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ZFOURGE

Visually Explore the Fields = http:/ zfourge.tamu.edu/DR2016/data.html. Galaxy formation and evolution at redshifts z 1. The FourStar Galaxy Evolution Survey (ZFOURGE) is a large and deep medium-band imaging survey aimed at establishing an observational benchmark of galaxy properties at redshift z 1. ZFOURGE survey is carried out using an extremely efficient near-infrared FOURSTAR instrument on the Magellan telescope, in three HST legacy fields: COSMOS, CDFS, and UDS.

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ZFOURGE | zfourge.tamu.edu Reviews
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Visually Explore the Fields = http:/ zfourge.tamu.edu/DR2016/data.html. Galaxy formation and evolution at redshifts z 1. The FourStar Galaxy Evolution Survey (ZFOURGE) is a large and deep medium-band imaging survey aimed at establishing an observational benchmark of galaxy properties at redshift z 1. ZFOURGE survey is carried out using an extremely efficient near-infrared FOURSTAR instrument on the Magellan telescope, in three HST legacy fields: COSMOS, CDFS, and UDS.
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ZFOURGE | zfourge.tamu.edu Reviews

https://zfourge.tamu.edu

Visually Explore the Fields = http:/ zfourge.tamu.edu/DR2016/data.html. Galaxy formation and evolution at redshifts z 1. The FourStar Galaxy Evolution Survey (ZFOURGE) is a large and deep medium-band imaging survey aimed at establishing an observational benchmark of galaxy properties at redshift z 1. ZFOURGE survey is carried out using an extremely efficient near-infrared FOURSTAR instrument on the Magellan telescope, in three HST legacy fields: COSMOS, CDFS, and UDS.

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zfourge.tamu.edu zfourge.tamu.edu
1

Publications | ZFOURGE

http://zfourge.tamu.edu/publications

The Fourstar Galaxy Evolution Survey (ZFOURGE): Ultraviolet to Far-Infrared Catalogs, Medium-Bandwidth Photometric Redshifts with Improved Accuracy, Stellar Masses, and Confirmation of Quiescent Galaxies to z 3.5. Straatman et al. 2016,. Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25. Rees et al. 2016,. Monthly Notices of the Royal Astronomical Society. Forrest et al. 2016,. Tomczak et al. 2016, Astrophysical Journal. Straatm...

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Data | ZFOURGE

http://zfourge.tamu.edu/DR2016/data.html

Visually explore the fields. For ZFOURGE data inquiries (e.g. catalogs, photometry), please contact Caroline Straatman [straatman AT mpia.de], Ivo Labbe [ivo AT strw.leidenuniv.nl], or Lee Spitler [lee.spitler AT mq.edu.au]. For website issues (e.g. broken links, info updates), please contact Kim-Vy Tran [kimvy.tran AT tamu.edu].

3

Survey | ZFOURGE

http://zfourge.tamu.edu/survey

5 sigma AB magnitude depths (CDFS, COSMOS, UDS; D=0.6” apertures). Ks depths correspond to a co-addition of the Fourstar imaging with public Ks-band imaging. 03 32 27, -27 45 52]. 128 sq. arcmin]. 10 00 31, 02 17 03]. 135 sq. arcmin]. 02 17 15, -05 11 53]. 189 sq. arcmin]. Completeness corrected number counts for each field observed with ZFOURGE. Sources with.

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Team | ZFOURGE

http://zfourge.tamu.edu/team

5

Science | ZFOURGE

http://zfourge.tamu.edu/science

The FourStar Galaxy Evolution Survey (ZFOURGE) aims to establish an observational benchmark of galaxy properties at z 1 by deriving 1-2% accurate redshifts of 60,000 galaxies at 1 z 3. Most normal L galaxies during this crucial epoch are too faint for spectroscopy, which has forced us to rely on inaccurate broadband photometric redshifts in the past. In response, we have equipped FourStar. With innovative medium-bandwidth filters from 1 1.8μm. Which enable accurate and robust redshifts to z = 3.5. The ev...

