A warm Spitzer survey of the LSST/DES 'Deep drilling' fields

Mark Lacy; Duncan Farrah; Niel Brandt; Masao Sako; Gordon Richards; Ray Norris; Susan Ridgway; Jose Afonso; Robert Brunner; Dave Clements; Asantha Cooray; Giovanni Covone; Chris D'Andrea; Mark Dickinson; Harry Ferguson; Joshua Frieman; Ravi Gupta; Evanthia Hatziminaoglou; Matt Jarvis; Amy Kimball; Lori Lubin; Minnie Mao; Lucia Marchetti; Jean-Christophe Mauduit; Simona Mei; Jeffrey Newman; Robert Nichol; Seb Oliver; Ismael Perez-Fournon; Marguerite Pierre; Huub Rottgering; Nick Seymour; Ian Smail; Jason Surace; Paul Thorman; Mattia Vaccari; Aprajita Verma; Gillian Wilson; Michael Wood-Vasey; Rachel Cane; Risa Wechsler; Paul Martini; August Evrard; Richard McMahon; Kirk Borne; Diego Capozzi; Jiashang Huang; Claudia Lagos; Chris Lidman; Claudia Maraston; Janine Pforr; Anna Sajina; Rachel Somerville; Michael Strauss; Kristen Jones; Wayne Barkhouse; Michael Cooper; David Ballantyne; Preshanth Jagannathan; Eric Murphy; Isabella Pradoni; Nicholas Suntzeff; Ricardo Covarrubias; Lee Spitler

A warm Spitzer survey of the LSST/DES 'Deep drilling' fields

Mark Lacy, Duncan Farrah, Niel Brandt, Masao Sako, Gordon Richards, Ray Norris, Susan Ridgway, Jose Afonso, Robert Brunner, Dave Clements, Asantha Cooray, Giovanni Covone, Chris D'Andrea, Mark Dickinson, Harry Ferguson, Joshua Frieman, Ravi Gupta, Evanthia Hatziminaoglou, Matt Jarvis, Amy KimballLori Lubin, Minnie Mao, Lucia Marchetti, Jean-Christophe Mauduit, Simona Mei, Jeffrey Newman, Robert Nichol, Seb Oliver, Ismael Perez-Fournon, Marguerite Pierre, Huub Rottgering, Nick Seymour, Ian Smail, Jason Surace, Paul Thorman, Mattia Vaccari, Aprajita Verma, Gillian Wilson, Michael Wood-Vasey, Rachel Cane, Risa Wechsler, Paul Martini, August Evrard, Richard McMahon, Kirk Borne, Diego Capozzi, Jiashang Huang, Claudia Lagos, Chris Lidman, Claudia Maraston, Janine Pforr, Anna Sajina, Rachel Somerville, Michael Strauss, Kristen Jones, Wayne Barkhouse, Michael Cooper, David Ballantyne, Preshanth Jagannathan, Eric Murphy, Isabella Pradoni, Nicholas Suntzeff, Ricardo Covarrubias, Lee Spitler

Research School of Astronomy & Astrophysics

Research output: Other contribution

Abstract

We propose a warm Spitzer survey to microJy depth of the four predefined Deep Drilling Fields (DDFs) for the Large Synoptic Survey Telescope (LSST) (three of which are also deep drilling fields for the Dark Energy Survey (DES)). Imaging these fields with warm Spitzer is a key component of the overall success of these projects, that address the 'Physics of the Universe' theme of the Astro2010 decadal survey. With deep, accurate, near-infrared photometry from Spitzer in the DDFs, we will generate photometric redshift distributions to apply to the surveys as a whole. The DDFs are also the areas where the supernova searches of DES and LSST are concentrated, and deep Spitzer data is essential to obtain photometric redshifts, stellar masses and constraints on ages and metallicities for the >10000 supernova host galaxies these surveys will find. This 'DEEPDRILL' survey will also address the 'Cosmic Dawn' goal of Astro2010 through being deep enough to find all the >10^11 solar mass galaxies within the survey area out to z~6. DEEPDRILL will complete the final 24.4 square degrees of imaging in the DDFs, which, when added to the 14 square degrees already imaged to this depth, will map a volume of 1-Gpc^3 at z>2. It will find ~100 > 10^11 solar mass galaxies at z~5 and ~40 protoclusters at z>2, providing targets for JWST that can be found in no other way. The Spitzer data, in conjunction with the multiwavelength surveys in these fields, ranging from X-ray through far-infrared and cm-radio, will comprise a unique legacy dataset for studies of galaxy evolution.

