Article
Astronomy & Astrophysics
B. Novosyadlyj, Yu. Kulinich, B. Melekh, V. Shulga
Summary: This study examines the formation and destruction of the first molecules during the Dark Ages and Cosmic Dawn, evaluating the luminosity of protogalaxy clumps (halos) in molecular lines. The impact of photodissociation processes on molecules like H-2 and HD is significant before full reionization, while the number density of helium hydride ions HeH+ shows complicated dependences on halo kinetic temperature and models of the first light. The brightness temperature evolution of individual halos in rotational lines of certain molecules does not exceed microkelvin, but detection could provide important insights into physical processes during the formation of the first stars and galaxies.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Tomas Soltinski, James S. Bolton, Nina Hatch, Martin G. Haehnelt, Laura C. Keating, Girish Kulkarni, Ewald Puchwein, Jonathan Chardin, Dominique Aubert
Summary: Late end of reionization at redshift z similar or equal to 5.3 is consistent with observed spatial variations in the Ly alpha forest transmission and the deficit of Ly alpha emitting galaxies around extended Ly alpha absorption troughs at z = 5.5. Strong 21-cm forest absorbers are predicted to persist until z = 6 in a model with only modest IGM pre-heating. A null-detection of 21-cm forest absorbers at z similar or equal to 6 with SKA1-low or possibly LOFAR could provide valuable lower limit information on the soft X-ray background at high redshift and the temperature of the pre-reionization IGM.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Tomas Soltinsky, James S. Bolton, Margherita Molaro, Nina Hatch, Martin G. Haehnelt, Laura C. Keating, Girish Kulkarni, Ewald Puchwein
Summary: Enhanced ionizing radiation near redshift z(sic) 6 quasars leads to short periods of intergalactic Ly alpha transmission in the blue part of the quasar Ly alpha emission lines. Most of these Ly alpha near-zones correspond to quasars with optically/UV bright lifetimes of t(Q) 10(5) -10(7) yr. However, the smallest Ly alpha near-zones require lifetimes as short as t(Q) (sic)10(4) yr, posing a challenge to the growth of 10(9) M-? black holes at z(sic) 6. Longer accretion timescales are only possible if black holes primarily grow in an obscured phase or if the quasars exhibit variability on timescales similar to the equilibriation time for ionized hydrogen. Distinguishing between young quasars and older quasars with episodic accretion based on Ly alpha absorption alone is difficult. Therefore, the presence of proximate 21-cm absorption around z(sic) 6 radio-loud quasars is predicted as a signature. 21-cm absorption in the spectra of radio-loud quasars should be observable when the intergalactic hydrogen is modestly pre-heated by the X-ray background and the spin temperature T-S(sic) 10(2) K prior to any quasar heating. The extent of proximate 21-cm absorption depends on the integrated lifetime of the quasar. Evidence of proximate 21-cm absorption from the diffuse intergalactic medium within 2-3 pMpc of a (radio-loud) quasar would support a short quasar lifetime of t(Q) (sic) 10(5) yr and provide additional constraints on models for high-redshift black hole growth.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Philippa S. Cole, Joseph Silk
Summary: The production and existence of primordial black holes can impact the primordial power spectrum and matter power spectrum, potentially leading to observable effects on the 21 cm power spectrum. It is crucial to include the contribution from primordial fluctuations in predicting the 21 cm signal in order to avoid underestimation.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Yuxiang Qin, J. Stuart B. Wyithe, Pascal A. Oesch, Garth D. Illingworth, Ecaterina Leonova, Simon J. Mutch, Rohan P. Naidu
