SDSS-IV eBOSS emission-line galaxy pilot survey

Comparat, J.; Delubac, T.; Jouvel, S.; Raichoor, Anand; Kneib, J. -P.; Yèche, C.; Abdalla, F. B.; Le Cras, C.; Maraston, C.; Wilkinson, D. M.; Zhu, G.; Jullo, E.; Prada, Francisco; Schlegel, D.; Xu, Z.; Zou, Hu; Bautista, Julian; Bizyaev, Dmitry; Bolton, A.; Brownstein, J. R.; Dawson, Kyle; Escoffier, Stephanie; Gaulme, P.; Kinemuchi, K.; Malanushenko, E.; Mariappan, V.; Newman, J. A.; Oravetz, D.; Pan, K.; Percival, Will J.; Prakash, A.; Schneider, D. P.; Simmons, A.; Abbott, T. M. C.; Allam, S.; Banerji, M.; Benoit-Lévy, A.; Bertin, E.; Brooks, D.; Capozzi, D.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, Jorge; Castander, Francisco J.; Cunha, C. E.; da Costa, L. N.; Desai, S.; Doel, P.; Eifler, T. F.; Estrada, J.; Flaugher, B.; Fosalba, Pablo; Frieman, J.; Gaztañaga, Enrique; Gerdes, D. W.; Gruen, D.; Gruendl, R. A.; Gutierrez, G.; Honscheid, K.; James, D. J.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; Lima, M.; Maia, M. A. G.; March, M.; Marshall, J. L.; Miquel, R.; Plazas, A. A.; Reil, K.; Roe, N.; Romer, A. K.; Roodman, A.; Rykoff, E. S.; Sako, M.; Sanchez, E.; Scarpine, V.; Sevilla-Noarbe, I.; Soares-Santos, M.; Sobreira, F.; Suchyta, E.; Swanson, M. E. C.; Tarlé, Gregory; Thaler, J.; Thomas, D.; Walker, A. R.; Zhang, Y.

SDSS-IV eBOSS emission-line galaxy pilot survey

The Sloan Digital Sky Survey IV extended Baryonic Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) will observe 195 000 emission-line galaxies (ELGs) to measure the baryonic acoustic oscillation (BAO) standard ruler at redshift 0.9. To test different ELG selection algorithms, 9000 spectra were obser...

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Autores:	Comparat, J., Delubac, T., Jouvel, S., Raichoor, Anand, Kneib, J. -P., Yèche, C., Abdalla, F. B., Le Cras, C., Maraston, C., Wilkinson, D. M., Zhu, G., Jullo, E., Prada, Francisco, Schlegel, D., Xu, Z., Zou, Hu, Bautista, Julian, Bizyaev, Dmitry, Bolton, A., Brownstein, J. R., Dawson, Kyle, Escoffier, Stephanie, Gaulme, P., Kinemuchi, K., Malanushenko, E., Mariappan, V., Newman, J. A., Oravetz, D., Pan, K., Percival, Will J., Prakash, A., Schneider, D. P., Simmons, A., Abbott, T. M. C., Allam, S., Banerji, M., Benoit-Lévy, A., Bertin, E., Brooks, D., Capozzi, D., Carnero Rosell, A., Carrasco Kind, M., Carretero, Jorge, Castander, Francisco J., Cunha, C. E., da Costa, L. N., Desai, S., Doel, P., Eifler, T. F., Estrada, J., Flaugher, B., Fosalba, Pablo, Frieman, J., Gaztañaga, Enrique, Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Marshall, J. L., Miquel, R., Plazas, A. A., Reil, K., Roe, N., Romer, A. K., Roodman, A., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarlé, Gregory, Thaler, J., Thomas, D., Walker, A. R., Zhang, Y.
