An international team of scientists led by Rutgers University astrophysicists has discovered 10 new massive galaxy clusters from a large, uniform survey of the southern sky. The survey was conducted using a breakthrough technique that detects "shadows" of galaxy clusters on the cosmic microwave background radiation, a relic of the "big bang" that gave birth to the universe.
In a paper published in the Nov. 10 issue of The Astrophysical Journal, the Rutgers scientists and collaborators at the Pontifical Catholic University of Chile (PUC) describe their visual telescope observations of these galaxy clusters, which were essential to verify the cosmic shadow sightings. Both observations will help scientists better understand how the universe was born and continues to evolve.
The research began in 2008 with a new radio telescope in the Atacama Desert of Chile -- one of the driest places on Earth. The instrument, known as the Atacama Cosmology Telescope (ACT), collects millimeter-length radio waves that reveal images of the otherwise invisible cosmic background radiation. Millimeter waves are easily blocked by water vapor, hence the telescope's home high in the Andes Mountains of northern Chile, where there is barely any atmospheric moisture.
"The groundbreaking observations at Atacama, led by Lyman Page of Princeton University, surveyed large areas of the sky to reveal shadows that pointed astronomers to these previously unseen massive galaxy clusters," said Felipe Menanteau, a research scientist in physics and astronomy, School of Arts and Sciences, at Rutgers.
Theorists Rashid Sunyaev and Yakov Zel'dovich predicted the shadow phenomenon 40 years ago, now known as the Sunyaev-Zel'dovich effect, or S-Z effect. Shortly thereafter astronomers verified it by observing shadows cast by previously known galaxy clusters. The higher sensitivity and resolution of ACT now makes it practical for astronomers to essentially reverse the procedure -- to search the cosmic background radiation for shadows that indicate the presence of unseen clusters.
"The 'shadows' that ACT revealed are not shadows in the traditional sense, as they are not caused by the galaxy clusters blocking light from another source," said Jack Hughes, professor of physics and astronomy at Rutgers. "Rather, the hot gases within the galaxy clusters cause a tiny fraction of the cosmic background radiation to shift to higher energies, which then makes them appear as shadows in one of ACT's observing bands."
Cosmic background radiation was first observed by two Bell Labs astronomers in New Jersey back in the 1960s, a discovery that earned them the Nobel Prize in Physics in 1978.
Hughes and Menanteau worked with Chilean professors Leopoldo Infante and Felipe Barrientos to collect optical images of dozens of candidates, which led to the discovery of ten entirely new massive galaxy clusters. The Rutgers and PUC team, which also included PUC undergraduate student Jorge González, worked on two optical telescopes in Chile over the course of seven nights during October and December of 2009.
"We knew the experiment was working when we could see the giant clusters clearly, even in the raw images as they came through the telescope," said Menanteau.
"The technical challenges involved in exploiting the S-Z technique are daunting, and it is fantastic to see this method working so well," said Priyamvada Natarajan, professor of astronomy and physics at Yale University and a leading theoretical cosmologist not affiliated with the study. "It will build our inventory of the most massive and distant clusters in the universe, which will provide important constraints on the currently accepted cosmological model. I am personally excited to see the large number of strong lensing clusters that ACT is turning up."
The Rutgers and PUC observations were funded by the National Science Foundation's Partnerships for International Research and Education, in an award to Princeton with sub-awards to Rutgers and the University of Pennsylvania. The astronomers carried out their optical observations on the SOAR telescope in Cerro Pachón and the NTT in La Silla. The Atacama Cosmology Telescope project is funded by the National Science Foundation.
- Felipe Menanteau, Jorge González, Jean-Baptiste Juin, Tobias A. Marriage, Erik D. Reese, Viviana Acquaviva, Paula Aguirre, John William Appel, Andrew J. Baker, L. Felipe Barrientos, Elia S. Battistelli, J. Richard Bond, Sudeep Das, Amruta J. Deshpande, Mark J. Devlin, Simon Dicker, Joanna Dunkley, Rolando Dünner, Thomas Essinger-Hileman, Joseph W. Fowler, Amir Hajian, Mark Halpern, Matthew Hasselfield, Carlos Hernández-Monteagudo, Matt Hilton, Adam D. Hincks, Renée Hlozek, Kevin M. Huffenberger, John P. Hughes, Leopoldo Infante, Kent D. Irwin, Jeff Klein, Arthur Kosowsky, Yen-Ting Lin, Danica Marsden, Kavilan Moodley, Michael D. Niemack, Michael R. Nolta, Lyman A. Page, Lucas Parker, Bruce Partridge, Neelima Sehgal, Jon Sievers, David N. Spergel, Suzanne T. Staggs, Daniel Swetz, Eric Switzer, Robert Thornton, Hy Trac, Ryan Warne, Ed Wollack. The Atacama Cosmology Telescope: Physical Properties and Purity of a Galaxy Cluster Sample Selected via the Sunyaev-Zel'dovich Effect. The Astrophysical Journal, 2010; 723 (2): 1523 DOI: 10.1088/0004-637X/723/2/1523
Cite This Page: