Menéndez-Delmestre, Karín and Capak, Peter and Sheth, Kartik (2016) High-Redshift Protoclusters Traced by Submillimeter Galaxies: Tracing Star Formation Activity out to z > 4. In: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? IAU Symposium Proceedings Series. No.315. Cambridge University Press , Cambridge, pp. 1-2. ISBN 978-1-107-13520-8 http://resolver.caltech.edu/CaltechAUTHORS:20170109-144441145
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Clustering analysis indicate that at z ~ 2 submm-selected galaxies (SMGs) reside in very massive halos (M_(DM) > 5 × 10^(13)), suggesting that SMGs trace high-density environments that evolve into rich galaxy clusters. Conversely, recent work suggests that SMGs are tracers of a broader range of environments, including structures with more modest masses caught in highly active periods; since galaxies in these structures are likely caught during episodes of peak starbursts, SMGs may be tracers of a wider range of environments beyond the progenitors of todays very rich clusters, opening a window for a more complete exploration of the details underpinning the process of galaxy evolution in concert with the assembly of the large scale structure (LSS). We have undertaken a large observing program comprising deep narrow-band Ly-alpha imaging and multi-object spectroscopy using Palomar/Keck/Magellan/Gemini telescopes to probe for galaxy overdensities in SMG environments at z ~ 1 − 5. With ~200 spectroscopically-confirmed Ly-alpha emitters, we are in a position to gauge the level of galaxy overdensity in these regions.
|Item Type:||Book Section|
|Additional Information:||© 2016 International Astronomical Union. Published online: 12 September 2016.|
|Group:||COSMOS, Infrared Processing and Analysis Center (IPAC)|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||09 Jan 2017 23:36|
|Last Modified:||09 Jan 2017 23:36|
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