Original language	English
Publication status	Published - 1 Dec 2014

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https://ui.adsabs.harvard.edu/abs/2014sptz.prop11086L

Cite this

Lacy, M., Farrah, D., Brandt, N., Sako, M., Richards, G., Norris, R., Ridgway, S., Afonso, J., Brunner, R., Clements, D., Cooray, A., Covone, G., D'Andrea, C., Dickinson, M., Ferguson, H., Frieman, J., Gupta, R., Hatziminaoglou, E., Jarvis, M., ... Spitler, L. (2014, Dec 1). A warm Spitzer survey of the LSST/DES 'Deep drilling' fields. https://ui.adsabs.harvard.edu/abs/2014sptz.prop11086L

@misc{52784f0cdcf44818a8fffe50b6960727,

title = "A warm Spitzer survey of the LSST/DES 'Deep drilling' fields",

abstract = "We propose a warm Spitzer survey to microJy depth of the four predefined Deep Drilling Fields (DDFs) for the Large Synoptic Survey Telescope (LSST) (three of which are also deep drilling fields for the Dark Energy Survey (DES)). Imaging these fields with warm Spitzer is a key component of the overall success of these projects, that address the 'Physics of the Universe' theme of the Astro2010 decadal survey. With deep, accurate, near-infrared photometry from Spitzer in the DDFs, we will generate photometric redshift distributions to apply to the surveys as a whole. The DDFs are also the areas where the supernova searches of DES and LSST are concentrated, and deep Spitzer data is essential to obtain photometric redshifts, stellar masses and constraints on ages and metallicities for the >10000 supernova host galaxies these surveys will find. This 'DEEPDRILL' survey will also address the 'Cosmic Dawn' goal of Astro2010 through being deep enough to find all the >10^11 solar mass galaxies within the survey area out to z~6. DEEPDRILL will complete the final 24.4 square degrees of imaging in the DDFs, which, when added to the 14 square degrees already imaged to this depth, will map a volume of 1-Gpc^3 at z>2. It will find ~100 > 10^11 solar mass galaxies at z~5 and ~40 protoclusters at z>2, providing targets for JWST that can be found in no other way. The Spitzer data, in conjunction with the multiwavelength surveys in these fields, ranging from X-ray through far-infrared and cm-radio, will comprise a unique legacy dataset for studies of galaxy evolution.",

author = "Mark Lacy and Duncan Farrah and Niel Brandt and Masao Sako and Gordon Richards and Ray Norris and Susan Ridgway and Jose Afonso and Robert Brunner and Dave Clements and Asantha Cooray and Giovanni Covone and Chris D'Andrea and Mark Dickinson and Harry Ferguson and Joshua Frieman and Ravi Gupta and Evanthia Hatziminaoglou and Matt Jarvis and Amy Kimball and Lori Lubin and Minnie Mao and Lucia Marchetti and Jean-Christophe Mauduit and Simona Mei and Jeffrey Newman and Robert Nichol and Seb Oliver and Ismael Perez-Fournon and Marguerite Pierre and Huub Rottgering and Nick Seymour and Ian Smail and Jason Surace and Paul Thorman and Mattia Vaccari and Aprajita Verma and Gillian Wilson and Michael Wood-Vasey and Rachel Cane and Risa Wechsler and Paul Martini and August Evrard and Richard McMahon and Kirk Borne and Diego Capozzi and Jiashang Huang and Claudia Lagos and Chris Lidman and Claudia Maraston and Janine Pforr and Anna Sajina and Rachel Somerville and Michael Strauss and Kristen Jones and Wayne Barkhouse and Michael Cooper and David Ballantyne and Preshanth Jagannathan and Eric Murphy and Isabella Pradoni and Nicholas Suntzeff and Ricardo Covarrubias and Lee Spitler",

year = "2014",

month = dec,

day = "1",

language = "English",

type = "Other",

}

Lacy, M, Farrah, D, Brandt, N, Sako, M, Richards, G, Norris, R, Ridgway, S, Afonso, J, Brunner, R, Clements, D, Cooray, A, Covone, G, D'Andrea, C, Dickinson, M, Ferguson, H, Frieman, J, Gupta, R, Hatziminaoglou, E, Jarvis, M, Kimball, A, Lubin, L, Mao, M, Marchetti, L, Mauduit, J-C, Mei, S, Newman, J, Nichol, R, Oliver, S, Perez-Fournon, I, Pierre, M, Rottgering, H, Seymour, N, Smail, I, Surace, J, Thorman, P, Vaccari, M, Verma, A, Wilson, G, Wood-Vasey, M, Cane, R, Wechsler, R, Martini, P, Evrard, A, McMahon, R, Borne, K, Capozzi, D, Huang, J, Lagos, C, Lidman, C, Maraston, C, Pforr, J, Sajina, A, Somerville, R, Strauss, M, Jones, K, Barkhouse, W, Cooper, M, Ballantyne, D, Jagannathan, P, Murphy, E, Pradoni, I, Suntzeff, N, Covarrubias, R & Spitler, L 2014, A warm Spitzer survey of the LSST/DES 'Deep drilling' fields.. <https://ui.adsabs.harvard.edu/abs/2014sptz.prop11086L>

