activity
20102026
most citedDust grain growth in the interstellar medium of 5<z<6.5 quasars

107 citations · 209 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2026

SN 2022riv in RX J2129: Discovery, Spectroscopic Classification, and Microlensing of a Strongly Lensed Type Ia Supernova from JWST and HST Observations

Birendra Dhanasingham, Patrick L. Kelly, Wenlei Chen +27

The multiply imaged SN 2022riv was discovered through a search of galaxy cluster fields as part of a Hubble Space Telescope (HST) SNAP program to find highly magnified stars. The s…

astro-ph.GA2025★ 1 cited

Dust removal timescale in galaxies across cosmic time

Aleksandra Leśniewska, Jens Hjorth, Christa Gall

Understanding the evolution of dust in galaxies is crucial because it affects the dynamics and cooling of gas, star formation, and chemical evolution. Recent work on dust removal i…

astro-ph.IM2025

AAS2RTO: Automated Alert Streams to Real-Time Observations: Preparing for rapid follow-up of transient objects in the era of LSST

Aidan Sedgewick, Christa Gall, Luca Izzo +4

The upcoming Vera C. Rubin Legacy Survey of Space and Time (LSST) will discover tens of thousands of astrophysical transients per night, far outpacing available spectroscopic follo…

astro-ph.GA2024

The Fate of the Interstellar Medium in Early-type Galaxies. V. AGN Feedback from Optical Spectral Classification

Oleh Ryzhov, Michał J. Michałowski, J. Nadolny +6

Quenching of star-formation plays a fundamental role in galaxy evolution. This process occurs due to the removal of the cold interstellar medium (ISM) or stabilization against coll…

astro-ph.CO2024★ 5 cited

The Hubble Constant from Blue Type Ia Supernovae

Christa Gall, Luca Izzo, Radoslaw Wojtak +1

There is a persistent tension of about between the value of the Hubble constant, as derived from the local distance ladder vs. the cosmic microwave background, signaling ei…

astro-ph.GA2024★ 1 cited

Rapid Dust Formation in the Early Universe

Danial Langeroodi, Jens Hjorth, Andrea Ferrara +1

Interstellar dust links the formation of the first stars to the rocky planet we inhabit by playing a pivotal role in the cooling and fragmentation of molecular clouds, and catalyzi…

astro-ph.GA2024★ 5 cited

The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies

Jakub Nadolny, Michał J. Michałowski, Massimiliano Parente +6

Removing cold interstellar medium (ISM) from a galaxy is central to quenching star formation. However, the exact mechanism of this process remains unclear. The objective of this wo…

astro-ph.GA2024★ 14 cited

The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation

Michał J. Michałowski, C. Gall, J. Hjorth +15

Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that…

astro-ph.GA2019★ 33 cited

The fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removal

Michał J. Michałowski, J. Hjorth, C. Gall +12

An important aspect of quenching star formation is the removal of the cold interstellar medium (ISM; non-ionised gas and dust) from a galaxy. In addition, dust grains can be destro…

astro-ph.GA2018★ 43 cited

Maximally dusty star-forming galaxies: Supernova dust production and recycling in Local Group and high-redshift galaxies

Christa Gall, Jens Hjorth

Motivated by recent observations suggesting that core-collapse supernovae may on average produce ~0.3 M_sun of dust, we explore a simple dust production scenario which applies to s…

astro-ph.CO2010★ 107 cited

Dust grain growth in the interstellar medium of 5<z<6.5 quasars

Michał J. Michałowski, Eric J. Murphy, Jens Hjorth +3

We investigate whether stellar dust sources i.e. asymptotic giant branch (AGB) stars and supernovae (SNe) can account for dust detected in 5<z<6.5 quasars (QSOs). We calculate the…