Search Results - "POPE, Alexandra"
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CO Emission in Infrared-selected Active Galactic Nuclei
Published in The Astrophysical journal (01-07-2019)“…In order to better understand how active galactic nuclei (AGNs) affect the interstellar media of their host galaxies, we perform a meta-analysis of the CO…”
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The Constant Average Relationship between Dust-obscured Star Formation and Stellar Mass from z = 0 to z = 2.5
Published in The Astrophysical journal (01-12-2017)“…The total star formation budget of galaxies consists of the sum of the unobscured star formation, as observed in the rest-frame ultraviolet (UV), together with…”
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3
Quenching of star formation from a lack of inflowing gas to galaxies
Published in Nature (London) (23-09-2021)“…Star formation in half of massive galaxies was quenched by the time the Universe was 3 billion years old 1 . Very low amounts of molecular gas seem to be…”
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Dust-enshrouded AGNs Can Dominate Host-galaxy-scale Cold Dust Emission
Published in The Astrophysical journal (01-11-2021)“…Abstract It is widely assumed that long-wavelength infrared (IR) emission from cold dust ( T ∼ 20–40 K) is a reliable tracer of star formation even in the…”
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First Constraints on the Interstellar Medium Conditions of a Low-mass, Highly Obscured z = 4.27 Main-sequence Galaxy
Published in The Astrophysical journal (01-07-2024)“…Abstract We present the molecular gas content and interstellar medium conditions of MACS J0717_Az9, a strong gravitationally lensed z = 4.273, M * ≃ 2 × 10 9 M…”
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STAR FORMATION AND AGN ACTIVITY IN GALAXY CLUSTERS FROM z = 1-2: A MULTI-WAVELENGTH ANALYSIS FEATURING HERSCHEL/PACS
Published in The Astrophysical journal (01-07-2016)“…ABSTRACT We present a detailed, multi-wavelength study of star formation (SF) and active galactic nucleus (AGN) activity in 11 near-infrared (IR) selected,…”
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Measuring Star Formation and Black Hole Accretion Rates in Tandem Using Mid-infrared Spectra of Local Infrared Luminous Galaxies
Published in The Astrophysical journal (01-07-2022)“…Abstract We present the results of a stacking analysis performed on Spitzer/Infrared Spectrograph high-resolution mid-infrared (mid-IR) spectra of luminous…”
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The Past and Future of Mid-Infrared Studies of AGN
Published in Universe (Basel) (27-06-2022)“…Observational studies of AGN in the mid-infrared regime are crucial to our understanding of AGN and their role in the evolution of galaxies. Mid-IR-based…”
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Measuring the Total Ultraviolet Light from Galaxy Clusters at z = 0.5–1.6: The Balance of Obscured and Unobscured Star Formation
Published in The Astrophysical journal (01-03-2022)“…Abstract Combined observations from UV to IR wavelengths are necessary to fully account for the star formation in galaxy clusters. Low-mass galaxies with log (…”
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THE ROLE OF STAR FORMATION AND AGN IN DUST HEATING OF Z = 0.3-2.8 Galaxies. II. INFORMING IR AGN FRACTION ESTIMATES THROUGH SIMULATIONS
Published in The Astrophysical journal (10-12-2016)“…ABSTRACT A key question in extragalactic studies is the determination of the relative roles of stars and active galactic nuclei (AGNs) in powering dusty…”
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The IR Compactness of Dusty Galaxies Sets Star Formation and Dust Properties at z ∼ 0–2
Published in The Astrophysical journal (01-10-2023)“…Abstract The surface densities of gas, dust, and stars provide a window into the physics of star formation that, until the advent of high-resolution…”
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Mid-Infrared Spectral Diagnosis of Submillimeter Galaxies
Published in The Astrophysical journal (10-03-2008)“…We present deep mid-IR spectroscopy with Spitzer of 13 SMGs in the GOODS-N field. We find strong PAH emission in all of our targets, which allows us to measure…”
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Tracing the Total Stellar Mass and Star Formation of High-redshift Protoclusters
Published in The Astrophysical journal (01-11-2023)“…Abstract As the progenitors of present-day galaxy clusters, protoclusters are excellent laboratories to study galaxy evolution. Since existing observations of…”
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Broad Emission Lines in Optical Spectra of Hot, Dust-obscured Galaxies Can Contribute Significantly to JWST/NIRCam Photometry
Published in Astrophysical journal. Letters (01-04-2023)“…Abstract Selecting the first galaxies at z > 7 − 10 from JWST surveys is complicated by z < 6 contaminants with degenerate photometry. For example, strong…”
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Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at z ∼ 1.4
Published in The Astrophysical journal (01-03-2022)“…Abstract We present the average gas properties derived from Atacama Large Millimeter Array (ALMA) Band 6 dust continuum imaging of 126 massive (log M ⋆ / M ⊙ ≳…”
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Measuring the Heating and Cooling of the Interstellar Medium at High Redshift: PAH and [C ii] Observations of the Same Star-forming Galaxies at z ∼ 2
Published in The Astrophysical journal (01-04-2020)“…Star formation depends critically on cooling mechanisms in the interstellar medium (ISM); however, thermal properties of gas in galaxies at the peak epoch of…”
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ALMA Reveals a Stable Rotating Gas Disk in a Paradoxical Low-mass, Ultradusty Galaxy at z = 4.274
Published in Astrophysical journal. Letters (01-07-2023)“…Abstract We report ALMA detections of [C ii ] and a dust continuum in Az9, a multiply imaged galaxy behind the Frontier Field cluster MACS J0717.5+3745. The…”
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The X-Ray and Mid-infrared Luminosities in Luminous Type 1 Quasars
Published in The Astrophysical journal (10-03-2017)“…Several recent studies have reported different intrinsic correlations between the active galactic nucleus (AGN) mid-IR luminosity ( ) and the rest-frame 2-10…”
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The One-hundred-deg2 DECam Imaging in Narrowbands (ODIN): Survey Design and Science Goals
Published in The Astrophysical journal (05-02-2024)“…We describe the survey design and science goals for One-hundred-deg2 DECam Imaging in Narrowbands (ODIN), a NOIRLab survey using the Dark Energy Camera (DECam)…”
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GOODS-HERSCHEL: IMPACT OF ACTIVE GALACTIC NUCLEI AND STAR FORMATION ACTIVITY ON INFRARED SPECTRAL ENERGY DISTRIBUTIONS AT HIGH REDSHIFT
Published in The Astrophysical journal (10-11-2012)“…We explore the effects of active galactic nuclei (AGNs) and star formation activity on the infrared (0.3-1000 mu m) spectral energy distributions (SEDs) of…”
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