140 citations · 1.2k across the 26 of their papers we have counts for
25 papers
ALMA reveals a stable rotating gas disk in a paradoxical low-mass, ultra-dusty galaxy at z = 4.274
Alexandra Pope, Jed McKinney, Patrick Kamieneski +13
We report ALMA detections of [CII] and dust continuum in Az9, a multiply-imaged galaxy behind the Frontier Field cluster MACSJ0717.5+3745. The bright [CII] emission line provides a…
The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
Caro Derkenne, Richard M. McDermid, Adriano Poci +20
We investigate the impact of environment on the internal mass distribution of galaxies using the Middle Ages Galaxy Properties with Integral field spectroscopy (MAGPI) survey. We u…
Constraining the LyC escape fraction from LEGUS star clusters with SIGNALS HII region observations: A pilot study of NGC 628
J. W. Teh, K. Grasha, M. R. Krumholz +23
The ionising radiation of young and massive stars is a crucial form of stellar feedback. Most ionising (Lyman-continuum; LyC, ) photons are absorbed close to the stars tha…
Spatially resolved dust properties and quasar-galaxy decomposition of a HyLIRG at z = 4.4
Takafumi Tsukui, Emily Wisnioski, Mark R. Krumholz +1
We report spatially resolved dust properties of the quasar host galaxy BRI 1335-0417 at redshift constrained by the ALMA observations. The dust temperature map, derived f…
Metallicity Gradient of Barred Galaxies with TYPHOON
Qian-Hui Chen, Kathryn Grasha, Andrew J. Battisti +5
Bars play an important role in mixing material in the inner regions of galaxies and stimulating radial migration. Previous observations have found evidence for the impact of a bar…
Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
Rongjun Huang, Andrew J. Battisti, Kathryn Grasha +4
Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass (), evolves…
A geostatistical analysis of multiscale metallicity variations in galaxies [II]: Predicting the metallicities of Hii and diffuse ionised gas regions via universal kriging
Benjamin Metha, Michele Trenti, Tingjin Chu +1
The metallicity of diffuse ionised gas (DIG) cannot be determined using strong emission line diagnostics, which are calibrated to calculate the metallicity of Hii regions. Because…
The average dust attenuation curve at z~1.3 based on HST grism surveys
A. J. Battisti, M. B. Bagley, I. Baronchelli +12
We present the first characterisation of the average dust attenuation curve at by combining rest-frame ultraviolet through near-IR photometry with Balmer decrement ($\ma…
Metallicity, ionization parameter, and pressure variations of HII regions in the TYPHOON spiral galaxies
K. Grasha, Q. H. Chen, A. J. Battisti +12
We present a spatially-resolved HII region study of the gas-phase metallicity, ionization parameter, and ISM pressure maps of 6 local star-forming and face-on spiral galaxies from…
The UV 2175Å Attenuation Bump and its Correlation with PAH Emission at z~2
Irene Shivaei, Leindert Boogaard, Tanio Díaz-Santos +10
The UV bump is a broad absorption feature centered at 2175Å that is seen in the attenuation/extinction curve of some galaxies, but its origin is not well known. Here, we use a samp…
Spectroscopically Identified Emission Line Galaxy Pairs in the WISP survey
Y. Sophia Dai, Matthew M. Malkan, Harry I. Teplitz +20
We identify a sample of spectroscopically measured emission line galaxy (ELG) pairs up to z=1.6 from the WFC3 Infrared Spectroscopic Parallels (WISP) survey. WISP obtained slitless…
Revisiting Attenuation Curves: the Case of NGC 3351
Daniela Calzetti, Andrew J. Battisti, Irene Shivaei +14
Multi-wavelength images from the farUV (~0.15 micron) to the sub-millimeter of the central region of the galaxy NGC 3351 are analyzed to constrain its stellar populations and dust…
The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
C. Foster, J. T. Mendel, C. D. P. Lagos +40
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical dri…
The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to
Sarah Leslie, Eva Schinnerer, Daizhong Liu +17
We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR) - stellar mass () relation, called the main sequence of star-forming g…
The MOSDEF Survey: the Variation of the Dust Attenuation Curve with Metallicity
Irene Shivaei, Naveen Reddy, George Rieke +14
We derive the UV-optical stellar dust attenuation curve of galaxies at z=1.4-2.6 as a function of gas-phase metallicity. We use a sample of 218 star-forming galaxies, excluding tho…
The Strength of the 2175Å Feature in the Attenuation Curves of Galaxies at 0.1<z<3
A. J. Battisti, E. da Cunha, I. Shivaei +1
We update the spectral modeling code MAGPHYS to include a 2175Å absorption feature in its UV-to-near-IR dust attenuation prescription. This allows us to determine the strength of t…
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ~700 Galaxies at z=0.5-6
Daizhong Liu, P. Lang, B. Magnelli +21
The rich information on (sub)millimeter dust continuum emission from distant galaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA) archive is contained in thou…
Spitzer catalog of Herschel-selected ultrared dusty, star-forming galaxies
Jingzhe Ma, Asantha Cooray, Hooshang Nayyeri +24
The largest Herschel extragalactic surveys, H-ATLAS and HerMES, have selected a sample of "ultrared" dusty, star-forming galaxies (DSFGs) with rising SPIRE flux densities ($S_{500}…
MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts
A. J. Battisti, E. da Cunha, K. Grasha +7
We present an enhanced version of the multiwavelength spectral modeling code MAGPHYS that allows the estimation of galaxy photometric redshift and physical properties (e.g., stella…
Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC4449
D. Calzetti, G. W. Wilson, B. T. Draine +17
We investigate the relation between gas and star formation in sub-galactic regions, ~360 pc to ~1.5 kpc in size, within the nearby starburst dwarf NGC4449, in order to separate the…
Characterizing Dust Attenuation in Local Star Forming Galaxies: Inclination Effects and the 2175Å Feature
A. J. Battisti, D. Calzetti, R. -R. Chary
We characterize the influence that inclination has on the shape and normalization in average dust attenuation curves derived from a sample of ~10,000 local star-forming galaxies. T…
Early Science with the Large Millimeter Telescope: Detection of dust emission in multiple images of a normal galaxy at lensed by a Frontier Fields cluster
Alexandra Pope, Alfredo Montana, Andrew Battisti +32
We directly detect dust emission in an optically-detected, multiply-imaged galaxy lensed by the Frontier Fields cluster MACSJ0717.5+3745. We detect two images of the same galaxy at…
Continuous Mid-Infrared Star Formation Rate Indicators: Diagnostics for 0<z<3 Star Forming Galaxies
A. J. Battisti, D. Calzetti, B. D. Johnson +1
We present continuous, monochromatic star formation rate (SFR) indicators over the mid-infrared wavelength range of 6-70 micron. We use a sample of 58 star forming galaxies (SFGs)…
The Dense Gas Mass Fraction of Molecular Clouds in the Milky Way
Andrew J. Battisti, Mark H. Heyer
The mass fraction of dense gas within giant molecular clouds (GMCs) of the Milky Way is investigated using 13CO data from the FCRAO Galactic Plane Surveys and the Bolocam Galactic…