CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY

Norman A. Grogin; Dale D. Kocevski; S. M. Faber; Henry C. Ferguson; Anton M. Koekemoer; Adam G. Riess; Viviana Acquaviva; David M. Alexander; Omar Almaini; Matthew L. N. Ashby; Marco Barden; Eric F. Bell; Frederic Bournaud; Thomas M. Brown; Karina I. Caputi; Stefano Casertano; Paolo Cassata; Marco Castellano; Peter Challis; Ranga-Ram Chary; Edmond Cheung; Michele Cirasuolo; Christopher J. Conselice; Asantha Roshan Cooray; Darren J. Croton; Emanuele Daddi; Tomas Dahlen; Romeel Dave; Duilia F. de Mello; Avishai Dekel; Mark Dickinson; Timothy Dolch; Jennifer L. Donley; James S. Dunlop; Aaron A. Dutton; David Elbaz; Giovanni G. Fazio; Alexei V. Filippenko; Steven L. Finkelstein; Adriano Fontana; Jonathan P. Gardner; Peter M. Garnavich; Eric Gawiser; Mauro Giavalisco; Andrea Grazian; Yicheng Guo; Nimish P. Hathi; Boris Haeussler; Philip F. Hopkins; Jia-Sheng Huang; Kuang-Han Huang; Saurabh W. Jha; Jeyhan S. Kartaltepe; Robert P. Kirshner; David C. Koo; Kamson Lai; Kyoung-Soo Lee; Weidong Li; Jennifer M. Lotz; Ray A. Lucas; Piero Madau; Patrick J. McCarthy; Elizabeth J. McGrath; Daniel H. McIntosh; Ross J. McLure; Bahram Mobasher; Leonidas A. Moustakas; Mark Mozena; Kirpal Nandra; Jeffrey A. Newman; Sami-Matias Niemi; Kai G. Noeske; Casey J. Papovich; Laura Pentericci; Alexandra Pope; Joel R. Primack; Abhijith Rajan; Swara Ravindranath; Naveen A. Reddy; Alvio Renzini; Hans-Walter Rix; Aday R. Robaina; Steven A. Rodney; David J. Rosario; Piero Rosati; Sara Salimbeni; Claudia Scarlata; Brian Siana; Luc Simard; Joseph Smidt; Rachel S. Somerville; Hyron Spinrad; Amber N. Straughn; Louis-Gregory Strolger; Olivia Telford; Harry I. Teplitz; Jonathan R. Trump; Arjen van der Wel; Carolin Villforth; Risa H. Wechsler; Benjamin J. Weiner; Tommy Wiklind; Vivienne Wild; Grant Wilson; Stijn Wuyts; Hao-Jing Yan; Min S. Yun

