The Dynamic Infrared Sky

Kavli Affiliate: Rob Simcoe | First 5 Authors: Mansi M. Kasliwal, Scott Adams, Igor Andreoni, Michael Ashley, Nadia Blagorodnova | Summary: Opening up the dynamic infrared sky for systematic time-domain exploration would yield many scientific advances. Multi-messenger pursuits such as localizing gravitational waves from neutron star mergers and quantifying the nucleosynthetic yields require the infrared. […]


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A close look at the dwarf AGN of NGC 4395: optical and near-IR integral field spectroscopy

Kavli Affiliate: Luis Ho | First 5 Authors: Carine Brum, Marlon R. Diniz, Rogemar A. Riffel, Alberto Rodriguez-Ardila, Luis Ho | Summary: Intermediate mass black holes (10$^3$-10$^5$ M$_odot$) in the center of dwarf galaxies are believed to be analogous to growing Active Galactic Nuclei (AGN) in the early Universe. Their characterization can provide insight about […]


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Cosmology with the Highly Redshifted 21cm Line

Kavli Affiliate: Jacqueline Hewitt | First 5 Authors: Adrian Liu, James Aguirre, Yacine Ali-Haimoud, Marcelo Alvarez, Adam Beardsley | Summary: In addition to being a probe of Cosmic Dawn and Epoch of Reionization astrophysics, the 21cm line at $z>6$ is also a powerful way to constrain cosmology. Its power derives from several unique capabilities. First, […]


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The Transiting Multi-planet System HD15337: Two Nearly Equal-mass Planets Straddling the Radius Gap

Kavli Affiliate: Robert Goeke | First 5 Authors: Davide Gandolfi, Luca Fossati, John H. Livingston, Keivan G. Stassun, Sascha Grziwa | Summary: We report the discovery of a super-Earth and a sub-Neptune transiting the star HD 15337 (TOI-402, TIC 120896927), a bright (V=9) K1 dwarf observed by the Transiting Exoplanet Survey Satellite (TESS) in Sectors […]


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The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory

Kavli Affiliate: Slawomir Gras | First 5 Authors: David Reitze, Rich Abbott, Carl Adams, Rana Adhikari, Nancy Aggarwal | Summary: Recent gravitational-wave observations from the LIGO and Virgo observatories have brought a sense of great excitement to scientists and citizens the world over. Since September 2015,10 binary black hole coalescences and one binary neutron star […]


Continue.. The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory

The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory

Kavli Affiliate: Slawomir Gras | First 5 Authors: David Reitze, Rich Abbott, Carl Adams, Rana Adhikari, Nancy Aggarwal | Summary: Recent gravitational-wave observations from the LIGO and Virgo observatories have brought a sense of great excitement to scientists and citizens the world over. Since September 2015,10 binary black hole coalescences and one binary neutron star […]


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Mapping the Inner Structure of Quasars with Time-Domain Spectroscopy

Kavli Affiliate: Luis Ho | First 5 Authors: Yue Shen, Scott Anderson, Edo Berger, W. N. Brandt, Gisella De Rosa | Summary: The ubiquitous variability of quasars across a wide range of wavelengths and timescales encodes critical information about the structure and dynamics of the circumnuclear emitting regions that are too small to be directly […]


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Dark Matter Science in the Era of LSST

Kavli Affiliate: Patricia R. Burchat | First 5 Authors: Keith Bechtol, Alex Drlica-Wagner, Kevork N. Abazajian, Muntazir Abidi, Susmita Adhikari | Summary: Astrophysical observations currently provide the only robust, empirical measurements of dark matter. In the coming decade, astrophysical observations will guide other experimental efforts, while simultaneously probing unique regions of dark matter parameter space. […]


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Electromagnetic probes of primordial black holes as dark matter

Kavli Affiliate: A. C. Davis | First 5 Authors: Y. Ali-Haimoud, S. Clesse, J. Garcia-Bellido, A. Kashlinsky, L. Wyrzykowski | Summary: The LIGO discoveries have rekindled suggestions that primordial black holes (BHs) may constitute part to all of the dark matter (DM) in the Universe. Such suggestions came from 1) the observed merger rate of […]


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