Summary: This study investigates the Ly alpha IGM transmission and environment of bright galaxies during the epoch of reionization. It reveals that brighter galaxies are less affected by damping-wing absorption, while the transmission of fainter galaxies depends on UV luminosity. The brightest sources are located in the largest ionized regions, leading to a lower incidence of Ly alpha detection in fainter galaxies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Multidisciplinary Sciences
Guido Roberts-Borsani, Tommaso Treu, Wenlei Chen, Takahiro Morishita, Eros Vanzella, Adi Zitrin, Pietro Bergamini, Marco Castellano, Adriano Fontana, Karl Glazebrook, Claudio Grillo, Patrick L. Kelly, Emiliano Merlin, Themiya Nanayakkara, Diego Paris, Piero Rosati, Lilan Yang, Ana Acebron, Andrea Bonchi, Kit Boyett, Marusa Bradac, Gabriel Brammer, Tom Broadhurst, Antonello Calabro, Jose M. Diego, Alan Dressler, Lukas J. Furtak, Alexei V. Filippenko, Alaina Henry, Anton M. Koekemoer, Nicha Leethochawalit, Matthew A. Malkan, Charlotte Mason, Amata Mercurio, Benjamin Metha, Laura Pentericci, Justin Pierel, Steven Rieck, Namrata Roy, Paola Santini, Victoria Strait, Robert Strausbaugh, Michele Trenti, Benedetta Vulcani, Lifan Wang, Xin Wang, Rogier A. Windhorst
Summary: In the early universe, sources of ultraviolet photons played a crucial role in ionizing intergalactic hydrogen, making the universe transparent to UV radiation. Fainter galaxies that are surrounded by neutral gas were believed to dominate the photon budget. By using the James Webb Space Telescope and gravitational lensing, the ultra-faint galaxy JD1 was spectroscopically confirmed at a redshift of z = 9.79, showing a compact and complex morphology with low stellar mass and subsolar metallicity.
Article
Astronomy & Astrophysics
Ting-Yi Lu, Tomotsugu Goto, Tetsuya Hashimoto, Daryl Joe D. Santos, Yi Hang Valerie Wong, Seong Jin Kim, Tiger Y-Y Hsiao, Ece Kilerci, Simon C-C Ho, Tohru Nagao, Yoshiki Matsuoka, Masafusa Onoue, Yoshiki Toba
Summary: Revealing the history of cosmic hydrogen reionization is a crucial goal in modern cosmology. This study uses a sample of 93 quasars discovered in the Subaru High-z Exploration of Low-Luminosity Quasars project to further constrain the reionization history. The results show that reionization ended at z less than or similar to 6. However, the uncertainty in the data prevents a conclusion on the redshift evolution of near-zone size being affected by reionization.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Tomas Ondro, Rudolf Galis
Summary: The article studied the temperature-density relation of the intergalactic medium in the range 1.6 <= z < 2.0, using Lyman alpha forest decomposition and an iterative fitting procedure to calibrate measurements against mock data. The results showed a decreasing trend in temperature at mean density predicted by various models at lower redshifts, while power-law index values were close to 1.6 as expected in models assuming balance of photoheating with adiabatic cooling after reionization events.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Janakee Raste, Girish Kulkarni, Laura C. Keating, Martin G. Haehnelt, Jonathan Chardin, Dominique Aubert
Summary: Advancements in understanding the intergalactic medium at redshifts z = 5-6 have been made through the discovery of quasars with z > 6, shedding light on the late end of hydrogen reionization and the existence of neutral hydrogen "islands." Radiative transfer simulations suggest implications for the 21-cm power spectrum signal and its potential detection by experiments such as hera, ska, lofar, and mwa, with values significantly higher than conventional models. This redshift range offers attractive conditions for detection, with low sky temperature and a greater abundance of multiwavelength data.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Teresita Suarez, Avery Meiksin
Summary: Observations of intergalactic low ionization metal absorption systems at high redshifts suggest that these systems may be pressure-confined clouds controlled by the expected pressure of galactic haloes. Some of the observed ratios require extending conventional radiative transfer models to spherical (or cylindrical) clouds to accurately describe the column density ratios.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Molly Wolfson, Joseph F. Hennawi, Frederick B. Davies, Jose Onorbe