doi:10.1088/0067-0049/197/2/35

CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY

Norman A. Grogin^*, Dale D. Kocevski, S. M. Faber, Henry C. Ferguson, Anton M. Koekemoer, Adam G. Riess, Viviana Acquaviva, David M. Alexander, Omar Almaini, Matthew L. N. Ashby, Marco Barden, Eric F. Bell, Frederic Bournaud, Thomas M. Brown, Karina I. Caputi, Stefano Casertano, Paolo Cassata, Marco Castellano, Peter Challis, Ranga-Ram CharyEdmond Cheung, Michele Cirasuolo, Christopher J. Conselice, Asantha Roshan Cooray, Darren J. Croton, Emanuele Daddi, Tomas Dahlen, Romeel Dave, Duilia F. de Mello, Avishai Dekel, Mark Dickinson, Timothy Dolch, Jennifer L. Donley, James S. Dunlop, Aaron A. Dutton, David Elbaz, Giovanni G. Fazio, Alexei V. Filippenko, Steven L. Finkelstein, Adriano Fontana, Jonathan P. Gardner, Peter M. Garnavich, Eric Gawiser, Mauro Giavalisco, Andrea Grazian, Yicheng Guo, Nimish P. Hathi, Boris Haeussler, Philip F. Hopkins, Jia-Sheng Huang, Kuang-Han Huang, Saurabh W. Jha, Jeyhan S. Kartaltepe, Robert P. Kirshner, David C. Koo, Kamson Lai, Kyoung-Soo Lee, Weidong Li, Jennifer M. Lotz, Ray A. Lucas, Piero Madau, Patrick J. McCarthy, Elizabeth J. McGrath, Daniel H. McIntosh, Ross J. McLure, Bahram Mobasher, Leonidas A. Moustakas, Mark Mozena, Kirpal Nandra, Jeffrey A. Newman, Sami-Matias Niemi, Kai G. Noeske, Casey J. Papovich, Laura Pentericci, Alexandra Pope, Joel R. Primack, Abhijith Rajan, Swara Ravindranath, Naveen A. Reddy, Alvio Renzini, Hans-Walter Rix, Aday R. Robaina, Steven A. Rodney, David J. Rosario, Piero Rosati, Sara Salimbeni, Claudia Scarlata, Brian Siana, Luc Simard, Joseph Smidt, Rachel S. Somerville, Hyron Spinrad, Amber N. Straughn, Louis-Gregory Strolger, Olivia Telford, Harry I. Teplitz, Jonathan R. Trump, Arjen van der Wel, Carolin Villforth, Risa H. Wechsler, Benjamin J. Weiner, Tommy Wiklind, Vivienne Wild, Grant Wilson, Stijn Wuyts, Hao-Jing Yan, Min S. Yun

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is designed to document the first third of galactic evolution, over the approximate redshift (z) range 8-1.5. It will image >250,000 distant galaxies using three separate cameras on the Hubble Space Telescope, from the mid-ultraviolet to the near-infrared, and will find and measure Type Ia supernovae at z > 1.5 to test their accuracy as standardizable candles for cosmology. Five premier multi-wavelength sky regions are selected, each with extensive ancillary data. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to a stellar mass of 10(9)M(circle dot) to z approximate to 2, reaching the knee of the ultraviolet luminosity function of galaxies to z approximate to 8. The survey covers approximately 800 arcmin(2) and is divided into two parts. The CANDELS/Deep survey (5 sigma point-source limit H = 27.7 mag) covers similar to 125 arcmin(2) within Great Observatories Origins Deep Survey (GOODS)-N and GOODS-S. The CANDELS/Wide survey includes GOODS and three additional fields (Extended Groth Strip, COSMOS, and Ultra-deep Survey) and covers the full area to a 5 sigma point-source limit of H greater than or similar to 27.0 mag. Together with the Hubble Ultra Deep Fields, the strategy creates a three-tiered "wedding-cake" approach that has proven efficient for extragalactic surveys. Data from the survey are nonproprietary and are useful for a wide variety of science investigations. In this paper, we describe the basic motivations for the survey, the CANDELS team science goals and the resulting observational requirements, the field selection and geometry, and the observing design. The Hubble data processing and products are described in a companion paper.

Original language	English
Article number	35
Number of pages	39
Journal	Astrophysical Journal Supplement Series
Volume	197
Issue number	2
DOIs	https://doi.org/10.1088/0067-0049/197/2/35
Publication status	Published - Dec 2011

Keywords

cosmology: observations
galaxies: high-redshift
HUBBLE-SPACE-TELESCOPE
STAR-FORMING GALAXIES
ACTIVE GALACTIC NUCLEI
LYMAN-BREAK GALAXIES
SUPERMASSIVE BLACK-HOLES
EXTENDED GROTH-STRIP
GOODS-SOUTH FIELD
SIMILAR-TO 7
REST-FRAME ULTRAVIOLET
EARLY RELEASE SCIENCE

