Reionization and the Cosmic Dawn with the Square Kilometre Array

Leon V. E. Koopmans; Filipe A. Abdalla; Gianni Bernardi; Benedetta Ciardi; Soobash Daiboo; A. G. de Bruyn; Kanan K. Datta; Heino Falcke; Andrea Ferrara; Ilian T. Iliev; Fabio Iocco; Vibor Jelic; Hannes Jensen; Ronniy Joseph; Panos Labroupoulos; Avery Meiksin; Andrei Mesinger; Andre R. Offringa; V. N. Pandey; Jonathan R. Pritchard; Mario G. Santos; Dominik J. Schwarz; Benoit Semelin; Harish Vedantham; Sarod Yatawatta; Saleem Zaroubi; G. Mellema

doi:10.1007/s10686-013-9334-5

Reionization and the Cosmic Dawn with the Square Kilometre Array

Leon V. E. Koopmans, Filipe A. Abdalla, Gianni Bernardi, Benedetta Ciardi, Soobash Daiboo, A. G. de Bruyn, Kanan K. Datta, Heino Falcke, Andrea Ferrara, Ilian T. Iliev, Fabio Iocco, Vibor Jelic, Hannes Jensen, Ronniy Joseph, Panos Labroupoulos, Avery Meiksin, Andrei Mesinger, Andre R. Offringa, V. N. Pandey, Jonathan R. PritchardMario G. Santos, Dominik J. Schwarz, Benoit Semelin, Harish Vedantham, Sarod Yatawatta, Saleem Zaroubi, G. Mellema

Onderzoeksoutput: Article › Academic › peer review

247 Citaten (Scopus)

Samenvatting

The Square Kilometre Array (SKA) will have a low frequency component (SKA-low) which has as one of its main science goals the study of the redshifted 21 cm line from the earliest phases of star and galaxy formation in the Universe. This 21 cm signal provides a new and unique window both on the time of the formation of the first stars and accreting black holes and the subsequent period of substantial ionization of the intergalactic medium. The signal will teach us fundamental new things about the earliest phases of structure formation, cosmology and even has the potential to lead to the discovery of new physical phenomena. Here we present a white paper with an overview of the science questions that SKA-low can address, how we plan to tackle these questions and what this implies for the basic design of the telescope.

Originele taal-2	English
Pagina's (van-tot)	235-318
Aantal pagina's	84
Tijdschrift	Experimental Astronomy
Volume	36
Nummer van het tijdschrift	1
DOI's	https://doi.org/10.1007/s10686-013-9334-5
Status	Published - aug.-2013

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10.1007/s10686-013-9334-5

http://adsabs.harvard.edu/abs/2013ExA....36..235M

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Reionization and the Cosmic Dawn with the Square Kilometre Array
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Koopmans, L. V. E., Abdalla, F. A., Bernardi, G., Ciardi, B., Daiboo, S., de Bruyn, A. G., Datta, K. K., Falcke, H., Ferrara, A., Iliev, I. T., Iocco, F., Jelic, V., Jensen, H., Joseph, R., Labroupoulos, P., Meiksin, A., Mesinger, A., Offringa, A. R., Pandey, V. N., ... Mellema, G. (2013). Reionization and the Cosmic Dawn with the Square Kilometre Array. Experimental Astronomy, 36(1), 235-318. https://doi.org/10.1007/s10686-013-9334-5

@article{f4cb5a4c0f6e437b928d4c59472e8ba7,

title = "Reionization and the Cosmic Dawn with the Square Kilometre Array",

abstract = "The Square Kilometre Array (SKA) will have a low frequency component (SKA-low) which has as one of its main science goals the study of the redshifted 21 cm line from the earliest phases of star and galaxy formation in the Universe. This 21 cm signal provides a new and unique window both on the time of the formation of the first stars and accreting black holes and the subsequent period of substantial ionization of the intergalactic medium. The signal will teach us fundamental new things about the earliest phases of structure formation, cosmology and even has the potential to lead to the discovery of new physical phenomena. Here we present a white paper with an overview of the science questions that SKA-low can address, how we plan to tackle these questions and what this implies for the basic design of the telescope.",

keywords = "Cosmology: Observations, Dark ages, Reionization, First stars, Diffuse radiation, Intergalactic medium, Radio lines: General, Techniques: Interferometric, 21 CENTIMETER FLUCTUATIONS, MURCHISON-WIDEFIELD-ARRAY, REDSHIFTED 21-CM MAPS, SOUTH-POLE TELESCOPE, LY-ALPHA EMITTERS, INFRARED BACKGROUND EXCESS, SMALL-SCALE FLUCTUATIONS, ULTRA-DEEP-FIELD, H-II REGIONS, INTERGALACTIC MEDIUM",

