activity
20162026
most citedA Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team

2.3k citations · 5.2k across the 79 of their papers we have counts for

collaborators
Showing 2022Show all

11 papers · 1 filter

astro-ph.GA2022★ 22 cited

PHANGS-JWST First Results: Stellar Feedback-Driven Excitation and Dissociation of Molecular Gas in the Starburst Ring of NGC 1365?

Daizhong Liu, Eva Schinnerer, Yixian Cao +36

We compare embedded young massive star clusters (YMCs) to (sub-)millimeter line observations tracing the excitation and dissociation of molecular gas in the starburst ring of NGC 1…

astro-ph.GA2022★ 9 cited

Peekaboo: the extremely metal poor dwarf galaxy HIPASS J1131-31

I. D. Karachentsev, L. N. Makarova, B. S. Koribalski +3

The dwarf irregular galaxy HIPASS J1131-31 was discovered as a source of HI emission at low redshift in such close proximity of a bright star that we call it Peekaboo. The galaxy r…

astro-ph.GA2022★ 131 cited

The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular resolution in Nearby GalaxieS

Janice C. Lee, Karin M. Sandstrom, Adam K. Leroy +74

The PHANGS collaboration has been building a reference dataset for the multi-scale, multi-phase study of star formation and the interstellar medium in nearby galaxies. With the suc…

astro-ph.GA2022★ 73 cited

PHANGS-JWST First Results: A statistical view on bubble evolution in NGC628

Elizabeth J. Watkins, Ashley Barnes, Kiana F. Henny +49

The first JWST observations of nearby galaxies have unveiled a rich population of bubbles that trace the stellar feedback mechanisms responsible for their creation. Studying these…

astro-ph.GA2022★ 1 cited

PHANGS-JWST First Results: Dust embedded star clusters in NGC 7496 selected via 3.3 m PAH emission

Jimena Rodriguez, Janice Lee, Bradley Whitmore +38

The earliest stages of star formation occur enshrouded in dust and are not observable in the optical. Here we leverage the extraordinary new high-resolution infrared imaging from J…

astro-ph.CO2022★ 20 cited

Comparative Analysis of TRGBs (CATs) from Unsupervised, Multi-Halo-Field Measurements: Contrast is Key

J. Wu, D. Scolnic, A. G. Riess +5

The Tip of the Red Giant Branch (TRGB) is an apparent discontinuity in the color-magnitude diagram (CMD) along the giant branch due to the end of the red giant evolutionary phase a…

astro-ph.GA2022★ 25 cited

PHANGS: Constraining Star Formation Timescales Using the Spatial Correlations of Star Clusters and Giant Molecular Clouds

Jordan A. Turner, Daniel A. Dale, James Lilly +22

In the hierarchical view of star formation, giant molecular gas clouds (GMCs) undergo fragmentation to form small-scale structures made up of stars and star clusters. Here we study…

astro-ph.CO2022★ 148 cited

Cosmicflows-4

R. Brent Tully, Ehsan Kourkchi, Hélène M. Courtois +14

With Cosmicflows-4, distances are compiled for 55,877 galaxies gathered into 38,065 groups. Eight methodologies are employed, with the largest numbers coming from the correlations…

astro-ph.CO2022★ 2 cited

Worry No More, The Hubble Tension is Relieved: A Truly Direct Measurement of the Hubble Constant from Mooniversal Expansion

Gagandeep S. Anand, Zachary R. Claytor, Ryan Dungee

Using sedimentary and eclipse-based measurements of the lunar recession velocity, we derive a new local-Universe measurement of the Hubble constant () from the recession rate…

astro-ph.GA2022★ 12 cited

Around the Spindle galaxy: the dark halo mass of NGC3115

I. D. Karachentsev, L. N. Makarova, G. S. Anand +1

We report observations of five dwarf galaxies in the vicinity of the luminous S0 galaxy NGC 3115 performed with the Advanced Camera for Surveys on the Hubble Space Telescope. Their…

astro-ph.GA2022★ 33 cited

Planetary Nebula Luminosity Function distances for 19 galaxies observed by PHANGS-MUSE

Fabian Scheuermann, Kathryn Kreckel, Gagandeep S. Anand +15

We provide new planetary nebula luminosity function (PNLF) distances to 19 nearby spiral galaxies that were observed with VLT/MUSE by the PHANGS collaboration. Emission line ratios…