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10.1088/0067-0049/197/2/35

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Grogin, N. A., Kocevski, D. D., Faber, S. M., Ferguson, H. C., Koekemoer, A. M., Riess, A. G., Acquaviva, V., Alexander, D. M., Almaini, O., Ashby, M. L. N., Barden, M., Bell, E. F., Bournaud, F., Brown, T. M., Caputi, K. I., Casertano, S., Cassata, P., Castellano, M., Challis, P., ... Yun, M. S. (2011). CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY. Astrophysical Journal Supplement Series, 197(2), Article 35. https://doi.org/10.1088/0067-0049/197/2/35

@article{de3dc0e576f54fb982652f3ba0a2ca52,

title = "CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY",

abstract = "The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is designed to document the first third of galactic evolution, over the approximate redshift (z) range 8-1.5. It will image >250,000 distant galaxies using three separate cameras on the Hubble Space Telescope, from the mid-ultraviolet to the near-infrared, and will find and measure Type Ia supernovae at z > 1.5 to test their accuracy as standardizable candles for cosmology. Five premier multi-wavelength sky regions are selected, each with extensive ancillary data. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to a stellar mass of 10(9)M(circle dot) to z approximate to 2, reaching the knee of the ultraviolet luminosity function of galaxies to z approximate to 8. The survey covers approximately 800 arcmin(2) and is divided into two parts. The CANDELS/Deep survey (5 sigma point-source limit H = 27.7 mag) covers similar to 125 arcmin(2) within Great Observatories Origins Deep Survey (GOODS)-N and GOODS-S. The CANDELS/Wide survey includes GOODS and three additional fields (Extended Groth Strip, COSMOS, and Ultra-deep Survey) and covers the full area to a 5 sigma point-source limit of H greater than or similar to 27.0 mag. Together with the Hubble Ultra Deep Fields, the strategy creates a three-tiered {"}wedding-cake{"} approach that has proven efficient for extragalactic surveys. Data from the survey are nonproprietary and are useful for a wide variety of science investigations. In this paper, we describe the basic motivations for the survey, the CANDELS team science goals and the resulting observational requirements, the field selection and geometry, and the observing design. The Hubble data processing and products are described in a companion paper.",

keywords = "cosmology: observations, galaxies: high-redshift, HUBBLE-SPACE-TELESCOPE, STAR-FORMING GALAXIES, ACTIVE GALACTIC NUCLEI, LYMAN-BREAK GALAXIES, SUPERMASSIVE BLACK-HOLES, EXTENDED GROTH-STRIP, GOODS-SOUTH FIELD, SIMILAR-TO 7, REST-FRAME ULTRAVIOLET, EARLY RELEASE SCIENCE",

