A massive AGB donor in Scutum X-1: Identification of the first Mira variable in an X-ray binary

Kavli Affiliate: Robert Simcoe | First 5 Authors: Kishalay De, Deepto Chakrabarty, Roberto Soria, Michael C. B. Ashley, Charlie Conroy | Summary: The symbiotic X-ray binary Sct X-1 was suggested as the first known neutron star accreting from a red supergiant companion. Although known for nearly 50 years, detailed characterization of the donor remains lacking, […]


Continue.. A massive AGB donor in Scutum X-1: Identification of the first Mira variable in an X-ray binary

A massive AGB donor in Scutum X-1: Identification of the first Mira variable in an X-ray binary

Kavli Affiliate: Robert Simcoe | First 5 Authors: Kishalay De, Deepto Chakrabarty, Roberto Soria, Michael C. B. Ashley, Charlie Conroy | Summary: The symbiotic X-ray binary Sct X-1 was suggested as the first known neutron star accreting from a red supergiant companion. Although known for nearly 50 years, detailed characterization of the donor remains lacking, […]


Continue.. A massive AGB donor in Scutum X-1: Identification of the first Mira variable in an X-ray binary

Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Kavli Affiliate: Marshall Bautz | First 5 Authors: Tanmoy Chattopadhyay, Sven Herrmann, Peter Orel, R. Glenn Morris, Gregory Prigozhin | Summary: The broad energy response, low electronic read noise, and good energy resolution have made X-ray Charge-Coupled Devices (CCDs) an obvious choice for developing soft X-ray astronomical instruments over the last half century. They also […]


Continue.. Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Kavli Affiliate: Marshall Bautz | First 5 Authors: Tanmoy Chattopadhyay, Sven Herrmann, Peter Orel, R. Glenn Morris, Gregory Prigozhin | Summary: The broad energy response, low electronic read noise, and good energy resolution have made X-ray Charge-Coupled Devices (CCDs) an obvious choice for developing soft X-ray astronomical instruments over the last half century. They also […]


Continue.. Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in Illustris-TNG

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Jubee Sohn, Margaret J. Geller, Mark Vogelsberger, Ivana Danjanov, | Summary: We use the Illustris-TNG simulations to explore the dynamic scaling relation between massive clusters and their central galaxies (BCGs). The Illustris TNG300-1 simulation we use includes 280 massive clusters with $M_{200} > 10^{14}$ M$_{odot}$ enabling a […]


Continue.. Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in Illustris-TNG

Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Jubee Sohn, Margaret J. Geller, Mark Vogelsberger, Ivana Damjanov, | Summary: We use the IllustrisTNG simulations to explore the dynamic scaling relation between massive clusters and their central galaxies (BCGs). The Illustris TNG300-1 simulation we use includes 280 massive clusters with $M_{200} > 10^{14}$ M$_{odot}$ enabling a […]


Continue.. Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG

H$_2$-dominated Atmosphere as an Indicator of Second-generation Rocky White Dwarf Exoplanets

Kavli Affiliate: Sara Seager | First 5 Authors: Zifan Lin, Sara Seager, Sukrit Ranjan, Thea Kozakis, Lisa Kaltenegger | Summary: Following the discovery of the first exoplanet candidate transiting a white dwarf (WD), a "white dwarf opportunity" for characterizing the atmospheres of terrestrial exoplanets around WDs is emerging. Large planet-to-star size ratios and hence large […]


Continue.. H$_2$-dominated Atmosphere as an Indicator of Second-generation Rocky White Dwarf Exoplanets

TESS Revisits WASP-12: Updated Orbital Decay Rate and Constraints on Atmospheric Variability

Kavli Affiliate: Avi Shporer | First 5 Authors: Ian Wong, Avi Shporer, Shreyas Vissapragada, Michael Greklek-McKeon, Heather A. Knutson | Summary: After observing WASP-12 in the second year of the primary mission, the Transiting Exoplanet Survey Satellite (TESS) revisited the system in late 2021 during its extended mission. In this paper, we incorporate the new […]


Continue.. TESS Revisits WASP-12: Updated Orbital Decay Rate and Constraints on Atmospheric Variability

Photochemical Runaway in Exoplanet Atmospheres: Implications for Biosignatures

Kavli Affiliate: Sara Seager | First 5 Authors: Sukrit Ranjan, Sara Seager, Zhuchang Zhan, Daniel D. B. Koll, William Bains | Summary: About 2.5 billion years ago, microbes learned to harness plentiful Solar energy to reduce CO$_2$ with H$_2$O, extracting energy and producing O$_2$ as waste. O$_2$ production from this metabolic process was so vigorous […]


Continue.. Photochemical Runaway in Exoplanet Atmospheres: Implications for Biosignatures

An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment

Kavli Affiliate: Kiyoshi Masui | First 5 Authors: The CHIME Collaboration, Mandana Amiri, Kevin Bandura, Anja Boskovic, Tianyue Chen | Summary: The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a drift scan radio telescope operating across the 400-800 MHz band. CHIME is located at the Dominion Radio Astrophysical Observatory near Penticton, BC Canada. The instrument […]


Continue.. An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment