Search Publications

The CatWISE Preliminary Catalog: Motions from WISE and NEOWISE Data
DOI: 10.3847/1538-4365/ab7f2a Bibcode: 2020ApJS..247...69E

Teplitz, Harry I.; Schlegel, David J.; Mobasher, Bahram +19 more

CatWISE is a program to catalog sources selected from combined WISE and NEOWISE all-sky survey data at 3.4 and 4.6 &mgrm (W1 and W2). The CatWISE Preliminary Catalog consists of 900,849,014 sources measured in data collected from 2010 to 2016. This data set represents four times as many exposures and spans over 10 times as large a time baselin…

2020 The Astrophysical Journal Supplement Series
Gaia 105
Scaling K2. I. Revised Parameters for 222,088 K2 Stars and a K2 Planet Radius Valley at 1.9 R
DOI: 10.3847/1538-4365/ab7230 Bibcode: 2020ApJS..247...28H

Schlieder, Joshua E.; Ciardi, David R.; Dressing, Courtney D. +3 more

Previous measurements of stellar properties for K2 stars in the Ecliptic Plane Input Catalog largely relied on photometry and proper motion measurements, with some added information from available spectra and parallaxes. Combining Gaia DR2 distances with spectroscopic measurements of effective temperatures, surface gravities, and metallicities fro…

2020 The Astrophysical Journal Supplement Series
Gaia 95
The R-Process Alliance: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo
DOI: 10.3847/1538-4365/ab9c19 Bibcode: 2020ApJS..249...30H

Grebel, Eva K.; Drout, Maria R.; Steinmetz, Matthias +22 more

This compilation is the fourth data release from the R-Process Alliance (RPA) search for r-process-enhanced stars and the second release based on "snapshot" high-resolution (R ∼ 30,000) spectra collected with the du Pont 2.5 m Telescope. In this data release, we propose a new delineation between the r-I and r-II stellar classes at $[\mathrm{Eu}/\m…

2020 The Astrophysical Journal Supplement Series
Gaia 91
Structure of Brightest Cluster Galaxies and Intracluster Light
DOI: 10.3847/1538-4365/ab733b Bibcode: 2020ApJS..247...43K

Brosch, N.; Schmidt, M.; Bender, R. +6 more

Observations of 170 local (z ≲ 0.08) galaxy clusters in the northern hemisphere have been obtained with the Wendelstein Telescope Wide Field Imager (WWFI). We correct for systematic effects such as point-spread function broadening, foreground star contamination, relative bias offsets, and charge persistence. Background inhomogeneities induced by s…

2020 The Astrophysical Journal Supplement Series
eHST 86
The Separation Distribution of Ultrawide Binaries across Galactic Populations
DOI: 10.3847/1538-4365/ab54c4 Bibcode: 2020ApJS..246....4T

Tian, Hai-Jun; Rix, Hans-Walter; Gould, Andrew +1 more

We present an extensive and pure sample of ultrawide binary stars with separations of 0.01 ≲ s/pc ≲ 1 in the solar neighborhood. Using data from Gaia DR2, we define kinematic subpopulations via the systems’ tangential velocities, I.e., disk-like (V ⊥,tot ≤ 40 km s-1), intermediate (V ⊥,tot = 40-85 km s-1

2020 The Astrophysical Journal Supplement Series
Gaia 76
Morpheus: A Deep Learning Framework for the Pixel-level Analysis of Astronomical Image Data
DOI: 10.3847/1538-4365/ab8868 Bibcode: 2020ApJS..248...20H

Hausen, Ryan; Robertson, Brant E.

We present Morpheus, a new model for generating pixel-level morphological classifications of astronomical sources. Morpheus leverages advances in deep learning to perform source detection, source segmentation, and morphological classification pixel-by-pixel via a semantic segmentation algorithm adopted from the field of computer vision. By utilizi…

2020 The Astrophysical Journal Supplement Series
eHST 74
Anticorrelation between the Bulk Speed and the Electron Temperature in the Pristine Solar Wind: First Results from the Parker Solar Probe and Comparison with Helios
DOI: 10.3847/1538-4365/ab61fc Bibcode: 2020ApJS..246...62M

Maksimovic, M.; Bale, S. D.; Štverák, Š. +25 more

We discuss the solar wind electron temperatures Te as measured in the nascent solar wind by Parker Solar Probe during its first perihelion pass. The measurements have been obtained by fitting the high-frequency part of quasi-thermal noise spectra recorded by the Radio Frequency Spectrometer. In addition we compare these measurements wit…

2020 The Astrophysical Journal Supplement Series
Ulysses 70
Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey
DOI: 10.3847/1538-4365/ab5f13 Bibcode: 2020ApJS..247...12S

Mahler, Guillaume; Rigby, Jane R.; Whitaker, Katherine E. +13 more

We present strong gravitational lensing models for 37 galaxy clusters from the Sloan Digital Sky Survey Giant Arcs Survey. We combine data from multi-band Hubble Space Telescope Wide Field Camera 3 (WFC3) imaging, with ground-based imaging and spectroscopy from Magellan, Gemini, Apache Point Observatory, and the Multiple Mirror Telescope, in order…

2020 The Astrophysical Journal Supplement Series
eHST 70
The SUPERWIDE Catalog: A Catalog of 99,203 Wide Binaries Found in Gaia and Supplemented by the SUPERBLINK High Proper Motion Catalog
DOI: 10.3847/1538-4365/ab79a6 Bibcode: 2020ApJS..247...66H

Hartman, Zachary D.; Lépine, Sébastien

We present a catalog of 99,203 wide binary systems, initially identified as common proper motion (CPM) pairs from a subset of ∼5.2 million stars with proper motions µ > 40 mas yr-1, selected from Gaia data release 2 (DR2) and the SUPERBLINK high proper motion catalog. CPM pairs are found by searching for pairs of stars with ang…

2020 The Astrophysical Journal Supplement Series
Gaia 68
Solar System Objects Observed with TESS—First Data Release: Bright Main-belt and Trojan Asteroids from the Southern Survey
DOI: 10.3847/1538-4365/ab64f0 Bibcode: 2020ApJS..247...26P

Pál, András; Kalup, Csilla; Szakáts, Róbert +10 more

Compared with previous space-borne surveys, the Transiting Exoplanet Survey Satellite (TESS) provides a unique and new approach to observe solar system objects. While its primary mission avoids the vicinity of the ecliptic plane by approximately six degrees, the scale height of the solar system debris disk is large enough to place various small bo…

2020 The Astrophysical Journal Supplement Series
Gaia 63