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Astrophysical Journal Letters, ISSN 2041-8205, 08/2018, Volume 863, Issue 1
Journal Article
Nature, ISSN 0028-0836, 2014, Volume 506, Issue 7487, pp. 197 - 199
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 09/2018, Volume 865, Issue 1, p. L9
Observations of high-redshift quasars indicate that supermassive black holes (SMBHs) with masses greater than similar to 10(9) M-circle dot were assembled... 
galaxies: high-redshift | ORIGIN | QUASAR | ASTRONOMY & ASTROPHYSICS | GROWTH | ACCRETION | UNIVERSE | COSMOLOGICAL SIMULATIONS | FEEDBACK | HALOES | PAIRS | Collapse | Quasars | Red shift | Galaxies | Black holes | Population III stars | Space telescopes | Stellar evolution | Mass ratios | X ray telescopes | Infrared telescopes | Halos | Stellar mass | Big bang cosmology | Telescopes | Physics - Astrophysics of Galaxies
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 2, p. 178
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2018, Volume 475, Issue 4, pp. 5246 - 5256
Journal Article
Nature, ISSN 0028-0836, 2012, Volume 486, Issue 7405, pp. 70 - 73
Dark and baryonic matter moved at different velocities in the early Universe, which strongly suppressed star formation in some regions(1). This was... 
COSMOLOGICAL REIONIZATION | POPULATION | POWER SPECTRUM | FLUCTUATIONS | MULTIDISCIPLINARY SCIENCES | EPOCH | DARK-MATTER | UNIVERSE | RADIATION | EARLY GALAXIES | Research | Properties | Hydrogen | Dark matter (Astronomy) | Studies | Cosmology | Stars & galaxies | Astronomy | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2014, Volume 445, Issue 1, pp. 1056 - 1063
High-redshift quasar observations imply that supermassive black holes (SMBHs) larger than similar to 10(9) M-circle dot formed before z similar to 6. That such... 
Quasars: supermassive black holes - cosmology: theory | COSMIC REIONIZATION | FLUCTUATIONS | ASTRONOMY & ASTROPHYSICS | GAS | 1ST STARS | DARK-MATTER | ACCRETION | quasars: supermassive black holes | GALAXIES | FEEDBACK | cosmology: theory
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2015, Volume 453, Issue 4, pp. 4457 - 4467
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 07/2016, Volume 460, Issue 1, pp. L59 - L63
We explore the formation of massive high-redshift Population III (Pop III) galaxies through photoionization feedback. We consider dark matter haloes formed... 
High-redshift-cosmology | Stars | Population III-galaxies | theory | HYDROGEN | BLACK-HOLE FORMATION | stars: Population III | REIONIZATION | ASTRONOMY & ASTROPHYSICS | STAR-FORMATION | DARK-MATTER | 1ST STARS | SIMULATIONS | SUPPRESSION | galaxies: high-redshift | cosmology: theory
Journal Article
Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, 11/2010, Volume 2010, Issue 11, pp. 016 - 16
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 3, pp. 2722 - 2727
The recent discovery of the gravitational wave source GW150914 has revealed a coalescing binary black hole (BBH) with masses of similar to 30 M-circle dot.... 
Stars: Population III | Gravitational waves | Black hole physics | IMPACT | stars: Population III | EVOLUTION | black hole physics | ASTRONOMY & ASTROPHYSICS | STAR-FORMATION | 1ST STARS | gravitational waves | MERGERS | METALLICITY | GALAXIES | RADIATIVE FEEDBACK
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2015, Volume 450, Issue 3, pp. 2506 - 2506
Constraining the properties of Population III (Pop III) stars will be very challenging because they reside in small galaxies at high redshift which will be... 
Red shift | Galaxies | Population III stars | Symbols | Stars | Emission | Mapping | Density | Three dimensional
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2015, Volume 453, Issue 2, pp. 1692 - 1700
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 453, Issue 4, pp. 4456 - 4456
Recently, Planck measured a value of the cosmic microwave background (CMB) optical depth due to electron scattering of T = 0.066 plus or minus 0.016. Here we... 
Enrichment | Accretion | Feedback | Population III stars | Stars | Cosmic microwave background | Formations | Density
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 453, Issue 2, pp. 1692 - 1692
We propose high-velocity collisions of protogalaxies as a new pathway to form supermassive stars (SMSs) with masses of ~10... M... at high redshift (z > 10).... 
Collapse | Clouds | Symbols | Collisions | Emission | Black holes (astronomy) | Dynamical systems | Density
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2014, Volume 445, Issue 1, pp. 1056 - 1056
High-redshift quasar observations imply that supermassive black holes (SMBHs) larger than similar to 10 super(9) M. formed before z = 6. That such large SMBHs... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2014, Volume 445, Issue 1, pp. 1056 - 1056
High-redshift quasar observations imply that supermassive black holes (SMBHs) larger than similar to 10 super(9) M. formed before z = 6. That such large SMBHs... 
Collapse | Quasars | Halos | Cooling | Thresholds | Mathematical analysis | Stars | Black holes (astronomy)
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 3, pp. 2722 - 2722
The recent discovery of the gravitational wave source GW150914 has revealed a coalescing binary black hole (BBH) with masses of ~30 M... Previous proposals for... 
Origins | Ionizing radiation | Ionization | Gravitational waves | Binary stars | Stars | Black holes (astronomy) | Spectra
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 2014, Volume 437, Issue 1, pp. L36 - L40
We present the first complete calculation of the history of the inhomogeneous 21 cm signal from neutral hydrogen during the era of the first stars. We use... 
Galaxies: high redshift | Cosmology: theory | Intergalactic medium | Galaxies: formation | LYMAN-WERNER | intergalactic medium | SUPPRESSION | RADIATION | cosmology: theory | EARLY GALAXIES | 21-CM | galaxies: formation | HYDROGEN | FLUCTUATIONS | ASTRONOMY & ASTROPHYSICS | galaxies: high redshift | EPOCH | SIMULATIONS | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 2014, Volume 442, Issue 1, pp. L100 - L104
Explaining the existence of supermassive black holes larger than similar to 10(9) M-circle dot at redshifts z greater than or similar to 6 remains an open... 
Quasars: supermassive black holes | Cosmology: theory | DARK-MATTER HALOES | STAR-FORMATION | cosmology: theory | PROTOGALAXIES | LYMAN | ASTRONOMY & ASTROPHYSICS | ACCRETION | quasars: supermassive black holes | REDSHIFT | VIRIAL TEMPERATURES | SIMULATIONS | 10 K | 1ST GALAXIES | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
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