Zobrazeno 1 - 10
of 54
pro vyhledávání: '"Blaylock, Myra"'
Publikováno v:
In Process Safety and Environmental Protection May 2023 173:22-38
Autor:
Hsieh, Alan S., Brown, Kenneth A., deVelder, Nathaniel B., Herges, Thomas G., Knaus, Robert C., Sakievich, Philip J., Cheung, Lawrence C., Houchens, Brent C., Blaylock, Myra L., Maniaci, David C.
Publikováno v:
In Journal of Wind Engineering & Industrial Aerodynamics November 2021 218
Autor:
Mangala Gitushi, Kevin1 (AUTHOR), Blaylock, Myra2 (AUTHOR), Hecht, Ethan S.2 (AUTHOR) ehecht@sandia.gov
Publikováno v:
Energies (19961073). Feb2023, Vol. 16 Issue 4, p1580. 15p.
Autor:
Quiroz-Arita, Carlos, Blaylock, Myra L., Gharagozloo, Patricia E., Bradley, Thomas H., Dempster, Thomas, McGowen, John, Davis, Ryan W.
Publikováno v:
In Bioresource Technology Reports June 2020 10
Autor:
Perez-Gonzalez, Pablo G., Rieke, George H., Villar, Victor, Barro, Guillermo, Blaylock, Myra, Egami, Eiichi, Gallego, Jesus, de Paz, Armando Gil, Pascual, Sergio, Zamorano, Jaime, Donley, Jennifer L.
Publikováno v:
ApJ, 675(1), p. 234 (2008)
Using a sample of ~28,000 sources selected at 3.6-4.5 microns with Spitzer observations of the HDF-N, the CDF-S, and the Lockman Hole (surveyed area: ~664 arcmin^2), we study the evolution of the stellar mass content of the Universe at 0
Externí odkaz:
http://arxiv.org/abs/0709.1354
Autor:
Bai, Lei, Marcillac, Delphine, Rieke, George H., Rieke, Marcia J., Tran, Kim-Vy H., Hinz, Joannah L., Rudnick, Gregory, Kelly, Douglas M., Blaylock, Myra
Publikováno v:
Astrophys.J.664:181-197,2007
We study the infrared (IR) properties of galaxies in the cluster MS 1054-03 at z=0.83 by combining MIPS 24 micron data with spectra of more than 400 galaxies and a very deep K-band selected catalog. 19 IR cluster members are selected spectroscopicall
Externí odkaz:
http://arxiv.org/abs/0704.0953
Autor:
Dole, Herve, Lagache, Guilaine, Puget, Jean-Loup, Caputi, Karina I., Fernandez-Conde, Nestor, Floc'h, Emeric Le, Papovich, Casey, Perez-Gonzalez, Pablo G., Rieke, George H., Blaylock, Myra
Aims. We quantify the contributions of 24um galaxies to the Far-Infrared (FIR) Background at 70 and 160um. We provide new estimates of the Cosmic Infrared Background (CIB), and compare it with the Cosmic Optical Background (COB). Methods. Using Spitz
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603208
Autor:
Bai, Lei, Rieke, George H., Rieke, Marcia J., Hinz, Joannah L., Kelly, Douglas M., Blaylock, Myra
Publikováno v:
Astrophys.J.639:827-837,2006
Using mid-IR and optical data, we deduce the total infrared (IR) luminosities of galaxies in the Coma cluster and present their infrared luminosity function (LF). The shape of the overall Coma IR LF does not show significant differences from the IR L
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512069
Autor:
Perez-Gonzalez, Pablo G., Rieke, George H., Egami, Eiichi, Alonso-Herrero, Almudena, Dole, Herve, Papovich, Casey, Blaylock, Myra, Jones, Jessica, Rieke, Marcia, Rigby, Jane, Barmby, Pauline, Fazio, Giovanni G., Huang, Jiasheng, Martin, Christopher
Publikováno v:
Astrophys.J.630:82-107,2005
We use a 24 micron selected sample containing more than 8,000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3. We obtain photometric redshifts for most of the sources in our survey using a method based on
Externí odkaz:
http://arxiv.org/abs/astro-ph/0505101
Akademický článek
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