COSMOS data across many different wavelengths, including X-ray, infrared and radio, has been used to set the record for the most distant galaxy cluster ever discovered. We may be seeing the cluster, named CL J1001+0220, just after it's formation and while it is in the process of a big 'baby-boom' of star formation.
A further 1500h of Spitzer time has been awarded to complete a survey of the COSMOS field. The program has been approved in Spitzer Cycle-13 to PI I. Labbe and COSMOS Co-I Karina Caputi. This will complete the legacy of Spitzer/IRAC over COSMOS by extending the deep coverage to cover the full 1.8 sq degree field, producing a nearly homogenous and contiguous map unparalleled in terms of area and depth. This will complement ongoing optical-to-NIR surveys and reconfirm COSMOS as a unique field for probing the bright end of the z=6-11 universe and the formation of large-scale structures.
Several hours of highly competitive Atacama Large Millimeter Array (ALMA) Cycle 4 time has been awarded to COSMOS astronomers to target various objects in the COSMOS field. ALMA is a revolutionary millimetre/sub-millimeter telescope and COSMOS astronomers will use it to gain a deeper understanding of how galaxies formed and evolved. They will study how the galaxy environment impacts star formation, examine the sizes and structures of enigmatic sub-millimetre galaxies, reveal the properties of galaxies in the high redshift Universe, and more. Congratulations to everyone involved! See the full article for details of the successful proposals.
Quiescent galaxies do not form stars anymore, however, their population averaged size is increasing over time. Using stacked zCOSMOS spectra, Fagioli et al. measured their ages as a function of size and find that small galaxies are older than large ones. This indicates that the increase of the average size of quiescent galaxies with cosmic time is due to the addition of newly quenched, bigger star-forming galaxies at later times to the quiescent population. This is not true anymore for the most massive galaxies, which individually grow in size, possibly due to dry mergers.
This new study uses the COSMOS survey to measure the local environment (density) around galaxies at z < 3 and connects it to their star formation rates. The study suggests that the shutdown of star formation due to galaxies falling into dense environment (e.g., causing stripping and heating of gas) is dominant at z < 1. At higher redshifts, quenching of star formation is likely triggered by galaxy internal processes (feedback, etc).
A new paper by COSMOS member Andreas Faisst and team shows how to use Spitzer colors to derive emission line properties of 3 < z < 6 galaxies. Optical emission lines at z > 4 cannot be measured spectroscopically with current facilities. Since emission lines "contaminate" the Spitzer 3.6um and 4.5um channels, these can be used to estimate optical line emission without the need of spectra. The study of emission lines provides important information about galaxy formation in the early universe and also provides a sample of galaxies for future JWST follow-up. The ApJ paper is in print and can be retrieved here: http://stacks.iop.org/0004-637X/821/122
Winds and outflows of gas in quasars are thought to have a significant impact on their host galaxies. A group of researchers, led by COSMOS's Marcella Brusa, have mapped the kinematics of quasar XID5395, a merging luminous quasar at z=1.5. The team identified this curious object using extensive COSMOS multiwavength data. They then observed XID5395 with the Subaru telescope and the ESO/SINFONI spectrograph and found the quasar to be in a turbulent situation. Winds up to 1300km/s, induced by the nuclear activity, are sweeping the surrounding gas outwards. It is thought that this will halt, or 'quench', star formation in the host galaxy of the quasar. XID5395 gives us a rare opportunity to see strong feedback in action and to study how this phenomenon impacts the evolutionary pathways of galaxies. Click here to read more about this galaxy caught in its life-changing phase.
COSMOS researcher Caitlin Casey has found that the formation of the most massive structures in the Universe — clusters of galaxies — happened with a bang! This conclusion was reached after looking in detail at galaxy protoclusters - collections of galaxies in the early Universe that may eventually form a galaxy cluster.
ESO’s VISTA survey telescope has spied a horde of previously hidden massive galaxies that existed when the Universe was in its infancy. By discovering and studying more of these galaxies than ever before, astronomers have, for the first time, found out exactly when such monster galaxies first appeared. Read the full press release here.
Researchers have found that 'starburst' galaxies in the Universe 9 billion years ago were more efficient at forming stars than average galaxies today. 'Starburst' galaxies display unusually huge bursts of newly-formed stars and are likely caused by a collision between two large galaxies. A new study published in Astrophysical Journal letters on October 15, led by John Silverman at the Kavli Institute for the Physics and Mathematics of the Universe, has helped to understand exactly why such huge bursts of star formation occur. The researchers used the new, sensitive Atacama Large Millimeter Array (ALMA) in Chile to study carbon monoxide (CO) gas in seven starburst galaxies that existed when the Universe was only four billion years old. They found that the amount of CO gas in these galaxies is not special, but that these galaxies seem to be particularly efficient at turning their gas into stars. This study also relied on a variety of powerful telescopes available through the COSMOS survey, including the Spitzer Observatory, the Herschel Observatory and the Subaru Telescope.
A research team, led by ETH Zurich researcher Benny Trakhtenbrot, has discovered a gigantic black hole that is much more massive than we expect it to be.
CONFIRMED: Galaxies contained far less dust in the early stages of their evolution! Using ALMA, COSMOS team leader Peter Capak and collaborators picked up the signature of [CII] (emitted by gas) and continuum (emitted by dust) in nine 'normal' galaxies at redshift 5 to 6 - only 1 billion years after the Big Bang.
We revealed the detailed shape and evolutionary behavior of the X-ray luminosity function of active galactic nuclei between 1