Tipo de recurso:	artículo
Fecha de publicación:	2016
País:	España
Institución:	Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:	DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:	oai:digital.csic.es:10261/394055
Acceso en línea:	http://hdl.handle.net/10261/394055
Access Level:	acceso abierto
Palabra clave:	Large-scale structure of Universe Galaxies: general Methods: observational

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oai_identifier_str	oai:digital.csic.es:10261/394055
network_acronym_str	ES
network_name_str	España
title	SDSS-IV eBOSS emission-line galaxy pilot survey
spellingShingle	SDSS-IV eBOSS emission-line galaxy pilot survey Comparat, J. Large-scale structure of Universe Galaxies: general Methods: observational
title_short	SDSS-IV eBOSS emission-line galaxy pilot survey
title_full	SDSS-IV eBOSS emission-line galaxy pilot survey
title_fullStr	SDSS-IV eBOSS emission-line galaxy pilot survey
title_full_unstemmed	SDSS-IV eBOSS emission-line galaxy pilot survey
title_sort	SDSS-IV eBOSS emission-line galaxy pilot survey
author	Comparat, J.
author_facet	Comparat, J. Delubac, T. Jouvel, S. Raichoor, Anand Kneib, J. -P. Yèche, C. Abdalla, F. B. Le Cras, C. Maraston, C. Wilkinson, D. M. Zhu, G. Jullo, E. Prada, Francisco Schlegel, D. Xu, Z. Zou, Hu Bautista, Julian Bizyaev, Dmitry Bolton, A. Brownstein, J. R. Dawson, Kyle Escoffier, Stephanie Gaulme, P. Kinemuchi, K. Malanushenko, E. Mariappan, V. Newman, J. A. Oravetz, D. Pan, K. Percival, Will J. Prakash, A. Schneider, D. P. Simmons, A. Abbott, T. M. C. Allam, S. Banerji, M. Benoit-Lévy, A. Bertin, E. Brooks, D. Capozzi, D. Carnero Rosell, A. Carrasco Kind, M. Carretero, Jorge Castander, Francisco J. Cunha, C. E. da Costa, L. N. Desai, S. Doel, P. Eifler, T. F. Estrada, J. Flaugher, B. Fosalba, Pablo Frieman, J. Gaztañaga, Enrique Gerdes, D. W. Gruen, D. Gruendl, R. A. Gutierrez, G. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M. A. G. March, M. Marshall, J. L. Miquel, R. Plazas, A. A. Reil, K. Roe, N. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Sanchez, E. Scarpine, V. Sevilla-Noarbe, I. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarlé, Gregory Thaler, J. Thomas, D. Walker, A. R. Zhang, Y.
author_role	author
author2	Delubac, T. Jouvel, S. Raichoor, Anand Kneib, J. -P. Yèche, C. Abdalla, F. B. Le Cras, C. Maraston, C. Wilkinson, D. M. Zhu, G. Jullo, E. Prada, Francisco Schlegel, D. Xu, Z. Zou, Hu Bautista, Julian Bizyaev, Dmitry Bolton, A. Brownstein, J. R. Dawson, Kyle Escoffier, Stephanie Gaulme, P. Kinemuchi, K. Malanushenko, E. Mariappan, V. Newman, J. A. Oravetz, D. Pan, K. Percival, Will J. Prakash, A. Schneider, D. P. Simmons, A. Abbott, T. M. C. Allam, S. Banerji, M. Benoit-Lévy, A. Bertin, E. Brooks, D. Capozzi, D. Carnero Rosell, A. Carrasco Kind, M. Carretero, Jorge Castander, Francisco J. Cunha, C. E. da Costa, L. N. Desai, S. Doel, P. Eifler, T. F. Estrada, J. Flaugher, B. Fosalba, Pablo Frieman, J. Gaztañaga, Enrique Gerdes, D. W. Gruen, D. Gruendl, R. A. Gutierrez, G. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M. A. G. March, M. Marshall, J. L. Miquel, R. Plazas, A. A. Reil, K. Roe, N. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Sanchez, E. Scarpine, V. Sevilla-Noarbe, I. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarlé, Gregory Thaler, J. Thomas, D. Walker, A. R. Zhang, Y.
