Search Results - "Meisner, Aaron"
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MODELING THERMAL DUST EMISSION WITH TWO COMPONENTS: APPLICATION TO THE PLANCK HIGH FREQUENCY INSTRUMENT MAPS
Published in The Astrophysical journal (10-01-2015)“…We apply the Finkbeiner et al. two-component thermal dust emission model to the Planck High Frequency Instrument maps. This parameterization of the…”
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unTimely: a Full-sky, Time-domain unWISE Catalog
Published in The Astronomical journal (01-02-2023)“…Abstract We present the unTimely Catalog, a deep time-domain catalog of detections based on Wide-field Infrared Survey Explorer (WISE) and NEOWISE observations…”
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A new physical interpretation of optical and infrared variability in quasars
Published in Monthly notices of the Royal Astronomical Society (11-11-2018)“…Changing-look quasars are a recently identified class of active galaxies in which the strong UV continuum and/or broad optical hydrogen emission lines…”
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A CASE AGAINST SPINNING PAHS AS THE SOURCE OF THE ANOMALOUS MICROWAVE EMISSION
Published in The Astrophysical journal (10-08-2016)“…ABSTRACT We employ an all-sky map of the anomalous microwave emission (AME) produced by component separation of the microwave sky to study correlations between…”
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A Mid-IR Selected Changing-look Quasar and Physical Scenarios for Abrupt AGN Fading
Published in The Astrophysical journal (01-09-2018)“…We report a new changing-look quasar, WISE J105203.55+151929.5 at z = 0.303, found by identifying highly mid-IR-variable quasars in the Wide-field Infrared…”
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The clustering of DESI-like luminous red galaxies using photometric redshifts
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT We present measurements of the redshift-dependent clustering of a DESI-like luminous red galaxy (LRG) sample selected from the Legacy Survey imaging…”
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A FULL-SKY, HIGH-RESOLUTION ATLAS OF GALACTIC 12 μm DUST EMISSION WITH WISE
Published in The Astrophysical journal (20-01-2014)“…We describe our custom processing of the entire Wide-field Infrared Survey Explorer (WISE) 12 mu m imaging data set, and present a high-resolution, full-sky…”
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WISE 2150-7520AB: A Very Low-mass, Wide Comoving Brown Dwarf System Discovered through the Citizen Science Project Backyard Worlds: Planet 9
Published in The Astrophysical journal (01-02-2020)“…We report the discovery of WISE 2150-7520AB (W2150AB): a widely separated (∼341 au) very low-mass L1 + T8 co-moving system. The system consists of the…”
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Rapidly evolving Galactic plane outbursts in NEOWISE: revisiting the Galactic nova rate with the first all-sky search in the mid-infrared
Published in Monthly notices of the Royal Astronomical Society (08-06-2023)“…ABSTRACT The Galactic nova rate is intimately linked to our understanding of its chemical enrichment and progenitor channels of Type Ia supernovae. Yet past…”
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Long-term 4.6 μm Variability in Brown Dwarfs and a New Technique for Identifying Brown Dwarf Binary Candidates
Published in The Astronomical journal (01-06-2023)“…Abstract Using a sample of 361 nearby brown dwarfs, we have searched for 4.6 μ m variability, indicative of large-scale rotational modulations or large-scale,…”
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Exploring the Extremes: Characterizing a New Population of Old and Cold Brown Dwarfs
Published in The Astronomical journal (01-08-2023)“…Abstract Mapping out the populations of thick disk and halo brown dwarfs is important for understanding the metallicity dependence of low-temperature…”
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DECam Multimessenger Astrophysics Pipeline. I. From Raw Data to Single-exposure Candidates
Published in The Astronomical journal (01-10-2024)“…Abstract We introduce a pipeline that performs rapid image subtraction and source selection to detect transients, with a focus on identifying…”
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The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
Published in The Astrophysical journal. Supplement series (01-02-2023)“…Abstract Deep optical and near-infrared imaging of the entire Galactic plane is essential for understanding our Galaxy’s stars, gas, and dust. The second data…”
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A New Population of Mid-infrared-selected Tidal Disruption Events: Implications for Tidal Disruption Event Rates and Host Galaxy Properties
Published in The Astrophysical journal (01-02-2024)“…Abstract Most tidal disruption events (TDEs) are currently found in time-domain optical and soft X-ray surveys, both of which are prone to significant…”
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Siena Galaxy Atlas 2020
Published in The Astrophysical journal. Supplement series (01-11-2023)“…Abstract We present the 2020 version of the Siena Galaxy Atlas (SGA-2020), a multiwavelength optical and infrared imaging atlas of 383,620 nearby galaxies. The…”
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Simulating Brown Dwarf Observations for Various Mass Functions, Birthrates, and Low-mass Cutoffs
Published in The Astrophysical journal (01-10-2024)“…Abstract After decades of brown dwarf discovery and follow-up, we can now infer the functional form of the mass distribution within 20 pc, which serves as a…”
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A Luminous Dust-obscured Tidal Disruption Event Candidate in a Star-forming Galaxy at 42 Mpc
Published in Astrophysical journal. Letters (01-05-2023)“…Abstract While the vast majority of tidal disruption events (TDEs) have been identified by wide-field sky surveys in the optical and X-ray bands, recent…”
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An infrared transient from a star engulfing a planet
Published in Nature (London) (04-05-2023)“…Planets with short orbital periods (roughly under 10 days) are common around stars like the Sun 1 , 2 . Stars expand as they evolve and thus we expect their…”
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WISEA J041451.67-585456.7 and WISEA J181006.18-101000.5: The First Extreme T-type Subdwarfs?
Published in The Astrophysical journal (01-07-2020)“…We present the discoveries of WISEA J041451.67−585456.7 and WISEA J181006.18−101000.5, two low-temperature (1200-1400 K), high proper motion T-type subdwarfs…”
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An Investigation of New Brown Dwarf Spectral Binary Candidates From the Backyard Worlds: Planet 9 Citizen Science Initiative
Published in The Astronomical journal (01-12-2023)“…Abstract We present three new brown dwarf spectral-binary candidates: CWISE J072708.09−360729.2, CWISE J103604.84−514424.4, and CWISE J134446.62−732053.9,…”
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