Rapidly Evolving And Luminous Transients From PAN-STARRS1
Presents rapidly evolving and luminous transients discovered by Pan-STARRS1.
Presents rapidly evolving and luminous transients discovered by Pan-STARRS1.
The AAS will no longer print physical copies of its flagship journals the ApJ and AJ. What does this mean for our field?
Harvard University Department of Astronomy PhD thesis published 2014.
How Dylan Nelson produced amazing, interactive visualizations of the Illustris simulation
Studies the interaction between SN 2012ap and DIB carriers.
Panchromatic observations of SN 2009ip, revealing massive star envelope ejection.
Douglas Adams' fictional Ford Prefect famously warned us of eddies in the spacetime continuum. Has the IBEX spacecraft now found evidence that they really exist?
Proposes a novel method for creating interactive software modules as part of graduate-level education, focusing on astronomy examples.
Investigates the use of galaxy colors, particularly UV and optical, to enhance the accuracy of photometric metallicity estimations for star-forming galaxies.
An article for PolicyLab about the Obama administration's failure to act on climate regulation in the airline industry.
SN 2012au as a link between superluminous SNe and their fainter counterparts.
Reports the discovery and analysis of PS1-12sk, a peculiar Type Ibn supernova, originating from a helium-rich progenitor in a brightest cluster galaxy environment.
Multi-wavelength study of SN 2011ei, a Type IIb SN with inefficient shock breakout.
A blog post for Scientific American introducing Astrobites.
A GradHacker / InsideHigherEd article from 2013 announcing the first ComSciCon conference.
Observational surveys looking for the smallest super-massive black holes come up empty; could they be hiding in plain sight?
Presents the metallicity profile of the Andromeda galaxy (M31) derived from spectroscopic analysis of a large sample of HII regions and planetary nebulae.
The Prisoner's Dilemma is one of the classic problems in game theory, first posed in 1950 and studied exhaustively for generations. Remarkably, a new solution has been discovered that prompts us to re-examine long held principles.
Describes SN 2010ay, a bright Type Ic supernova with broad spectral lines, found in a host galaxy with low metallicity, and discusses its implications for GRB progenitors.
Discusses strategies for preparing undergraduate students for research careers, highlighting the use of Astrobites for integrating current research into educational settings.