ZFIRE

A KeckMOSFIRE 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.

OVERVIEW

The domain zfire.swinburne.edu.au presently has an average traffic classification of zero (the smaller the better). We have crawled five pages within the website zfire.swinburne.edu.au and found two websites linking to zfire.swinburne.edu.au.
Pages Parsed
5
Links to this site
2

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LINKS TO ZFIRE.SWINBURNE.EDU.AU

Themiya Nanayakkara

Postdoc and Ex-Graduate student at Swinburne University of Technology. Infrared Astronomy, spectroscopy, extragalactic astrophysics. Centre for Astrophysics and Supercomputing, Swinburne University of Technology. Teams I have also participated in the Deeper-Wider-faster survey. Mauna Kea summit overlooking the Keck observatory.

WHAT DOES ZFIRE.SWINBURNE.EDU.AU LOOK LIKE?

Desktop Screenshot of zfire.swinburne.edu.au Mobile Screenshot of zfire.swinburne.edu.au Tablet Screenshot of zfire.swinburne.edu.au

ZFIRE.SWINBURNE.EDU.AU SERVER

We diagnosed that a single root page on zfire.swinburne.edu.au took four thousand four hundred and six milliseconds to download. I could not discover a SSL certificate, so therefore we consider zfire.swinburne.edu.au not secure.
Load time
4.406 sec
SSL
NOT SECURE
IP
136.186.1.61

SERVER SOFTWARE

We discovered that this domain is using the Apache/2.2.29 (Unix) DAV/2 mod_ssl/2.2.29 OpenSSL/1.0.1e-fips os.

SITE TITLE

ZFIRE

DESCRIPTION

A KeckMOSFIRE 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.

PARSED CONTENT

The domain states the following, "A KeckMOSFIRE spectroscopic survey of star-forming galaxies in rich enviornments during cosmic-noon." I observed that the web page also stated " 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." They also stated " ZFIRE combines imaging from the Hubble Space Telescope. With deep spectroscopy from Keck Observatory."

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