TY - GEN

T1 - A warm Spitzer survey of the LSST/DES 'Deep drilling' fields

AU - Lacy, Mark

AU - Farrah, Duncan

AU - Brandt, Niel

AU - Sako, Masao

AU - Richards, Gordon

AU - Norris, Ray

AU - Ridgway, Susan

AU - Afonso, Jose

AU - Brunner, Robert

AU - Clements, Dave

AU - Cooray, Asantha

AU - Covone, Giovanni

AU - D'Andrea, Chris

AU - Dickinson, Mark

AU - Ferguson, Harry

AU - Frieman, Joshua

AU - Gupta, Ravi

AU - Hatziminaoglou, Evanthia

AU - Jarvis, Matt

AU - Kimball, Amy

AU - Lubin, Lori

AU - Mao, Minnie

AU - Marchetti, Lucia

AU - Mauduit, Jean-Christophe

AU - Mei, Simona

AU - Newman, Jeffrey

AU - Nichol, Robert

AU - Oliver, Seb

AU - Perez-Fournon, Ismael

AU - Pierre, Marguerite

AU - Rottgering, Huub

AU - Seymour, Nick

AU - Smail, Ian

AU - Surace, Jason

AU - Thorman, Paul

AU - Vaccari, Mattia

AU - Verma, Aprajita

AU - Wilson, Gillian

AU - Wood-Vasey, Michael

AU - Cane, Rachel

AU - Wechsler, Risa

AU - Martini, Paul

AU - Evrard, August

AU - McMahon, Richard

AU - Borne, Kirk

AU - Capozzi, Diego

AU - Huang, Jiashang

AU - Lagos, Claudia

AU - Lidman, Chris

AU - Maraston, Claudia

AU - Pforr, Janine

AU - Sajina, Anna

AU - Somerville, Rachel

AU - Strauss, Michael

AU - Jones, Kristen

AU - Barkhouse, Wayne

AU - Cooper, Michael

AU - Ballantyne, David

AU - Jagannathan, Preshanth

AU - Murphy, Eric

AU - Pradoni, Isabella

AU - Suntzeff, Nicholas

AU - Covarrubias, Ricardo

AU - Spitler, Lee

PY - 2014/12/1

Y1 - 2014/12/1

N2 - We propose a warm Spitzer survey to microJy depth of the four predefined Deep Drilling Fields (DDFs) for the Large Synoptic Survey Telescope (LSST) (three of which are also deep drilling fields for the Dark Energy Survey (DES)). Imaging these fields with warm Spitzer is a key component of the overall success of these projects, that address the 'Physics of the Universe' theme of the Astro2010 decadal survey. With deep, accurate, near-infrared photometry from Spitzer in the DDFs, we will generate photometric redshift distributions to apply to the surveys as a whole. The DDFs are also the areas where the supernova searches of DES and LSST are concentrated, and deep Spitzer data is essential to obtain photometric redshifts, stellar masses and constraints on ages and metallicities for the >10000 supernova host galaxies these surveys will find. This 'DEEPDRILL' survey will also address the 'Cosmic Dawn' goal of Astro2010 through being deep enough to find all the >10^11 solar mass galaxies within the survey area out to z~6. DEEPDRILL will complete the final 24.4 square degrees of imaging in the DDFs, which, when added to the 14 square degrees already imaged to this depth, will map a volume of 1-Gpc^3 at z>2. It will find ~100 > 10^11 solar mass galaxies at z~5 and ~40 protoclusters at z>2, providing targets for JWST that can be found in no other way. The Spitzer data, in conjunction with the multiwavelength surveys in these fields, ranging from X-ray through far-infrared and cm-radio, will comprise a unique legacy dataset for studies of galaxy evolution.

AB - We propose a warm Spitzer survey to microJy depth of the four predefined Deep Drilling Fields (DDFs) for the Large Synoptic Survey Telescope (LSST) (three of which are also deep drilling fields for the Dark Energy Survey (DES)). Imaging these fields with warm Spitzer is a key component of the overall success of these projects, that address the 'Physics of the Universe' theme of the Astro2010 decadal survey. With deep, accurate, near-infrared photometry from Spitzer in the DDFs, we will generate photometric redshift distributions to apply to the surveys as a whole. The DDFs are also the areas where the supernova searches of DES and LSST are concentrated, and deep Spitzer data is essential to obtain photometric redshifts, stellar masses and constraints on ages and metallicities for the >10000 supernova host galaxies these surveys will find. This 'DEEPDRILL' survey will also address the 'Cosmic Dawn' goal of Astro2010 through being deep enough to find all the >10^11 solar mass galaxies within the survey area out to z~6. DEEPDRILL will complete the final 24.4 square degrees of imaging in the DDFs, which, when added to the 14 square degrees already imaged to this depth, will map a volume of 1-Gpc^3 at z>2. It will find ~100 > 10^11 solar mass galaxies at z~5 and ~40 protoclusters at z>2, providing targets for JWST that can be found in no other way. The Spitzer data, in conjunction with the multiwavelength surveys in these fields, ranging from X-ray through far-infrared and cm-radio, will comprise a unique legacy dataset for studies of galaxy evolution.

M3 - Other contribution

ER -

A warm Spitzer survey of the LSST/DES 'Deep drilling' fields

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