Zobrazeno 1 - 10
of 442
pro vyhledávání: '"E. Abramson"'
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 2, p 93 (2023)
We study the recent star formation histories (SFHs) of 575 intermediate-mass galaxies (IMGs, 10 ^9 ≤ M / M _⊙ ≤ 10 ^10 ) in COSMOS at 0.3 < z < 0.4 by comparing their H α and UV luminosities. These two measurements trace star formation rates (
Externí odkaz:
https://doaj.org/article/3752f752a0d64a7d95c0a3a68cb09cd6
Autor:
Nayon Park, Ryan A. Beck, Kevin K. Hoang, Dylan M. Ladd, Jared E. Abramson, Ricardo A. Rivera-Maldonado, Hao A. Nguyen, Madison Monahan, Gerald T. Seidler, Michael F. Toney, Xiaosong Li, Brandi M. Cossairt
Publikováno v:
Inorganic Chemistry. 62:6674-6687
Autor:
Jared E. Abramson, William M. Holden, Ricardo A. Rivera-Maldonado, Alexandra Velian, Brandi M. Cossairt, Gerald T. Seidler
Publikováno v:
Journal of Analytical Atomic Spectrometry. 38:1125-1134
We report a compact laboratory-based, high resolution X-ray emission spectrometer installed in a glovebox for simultaneous measurement of phosphorus Kα and Kβ spectra of air-sensitive materials.
Autor:
Brian Lefchak, Susan Bostwick, Sarah Collins Rossetti, Kenneth Shen, Jessica Ancker, Kenrick Cato, E Abramson, Charlene Thomas, Linda Gerber, Amanda Moy, Mohit M. Sharma, Jonathan Edmond Elias
Publikováno v:
Applied Clinical Informatics.
BACKGROUND: A growing body of literature has linked usability limitations within electronic health records (EHRs) to adverse outcomes which may in turn affect EHR system transitions. NewYork-Presbyterian Hospital (NYP), Columbia University College of
Publikováno v:
X-Ray Spectrometry. 51:151-162
Akademický článek
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Autor:
Tommaso Treu, G. B. Brammer, T. Morishita, Patrick L. Kelly, Tucker Jones, Michele Trenti, Massimo Stiavelli, Benedetta Vulcani, Louis E. Abramson, Xin Wang
Publikováno v:
Proceedings of the International Astronomical Union. 15:50-54
We study star formation and metallicity enrichment histories of 24 massive galaxies at 1.6 < z < 2.5. Deep slitless spectroscopy + imaging data set collected from multiple HST surveys allows robust determination of their SEDs. Our new SED modeling wi
Autor:
Eros Vanzella, Lucia Guaita, Laura Pentericci, Marusa Bradac, Kasper B. Schmidt, Tucker Jones, Ricardo Amorín, Alaina Henry, Adriano Fontana, Tommaso Treu, Austin Hoag, Michele Trenti, Matthew A. Malkan, Charlotte Mason, Louis E. Abramson
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 485, iss 3
Mason, Charlotte A; Fontana, Adriano; Treu, Tommaso; Schmidt, Kasper B; Hoag, Austin; Abramson, Louis; et al.(2019). Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic Survey. Monthly Notices of the Royal Astronomical Society, 485(3), 3947-3969. doi: 10.1093/mnras/stz632. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/58n3m7q1
Mason, Charlotte A; Fontana, Adriano; Treu, Tommaso; Schmidt, Kasper B; Hoag, Austin; Abramson, Louis; et al.(2019). Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic Survey. Monthly Notices of the Royal Astronomical Society, 485(3), 3947-3969. doi: 10.1093/mnras/stz632. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/58n3m7q1
Detections and non-detections of Lyman alpha (Ly$\alpha$) emission from $z>6$ galaxies ($ 7, where Ly$\alpha$ redshifts to near infra-red wavelengths. Here we present a search for z > 7.2 Ly$\alpha$ emission in 53 intrinsically faint Lyman Break Gala
Autor:
Daniel D. Kelson, Louis E. Abramson
Publikováno v:
Research Notes of the AAS. 6:162
Multiple investigations support describing galaxy growth as a stochastic process with correlations over a range of timescales governed by a parameter, $H$, empirically and theoretically constrained to be near unity. Here, we show that the distributio
Autor:
Peter R. Williams, Keith Horne, Håkon Dahle, Stefano Valenti, Keren Sharon, Aaron J. Barth, Louis E. Abramson, Michael D. Gladders, Karianne Dyrland, Tommaso Treu, Brendon J. Brewer
We present CIV BLR modeling results for the multiply imaged $z=2.805$ quasar SDSS J2222+2745. Using data covering a 5.3 year baseline after accounting for gravitational time delays, we find models that can reproduce the observed emission-line spectra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0ea6195ebeb8fe67bc5a0ae08256b38
http://arxiv.org/abs/2103.10961
http://arxiv.org/abs/2103.10961