author = "Grogin, {Norman A.} and Kocevski, {Dale D.} and Faber, {S. M.} and Ferguson, {Henry C.} and Koekemoer, {Anton M.} and Riess, {Adam G.} and Viviana Acquaviva and Alexander, {David M.} and Omar Almaini and Ashby, {Matthew L. N.} and Marco Barden and Bell, {Eric F.} and Frederic Bournaud and Brown, {Thomas M.} and Caputi, {Karina I.} and Stefano Casertano and Paolo Cassata and Marco Castellano and Peter Challis and Ranga-Ram Chary and Edmond Cheung and Michele Cirasuolo and Conselice, {Christopher J.} and Cooray, {Asantha Roshan} and Croton, {Darren J.} and Emanuele Daddi and Tomas Dahlen and Romeel Dave and {de Mello}, {Duilia F.} and Avishai Dekel and Mark Dickinson and Timothy Dolch and Donley, {Jennifer L.} and Dunlop, {James S.} and Dutton, {Aaron A.} and David Elbaz and Fazio, {Giovanni G.} and Filippenko, {Alexei V.} and Finkelstein, {Steven L.} and Adriano Fontana and Gardner, {Jonathan P.} and Garnavich, {Peter M.} and Eric Gawiser and Mauro Giavalisco and Andrea Grazian and Yicheng Guo and Hathi, {Nimish P.} and Boris Haeussler and Hopkins, {Philip F.} and Jia-Sheng Huang and Kuang-Han Huang and Jha, {Saurabh W.} and Kartaltepe, {Jeyhan S.} and Kirshner, {Robert P.} and Koo, {David C.} and Kamson Lai and Kyoung-Soo Lee and Weidong Li and Lotz, {Jennifer M.} and Lucas, {Ray A.} and Piero Madau and McCarthy, {Patrick J.} and McGrath, {Elizabeth J.} and McIntosh, {Daniel H.} and McLure, {Ross J.} and Bahram Mobasher and Moustakas, {Leonidas A.} and Mark Mozena and Kirpal Nandra and Newman, {Jeffrey A.} and Sami-Matias Niemi and Noeske, {Kai G.} and Papovich, {Casey J.} and Laura Pentericci and Alexandra Pope and Primack, {Joel R.} and Abhijith Rajan and Swara Ravindranath and Reddy, {Naveen A.} and Alvio Renzini and Hans-Walter Rix and Robaina, {Aday R.} and Rodney, {Steven A.} and Rosario, {David J.} and Piero Rosati and Sara Salimbeni and Claudia Scarlata and Brian Siana and Luc Simard and Joseph Smidt and Somerville, {Rachel S.} and Hyron Spinrad and Straughn, {Amber N.} and Louis-Gregory Strolger and Olivia Telford and Teplitz, {Harry I.} and Trump, {Jonathan R.} and {van der Wel}, Arjen and Carolin Villforth and Wechsler, {Risa H.} and Weiner, {Benjamin J.} and Tommy Wiklind and Vivienne Wild and Grant Wilson and Stijn Wuyts and Hao-Jing Yan and Yun, {Min S.}",

year = "2011",

month = dec,

doi = "10.1088/0067-0049/197/2/35",

language = "English",

volume = "197",

journal = "Astrophysical Journal Supplement Series",

issn = "0067-0049",

publisher = "American Astronomical Society",

number = "2",

}

Grogin, NA, Kocevski, DD, Faber, SM, Ferguson, HC, Koekemoer, AM, Riess, AG, Acquaviva, V, Alexander, DM, Almaini, O, Ashby, MLN, Barden, M, Bell, EF, Bournaud, F, Brown, TM, Caputi, KI, Casertano, S, Cassata, P, Castellano, M, Challis, P, Chary, R-R, Cheung, E, Cirasuolo, M, Conselice, CJ, Cooray, AR, Croton, DJ, Daddi, E, Dahlen, T, Dave, R, de Mello, DF, Dekel, A, Dickinson, M, Dolch, T, Donley, JL, Dunlop, JS, Dutton, AA, Elbaz, D, Fazio, GG, Filippenko, AV, Finkelstein, SL, Fontana, A, Gardner, JP, Garnavich, PM, Gawiser, E, Giavalisco, M, Grazian, A, Guo, Y, Hathi, NP, Haeussler, B, Hopkins, PF, Huang, J-S, Huang, K-H, Jha, SW, Kartaltepe, JS, Kirshner, RP, Koo, DC, Lai, K, Lee, K-S, Li, W, Lotz, JM, Lucas, RA, Madau, P, McCarthy, PJ, McGrath, EJ, McIntosh, DH, McLure, RJ, Mobasher, B, Moustakas, LA, Mozena, M, Nandra, K, Newman, JA, Niemi, S-M, Noeske, KG, Papovich, CJ, Pentericci, L, Pope, A, Primack, JR, Rajan, A, Ravindranath, S, Reddy, NA, Renzini, A, Rix, H-W, Robaina, AR, Rodney, SA, Rosario, DJ, Rosati, P, Salimbeni, S, Scarlata, C, Siana, B, Simard, L, Smidt, J, Somerville, RS, Spinrad, H, Straughn, AN, Strolger, L-G, Telford, O, Teplitz, HI, Trump, JR, van der Wel, A, Villforth, C, Wechsler, RH, Weiner, BJ, Wiklind, T, Wild, V, Wilson, G, Wuyts, S, Yan, H-J & Yun, MS 2011, 'CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY', Astrophysical Journal Supplement Series, vol. 197, no. 2, 35. https://doi.org/10.1088/0067-0049/197/2/35

TY - JOUR

T1 - CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY

AU - Grogin, Norman A.

