B. Zuckerman
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View article: “I Call It a Self-Rape”: A Qualitative Study of Unwanted Sex Among Adult Men With Women
“I Call It a Self-Rape”: A Qualitative Study of Unwanted Sex Among Adult Men With Women Open
Research on men’s sexual victimization has primarily focused on the psychological impact of childhood abuse by male perpetrators and how societal beliefs about masculinity hinder disclosure. This study broadens the lens by exploring how ad…
View article: Silicate mineralogy and bulk composition of exoplanetary material in polluted white dwarfs
Silicate mineralogy and bulk composition of exoplanetary material in polluted white dwarfs Open
White dwarf planetary systems uniquely link the bulk elemental composition of exoplanetary material to the mineralogy as photospheric abundances can be compared to circumstellar dust mineralogy. This study re-examines Spitzer/IRS spectra o…
View article: Silicate mineralogy and bulk composition of exoplanetary material in polluted white dwarfs
Silicate mineralogy and bulk composition of exoplanetary material in polluted white dwarfs Open
White dwarf planetary systems uniquely link the bulk elemental composition of exoplanetary material to the mineralogy as photospheric abundances can be compared to circumstellar dust mineralogy. This study re-examines Spitzer/IRS spectra o…
View article: A machine-learning compositional study of exoplanetary material accreted onto five helium-atmosphere white dwarfs with <tt>cecilia</tt>
A machine-learning compositional study of exoplanetary material accreted onto five helium-atmosphere white dwarfs with cecilia Open
We present the first application of the machine learning (ML) pipeline cecilia to determine the physical parameters and photospheric composition of five metal-polluted He-atmosphere white dwarfs without well-characterized elemental abundan…
View article: A Machine-Learning Compositional Study of Exoplanetary Material Accreted Onto Five Helium-Atmosphere White Dwarfs with $\texttt{cecilia}$
A Machine-Learning Compositional Study of Exoplanetary Material Accreted Onto Five Helium-Atmosphere White Dwarfs with $\texttt{cecilia}$ Open
We present the first application of the Machine Learning (ML) pipeline $\texttt{cecilia}$ to determine the physical parameters and photospheric composition of five metal-polluted He-atmosphere white dwarfs without well-characterised elemen…
View article: Spectroscopic Observations of the GALEX Nearby Young Star Survey Sample. I. Nearby Moving Group Candidates
Spectroscopic Observations of the GALEX Nearby Young Star Survey Sample. I. Nearby Moving Group Candidates Open
The GALEX Nearby Young Star Search (GALNYSS) yielded the identification of more than 2000 late-type stars that, based on their ultraviolet and infrared colors and pre-Gaia proper motions, are potentially of age Pic and AB Dor moving groups…
View article: The 40 pc sample of white dwarfs from <i>Gaia</i>
The 40 pc sample of white dwarfs from <i>Gaia</i> Open
We present a comprehensive overview of a volume-complete sample of white dwarfs located within 40 pc of the Sun, a significant proportion of which were detected in Gaia Data Release 3 (DR3). Our DR3 sample contains 1076 spectroscopically c…
View article: Seven white dwarfs with circumstellar gas discs I: white dwarf parameters and accreted planetary abundances
Seven white dwarfs with circumstellar gas discs I: white dwarf parameters and accreted planetary abundances Open
Observations of planetary material polluting the atmospheres of white dwarfs are an important probe of the bulk composition of exoplanetary material. Medium- and high-resolution optical and ultraviolet spectroscopy of seven white dwarfs wi…
View article: Seven white dwarfs with circumstellar gas discs I: white dwarf parameters and accreted planetary abundances
Seven white dwarfs with circumstellar gas discs I: white dwarf parameters and accreted planetary abundances Open
Observations of planetary material polluting the atmospheres of white dwarfs are an important probe of the bulk composition of exoplanetary material. Medium- and high-resolution optical and ultraviolet spectroscopy of seven white dwarfs wi…
View article: A cool, magnetic white dwarf accreting planetary debris
A cool, magnetic white dwarf accreting planetary debris Open
We present an analysis of spectroscopic data of the cool, highly magnetic, and polluted white dwarf 2MASS J0916−4215. The atmosphere of the white dwarf is dominated by hydrogen, but numerous spectral lines of magnesium, calcium, titanium, …
View article: A giant planet candidate transiting a white dwarf
A giant planet candidate transiting a white dwarf Open
Astronomers have discovered thousands of planets outside the Solar System1, most of which orbit stars that will eventually evolve into red giants and then into white dwarfs. During the red giant phase, any close-orbiting planets will be en…
View article: An emerging and enigmatic spectral class of isolated DAe white dwarfs
An emerging and enigmatic spectral class of isolated DAe white dwarfs Open
Two recently discovered white dwarfs, WD J041246.84 + 754942.26 and WD J165335.21 − 100116.33, exhibit Hα and Hβ Balmer line emission similar to stars in the emerging DAHe class, yet intriguingly have not been found to have detectable magn…
View article: An emerging and enigmatic spectral class of isolated DAe white dwarfs
An emerging and enigmatic spectral class of isolated DAe white dwarfs Open
Two recently discovered white dwarfs, WDJ041246.84$+$754942.26 and WDJ165335.21$-$100116.33, exhibit H$α$ and H$β$ Balmer line emission similar to stars in the emerging DAHe class, yet intriguingly have not been found to have detectable ma…
View article: Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-infrared Spectroscopy
Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-infrared Spectroscopy Open
