Search Publications

Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in ∼100,000 SDSS and ∼20,000 CANDELS Galaxies
DOI: 10.3847/1538-4357/ab8a47 Bibcode: 2020ApJ...895..112G

Schawinski, Kevin; Urry, C. Megan; Powell, Meredith C. +3 more

We examine morphology-separated color-mass diagrams to study the quenching of star formation in ∼100,000 (z ∼ 0) Sloan Digital Sky Survey (SDSS) and ∼20,000 (z ∼ 1) Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS) galaxies. To classify galaxies morphologically, we developed Galaxy Morphology Network (GAMORNET), a convolutio…

2020 The Astrophysical Journal
eHST 46
Primordial black holes and gravitational waves in nonstandard cosmologies
DOI: 10.1103/PhysRevD.102.043522 Bibcode: 2020PhRvD.102d3522B

Mohanty, Subhendra; Parashari, Priyank; Bhattacharya, Sukannya

For primordial black holes (PBHs) to form a considerable fraction of cold dark matter, the required amplitude of primordial scalar perturbations is quite large (Pζ(k )∼10-2) if PBH is formed in radiation epoch. In alternate cosmological histories, where additional epoch of arbitrary equation of state precede radiation epoch, …

2020 Physical Review D
INTEGRAL 46
Detection of PAH Absorption and Determination of the Mid-infrared Diffuse Interstellar Extinction Curve from the Sight Line toward Cyg OB2-12
DOI: 10.3847/1538-4357/ab8cc3 Bibcode: 2020ApJ...895...38H

Draine, B. T.; Hensley, Brandon S.

The sight line toward the luminous blue hypergiant Cyg OB2-12 is widely used to study interstellar dust on account of its large extinction (AV ≃ 10 mag) and the fact that this extinction appears to be dominated by dust typical of the diffuse interstellar medium. We present a new analysis of archival Infrared Space Observatory Short Wave…

2020 The Astrophysical Journal
Gaia ISO 46
The Tidal Disruption Event AT 2018hyz II: Light-curve modelling of a partially disrupted star
DOI: 10.1093/mnras/staa2099 Bibcode: 2020MNRAS.497.1925G

Eftekhari, Tarraneh; Berger, Edo; Chornock, Ryan +18 more

AT 2018hyz (= ASASSN-18zj) is a tidal disruption event (TDE) located in the nucleus of a quiescent E+A galaxy at a redshift of z = 0.04573, first detected by the All-Sky Automated Survey for Supernovae (ASAS-SN). We present optical+UV photometry of the transient, as well as an X-ray spectrum and radio upper limits. The bolometric light curve of AT…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 46
The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching
DOI: 10.3847/1538-4357/ab5fd9 Bibcode: 2020ApJ...888...77W

Bell, Eric F.; D'Eugenio, Francesco; Franx, Marijn +11 more

We analyze the colors and sizes of 32 quiescent (UVJ-selected) galaxies with strong Balmer absorption (EW(Hδ) ≥ 4 Å) at z ∼ 0.8 drawn from DR2 of the LEGA-C survey to test the hypothesis that these galaxies experienced compact, central starbursts before quenching. These recently quenched galaxies, usually referred to as post-starburst galaxies, sp…

2020 The Astrophysical Journal
eHST 46
A closer look at the spur, blob, wiggle, and gaps in GD-1
DOI: 10.1093/mnras/staa917 Bibcode: 2020MNRAS.494.5315D

Gieles, M.; Erkal, D.; de Boer, T. J. L.

The GD-1 stream is one of the longest and coldest stellar streams discovered to date, and one of the best objects for constraining the dark matter properties of the Milky Way. Using data from Gaia DR2, we study the proper motions (PMs), distance, morphology, and density of the stream to uncover small-scale perturbations. The PM cleaned data show a…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 46
Clouds of Fluffy Aggregates: How They Form in Exoplanetary Atmospheres and Influence Transmission Spectra
DOI: 10.3847/1538-4357/ab44bd Bibcode: 2020ApJ...891..131O

Okuzumi, Satoshi; Tazaki, Ryo; Ohno, Kazumasa

Transmission spectrum surveys have suggested the ubiquity of high-altitude clouds in exoplanetary atmospheres. Theoretical studies have investigated the formation processes of the high-altitude clouds; however, cloud particles have been commonly approximated as compact spheres, which is not always true for solid mineral particles that likely const…

2020 The Astrophysical Journal
eHST 46
The unusual broad-band X-ray spectral variability of NGC 1313 X-1 seen with XMM-Newton, Chandra, and NuSTAR
DOI: 10.1093/mnras/staa1129 Bibcode: 2020MNRAS.494.6012W

Harrison, F. A.; Stern, D.; Fabian, A. C. +19 more

We present results from the major coordinated X-ray observing programme on the ULX NGC 1313 X-1 performed in 2017, combining XMM-Newton, Chandra, and NuSTAR, focusing on the evolution of the broad-band (∼0.3-30.0 keV) continuum emission. Clear and unusual spectral variability is observed, but this is markedly suppressed above ∼10-15 keV, qualitati…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46
Searching for ultra-fast outflows in AGN using variability spectra
DOI: 10.1093/mnras/staa265 Bibcode: 2020MNRAS.493.1088I

Schartel, N.; Santos-Lleó, M.; Buisson, D. J. K. +9 more

We present a qualitative search for ultra-fast outflows (UFOs) in excess variance spectra of radio-quiet active galactic nuclei (AGNs). We analyse 42 sources from the spectroscopic UFO detection sample, and an additional 22 different sources from the variability sample. A total of 58 sources have sufficient observational data from XMM-Newton EPIC-…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46
Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0
DOI: 10.3847/1538-4357/abbf59 Bibcode: 2020ApJ...904..107S

Hathi, Nimish P.; Kartaltepe, Jeyhan S.; Kocevski, Dale D. +30 more

Galaxy interactions and mergers are thought to play an important role in the evolution of galaxies. Studies in the nearby universe show a higher fraction of active galactic nuclei (AGNs) in interacting and merging galaxies than in their isolated counterparts, indicating that such interactions are important contributors to black hole growth. To inv…

2020 The Astrophysical Journal
eHST 46