Zobrazeno 1 - 10
of 2 866
pro vyhledávání: '"Balser A"'
Autor:
Bania, T. M., Balser, Dana S., Wenger, Trey V., Ireland, Spencer J., Anderson, L. D., Luisi, Matteo
Diffuse ionized gas pervades the disk of the Milky Way. We detect extremely faint emission from this Galactic Warm Ionized Medium (WIM) using the Green Bank Telescope to make radio recombination line (RRL) observations toward two Milky Way sight line
Externí odkaz:
http://arxiv.org/abs/2407.06396
Autor:
Balser, Dana S., Wenger, Trey V.
HII region heavy-element abundances throughout the Galactic disk provide important constraints to theories of the formation and evolution of the Milky Way. In LTE, radio recombination line (RRL) and free-free continuum emission are accurate extinctio
Externí odkaz:
http://arxiv.org/abs/2401.17969
Autor:
Anderson, L. D., Liu, B., Balser, Dana S., Bania, T. M., Haffner, L. M., Linville, Dylan J., Luisi, Matteo, Wenger, Trey V.
The ideal spectral averaging method depends on one's science goals and the available information about one's data. Including low-quality data in the average can decrease the signal-to-noise ratio (SNR), which may necessitate an optimization method or
Externí odkaz:
http://arxiv.org/abs/2310.09076
Autor:
Linville, Dylan J., Luisi, Matteo, Anderson, L. D., Liu, Bin, Bania, T. M., Balser, Dana S., Wenger, Trey V., Haffner, L. M., Mascoop, J. L.
The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by observing radio recombination line (RRL) emission from 4-8 GHz. The nominal survey zone is $32.3^{\circ}> {\ell} > -5^{\circ}$, $|b|<0.5^
Externí odkaz:
http://arxiv.org/abs/2310.01607
Standard stellar evolution models that only consider convection as a physical process to mix material inside of stars predict the production of significant amounts of 3He in low-mass stars (M < 2 Msun), with peak abundances of 3He/H ~ few x 10-3 by n
Externí odkaz:
http://arxiv.org/abs/2208.03395
Several recent investigations indicate the existence of gender-related systematic trends in the peer review of proposals for observations on astronomical facilities. This includes the National Radio Astronomy Observatory (NRAO) where there is evidenc
Externí odkaz:
http://arxiv.org/abs/2110.12488
Autor:
Balser, Dana S., Wenger, Trey V., Anderson, L. D., Armentrout, W. P., Bania, T. M., Dawson, J. R., Dickey, John M.
We investigate the kinematic properties of Galactic HII regions using radio recombination line (RRL) emission detected by the Australia Telescope Compact Array (ATCA) at 4-10 GHz and the Jansky Very Large Array (VLA) at 8-10 GHz. Our HII region sampl
Externí odkaz:
http://arxiv.org/abs/2108.06330
Autor:
Camacho, M. Catalina, Balser, Dorothy H., Furtado, Emily J., Rogers, Cynthia E., Schwarzlose, Rebecca F., Sylvester, Chad M., Barch, Deanna M.
Publikováno v:
In Journal of the American Academy of Child & Adolescent Psychiatry May 2024 63(5):549-560
Autor:
Wenger, Trey V., Dawson, J. R., Dickey, John M., Jordan, C. H., McClure-Griffiths, N. M., Anderson, L. D., Armentrout, W. P., Balser, Dana S., Bania, T. M.
The Southern HII Region Discovery Survey (SHRDS) is a 900 hour Australia Telescope Compact Array 4-10 GHz radio continuum and radio recombination line (RRL) survey of Galactic HII regions and infrared-identified HII region candidates in the southern
Externí odkaz:
http://arxiv.org/abs/2103.12199
Autor:
Anderson, L. D., Luisi, Matteo, Liu, Bin, Wenger, Trey V., Balser, Dana. S., Bania, T. M., Haffner, L. M., Linville, Dylan J., Mascoop, J. L.
The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by measuring $4-8$GHz radio recombination line (RRL) emission. The nominal survey zone is $32.3^{\circ}> l >-5^{\circ}$, $|b|<0.5^{\circ}$,
Externí odkaz:
http://arxiv.org/abs/2103.10466