Zobrazeno 1 - 10
of 87
pro vyhledávání: '"Zarija Lukić"'
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 1, p 46 (2024)
Dense gas in minihalos with masses of 10 ^6 −10 ^8 M _⊙ can shield themselves from reionization for ∼100 Myr after being exposed to the UV background. These self-shielded systems, often unresolved in cosmological simulations, can introduce stro
Externí odkaz:
https://doaj.org/article/1e1e57cf87be47489d5ccd0fa45de4f2
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 1, p 21 (2023)
Hydrodynamical cosmological simulations are a powerful tool for accurately predicting the properties of the intergalactic medium (IGM) and for producing mock skies that can be compared against observational data. However, the need to resolve density
Externí odkaz:
https://doaj.org/article/679f6cec74134f56a2e57d0d4ec532e1
Autor:
Tobias M. Schmidt, Gabor Worseck, Joseph F. Hennawi, J. Xavier Prochaska, Neil H. M. Crighton, Zarija Lukić, Jose Oñorbe
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 4 (2017)
The reionization of helium at z ~ 3 is the final phase transition of the intergalactic medium and supposed to be driven purely by quasars. The He ii transverse proximity effect—enhanced He ii transmission in a background sightline caused by the ion
Externí odkaz:
https://doaj.org/article/8eb93fecac3c4276b77df4dcdaff121f
Autor:
C. L. Morris, Konstantin Borozdin, Jeffrey Bacon, Elliott Chen, Zarija Lukić, Edward Milner, Haruo Miyadera, John Perry, Dave Schwellenbach, Derek Aberle, Wendi Dreesen, J. Andrew Green, George G. McDuff, Kanetada Nagamine, Michael Sossong, Candace Spore, Nathan Toleman
Publikováno v:
AIP Advances, Vol 2, Iss 4, Pp 042128-042128-7 (2012)
The passage of muons through matter is dominated by the Coulomb interaction with electrons and nuclei in the matter. The muon interaction with the electrons leads to continuous energy loss and stopping of the muons. The muon interaction with nuclei l
Externí odkaz:
https://doaj.org/article/a11b6227ee654bef9c6f158b8a2d7555
Autor:
C. L. Morris, Jeffrey Bacon, Konstantin Borozdin, Haruo Miyadera, John Perry, Evan Rose, Scott Watson, Tim White, Derek Aberle, J. Andrew Green, George G. McDuff, Zarija Lukić, Edward C. Milner
Publikováno v:
AIP Advances, Vol 3, Iss 8, Pp 082128-082128 (2013)
Muon tomography is a technique that uses cosmic ray muons to generate three dimensional images of volumes using information contained in the Coulomb scattering of the muons. Advantages of this technique are the ability of cosmic rays to penetrate sig
Externí odkaz:
https://doaj.org/article/7edd4912ead5419dae7728c315d09a07
Autor:
Haruo Miyadera, Konstantin N. Borozdin, Steve J. Greene, Zarija Lukić, Koji Masuda, Edward C. Milner, Christopher L. Morris, John O. Perry
Publikováno v:
AIP Advances, Vol 3, Iss 5, Pp 052133-052133 (2013)
A study of imaging the Fukushima Daiichi reactors with cosmic-ray muons to assess the damage to the reactors is presented. Muon scattering imaging has high sensitivity for detecting uranium fuel and debris even through thick concrete walls and a reac
Externí odkaz:
https://doaj.org/article/5e4df589add848a5a088fb0ae6c31f49
Autor:
Solène Chabanier, J D Emberson, Zarija Lukić, Jesus Pulido, Salman Habib, Esteban Rangel, Jean Sexton, Nicholas Frontiere, Michael Buehlmann
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 518:3754-3776
We compare two state-of-the-art numerical codes to study the overall accuracy in modeling the intergalactic medium and reproducing Lyman-$\alpha$ forest observables for DESI and high-resolution data sets. The codes employ different approaches to solv
Publikováno v:
The Astrophysical Journal. 941:42
Generating large volume hydrodynamical simulations for cosmological observables is a computationally demanding task necessary for next generation observations. In this work, we construct a novel fully convolutional variational auto-encoder (VAE) to s
Autor:
Molly Wolfson, Joseph F. Hennawi, Jose Oñorbe, Hector Hiss, Zarija Lukić, Frederick B. Davies
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 508(4), 5493-5513
The thermal state of the intergalactic medium (IGM) contains vital information about the epoch of reionization, one of the most transformative yet poorly understood periods in the young universe. This thermal state is encoded in the small-scale struc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd2622824ccaa060d6be1188430a63dd
http://arxiv.org/abs/2110.02828
http://arxiv.org/abs/2110.02828
Autor:
Zarija Lukić, Christian Rodriguez, Joseph F. Hennawi, J. Xavier Prochaska, Todd M. Tripp, Vikram Khaire, Michael Walther, Joseph N. Burchett, Jose Oñorbe
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 486:769-782
We present new measurements of the flux power-spectrum P(k) of the z < 0.5 H i Lyman-α Forest spanning scales $k \sim 0.001\!-\!0.1\, \mathrm{s \, km}^{-1}$. These results were derived from 65 far-ultraviolet quasar spectra (resolution $R \sim 18\,