optical-infrared astronomy, operates the international Gemini Observatory (a facility of NSF, NRC–Canada, ANID–Chile, MCTIC–Brazil, MINCyT–Argentina, and KASI–Republic of Korea), Kitt Peak National Observatory (KPNO), Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), and the Vera C. Rubin Observatory. It is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF and is headquartered in Tucson, Arizona. The astronomical community is honored to have the opportunity to conduct astronomical research on Iolkam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawaiʻi, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence that these sites have to the Tohono O’odham Nation, to the Native Hawaiian community, and to the local communities in Chile, respectively.

Contacts:

Amanda Kocz
Press and Internal Communications Officer
NSF’s NOIRLab
Cell: +1 626 524 5884
Email: akocz@aura-astronomy.org

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