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pro vyhledávání: '"Morgan, Dylan"'
Autor:
Klein, Benedikt P., Stoodley, Matthew A., Deyerling, Joel, Rochford, Luke A., Morgan, Dylan B., Hopkinson, David, Sullivan-Allsop, Sam, Eratam, Fulden, Sattler, Lars, Weber, Sebastian M., Hilt, Gerhard, Generalov, Alexander, Preobrajenski, Alexei, Liddy, Thomas, Williams, Leon B. S., Lee, Tien-Lin, Saywell, Alex, Gorbachev, Roman, Haigh, Sarah J., Allen, Christopher, Auwärter, Willi, Maurer, Reinhard J., Duncan, David A.
Chemical vapour deposition enables large-domain growth of ideal graphene, yet many applications of graphene require the controlled inclusion of specific defects. We present a one-step chemical vapour deposition procedure aimed at retaining the precur
Externí odkaz:
http://arxiv.org/abs/2411.02676
Autor:
Ismail, Idil, Chaudhuri, Shayantan, Morgan, Dylan, Woodgate, Christopher D., Fakhoury, Ziad, Targett, James M., Pilgrim, Charlie, Maino, Carlo
This article is intended as a guide for new graduate students in the field of computational science. With the increasing influx of students from diverse backgrounds joining the ever-popular field, this short guide aims to help students navigate throu
Externí odkaz:
http://arxiv.org/abs/2310.13514
Autor:
Morgan, Dylan Parker
I present a study of close white dwarf (WD) and M dwarf (dM) binary systems (WD+dM) to examine the effects that close companions have on the magnetic field generation in dMs. Using the Sloan Digital Sky Survey (SDSS) Data Release 8 spectroscopic data
Externí odkaz:
https://hdl.handle.net/2144/20874
Autor:
Skinner, Julie N., Morgan, Dylan P., West, Andrew A., Lepine, Sebastien, Thorstensen, John R.
We present an activity and kinematic analysis of high proper motion white dwarf-M dwarf binaries (WD+dMs) found in the SUPERBLINK survey, 178 of which are new identifications. To identify WD+dMs, we developed a UV-optical-IR color criterion and condu
Externí odkaz:
http://arxiv.org/abs/1707.08576
We present a study of the statistical flare rates of M dwarfs (dMs) with close white dwarf (WD) companions (WD+dM; typical separations < 1 au). Our previous analysis demonstrated that dMs with close WD companions are more magnetically active than the
Externí odkaz:
http://arxiv.org/abs/1602.06296
Akademický článek
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Autor:
Sesar, Branimir, Ivezić, Željko, Stuart, J. Scott, Morgan, Dylan M., Becker, Andrew C., Sharma, Sanjib, Palaversa, Lovro, Jurić, Mario, Wozniak, Przemyslaw, Oluseyi, Hakeem
We present a sample of ~5,000 RR Lyrae stars selected from the recalibrated LINEAR dataset and detected at heliocentric distances between 5 kpc and 30 kpc over ~8,000 deg^2 of sky. The coordinates and light curve properties, such as period and Ooster
Externí odkaz:
http://arxiv.org/abs/1305.2160
Autor:
Morgan, Dylan P., West, Andrew A., Garcés, Ane, Catalán, Silvia, Dhital, Saurav, Fuchs, Miriam, Silvestri, Nicole M.
We present a study of close white dwarf and M dwarf (WD+dM) binary systems and examine the effect that a close companion has on the magnetic field generation in M dwarfs. We use a base sample of 1602 white dwarf -- main sequence binaries from Rebassa
Externí odkaz:
http://arxiv.org/abs/1205.6806
Autor:
Sesar, Branimir, Stuart, J. Scott, Ivezić, Željko, Morgan, Dylan P., Becker, Andrew C., Woźniak, Przemysław
We describe photometric recalibration of data obtained by the asteroid survey LINEAR. Although LINEAR was designed for astrometric discovery of moving objects, the dataset described here contains over 5 billion photometric measurements for about 25 m
Externí odkaz:
http://arxiv.org/abs/1109.5227
Autor:
West, Andrew A., Morgan, Dylan P., Bochanski, John J., Andersen, Jan Marie, Bell, Keaton J., Kowalski, Adam F., Davenport, James R. A., Hawley, Suzanne L., Schmidt, Sarah J., Bernat, David, Hilton, Eric J., Muirhead, Philip, Covey, Kevin R., Rojas-Ayala, Barbara, Schlawin, Everett, Gooding, Mary, Schluns, Kyle, Dhital, Saurav, Pineda, J. Sebastian, Jones, David O.
We present a spectroscopic catalog of 70,841 visually inspected M dwarfs from the seventh data release of the Sloan Digital Sky Survey (SDSS). For each spectrum, we provide measurements of the spectral type, a number of molecular bandheads, and the H
Externí odkaz:
http://arxiv.org/abs/1101.1082