Wine and Cheese Spring 2020: Difference between revisions

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'''Deprojecting Astronomical Sky Maps'''<br>
'''Deprojecting Astronomical Sky Maps'''<br>
We see the sky in 2D but, in order to conduct astrophysical studies, we need 3D information. I will show how to take any large-scale map of the sky, at any wavelength, and extract 3D extragalactic information from it using clustering measurements. I will then apply this technique to observations of galaxies and diffuse components across the electromagnetic spectrum.
We see the sky in 2D but, in order to conduct astrophysical studies, we need 3D information. I will show how to take any large-scale map of the sky, at any wavelength, and extract 3D extragalactic information from it using clustering measurements. I will then apply this technique to observations of galaxies and diffuse components across the electromagnetic spectrum.
=10 February =
==Alberto Bolatto (UMd) ==
'''Synergies Between IFU and Molecular Gas Surveys'''
The internal structure of galaxies harbors important clues of the processes that shape their evolution. The last several years have seen the completion of a number of galaxy surveys using Integral Field Units that produce complete spectroscopic mapping at optical wavelengths (MaNGA, CALIFA, SAMI). Those data have produced invaluable information about the stellar and ionized gas components of galaxies. Information about the neutral and molecular phases of the gas, the largest gas reservoirs, has however historically lagged behind. I will present some results from EDGE-CALIFA, a follow up of 126 CALIFA galaxies in CO emission that is currently starting to be expanded with ALMA, and I will discuss future prospects with existing and planned instruments, in particular the ngVLA (a proposal to the Astro2020 Decadal).

Revision as of 17:57, 31 January 2020

This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Spring 2020.

Wine and Cheese sessions with one talk will have a 50 minute talk with 10 minutes for questions. Sessions with two speakers will have two 25 minute talks, each with 5 minutes for questions. Sessions in the Graduate Student Series will have three 15 minute talks, each with 5 minutes for questions.

Back to W&C Schedule

3 February

Brice Menard (JHU)

Deprojecting Astronomical Sky Maps
We see the sky in 2D but, in order to conduct astrophysical studies, we need 3D information. I will show how to take any large-scale map of the sky, at any wavelength, and extract 3D extragalactic information from it using clustering measurements. I will then apply this technique to observations of galaxies and diffuse components across the electromagnetic spectrum.

10 February

Alberto Bolatto (UMd)

Synergies Between IFU and Molecular Gas Surveys The internal structure of galaxies harbors important clues of the processes that shape their evolution. The last several years have seen the completion of a number of galaxy surveys using Integral Field Units that produce complete spectroscopic mapping at optical wavelengths (MaNGA, CALIFA, SAMI). Those data have produced invaluable information about the stellar and ionized gas components of galaxies. Information about the neutral and molecular phases of the gas, the largest gas reservoirs, has however historically lagged behind. I will present some results from EDGE-CALIFA, a follow up of 126 CALIFA galaxies in CO emission that is currently starting to be expanded with ALMA, and I will discuss future prospects with existing and planned instruments, in particular the ngVLA (a proposal to the Astro2020 Decadal).