Search Results - "MOORE, Anna M"
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Andromeda's Parachute: A Bright Quadruply Lensed Quasar at z = 2.377
Published in The Astrophysical journal (01-06-2018)“…We present Keck Cosmic Web Imager spectroscopy of the four putative images of the lensed quasar candidate J014710+463040 recently discovered by Berghea et al…”
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A Sensitive Search for Supernova Emission Associated with the Extremely Energetic and Nearby GRB 221009A
Published in Astrophysical journal. Letters (01-06-2023)“…We report observations of the optical counterpart of the long gamma-ray burst GRB 221009A. Due to the extreme rarity of being both nearby (z = 0.151) and…”
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3
Direct evidence of AGN feedback: a post-starburst galaxy stripped of its gas by AGN-driven winds
Published in Monthly notices of the Royal Astronomical Society (01-11-2018)Get full text
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Palomar Gattini-IR: Survey Overview, Data Processing System, On-sky Performance and First Results
Published in Publications of the Astronomical Society of the Pacific (01-02-2020)“…Palomar Gattini-IR is a new wide-field, near-infrared (NIR) robotic time domain survey operating at Palomar Observatory. Using a 30 cm telescope mounted with a…”
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5
Resolving the H i in damped Lyman α systems that power star formation
Published in Nature (London) (02-06-2022)“…Reservoirs of dense atomic gas (primarily hydrogen) contain approximately 90 per cent of the neutral gas at a redshift of 3, and contribute to between 2 and 3…”
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A Population of Heavily Reddened, Optically Missed Novae from Palomar Gattini-IR: Constraints on the Galactic Nova Rate
Published in The Astrophysical journal (01-05-2021)“…Abstract The nova rate in the Milky Way remains largely uncertain, despite its vital importance in constraining models of Galactic chemical evolution as well…”
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Unveiling the dynamic infrared sky
Published in Nature astronomy (01-01-2019)“…Palomar Gattini-IR is the first of a number of infrared transient surveyors that will search the skies nightly, looking for ephemeral phenomena such as novae,…”
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Possible anticorrelations between pulsation amplitudes and the disc growth of Be stars in giant-outbursting Be X-ray binaries
Published in Monthly notices of the Royal Astronomical Society (09-10-2024)“…ABSTRACT The mechanism of X-ray outbursts in Be X-ray binaries remains a mystery, and understanding their circumstellar discs is crucial for a solution of the…”
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Ultra wide‐field infrared astronomy in Antarctica
Published in Astronomische Nachrichten (01-10-2023)“…The science enabled by the deep and high‐cadence survey that will be performed by the Vera Rubin Observatory has led to an increase of survey and follow‐up…”
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SRGA J181414.6-225604: A New Galactic Symbiotic X-Ray Binary Outburst Triggered by an Intense Mass-loss Episode of a Heavily Obscured Mira Variable
Published in The Astrophysical journal (01-08-2022)“…Abstract We present the discovery and multiwavelength characterization of SRGA J181414.6-225604, a Galactic hard X-ray transient discovered during the ongoing…”
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A survey for variable young stars with small telescopes: VI – Analysis of the outbursting Be stars NSW 284, gaia 19eyy, and VES 263
Published in Monthly notices of the Royal Astronomical Society (22-02-2023)“…ABSTRACT This paper is one in a series reporting results from small telescope observations of variable young stars. Here, we study the repeating outbursts of…”
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A Massive AGB Donor in Scutum X-1: Identification of the First Mira Variable in an X-Ray Binary
Published in Astrophysical journal. Letters (01-03-2022)“…Abstract The symbiotic X-ray binary Sct X-1 was suggested to be the first known neutron star accreting from a red supergiant companion. Although known for…”
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13
Extensive diffuse Lyman-α emission correlated with cosmic structure
Published in Nature astronomy (01-11-2023)“…The intergalactic medium represents the dominant reservoir of baryons at high redshift, traces the architecture of the cosmic web dominated by dark matter and…”
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Discovery of a 310 Day Period from the Enshrouded Massive System NaSt1 (WR 122)
Published in The Astrophysical journal (01-11-2021)“…Abstract We present optical and infrared (IR) light curves of NaSt1, also known as Wolf–Rayet 122, with observations from Palomar Gattini-IR (PGIR), the Zwicky…”
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15
Airglow and Aurorae at Dome A, Antarctica
Published in Publications of the Astronomical Society of the Pacific (01-06-2012)“…ABSTRACT Despite the absence of artificial light pollution at Antarctic plateau sites such as Dome A, other factors such as airglow, aurorae, and extended…”
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A Close Companion Search Around L Dwarfs Using Aperture Masking Interferometry and Palomar Laser Guide Star Adaptive Optics
Published in The Astrophysical journal (01-06-2010)“…We present a close companion search around 16 known early L dwarfs using aperture masking interferometry with Palomar laser guide star adaptive optics (LGS…”
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Palomar Gattini-IR: Survey Overview, Data Processing System, On-sky Performance and First Results
Published in Publications of the Astronomical Society of the Pacific (01-02-2020)“…Palomar Gattini-IR is a new wide-field, near-infrared (NIR) robotic time domain survey operating at Palomar Observatory. Using a 30 cm telescope mounted with a…”
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18
Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope
Published in Publications of the Astronomical Society of Japan (25-10-2010)“…Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to…”
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Operationally convenient, efficient asymmetric synthesis of enantiomerically pure 4-aminoglutamic acids via methylene dimerization of chiral glycine equivalents with dichloromethane
Published in Tetrahedron (26-06-2006)“…This paper presents a practical and efficient asymmetric synthesis of enantiomerically pure 4-aminoglutamic acids using a quite unusual methylene dimerization…”
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The first Palomar Gattini-IR catalog of J-band light curves: construction and public data release
Published 03-06-2024“…Palomar Gattini-IR is a wide-field, synoptic infrared time domain survey covering $\approx 15000$ sq. deg. of the sky at $\approx 1-3$ night cadence to a depth…”
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