author2_role	author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author
topic	Large-scale structure of Universe Galaxies: general Methods: observational
topic_facet	Large-scale structure of Universe Galaxies: general Methods: observational
description	The Sloan Digital Sky Survey IV extended Baryonic Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) will observe 195 000 emission-line galaxies (ELGs) to measure the baryonic acoustic oscillation (BAO) standard ruler at redshift 0.9. To test different ELG selection algorithms, 9000 spectra were observed with the SDSS spectrograph as a pilot survey based on data from several imaging surveys. First, using visual inspection and redshift quality flags, we show that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a reliable BAO measurement. We also show the correlations between sky emission, signal-to-noise ratio in the emission lines, and redshift error. Then we provide a detailed description of each target selection algorithm we tested and compare them with the requirements of the eBOSS experiment. As a result, we provide reliable redshift distributions for the different target selection schemes we tested. Finally, we determine an target selection algorithms that is best suited to be applied on DECam photometry because they fulfill the eBOSS survey efficiency requirements. © ESO, 2016.
publishDate	2016
format	article
url	http://hdl.handle.net/10261/394055
eu_rights_str_mv	openAccess
publisher	EDP Sciences
institution	Consejo Superior de Investigaciones Científicas (CSIC)
collection	DIGITAL.CSIC. Repositorio Institucional del CSIC
reponame_str	DIGITAL.CSIC. Repositorio Institucional del CSIC
instname_str	Consejo Superior de Investigaciones Científicas (CSIC)
spelling	SDSS-IV eBOSS emission-line galaxy pilot survey Comparat, J. Delubac, T. Jouvel, S. Raichoor, Anand Kneib, J. -P. Yèche, C. Abdalla, F. B. Le Cras, C. Maraston, C. Wilkinson, D. M. Zhu, G. Jullo, E. Prada, Francisco Schlegel, D. Xu, Z. Zou, Hu Bautista, Julian Bizyaev, Dmitry Bolton, A. Brownstein, J. R. Dawson, Kyle Escoffier, Stephanie Gaulme, P. Kinemuchi, K. Malanushenko, E. Mariappan, V. Newman, J. A. Oravetz, D. Pan, K. Percival, Will J. Prakash, A. Schneider, D. P. Simmons, A. Abbott, T. M. C. Allam, S. Banerji, M. Benoit-Lévy, A. Bertin, E. Brooks, D. Capozzi, D. Carnero Rosell, A. Carrasco Kind, M. Carretero, Jorge Castander, Francisco J. Cunha, C. E. da Costa, L. N. Desai, S. Doel, P. Eifler, T. F. Estrada, J. Flaugher, B. Fosalba, Pablo Frieman, J. Gaztañaga, Enrique Gerdes, D. W. Gruen, D. Gruendl, R. A. Gutierrez, G. Honscheid, K. James, D. J. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M. A. G. March, M. Marshall, J. L. Miquel, R. Plazas, A. A. Reil, K. Roe, N. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Sanchez, E. Scarpine, V. Sevilla-Noarbe, I. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarlé, Gregory Thaler, J. Thomas, D. Walker, A. R. Zhang, Y. Large-scale structure of Universe Galaxies: general Methods: observational The Sloan Digital Sky Survey IV extended Baryonic Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) will observe 195 000 emission-line galaxies (ELGs) to measure the baryonic acoustic oscillation (BAO) standard ruler at redshift 0.9. To test different ELG selection algorithms, 9000 spectra were observed with the SDSS spectrograph as a pilot survey based on data from several imaging surveys. First, using visual inspection and redshift quality flags, we show that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a reliable BAO measurement. We also show the correlations between sky emission, signal-to-noise ratio in the emission lines, and redshift error. Then we provide a detailed description of each target selection algorithm we tested and compare them with the requirements of the eBOSS experiment. As a result, we provide reliable