The deepest spectrum of the universe? Constraints on the Lyman continuum background at high redshift

The deepest spectrum of the universe? Constraints on the Lyman continuum background at high redshift

التفاصيل البيبلوغرافية
المؤلفون الرئيسيون:	Marleau, F, Bunker, A, Graham, JR
التنسيق:	Conference item
منشور في:	1999

مواد مشابهة

The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters
حسب: Sophia R. Flury, وآخرون
منشور في: (2022-01-01)

Multivariate Predictors of Lyman Continuum Escape. II. Predicting Lyman Continuum Escape Fractions for High-redshift Galaxies
حسب: Anne E. Jaskot, وآخرون
منشور في: (2024-01-01)

Multivariate Predictors of Lyman Continuum Escape. I. A Survival Analysis of the Low-redshift Lyman Continuum Survey
حسب: Anne E. Jaskot, وآخرون
منشور في: (2024-01-01)

The Low-redshift Lyman Continuum Survey: Optically Thin and Thick Mg ii Lines as Probes of Lyman Continuum Escape
حسب: Xinfeng Xu, وآخرون
منشور في: (2023-01-01)

Merging Signatures in an Offset Lyman Continuum Emitter at Redshift 3.8
حسب: Fang-Ting Yuan, وآخرون
منشور في: (2024-01-01)

The physics of indirect estimators of Lyman Continuum escape and their application to high-redshift JWST galaxies
حسب: Choustikov, N, وآخرون
منشور في: (2023)

The physics of indirect estimators of Lyman Continuum escape and their application to high-redshift JWST galaxies
حسب: Choustikov, N, وآخرون
منشور في: (2024)

Erratum: “The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters” (2022, ApJS, 260, 1)
حسب: Sophia R. Flury, وآخرون
منشور في: (2024-01-01)

Keck spectroscopy of faint 3 < z < 7 Lyman break galaxies - I. New constraints on cosmic reionization from the luminosity and redshift-dependent fraction of Lyman alpha emission
حسب: Stark, D, وآخرون
منشور في: (2010)

Spectroscopy of z similar to 7 candidate galaxies: using Lyman alpha to constrain the neutral fraction of hydrogen in the high-redshift universe
حسب: Caruana, J, وآخرون
منشور في: (2014)

Formation of the Lyman Continuum during Solar Flares
حسب: Shaun A. McLaughlin, وآخرون
منشور في: (2023-01-01)

Seeking the ultraviolet ionizing background at z approximate to 3 with the Keck telescope
حسب: Bunker, A, وآخرون
منشور في: (1998)

Interpreting the observed UV continuum slopes of high-redshift galaxies
حسب: Wilkins, S, وآخرون
منشور في: (2013)

Minihalo Model for the Low-Redshift Lyman alpha Absorbers Revisited
حسب: Lalović, A., وآخرون
منشور في: (2008-06-01)

GALICS III: Predicted properties for Lyman Break Galaxies at redshift 3
حسب: Blaizot, J, وآخرون
منشور في: (2003)

THE EVOLUTIONARY HISTORY OF LYMAN BREAK GALAXIES BETWEEN REDSHIFT 4 AND 6: OBSERVING SUCCESSIVE GENERATIONS OF MASSIVE GALAXIES IN FORMATION
حسب: Stark, D, وآخرون
منشور في: (2009)

Haro 11: The Spatially Resolved Lyman Continuum Sources
حسب: Lena Komarova, وآخرون
منشور في: (2024-01-01)

Testing Lyα Emitters and Lyman-break Galaxies as Tracers of Large-scale Structures at High Redshifts
حسب: Sang Hyeok Im, وآخرون
منشور في: (2024-01-01)

Constraints on the Lyman Continuum Escape from Low-mass Lensed Galaxies at 1.3 ≤ z ≤ 3.0
حسب: Intae Jung, وآخرون
منشور في: (2024-01-01)

Lyman Continuum Leakers at z > 3 in the GOODS-S Field: Starburst or Not?
حسب: Shuairu Zhu, وآخرون
منشور في: (2024-01-01)

The Lyman‐α Sky Background as Observed by New Horizons
حسب: G. Randall Gladstone, وآخرون
منشور في: (2018-08-01)

Lyman break galaxies and the star formation rate of the Universe at z approximate to 6
حسب: Stanway, E, وآخرون
منشور في: (2003)

Lyman break galaxies and the star formation rate of the Universe at z approximate to 6
حسب: Stanway, E, وآخرون
منشور في: (2003)

New methods for identifying Lyman continuum leakers and reionization-epoch analogues
حسب: Katz, H, وآخرون
منشور في: (2020)

MgII in the JWST era: a probe of lyman continuum escape?
حسب: Katz, H, وآخرون
منشور في: (2022)

One-line redshifts and searches for high-redshift Ly alpha emission
حسب: Stern, D, وآخرون
منشور في: (2000)

Detections of [C ii] 158 μm and [O iii] 88 μm in a Local Lyman Continuum Emitter, Mrk 54, and Its Implications to High-redshift ALMA Studies
حسب: Ryota Ura, وآخرون
منشور في: (2023-01-01)

The Magellan M2FS Spectroscopic Survey of High-redshift Galaxies: The Brightest Lyman-break Galaxies at z ∼ 6
حسب: Shuqi Fu, وآخرون
منشور في: (2024-01-01)

The Leakage of Lyman-continuum Photons from a Major Merger at z ∼ 1
حسب: Soumil Maulick, وآخرون
منشور في: (2024-01-01)

New constraints on the co-moving star formation rate in the redshift interval 6
حسب: Ellis, R, وآخرون
منشور في: (2006)

The Flux Auto- and Cross-Correlation of the Lyman-alpha Forest. I. Spectroscopy of QSO Pairs with Arcminute Separations and Similar Redshifts
حسب: Marble, A, وآخرون
منشور في: (2008)

My deepest gratitude...
حسب: Caio Augusto de Souza Nery
منشور في: (2024-05-01)

TEMPLATES: Direct Abundance Constraints for Two Lensed Lyman-break Galaxies
حسب: Brian Welch, وآخرون
منشور في: (2024-01-01)

Lyman Continuum Emission from Spectroscopically Confirmed Lyα Emitters at z ∼ 3.1
حسب: Yuchen Liu, وآخرون
منشور في: (2023-01-01)

Galaxies at high redshift and reionization
حسب: Bunker, A, وآخرون
منشور في: (2007)

On the lyman problem
حسب: Kolár Václav
منشور في: (2003-06-01)

The high redshift universe and cosmology
حسب: Hook, I
منشور في: (2013)

The Wide Field Imager Lyman-Alpha Search (WFILAS) for galaxies at redshift similar to 5.7 - I. A spatially compact Ly alpha emitting galaxy at redshift 5.721
حسب: Westra, E, وآخرون
منشور في: (2005)

Lyman Continuum Leakers in the AstroSat Ultraviolet Deep Field: Extreme-ultraviolet Emitters at the Cosmic Noon
حسب: Suraj Dhiwar, وآخرون
منشور في: (2024-01-01)

William James and the Deepest South
حسب: Alexandre Mendes
منشور في: (2022-05-01)