author = "Koopmans, {Leon V. E.} and Abdalla, {Filipe A.} and Gianni Bernardi and Benedetta Ciardi and Soobash Daiboo and {de Bruyn}, {A. G.} and Datta, {Kanan K.} and Heino Falcke and Andrea Ferrara and Iliev, {Ilian T.} and Fabio Iocco and Vibor Jelic and Hannes Jensen and Ronniy Joseph and Panos Labroupoulos and Avery Meiksin and Andrei Mesinger and Offringa, {Andre R.} and Pandey, {V. N.} and Pritchard, {Jonathan R.} and Santos, {Mario G.} and Schwarz, {Dominik J.} and Benoit Semelin and Harish Vedantham and Sarod Yatawatta and Saleem Zaroubi and G. Mellema",

year = "2013",

month = aug,

doi = "10.1007/s10686-013-9334-5",

language = "English",

volume = "36",

pages = "235--318",

journal = "Experimental Astronomy",

issn = "0922-6435",

publisher = "SPRINGER",

number = "1",

}

Koopmans, LVE, Abdalla, FA, Bernardi, G, Ciardi, B, Daiboo, S, de Bruyn, AG, Datta, KK, Falcke, H, Ferrara, A, Iliev, IT, Iocco, F, Jelic, V, Jensen, H, Joseph, R, Labroupoulos, P, Meiksin, A, Mesinger, A, Offringa, AR, Pandey, VN, Pritchard, JR, Santos, MG, Schwarz, DJ, Semelin, B, Vedantham, H, Yatawatta, S, Zaroubi, S & Mellema, G 2013, 'Reionization and the Cosmic Dawn with the Square Kilometre Array', Experimental Astronomy, vol. 36, nr. 1, blz. 235-318. https://doi.org/10.1007/s10686-013-9334-5

TY - JOUR

T1 - Reionization and the Cosmic Dawn with the Square Kilometre Array

AU - Koopmans, Leon V. E.

AU - Abdalla, Filipe A.

AU - Bernardi, Gianni

AU - Ciardi, Benedetta

AU - Daiboo, Soobash

AU - de Bruyn, A. G.

AU - Datta, Kanan K.

AU - Falcke, Heino

AU - Ferrara, Andrea

AU - Iliev, Ilian T.

AU - Iocco, Fabio

AU - Jelic, Vibor

AU - Jensen, Hannes

AU - Joseph, Ronniy

AU - Labroupoulos, Panos

AU - Meiksin, Avery

AU - Mesinger, Andrei

AU - Offringa, Andre R.

AU - Pandey, V. N.

AU - Pritchard, Jonathan R.

AU - Santos, Mario G.

AU - Schwarz, Dominik J.

AU - Semelin, Benoit

AU - Vedantham, Harish

AU - Yatawatta, Sarod

AU - Zaroubi, Saleem

AU - Mellema, G.

PY - 2013/8

Y1 - 2013/8

N2 - The Square Kilometre Array (SKA) will have a low frequency component (SKA-low) which has as one of its main science goals the study of the redshifted 21 cm line from the earliest phases of star and galaxy formation in the Universe. This 21 cm signal provides a new and unique window both on the time of the formation of the first stars and accreting black holes and the subsequent period of substantial ionization of the intergalactic medium. The signal will teach us fundamental new things about the earliest phases of structure formation, cosmology and even has the potential to lead to the discovery of new physical phenomena. Here we present a white paper with an overview of the science questions that SKA-low can address, how we plan to tackle these questions and what this implies for the basic design of the telescope.

AB - The Square Kilometre Array (SKA) will have a low frequency component (SKA-low) which has as one of its main science goals the study of the redshifted 21 cm line from the earliest phases of star and galaxy formation in the Universe. This 21 cm signal provides a new and unique window both on the time of the formation of the first stars and accreting black holes and the subsequent period of substantial ionization of the intergalactic medium. The signal will teach us fundamental new things about the earliest phases of structure formation, cosmology and even has the potential to lead to the discovery of new physical phenomena. Here we present a white paper with an overview of the science questions that SKA-low can address, how we plan to tackle these questions and what this implies for the basic design of the telescope.

KW - Cosmology: Observations

KW - Dark ages

KW - Reionization

KW - First stars

KW - Diffuse radiation

KW - Intergalactic medium

KW - Radio lines: General

KW - Techniques: Interferometric

KW - 21 CENTIMETER FLUCTUATIONS

KW - MURCHISON-WIDEFIELD-ARRAY

KW - REDSHIFTED 21-CM MAPS

KW - SOUTH-POLE TELESCOPE

KW - LY-ALPHA EMITTERS

KW - INFRARED BACKGROUND EXCESS

KW - SMALL-SCALE FLUCTUATIONS

KW - ULTRA-DEEP-FIELD

KW - H-II REGIONS

KW - INTERGALACTIC MEDIUM

U2 - 10.1007/s10686-013-9334-5

DO - 10.1007/s10686-013-9334-5

M3 - Article

SN - 0922-6435

VL - 36

SP - 235

EP - 318

JO - Experimental Astronomy

JF - Experimental Astronomy

IS - 1

ER -