Search Results - "Bechtol, K."
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Detailed Abundances in the Ultra-faint Magellanic Satellites Carina II and III
Published in The Astrophysical journal (20-01-2020)“…We present the first detailed elemental abundances in the ultra-faint Magellanic satellite galaxies Carina II (Car II) and Carina III (Car III). With…”
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EIGHT NEW MILKY WAY COMPANIONS DISCOVERED IN FIRST-YEAR DARK ENERGY SURVEY DATA
Published in The Astrophysical journal (01-07-2015)“…ABSTRACT We report the discovery of eight new Milky Way companions in of optical imaging data collected during the first year of the Dark Energy Survey (DES)…”
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The Dark Energy Survey Image Processing Pipeline
Published in Publications of the Astronomical Society of the Pacific (01-07-2018)“…The Dark Energy Survey (DES) is a five-year optical imaging campaign with the goal of understanding the origin of cosmic acceleration. DES performs a ∼5000…”
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Discovery of two neighbouring satellites in the Carina constellation with MagLiteS
Published in Monthly notices of the Royal Astronomical Society (21-04-2018)“…Abstract We report the discovery of two ultra-faint satellites in the vicinity of the Large Magellanic Cloud (LMC) in data from the Magellanic Satellites…”
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The southern stellar stream spectroscopic survey (S5): Overview, target selection, data reduction, validation, and early science
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…ABSTRACT We introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the…”
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Digging deeper into the Southern skies: a compact Milky Way companion discovered in first-year Dark Energy Survey data
Published in Monthly notices of the Royal Astronomical Society (01-05-2016)“…We use the first-year Dark Energy Survey (DES) data down to previously unprobed photometric depths to search for stellar systems in the Galactic halo,…”
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An r-process Enhanced Star in the Dwarf Galaxy Tucana III
Published in The Astrophysical journal (20-03-2017)“…Abstract Chemically peculiar stars in dwarf galaxies provide a window for exploring the birth environment of stars with varying chemical enrichment. We present…”
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Birds of a Feather? Magellan/IMACS Spectroscopy of the Ultra-faint Satellites Grus II, Tucana IV, and Tucana V
Published in The Astrophysical journal (01-04-2020)“…Abstract We present Magellan/IMACS spectroscopy of three recently discovered ultra-faint Milky Way satellites, Grus II, Tucana IV, and Tucana V. We measure…”
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SEARCH FOR SPATIALLY EXTENDED FERMI LARGE AREA TELESCOPE SOURCES USING TWO YEARS OF DATA
Published in The Astrophysical journal (01-09-2012)“…Spatial extension is an important characteristic for correctly associating [gamma]-ray-emitting sources with their counterparts at other wavelengths and for…”
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Ships Passing in the Night: Spectroscopic Analysis of Two Ultra-faint Satellites in the Constellation Carina
Published in The Astrophysical journal (20-04-2018)“…Abstract We present Magellan/IMACS, Anglo-Australian Telescope/AAOmega+2dF, and Very Large Telescope/GIRAFFE+FLAMES spectroscopy of the Carina II (Car II) and…”
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A Faint Halo Star Cluster Discovered in the Blanco Imaging of the Southern Sky Survey
Published in The Astrophysical journal (20-04-2019)“…We present the discovery of a faint, resolved stellar system, BLISS J0321+0438 (BLISS 1), found in Dark Energy Camera data from the first observing run of the…”
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12
Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C
Published in Science (American Association for the Advancement of Science) (27-03-2009)“…Gamma-ray bursts (GRBs) are highly energetic explosions signaling the death of massive stars in distant galaxies. The Gamma-ray Burst Monitor and Large Area…”
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Two Ultra-faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey
Published in The Astrophysical journal (20-02-2020)“…We report the discovery of two ultra-faint stellar systems found in early data from the DECam Local Volume Exploration survey (DELVE). The first system,…”
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14
Brown dwarf census with the Dark Energy Survey year 3 data and the thin disc scale height of early L types
Published in Monthly notices of the Royal Astronomical Society (11-11-2019)“…ABSTRACT In this paper we present a catalogue of 11 745 brown dwarfs with spectral types ranging from L0 to T9, photometrically classified using data from the…”
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A Deeper Look at DES Dwarf Galaxy Candidates: Grus i and Indus ii
Published in The Astrophysical journal (01-08-2021)“…Abstract We present deep g - and r -band Magellan/Megacam photometry of two dwarf galaxy candidates discovered in the Dark Energy Survey (DES), Grus i and…”
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SPATIALLY RESOLVING A STARBURST GALAXY AT HARD X-RAY ENERGIES: NuSTAR , CHANDRA , AND VLBA OBSERVATIONS OF NGC 253
Published in The Astrophysical journal (20-12-2014)“…Prior to the launch of NuSTAR, it was not feasible to spatially resolve the hard (E > 10 keV) emission from galaxies beyond the Local Group. The combined…”
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Expediting DECam Multimessenger Counterpart Searches with Convolutional Neural Networks
Published in The Astrophysical journal (01-01-2022)“…Abstract Searches for counterparts to multimessenger events with optical imagers use difference imaging to detect new transient sources. However, even with…”
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Astrometric Calibration and Performance of the Dark Energy Camera
Published in Publications of the Astronomical Society of the Pacific (01-07-2017)“…We characterize the ability of the Dark Energy Camera (DECam) to perform relative astrometry across its 500 Mpix, 3-deg2 science field of view and across four…”
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Chemical Abundance Analysis of Tucana III, the Second r-process Enhanced Ultra-faint Dwarf Galaxy
Published in The Astrophysical journal (10-09-2019)“…Abstract We present a chemical abundance analysis of four additional confirmed member stars of Tucana III, a Milky Way satellite galaxy candidate in the…”
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DeepZipper: A Novel Deep-learning Architecture for Lensed Supernovae Identification
Published in The Astrophysical journal (01-03-2022)“…Abstract Large-scale astronomical surveys have the potential to capture data on large numbers of strongly gravitationally lensed supernovae (LSNe). To…”
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