The evolution of the star-forming interstellar medium across cosmic time
LJ Tacconi, R Genzel, A Sternberg - Annual Review of …, 2020 - annualreviews.org
Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …
Star-forming galaxies at cosmic noon
NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …
star-formation history, which culminated around; this period is often nicknamed “cosmic …
The IllustrisTNG simulations: public data release
We present the full public release of all data from the TNG100 and TNG300 simulations of
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …
First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time
We present a new cosmological, magnetohydrodynamical simulation for galaxy formation:
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …
PHIBSS: unified scaling relations of gas depletion time and molecular gas fractions
This paper provides an update of our previous scaling relations between galaxy-integrated
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
Wet compaction to a blue nugget: a critical phase in galaxy evolution
We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for∼ 100,000 galaxies
IG Momcheva, GB Brammer… - The Astrophysical …, 2016 - iopscience.iop.org
We present reduced data and data products from the 3D-HST survey, a 248-orbit HST
Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five …
Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five …
A dynamically cold disk galaxy in the early Universe
The extreme astrophysical processes and conditions that characterize the early Universe
are expected to result in young galaxies that are dynamically different from those observed …
are expected to result in young galaxies that are dynamically different from those observed …
What causes the formation of discs and end of bursty star formation?
As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
The data reduction pipeline for the SDSS-IV MaNGA IFU galaxy survey
ABSTRACT Map** Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical
fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs …
fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs …