activity
20062026
most citedThe Mid-Infrared Spectrum of Star-Forming Galaxies: Global Properties of PAH Emission

967 citations · 4.9k across the 28 of their papers we have counts for

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15 papers · 1 filter

astro-ph.GA2026

JWST Whirlpool Galaxy Treasury: Mid-Infrared Emission in M51 and its Relation to Gas Column and Star Formation

Mansi Padave, Karin M. Sandstrom, Daniel A. Dale +25

Using JWST/MIRI imaging of M51 in eight broadband filters, we investigate correlations of mid-infrared emission from polycyclic aromatic hydrocarbons (PAHs) and dust continuum with…

astro-ph.GA2026★ 1 cited

Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST

Rupali Chandar, Miranda Caputo, Paul Goudfrooij +15

The Antennae galaxies merger produces the brightest infrared emission of any galaxy within ~20 Mpc, mostly from intense star formation taking place in supergiant molecular cloud co…

astro-ph.GA2025★ 4 cited

Physical Conditions of the Ionized Superwind in NGC 253 with VLT/MUSE

Serena A. Cronin, Alberto D. Bolatto, Enrico Congiu +7

We present an analysis of the H-emitting ionized gas in the warm phase of the NGC 253 outflow using integral field spectroscopy from the Multi Unit Spectroscopic Explorer (MUSE)…

astro-ph.GA2025★ 5 cited

Euclid: The potential of slitless infrared spectroscopy: A z=5.4 quasar and new ultracool dwarfs

E. Bañados, V. Le Brun, S. Belladitta +226

We demonstrate the potential of Euclid's slitless spectroscopy to discover high-redshift (z>5) quasars and their main photometric contaminant, ultracool dwarfs. Sensitive infrared…

astro-ph.GA2025★ 7 cited

Detection of Deuterated Hydrocarbon Nanoparticles in the Whirlpool Galaxy, M51

B. T. Draine, Karin Sandstrom, Daniel A. Dale +29

Deuteration of hydrocarbon material, including polycyclic aromatic hydrocarbons (PAHs), has been proposed to account for the low gas-phase abundances of D in the interstellar mediu…

astro-ph.GA2025

An Investigation of Disk Thickness in M51 from H-alpha, Pa-alpha, and Mid-Infrared Power Spectra

Bruce G. Elmegreen, Daniela Calzetti, Angela Adamo +27

Power spectra (PS) of high-resolution images of M51 (NGC 5194) taken with the Hubble Space Telescope and the James Webb Space Telescope have been examined for evidence of disk thic…

astro-ph.GA2024

ALESS-JWST: Joint (sub-)kiloparsec JWST and ALMA imaging of submillimeter galaxies reveals heavily obscured bulge formation events

Jacqueline A. Hodge, Elisabete da Cunha, Sarah Kendrew +25

We present JWST NIRCam imaging targeting 13 infrared-luminous () galaxies from the ALESS survey with uniquely deep, high-resolution…

astro-ph.GA2024

A Comparative Study of the Ground State Transitions of CO and [C I] as Molecular Gas Tracers at High Redshift

Marta Frias Castillo, Matus Rybak, Jacqueline A. Hodge +22

The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM)…

astro-ph.GA2017★ 642 cited

PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

L. J. Tacconi, R. Genzel, A. Saintonge +32

This paper provides an update of our previous scaling relations (Genzel et al.2015) between galaxy integrated molecular gas masses, stellar masses and star formation rates, in the…

astro-ph.GA2016★ 162 cited

ALMA spectroscopic survey in the Hubble Ultra Deep Field: Continuum number counts, resolved 1.2-mm extragalactic background, and properties of the faintest dusty star forming galaxies

M. Aravena, R. Decarli, F. Walter +31

We present an analysis of a deep (1=13 Jy) cosmological 1.2-mm continuum map based on ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field. In the 1 arcmin$^2…

astro-ph.GA2016★ 35 cited

Comparing [CII], HI, and CO dynamics of nearby galaxies

W. J. G. de Blok, F. Walter, J. -D. T Smith +12

The HI and CO components of the interstellar medium (ISM) are usually used to derive the dynamical mass M_dyn of nearby galaxies. Both components become too faint to be used as a t…

astro-ph.GA2015★ 38 cited

The Impact of Molecular Gas on Mass Models of Nearby Galaxies

Bradley S. Frank, W. J. G. de Blok, F. Walter +2

We present CO velocity fields and rotation curves for a sample of nearby galaxies, based on data from the HERACLES survey. We combine our data with literature THINGS, SINGS and KIN…

astro-ph.GA2014★ 31 cited

The Survey of Lines in M31 (SLIM): Investigating the Origins of [CII] Emission

M. J. Kapala, K. Sandstrom, B. Groves +7

The [CII] 158 micron line is one of the strongest emission lines observed in star-forming galaxies, and has been empirically measured to correlate with the star formation rate (SFR…

astro-ph.GA2014★ 24 cited

A far-IR view of the starburst driven superwind in NGC 2146

K. Kreckel, L. Armus, B. Groves +19

NGC 2146, a nearby luminous infrared galaxy (LIRG), presents evidence for outflows along the disk minor axis in all gas phases (ionized, neutral atomic and molecular). We present a…

astro-ph.GA2012★ 40 cited

A Study of Heating and Cooling of the ISM in NGC 1097 with Herschel-PACS and Spitzer-IRS

P. Beirao, L. Armus, G. Helou +38

NGC 1097 is a nearby Seyfert 1 galaxy with a bright circumnuclear starburst ring, a strong large-scale bar and an active nucleus. We present a detailed study of the spatial variati…