Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: HPB-Red, Dallas, TX, U.S.A.
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Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Labyrinth Books, Princeton, NJ, U.S.A.
EUR 68,05
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Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Basi6 International, Irving, TX, U.S.A.
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Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Romtrade Corp., STERLING HEIGHTS, MI, U.S.A.
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Editore: Cambridge University Press CUP, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Books Puddle, New York, NY, U.S.A.
EUR 126,25
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Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Majestic Books, Hounslow, Regno Unito
EUR 132,54
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Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Biblios, Frankfurt am main, HESSE, Germania
EUR 134,47
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Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: PBShop.store US, Wood Dale, IL, U.S.A.
EUR 148,59
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Editore: Cambridge University Press, Cambridge, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Grand Eagle Retail, Bensenville, IL, U.S.A.
EUR 155,00
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Aggiungi al carrelloHardcover. Condizione: new. Hardcover. Several Epoch of Reionization (EoR) experiments, for example, LOFAR, MWA and PAPER, are currently under way and producing results. These very deep observations not only set constraints on when and where the first sources formed in the early Universe and began (re)ionizing the predominantly neutral all-pervasive intergalactic medium, but they also provide high-quality data for cutting edge auxiliary foreground science. Obviously studying the physical origin of the foreground emission, whether Galactic or extragalactic, is a very exciting field in its own right and is of fundamental importance for perfecting the foreground removal techniques in the cosmological experiments. These proceedings of IAU S333 address both topics through giving the clearest and widest possible view on the EoR; presenting the state-of-the-art foreground science; and discussing challenges of upcoming and planned radio facilities such as HERA and SKA. Detecting the weak cosmological radiation emitted billions of years ago, from the time of the first 'stars', is difficult as emission from our Galaxy and other extragalactic sources intervenes. To get a clear view towards the early Universe, we therefore need to study the foreground emission in great detail. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.
Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: PBShop.store UK, Fairford, GLOS, Regno Unito
EUR 159,56
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Aggiungi al carrelloHardcover. Condizione: Brand New. 297 pages. 10.00x7.00x0.75 inches. In Stock.
Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
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Editore: Cambridge University Press, Cambridge, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: CitiRetail, Stevenage, Regno Unito
EUR 146,52
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Aggiungi al carrelloHardcover. Condizione: new. Hardcover. Several Epoch of Reionization (EoR) experiments, for example, LOFAR, MWA and PAPER, are currently under way and producing results. These very deep observations not only set constraints on when and where the first sources formed in the early Universe and began (re)ionizing the predominantly neutral all-pervasive intergalactic medium, but they also provide high-quality data for cutting edge auxiliary foreground science. Obviously studying the physical origin of the foreground emission, whether Galactic or extragalactic, is a very exciting field in its own right and is of fundamental importance for perfecting the foreground removal techniques in the cosmological experiments. These proceedings of IAU S333 address both topics through giving the clearest and widest possible view on the EoR; presenting the state-of-the-art foreground science; and discussing challenges of upcoming and planned radio facilities such as HERA and SKA. Detecting the weak cosmological radiation emitted billions of years ago, from the time of the first 'stars', is difficult as emission from our Galaxy and other extragalactic sources intervenes. To get a clear view towards the early Universe, we therefore need to study the foreground emission in great detail. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.
Editore: Cambridge University Press, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: Mispah books, Redhill, SURRE, Regno Unito
EUR 173,23
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Aggiungi al carrelloHardcover. Condizione: New. New. book.
Editore: Cambridge University Press, Cambridge, 2018
ISBN 10: 1107192463 ISBN 13: 9781107192461
Lingua: Inglese
Da: AussieBookSeller, Truganina, VIC, Australia
EUR 227,88
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Aggiungi al carrelloHardcover. Condizione: new. Hardcover. Several Epoch of Reionization (EoR) experiments, for example, LOFAR, MWA and PAPER, are currently under way and producing results. These very deep observations not only set constraints on when and where the first sources formed in the early Universe and began (re)ionizing the predominantly neutral all-pervasive intergalactic medium, but they also provide high-quality data for cutting edge auxiliary foreground science. Obviously studying the physical origin of the foreground emission, whether Galactic or extragalactic, is a very exciting field in its own right and is of fundamental importance for perfecting the foreground removal techniques in the cosmological experiments. These proceedings of IAU S333 address both topics through giving the clearest and widest possible view on the EoR; presenting the state-of-the-art foreground science; and discussing challenges of upcoming and planned radio facilities such as HERA and SKA. Detecting the weak cosmological radiation emitted billions of years ago, from the time of the first 'stars', is difficult as emission from our Galaxy and other extragalactic sources intervenes. To get a clear view towards the early Universe, we therefore need to study the foreground emission in great detail. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.