Search Publications

The SPTpol Extended Cluster Survey
DOI: 10.3847/1538-4365/ab6993 Bibcode: 2020ApJS..247...25B

Sharon, K.; Gladders, M. D.; Ade, P. A. R. +135 more

We describe the observations and resultant galaxy cluster catalog from the 2770 deg2 SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev-Zel'dovich (SZ) effect and confirmed with a combination of archival and targeted follow-up data, making particular use of data from the Dark Energy Survey (DES). With inco…

2020 The Astrophysical Journal Supplement Series
Gaia eHST 184
The ALPINE-ALMA [C II] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements
DOI: 10.3847/1538-4365/ab7ccd Bibcode: 2020ApJS..247...61F

Cimatti, A.; Pozzi, F.; Rodighiero, G. +37 more

We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey - the first large multiwavelength survey that aims at characterizing the gas and dust properties of 118 main-sequence galaxies at redshifts 4.4 < z < 5.9 via the measurement of […

2020 The Astrophysical Journal Supplement Series
Gaia eHST 141
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
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
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
High-resolution UV/Optical/IR Imaging of Jupiter in 2016-2019
DOI: 10.3847/1538-4365/ab775f Bibcode: 2020ApJS..247...58W

de Pater, Imke; Wong, Michael H.; Fletcher, Leigh N. +13 more

Imaging observations of Jupiter with high spatial resolution were acquired beginning in 2016, with a cadence of 53 days to coincide with atmospheric observations of the Juno spacecraft during each perijove pass. The Wide Field Camera 3 (WFC3) aboard the Hubble Space Telescope (HST) collected Jupiter images from 236 to 925 nm in 14 filters. The Nea…

2020 The Astrophysical Journal Supplement Series
eHST 40
HST/COS Observations of Quasar Outflows in the 500-1050 Å Rest Frame. I. The Most Energetic Outflows in the Universe and Other Discoveries
DOI: 10.3847/1538-4365/ab66af Bibcode: 2020ApJS..247...37A

Xu, Xinfeng; Kriss, Gerard A.; Arav, Nahum +2 more

The Hubble Space Telescope/Cosmic Origins Spectrograph (COS) has opened a new discovery space for studying quasar absorption outflows and their contribution to active galactic nucleus (AGN) feedback. Specifically, COS provides high-quality far-ultraviolet (FUV) spectra covering the diagnostic-rich 500-1050 Å rest frame (hereafter, EUV500) of mediu…

2020 The Astrophysical Journal Supplement Series
eHST 31
Microlensing Optical Depth and Event Rate in the OGLE-IV Galactic Plane Fields
DOI: 10.3847/1538-4365/ab9366 Bibcode: 2020ApJS..249...16M

Udalski, Andrzej; Mróz, Przemek; Szymański, Michał K. +10 more

Searches for gravitational microlensing events are traditionally concentrated on the central regions of the Galactic bulge but many microlensing events are expected to occur in the Galactic plane, far from the Galactic Center. Owing to the difficulty in conducting high-cadence observations of the Galactic plane over its vast area, which are necess…

2020 The Astrophysical Journal Supplement Series
eHST 30
X-Ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-mass X-Ray Binaries in Galactic Fields
DOI: 10.3847/1538-4365/ab9175 Bibcode: 2020ApJS..248...31L

Brandt, William N.; Tzanavaris, Panayiotis; Basu-Zych, Antara +10 more

We investigate X-ray binary (XRB) luminosity function (XLF) scaling relations for Chandra-detected populations of low-mass XRBs (LMXBs) within the footprints of 24 early-type galaxies. Our sample includes Chandra and Hubble Space Telescope observed galaxies at $D\lesssim 25$ Mpc that have estimates of the globular cluster (GC) specific frequency (…

2020 The Astrophysical Journal Supplement Series
Herschel eHST 29
The Next Generation Virgo Cluster Survey. XXXIV. Ultracompact Dwarf Galaxies in the Virgo Cluster
DOI: 10.3847/1538-4365/abad91 Bibcode: 2020ApJS..250...17L

Zhang, Hongxin; Liu, Chengze; Gwyn, Stephen +26 more

We present a study of ultracompact dwarf (UCD) galaxies in the Virgo cluster based mainly on imaging from the Next Generation Virgo Cluster Survey (NGVS). Using ∼100 deg2 of u*giz imaging, we have identified more than 600 candidate UCDs, from the core of Virgo out to its virial radius. Candidates have been selected through a combination…

2020 The Astrophysical Journal Supplement Series
Gaia eHST 28