AU - Kocevski, Dale D.

AU - Faber, S. M.

AU - Ferguson, Henry C.

AU - Koekemoer, Anton M.

AU - Riess, Adam G.

AU - Acquaviva, Viviana

AU - Alexander, David M.

AU - Almaini, Omar

AU - Ashby, Matthew L. N.

AU - Barden, Marco

AU - Bell, Eric F.

AU - Bournaud, Frederic

AU - Brown, Thomas M.

AU - Caputi, Karina I.

AU - Casertano, Stefano

AU - Cassata, Paolo

AU - Castellano, Marco

AU - Challis, Peter

AU - Chary, Ranga-Ram

AU - Cheung, Edmond

AU - Cirasuolo, Michele

AU - Conselice, Christopher J.

AU - Cooray, Asantha Roshan

AU - Croton, Darren J.

AU - Daddi, Emanuele

AU - Dahlen, Tomas

AU - Dave, Romeel

AU - de Mello, Duilia F.

AU - Dekel, Avishai

AU - Dickinson, Mark

AU - Dolch, Timothy

AU - Donley, Jennifer L.

AU - Dunlop, James S.

AU - Dutton, Aaron A.

AU - Elbaz, David

AU - Fazio, Giovanni G.

AU - Filippenko, Alexei V.

AU - Finkelstein, Steven L.

AU - Fontana, Adriano

AU - Gardner, Jonathan P.

AU - Garnavich, Peter M.

AU - Gawiser, Eric

AU - Giavalisco, Mauro

AU - Grazian, Andrea

AU - Guo, Yicheng

AU - Hathi, Nimish P.

AU - Haeussler, Boris

AU - Hopkins, Philip F.

AU - Huang, Jia-Sheng

AU - Huang, Kuang-Han

AU - Jha, Saurabh W.

AU - Kartaltepe, Jeyhan S.

AU - Kirshner, Robert P.

AU - Koo, David C.

AU - Lai, Kamson

AU - Lee, Kyoung-Soo

AU - Li, Weidong

AU - Lotz, Jennifer M.

AU - Lucas, Ray A.

AU - Madau, Piero

AU - McCarthy, Patrick J.

AU - McGrath, Elizabeth J.

AU - McIntosh, Daniel H.

AU - McLure, Ross J.

AU - Mobasher, Bahram

AU - Moustakas, Leonidas A.

AU - Mozena, Mark

AU - Nandra, Kirpal

AU - Newman, Jeffrey A.

AU - Niemi, Sami-Matias

AU - Noeske, Kai G.

AU - Papovich, Casey J.

AU - Pentericci, Laura

AU - Pope, Alexandra

AU - Primack, Joel R.

AU - Rajan, Abhijith

AU - Ravindranath, Swara

AU - Reddy, Naveen A.

AU - Renzini, Alvio

AU - Rix, Hans-Walter

AU - Robaina, Aday R.

AU - Rodney, Steven A.

AU - Rosario, David J.

AU - Rosati, Piero

AU - Salimbeni, Sara

AU - Scarlata, Claudia

AU - Siana, Brian

AU - Simard, Luc

AU - Smidt, Joseph

AU - Somerville, Rachel S.

AU - Spinrad, Hyron

AU - Straughn, Amber N.

AU - Strolger, Louis-Gregory

AU - Telford, Olivia

AU - Teplitz, Harry I.

AU - Trump, Jonathan R.

AU - van der Wel, Arjen

AU - Villforth, Carolin

AU - Wechsler, Risa H.

AU - Weiner, Benjamin J.

AU - Wiklind, Tommy

AU - Wild, Vivienne

AU - Wilson, Grant

AU - Wuyts, Stijn

AU - Yan, Hao-Jing

AU - Yun, Min S.

