The Effect of Dust Evolution and Traps on Inner Disk Water Enrichment

Kavli Affiliate: Gregory J. Herczeg | First 5 Authors: Anusha Kalyaan, Paola Pinilla, Sebastiaan Krijt, Andrea Banzatti, Giovanni Rosotti | Summary: Substructures in protoplanetary disks can act as dust traps that shape the radial distribution of pebbles. By blocking the passage of pebbles, the presence of gaps in disks may have a profound effect on […]


Continue.. The Effect of Dust Evolution and Traps on Inner Disk Water Enrichment

Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Kavli Affiliate: Vinothan N. Manoharan | First 5 Authors: Xander M. de Wit, Amelia W. Paine, Caroline Martin, Aaron M. Goldfain, Rees F. Garmann | Summary: Interferometric scattering microscopy (iSCAT) can image the dynamics of nanometer-scale systems. The typical approach to analyzing interferometric images involves intensive processing, which discards data and limits the precision of […]


Continue.. Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Kavli Affiliate: Vinothan N. Manoharan | First 5 Authors: Xander M. de Wit, Amelia W. Paine, Caroline Martin, Aaron M. Goldfain, Rees F. Garmann | Summary: Interferometric scattering microscopy (iSCAT) can image the dynamics of nanometer-scale systems. The typical approach to analyzing interferometric images involves intensive processing, which discards data and limits the precision of […]


Continue.. Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Kavli Affiliate: Vinothan N. Manoharan | First 5 Authors: Xander M. de Wit, Amelia W. Paine, Caroline Martin, Aaron M. Goldfain, Rees F. Garmann | Summary: Interferometric scattering microscopy (iSCAT) can image the dynamics of nanometer-scale systems. The typical approach to analyzing interferometric images involves intensive processing, which discards data and limits the precision of […]


Continue.. Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

Kavli Affiliate: Vinothan N. Manoharan | First 5 Authors: Xander M. de Wit, Amelia W. Paine, Caroline Martin, Aaron M. Goldfain, Rees F. Garmann | Summary: Interferometric scattering microscopy (iSCAT) can image the dynamics of nanometer-scale systems. The typical approach to analyzing interferometric images involves intensive processing, which discards data and limits the precision of […]


Continue.. Precise characterization of nanometer-scale systems using interferometric scattering microscopy and Bayesian analysis

BU Canis Minoris — the Most Compact Known Flat Doubly Eclipsing Quadruple System

Kavli Affiliate: Andrew Vanderburg | First 5 Authors: Theodor Pribulla, Tamás Borkovits, Rahul Jayaraman, Saul Rappaport, Tibor Mitnyan | Summary: We have found that the 2+2 quadruple star system BU CMi is currently the most compact quadruple system known, with an extremely short outer period of only 121 days. The previous record holder was TIC […]


Continue.. BU Canis Minoris — the Most Compact Known Flat Doubly Eclipsing Quadruple System

X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Nhut Truong, Annalisa Pillepich, Dylan Nelson, Ákos Bogdán, Gerrit Schellenberger | Summary: We derive predictions from state-of-the-art cosmological galaxy simulations for the spatial distribution of the hot circumgalactic medium (CGM, ${rm [0.1-1]R_{200c}}$) through its emission lines in the X-ray soft band ($[0.3-1.3]$ keV). In particular, we compare […]


Continue.. X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback

X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Nhut Truong, Annalisa Pillepich, Dylan Nelson, Ákos Bogdán, Gerrit Schellenberger | Summary: We derive predictions from state-of-the-art cosmological galaxy simulations for the spatial distribution of the hot circumgalactic medium (CGM, ${rm [0.1-1]R_{200c}}$) through its emission lines in the X-ray soft band ($[0.3-1.3]$ keV). In particular, we compare […]


Continue.. X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback

EIGER IV: The cool 10$^4$K circumgalactic environment of high-$z$ galaxies reveals remarkably efficient IGM enrichment

Kavli Affiliate: Robert A. Simcoe | First 5 Authors: Rongmon Bordoloi, Robert A. Simcoe, Jorryt Matthee, Daichi Kashino, Ruari Mackenzie | Summary: We report new observations of the cool diffuse gas around 29, $2.3<z<6.3$ galaxies, using deep JWST/NIRCam slitless grism spectroscopy around the sightline to the quasar J0100+2802. The galaxies span a stellar mass range […]


Continue.. EIGER IV: The cool 10$^4$K circumgalactic environment of high-$z$ galaxies reveals remarkably efficient IGM enrichment