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high-redshift research - lee spitler

https://sites.google.com/site/leespitler/high_redshift

My first high-redshift (distant) paper is about the discovery of a galaxy cluster located 10.5 billion light years from Earth. It was discovered in the first semester of imaging data from the Z-FOURGE survey. We are using medium-band filters on the new FourStar camera at the Magellan Baade telescope. To obtain distances to distant galaxies at unprecedented accuracies over a spatially-complete region of the sky. The scientific paper describing the galaxy cluster is available here.

zfire.swinburne.edu.au zfire.swinburne.edu.au

ZFIRE

http://zfire.swinburne.edu.au/data.html

We release galaxy redshift catalogue and 1D spectra for 2 cluster fields for observations carried out between 2013 2015 over 13 MOSFIRE nights. MOSFIRE nights were awarded to the ZFIRE program by a combination of Swinburne University (Program IDs- 2013A W163M, 2013B W160M, 2014A W168M, 2015A W193M), Australian National University (Program IDs- 2013B Z295M, 2014A Z225M, 2015A Z236M), and NASA (Program IDs- 2013A N105M, 2014A N121M) telescope time allocation committees. Release date: 4th July 2016.

zfire.swinburne.edu.au zfire.swinburne.edu.au

ZFIRE

http://zfire.swinburne.edu.au/team.html

Pindarie Winery, Barossa Valley, South Australia. Lyndoch Hill, Barossa Valley, South Australia. Keck-I Control Room, Waimea, Hawai'i. The ZFIRE Team recognizes and acknowledges the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

zfire.swinburne.edu.au zfire.swinburne.edu.au

ZFIRE

http://zfire.swinburne.edu.au/index.html

A Keck/MOSFIRE spectroscopic survey of star-forming galaxies in rich enviornments during cosmic-noon. With the growing number of confirmed galaxy clusters at z 2, it is now possible to track how baryons cycle between stars, winds, and the ISM when cluster galaxies are still forming a large fraction of their stars. ZFIRE combines imaging from the Hubble Space Telescope. With deep spectroscopy from Keck Observatory.

zfire.swinburne.edu.au zfire.swinburne.edu.au

ZFIRE PUBLICATIONS

http://zfire.swinburne.edu.au/publications.html

ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift 2.0. ZFIRE: SIMILAR STELLAR GROWTH IN H-Alpha EMITTING CLUSTER AND FIELD GALAXIES AT Z 2. ZFIRE: A KECK/MOSFIRE Spectroscopic Survey of Galaxies in Rich Environments at z 2. Cold-mode accretion: Driving the fundamental mass-metallicity relation at z 2. ZFIRE: The Kinematics of Star-Forming Galaxies as a Function of Environment at z 2. ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift 2.0. Kewley et al....

zfire.swinburne.edu.au zfire.swinburne.edu.au

ZFIRE

http://zfire.swinburne.edu.au/science.html

ZFIRE is a multi-year program with 12 nights awarded thus far on Keck (although 7 were lost to poor weather conditions). To reach the target depths for 3-5 galaxy clusters, the survey require 20 nights on Keck by 2017. The ZFIRE Team recognizes and acknowledges the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

saoastronews.wordpress.com saoastronews.wordpress.com

Sudden death of very early galaxies | SAO astro news

https://saoastronews.wordpress.com/2014/03/13/sudden-death-of-very-early-galaxies

About SAO astro news. Detection of gravitational waves →. Sudden death of very early galaxies. March 13, 2014. The first galaxies that formed in the universe might have matured sooner than expected. New results from an international team of astronomers, including researchers from Swinburne University, indicate that some of the most distance galaxies are much more ‘mature’ than expected. When we look into the distant universe, we are also looking back in time. The FourStar Galaxy Evolution ( ZFOURGE.

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Visually Explore the Fields = http:/ zfourge.tamu.edu/DR2016/data.html. Galaxy formation and evolution at redshifts z 1. The FourStar Galaxy Evolution Survey (ZFOURGE) is a large and deep medium-band imaging survey aimed at establishing an observational benchmark of galaxy properties at redshift z 1. ZFOURGE survey is carried out using an extremely efficient near-infrared FOURSTAR instrument on the Magellan telescope, in three HST legacy fields: COSMOS, CDFS, and UDS.

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