Summary: Fluctuations in Lyman-alpha forest transmission towards high-z quasars are affected by spatial fluctuations in the ultraviolet background, which are determined by the mean free path of ionizing photons. The autocorrelation function of Lyman-alpha forest flux can indicate the strength and scale of transmission fluctuations and is sensitive to the mean free path. By modeling mock data sets similar to the real data, we find that the precision of measuring the mean free path is comparable to direct measurements from quasar spectra stacking. Hypothetical high-resolution data can further reduce the error bars by approximately 40% at all redshifts.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
T-S Kim, B. P. Wakker, F. Nasir, R. F. Carswell, B. D. Savage, J. S. Bolton, A. J. Fox, M. Viel, M. G. Haehnelt, J. C. Charlton, B. E. Rosenwasser
Summary: A uniform analysis of the HI transmitted flux and Hi column density distribution in the low-density IGM as a function of redshift was conducted using spectra from different instruments. The evolution from higher to lower redshifts and the stability at z < 0.5 were observed, with significant variations along different sightlines. The shape of the column density distribution function at lower redshifts can be replicated by rotating a higher redshift distribution slightly, and there is an evolutionary break in absorption line number at z around 1.5. High-N-HI absorbers evolve more rapidly than low-N-HI absorbers, possibly due to stronger clustering at lower redshifts.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Aniket Bhagwat, Benedetta Ciardi, Erik Zackrisson, Joop Schaye
Summary: Dense, metal-rich regions shielded from stellar radiation can remain neutral during reionization and produce metal and 21 cm absorption lines. The simultaneous absorption of metals and 21 cm can complement each other as probes of gas properties. High-resolution radiation-hydrodynamical simulations are used to investigate the occurrence of aligned absorbers and their classifications.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
V D'Odorico, K. Finlator, S. Cristiani, G. Cupani, S. Perrotta, F. Calura, M. Centurion, G. Becker, T. A. M. Berg, S. Lopez, S. Ellison, E. Pomante
Summary: In this study, we investigate the abundance and distribution of metals in the high-redshift intergalactic medium and circum-galactic medium. Through the analysis of 147 quasars' high- and intermediate-resolution spectra, we find that the number density and column density distribution of Si iv absorption lines show significant changes in different redshift intervals, with a behavior consistent with that of C iv absorption lines. Furthermore, the study reveals the challenge of accurately predicting the properties of Si iv and C iv through numerical simulations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
T-s Kim, B. P. Wakker, F. Nasir, R. F. Carswell, B. D. Savage, J. S. Bolton, A. J. Fox, M. Viel, M. G. Haehnelt, J. C. Charlton, B. E. Rosenwasser
Summary: A new uniform analysis of the H I transmitted flux and column density distribution in the low-density IGM as a function of redshift was presented. The study confirmed previous conclusions and revealed evolution in flux and column density distribution with decreasing redshift, as well as variations in sightlines. High-NH absorbers were found to evolve more rapidly than low-N(H I ) absorbers, decreasing in number or cross-section over time.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Jose Onorbe, F. B. Davies, Z. Lukic, J. F. Hennawi, D. Sorini
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2019)
Article
Multidisciplinary Sciences