PY - 2011/12

Y1 - 2011/12

N2 - The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is designed to document the first third of galactic evolution, over the approximate redshift (z) range 8-1.5. It will image >250,000 distant galaxies using three separate cameras on the Hubble Space Telescope, from the mid-ultraviolet to the near-infrared, and will find and measure Type Ia supernovae at z > 1.5 to test their accuracy as standardizable candles for cosmology. Five premier multi-wavelength sky regions are selected, each with extensive ancillary data. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to a stellar mass of 10(9)M(circle dot) to z approximate to 2, reaching the knee of the ultraviolet luminosity function of galaxies to z approximate to 8. The survey covers approximately 800 arcmin(2) and is divided into two parts. The CANDELS/Deep survey (5 sigma point-source limit H = 27.7 mag) covers similar to 125 arcmin(2) within Great Observatories Origins Deep Survey (GOODS)-N and GOODS-S. The CANDELS/Wide survey includes GOODS and three additional fields (Extended Groth Strip, COSMOS, and Ultra-deep Survey) and covers the full area to a 5 sigma point-source limit of H greater than or similar to 27.0 mag. Together with the Hubble Ultra Deep Fields, the strategy creates a three-tiered "wedding-cake" approach that has proven efficient for extragalactic surveys. Data from the survey are nonproprietary and are useful for a wide variety of science investigations. In this paper, we describe the basic motivations for the survey, the CANDELS team science goals and the resulting observational requirements, the field selection and geometry, and the observing design. The Hubble data processing and products are described in a companion paper.

AB - The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is designed to document the first third of galactic evolution, over the approximate redshift (z) range 8-1.5. It will image >250,000 distant galaxies using three separate cameras on the Hubble Space Telescope, from the mid-ultraviolet to the near-infrared, and will find and measure Type Ia supernovae at z > 1.5 to test their accuracy as standardizable candles for cosmology. Five premier multi-wavelength sky regions are selected, each with extensive ancillary data. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to a stellar mass of 10(9)M(circle dot) to z approximate to 2, reaching the knee of the ultraviolet luminosity function of galaxies to z approximate to 8. The survey covers approximately 800 arcmin(2) and is divided into two parts. The CANDELS/Deep survey (5 sigma point-source limit H = 27.7 mag) covers similar to 125 arcmin(2) within Great Observatories Origins Deep Survey (GOODS)-N and GOODS-S. The CANDELS/Wide survey includes GOODS and three additional fields (Extended Groth Strip, COSMOS, and Ultra-deep Survey) and covers the full area to a 5 sigma point-source limit of H greater than or similar to 27.0 mag. Together with the Hubble Ultra Deep Fields, the strategy creates a three-tiered "wedding-cake" approach that has proven efficient for extragalactic surveys. Data from the survey are nonproprietary and are useful for a wide variety of science investigations. In this paper, we describe the basic motivations for the survey, the CANDELS team science goals and the resulting observational requirements, the field selection and geometry, and the observing design. The Hubble data processing and products are described in a companion paper.

KW - cosmology: observations

KW - galaxies: high-redshift

KW - HUBBLE-SPACE-TELESCOPE

KW - STAR-FORMING GALAXIES

KW - ACTIVE GALACTIC NUCLEI

KW - LYMAN-BREAK GALAXIES

KW - SUPERMASSIVE BLACK-HOLES

KW - EXTENDED GROTH-STRIP

KW - GOODS-SOUTH FIELD

KW - SIMILAR-TO 7

KW - REST-FRAME ULTRAVIOLET

KW - EARLY RELEASE SCIENCE

U2 - 10.1088/0067-0049/197/2/35

DO - 10.1088/0067-0049/197/2/35

M3 - Article

SN - 0067-0049

VL - 197

JO - Astrophysical Journal Supplement Series

JF - Astrophysical Journal Supplement Series

IS - 2

M1 - 35

ER -

CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY

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Keywords

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