Excess infrared flux from white dwarf stars is likely to arise from a dusty debris disk or a cool companion. In this work, we present near-infrared spectroscopic observations with Keck/MOSFIRE, Gemini/GNIRS, and Gemini/Flamingos-2 of seven…
View article: New Chondritic Bodies Identified in Eight Oxygen-bearing White Dwarfs
New Chondritic Bodies Identified in Eight Oxygen-bearing White Dwarfs Open
We present observations and analyses of eight white dwarf stars (WDs) that have accreted rocky material from their surrounding planetary systems. The spectra of these helium-atmosphere WDs contain detectable optical lines of all four major…
View article: Unusual Abundances from Planetary System Material Polluting the White Dwarf G238-44
Unusual Abundances from Planetary System Material Polluting the White Dwarf G238-44 Open
Ultraviolet and optical spectra of the hydrogen-dominated atmosphere white dwarf star G238-44 obtained with FUSE, Keck/HIRES, HST/COS, and HST/STIS reveal 10 elements heavier than helium: C, N, O, Mg, Al, Si, P, S, Ca, and Fe. G238-44 is o…
View article: <i>Gaia</i> white dwarfs within 40 pc – III. Spectroscopic observations of new candidates in the Southern hemisphere
<i>Gaia</i> white dwarfs within 40 pc – III. Spectroscopic observations of new candidates in the Southern hemisphere Open
We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the Southern hemisphere. Observations were performed mostly with the Very Large Telescope (X-Shooter) and Southern Astrophysical R…
View article: Infrared and optical detectability of Dyson spheres at white dwarf stars
Infrared and optical detectability of Dyson spheres at white dwarf stars Open
It has been hypothesized that advanced technological civilizations will construct giant space colonies and supporting infrastructures to orbit about their home stars. With data from recent satellites that operate at infrared and optical wa…
View article: V488 Per Revisited: No Strong Mid-infrared Emission Features and No Evidence for Stellar/substellar Companions
V488 Per Revisited: No Strong Mid-infrared Emission Features and No Evidence for Stellar/substellar Companions Open
We present characterization of the planetary system architecture for V488 Per, the dustiest main-sequence star known with a fractional infrared luminosity of ≈16%. Far-infrared imaging photometry confirms the existence of an outer planetar…
View article: Minimal Conditions for Survival of Technological Civilizations in the Face of Stellar Evolution
Minimal Conditions for Survival of Technological Civilizations in the Face of Stellar Evolution Open
The ease of interstellar rocket travel is an issue with implications for the long-term fate of our own and other civilizations and for the much-debated number of technological civilizations in the Galaxy. We show that the physical barrier …
View article: Oumuamua Is Not a Probe Sent to our Solar System by an Alien Civilization
Oumuamua Is Not a Probe Sent to our Solar System by an Alien Civilization Open
Oumuamua, the first known object of extrasolar origin seen to enter our Solar System, has multiple unusual characteristics that, taken together, are very difficult to explain with conventional astronomical entities like asteroids and comet…
View article: A giant planet candidate transiting a white dwarf
A giant planet candidate transiting a white dwarf Open
View article: Atmospheric Temperature Inversions and He i 5876 Core Profile Structure in White Dwarfs
Atmospheric Temperature Inversions and He i 5876 Core Profile Structure in White Dwarfs Open
We report distinctive core profiles in the strongest optical helium line, He i λ 5876, from high-resolution high-sensitivity observations of spectral type DB white dwarfs. By analyzing a sample of 40 stars from Keck/HIRES and VLT/UVES, we …
View article: Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign
Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign Open
We report the results of a ∼4 yr direct imaging survey of 104 stars to resolve and characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager (GPI) Exoplanet Survey. We targeted nearby (≲150 pc), young (…
View article: Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign
Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign Open
We report the results of a ${\sim}4$-year direct imaging survey of 104 stars to resolve and characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager Exoplanet Survey. We targeted nearby (${\lesssim}150…
View article: First Resolved Scattered-light Images of Four Debris Disks in Scorpius-Centaurus with the Gemini Planet Imager
First Resolved Scattered-light Images of Four Debris Disks in Scorpius-Centaurus with the Gemini Planet Imager Open
We present the first spatially resolved scattered-light images of four debris disks around members of the Scorpius-Centaurus (Sco-Cen) OB association with high-contrast imaging and polarimetry using the Gemini Planet Imager (GPI). All four…
View article: Why SETI Will Fail
Why SETI Will Fail Open
The union of space telescopes and interstellar spaceships guarantees that if extraterrestrial civilizations were common, someone would have come here long ago.
View article: Why SETI Will Fail
Why SETI Will Fail Open
The union of space telescopes and interstellar spaceships guarantees that if extraterrestrial civilizations were common, someone would have come here long ago.
View article: Compositions of Planetary Debris around Dusty White Dwarfs
Compositions of Planetary Debris around Dusty White Dwarfs Open
The photospheres of some white dwarfs (WDs) are “polluted” by accretion of material from their surrounding planetary debris. WDs with dust disks are often heavily polluted and high-resolution spectroscopic observations of these systems can…
View article: The Barium Abundance in the Young Star RZ Piscium
The Barium Abundance in the Young Star RZ Piscium Open
D'Orazi et al. (2009) found a barium overabundance up to 0.6 dex in clusters younger than 200 Myr compared to older clusters and the Sun.Oddly, while Ba is found to be overabundant, other s-process elements are not (D'Orazi et al. 2017).Th…