activity
20152026
most citedThe [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift

236 citations · 2.5k across the 90 of their papers we have counts for

collaborators
Showing 2022Show all

28 papers · 1 filter

astro-ph.GA2022★ 48 cited

PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365

Bradley C. Whitmore, Rupali Chandar, M. Jimena Rodríguez +28

A primary new capability of JWST is the ability to penetrate the dust in star forming galaxies to identify and study the properties of young star clusters that remain embedded in d…

astro-ph.GA2022★ 30 cited

PHANGS-JWST First Results: A Global and Moderately Resolved View of Mid-Infrared and CO Line Emission from Galaxies at the Start of the JWST Era

Adam K. Leroy, Alberto D. Bolatto, Karin Sandstrom +41

We explore the relationship between mid-infrared (mid-IR) and CO rotational line emission from massive star-forming galaxies, which is one of the tightest scalings in the local uni…

astro-ph.GA2022★ 49 cited

PHANGS-JWST First Results: Tracing the Diffuse ISM with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies

Karin M. Sandstrom, Eric W. Koch, Adam K. Leroy +43

JWST observations of polycyclic aromatic hydrocarbon (PAH) emission provide some of the deepest and highest resolution views of the cold interstellar medium (ISM) in nearby galaxie…

astro-ph.GA2022★ 1 cited

PHANGS-JWST First Results: Measuring PAH Properties across the multiphase ISM

Jérémy Chastenet, Jessica Sutter, Karin Sandstrom +26

Ratios of polycyclic aromatic hydrocarbon (PAH) vibrational bands are a promising tool for measuring the properties of the PAH population and their effect on star formation. The ph…

astro-ph.GA2022★ 9 cited

CI and CO in Nearby Spiral Galaxies -- I. Line Ratio and Abundance Variations at ~ 200 pc Scales

Daizhong Liu, Eva Schinnerer, Toshiki Saito +25

We present new neutral atomic carbon [CI](3P1-3P0) mapping observations within the inner ~7 kpc and ~4 kpc of the disks of NGC3627 and NGC4321 at a spatial resolution of 190 pc and…

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★ 40 cited

PHANGS-JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC1365

Eva Schinnerer, Eric Emsellem, Jonathan D. Henshaw +36

Large-scale bars can fuel galaxy centers with molecular gas, often leading to the development of dense ring-like structures where intense star formation occurs, forming a very diff…

astro-ph.GA2022★ 64 cited

PHANGS-JWST First Results: Destruction of the PAH molecules in HII regions probed by JWST and MUSE

Oleg V. Egorov, Kathryn Kreckel, Karin M. Sandstrom +30

Polycyclic aromatic hydrocarbons (PAHs) play a critical role in the reprocessing of stellar radiation and in balancing the heating and cooling processes in the interstellar medium…

astro-ph.GA2022★ 32 cited

PHANGS--JWST First Results: ISM structure on the turbulent Jeans scale in four disk galaxies observed by JWST and ALMA

Sharon E. Meidt, Erik Rosolowsky, Jiayi Sun +31

JWST/MIRI imaging of the nearby galaxies IC 5332, NGC 628, NGC 1365 and NGC 7496 from PHANGS reveals a richness of gas structures that in each case form a quasi-regular network of…

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★ 41 cited

PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628

Jaeyeon Kim, Mélanie Chevance, J. M. Diederik Kruijssen +33

The earliest stages of star formation, when young stars are still deeply embedded in their natal clouds, represent a critical phase in the matter cycle between gas clouds and young…

astro-ph.GA2022★ 63 cited

PHANGS-JWST First Results: Multi-wavelength view of feedback-driven bubbles (The Phantom Voids) across NGC 628

Ashley T. Barnes, Elizabeth J. Watkins, Sharon E. Meidt +51

We present a high-resolution view of bubbles within The Phantom Galaxy (NGC 628); a nearby (~10Mpc), star-forming (~2Msun/yr), face-on (i~9deg) grand-design spiral galaxy. With new…

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★ 20 cited

PHANGS-JWST First Results: Spurring on Star Formation: JWST Reveals Localised Star Formation in a Spiral Arm Spur of NGC 628

Thomas G. Williams, Jiayi Sun, Ashley T. Barnes +34

We combine JWST observations with ALMA CO and VLT-MUSE H data to examine off-spiral arm star formation in the face-on, grand-design spiral galaxy NGC 628. We focus on the northe…

astro-ph.GA2022★ 30 cited

PHANGS-JWST First Results: The Influence of Stellar Clusters on PAHs in Nearby Galaxies

Daniel A. Dale, Médéric Boquien, Ashley T. Barnes +28

We present a comparison of theoretical predictions of dust continuum and polycyclic aromatic hydrocarbon (PAH) emission with new JWST observations in three nearby galaxies: NGC 628…

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.GA2022★ 22 cited

A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259

Daizhong Liu, N. M. Förster Schreiber, R. Genzel +19

We present a high-resolution kinematic study of the massive main-sequence star-forming galaxy (SFG) SDSS J090122.37+181432.3 (J0901) at z=2.259, using 0.36 arcsec ALMA CO(3-2) and…

astro-ph.GA2022★ 16 cited

PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628

Nils Hoyer, Francesca Pinna, Albrecht W. H. Kamlah +28

We combine archival HST and new JWST imaging data, covering the ultraviolet to mid-infrared regime, to morphologically analyze the nuclear star cluster (NSC) of NGC 628, a grand-de…

astro-ph.GA2022★ 13 cited

COSMOS-Web: An Overview of the JWST Cosmic Origins Survey

Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos +82

We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations…

astro-ph.GA2022★ 25 cited

COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS

Malte Brinch, Thomas R. Greve, John R. Weaver +20

We conduct a systematic search for protocluster candidates at in the COSMOS field using the recently released COSMOS2020 source catalog. We select galaxies using a numbe…

astro-ph.GA2022★ 2 cited

Galaxy kinematics and mass estimates at from ionised gas and stars

Hannah Übler, Natascha M. Förster Schreiber, Arjen van der Wel +14

We compare ionised gas and stellar kinematics of 16 star-forming galaxies (, SFR=6-86 ) at using near-infrared integral field s…

astro-ph.GA2022★ 5 cited

Compact and variable radio emission from an active galaxy with supersoft X-ray emission

Lei Yang, Xinwen Shu, Fabao Zhang +15

RX J1301.9+2747 is a unique active galaxy with supersoft X-ray spectrum that lacks significant emission at energies above 2 keV. In addition, it is one of few galaxies displaying q…

astro-ph.GA2022★ 20 cited

AGN-driven Cold Gas Outflow of NGC 1068 Characterized by Dissociation-Sensitive Molecules

Toshiki Saito, Shuro Takano, Nanase Harada +11

Recent developments in (sub-)millimeter facilities have drastically changed the amount of information obtained from extragalactic spectral scans. In this paper, we present a featur…

astro-ph.GA2022★ 115 cited

Molecular Cloud Populations in the Context of Their Host Galaxy Environments: A Multiwavelength Perspective

Jiayi Sun, Adam K. Leroy, Erik Rosolowsky +35

We present a rich, multiwavelength, multiscale database built around the PHANGS-ALMA CO(2-1) survey and ancillary data. We use this database to present the distributions of mol…