Computing in science.

  title={Computing in science.},
  author={John I. Brauman},
  volume={261 5123},
A bottom-heavy initial mass function for the accreted blue-halo stars of the Milky Way
We use Gaia DR2 to measure the initial mass function (IMF) of stars within 250 pc and masses in the range 0.2 100 km/s or v_T > 200 km/s, and located above the isochrone on the HRD with metallicity
BAT AGN Spectroscopic Survey – XIII. The nature of the most luminous obscured AGN in the low-redshift universe
We present a multiwavelength analysis of 28 of the most luminous low-redshift narrow-line, ultra-hard X-ray-selected active galactic nuclei (AGN) drawn from the 70-month Swift/BAT all-sky survey,
3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3: Its Relation to Cluster Dynamics
We analyze the 3D morphology and kinematics of 13 open clusters (OCs) located within 500 pc of the Sun, using Gaia EDR 3 and kinematic data from the literature. Members of OCs are identified using
Exploring the relation between dust mass and galaxy properties using Dusty SAGE
We explore the relation between dust and several fundamental properties of simulated galaxies using the Dusty SAGE semi-analytic model. In addition to tracing the standard galaxy properties, Dusty
Eigenspectra: a framework for identifying spectra from 3D eclipse mapping
Planetary atmospheres are inherently 3D objects that can have strong gradients in latitude, longitude, and altitude. Secondary eclipse mapping is a powerful way to map the 3D distribution of the
Searching the Entirety of Kepler Data. I. 17 New Planet Candidates Including One Habitable Zone World
We present the results of an independent search of all ~200,000 stars observed over the four year Kepler mission (Q1-Q17) for multiplanet systems, using a three-transit minimum detection criteria to
The abundance and physical properties of O vii and O viii X-ray absorption systems in the EAGLE simulations
We use the EAGLE cosmological, hydrodynamical simulations to predict the column density and equivalent width distributions of intergalactic O vii ($E=574 \, \rm {eV}$) and O viii ($E=654 \, \rm
What chemists (or chemistry students) need to know about computing
Key points developed here include: the computer as a tool for learning study, research, and communication; hardware, software, computing concepts and other teaching concerns; and the appropriate place for chemistry computer usage instruction.
ShapeNet: Shape Constraint for Galaxy Image Deconvolution
Deep learning (DL) has shown remarkable results in solving inverse problems in various domains. In particular, the Tikhonet approach is very powerful in deconvolving optical astronomical images.