K. W. Bannister, A. T. Deller, C. Phillips, J. -P. Macquart, J. X. Prochaska, N. Tejos, S. D. Ryder, E. M. Sadler, R. M. Shannon, S. Simha, C. K. Day, M. McQuinn, F. O. North-Hickey, S. Bhandari, W. R. Arcus, V. N. Bennert, J. Burchett, M. Bouwhuis, R. Dodson, R. D. Ekers, W. Farah, C. Flynn, C. W. James, M. Kerr, E. Lenc, E. K. Mahony, J. O'Meara, S. Oslowski, H. Qiu, T. Treu, T. J. Bateman, D. C. -J. Bock, R. J. Bolton, A. Brown, J. D. Bunton, A. P. Chippendale, F. R. Cooray, T. Cornwell, N. Gupta, D. B. Hayman, M. Kesteven, B. S. Koribalski, A. MacLeod, N. M. McClure-Griffiths, S. Neuhold, R. P. Norris, M. A. Pilawa, R. -Y. Qiao, J. Reynolds, D. N. Roxby, T. W. Shimwell, M. A. Voronkov, C. D. Wilson
Article
Astronomy & Astrophysics
Fahad Nasir, Christopher Cain, Anson D'Aloisio, Nakul Gangolli, Matthew McQuinn
Summary: Becker et al. measured the mean free path of Lyman-limit photons in the intergalactic medium at z = 6, indicating significant role of absorptions in reionization. They studied physical properties of ionizing photon sinks in the wake of ionization fronts using radiative hydrodynamic simulations. The contributions of self-shielding systems to the opacity decrease over time as the intergalactic medium evolves.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Sultan Hassan, Romeel Dave, Matthew McQuinn, Rachel S. Somerville, Laura C. Keating, Daniel Angles-Alcazar, Francisco Villaescusa-Navarro, David N. Spergel
Summary: Traditional large-scale models of reionization usually use simple deterministic relations between halo mass and luminosity to predict reionization. This study examines the impact of using more detailed models for ionizing sources and finds that the scatter in the relation between dark matter halos and star formation affects the model. However, at the power spectrum level, the ionization morphology remains mostly unchanged regardless of the variability in the number of sources or escape fraction.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Daniel R. Piacitelli, Erik Solhaug, Yakov Faerman, Matthew McQuinn
Summary: Motivated by the development of integral field units (IFUs) on ground telescopes and proposals for ultraviolet-sensitive space telescopes, this research explores the potential of using emission lines to study the circumgalactic medium (CGM) and its relationship to galaxy formation. The study identifies O III 5007 angstrom, N II 6583 angstrom, O v 630 angstrom, and O VI 1032,1038 angstrom as the most promising emission lines for detection. Formulas are provided to simplify the application of these estimates to other samples and scenarios. The study also discusses the detectability of C III 978 angstrom, C IV 1548 angstrom, H alpha, and hydrogen n > 2 Ly-series lines.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Christopher Cain, Anson D'Aloisio, Vid Irsic, Matthew McQuinn, Hy Trac
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Vid Irsic, Huangyu Xiao, Matthew McQuinn
Article
Astronomy & Astrophysics
Frederick B. Davies, Joseph F. Hennawi, Anna-Christina Eilers
ASTROPHYSICAL JOURNAL LETTERS
(2019)
Article
Astronomy & Astrophysics
Anson D'Aloisio, Matthew McQuinn, Oliver Maupin, Frederick B. Davies, Hy Tracy, Spencer Fuller, Phoebe R. Upton Sanderbeck
ASTROPHYSICAL JOURNAL
(2019)
Article
Astronomy & Astrophysics
Frederick B. Davies, Joseph F. Hennawi, Eduardo Banados, Zarija Lukic, Roberto Decarli, Xiaohui Fan, Emanuele P. Farina, Chiara Mazzucchelli, Hans-Walter Rix, Bram P. Venemans, Fabian Walter, Feige Wang, Jinyi Yang
ASTROPHYSICAL JOURNAL
(2018)
Article
Astronomy & Astrophysics
Anna-Christina Eilers, Joseph F. Hennawi, Frederick B. Davies
ASTROPHYSICAL JOURNAL
(2018)
Article
Astronomy & Astrophysics
George D. Becker, Frederick B. Davies, Steven R. Furlanetto, Matthew A. Malkan, Elisa Boera, Craig Douglass
ASTROPHYSICAL JOURNAL
(2018)
Article
Astronomy & Astrophysics
Tobias M. Schmidt, Joseph F. Hennawi, Gabor Worseck, Frederick B. Davies, Zarija Lukic, Jose Onorbe
ASTROPHYSICAL JOURNAL
(2018)
Article
Astronomy & Astrophysics
Matthew McQuinn, Jessica K. Werk
ASTROPHYSICAL JOURNAL
(2018)