redshift distributions for the different target selection schemes we tested. Finally, we determine an target selection algorithms that is best suited to be applied on DECam photometry because they fulfill the eBOSS survey efficiency requirements. © ESO, 2016. J.C .and F.P. acknowledge support from the Spanish MICINNs Consolider-Ingenio 2010 Programme under grant MultiDark CSD2009-00064, MINECO Centro de Excelencia Severo Ochoa Programme under the grants SEV-2012-0249, FPA2012-34694, and the projects AYA2014-60641-C2-1-P and AYA2012-31101. We also thank the Lawrence Berkeley National Laboratory for its hospitality. F.P. acknowledges the spanish MEC Salvador de Madariaga program, Ref. PRX14/00444. T.D. and J.P.K. acknowledge support from the LIDA ERC advanced grant. AR acknowledges funding from the P2IO LabEx (ANR-10-LABX-0038) in the framework Investissements d’Avenir (ANR- 11-IDEX-0003-01) managed by the French National Research Agency (ANR). E.J. acknowledges the support of CNRS and the Labex OCEVU. This paper represents an effort by the SDSS-III, SDSS-IV and DES collaborations. Funding for SDSS-III was provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS web site is http://www.sdss.org. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatory of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, Yale University and the french participation group. Funding for the DES Projects has been provided by the US Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical AstronomyObservatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University. The DES data management system is supported by the National Science Foundation under Grant Number AST-1138766. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2012-39559, ESP2013-48274, FPA2013-47986, and Centro de Excelencia Severo Ochoa SEV-2012-0234. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007−2013) including ERC grant agreements 240672, 291329, and 306478. We are grateful for the extraordinary contributions of our CTIO colleagues and the DECam Construction, Commissioning and Science Verification teams in achieving the excellent instrument and telescope conditions that have made this work possible. The success of this project also relies critically on the expertise and dedication of the DES Data Management group. This paper includes targets derived from the images of the Wide-Field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This paper has gone through internal review by the DES collaboration. EDP Sciences http://hdl.handle.net/10261/394055
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publishDateSort	2016
author_browse	Abbott, T. M. C. Abdalla, F. B. Allam, S. Banerji, M. Bautista, Julian Benoit-Lévy, A. Bertin, E. Bizyaev, Dmitry Bolton, A. Brooks, D. Brownstein, J. R. Capozzi, D. Carnero Rosell, A. Carrasco Kind, M. Carretero, Jorge Castander, Francisco J. Comparat, J. Cunha, C. E. Dawson, Kyle Delubac, T. Desai, S. Doel, P. Eifler, T. F. Escoffier, Stephanie Estrada, J. Flaugher, B. Fosalba, Pablo Frieman, J. Gaulme, P. Gaztañaga, Enrique Gerdes, D. W. Gruen, D. Gruendl, R. A. Gutierrez, G. Honscheid, K. James, D. J. Jouvel, S. Jullo, E. Kinemuchi, K. Kneib, J. -P. Kuehn, K. Kuropatkin, N. Lahav, O. Le Cras, C. Lima, M. Maia, M. A. G. Malanushenko, E. Maraston, C. March, M. Mariappan, V. Marshall, J. L. Miquel, R. Newman, J. A. Oravetz, D. Pan, K. Percival, Will J. Plazas, A. A. Prada, Francisco Prakash, A. Raichoor, Anand Reil, K. Roe, N. Romer, A. K. Roodman, A. Rykoff, E. S. Sako, M. Sanchez, E. Scarpine, V. Schlegel, D. Schneider, D. P. Sevilla-Noarbe, I. Simmons, A. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E. C. Tarlé, Gregory Thaler, J. Thomas, D. Walker, A. R. Wilkinson, D. M. Xu, Z. Yèche, C. Zhang, Y. Zhu, G. Zou, Hu da Costa, L. N.
publisherStr	EDP Sciences
score	6,9303427

SDSS-IV eBOSS emission-line galaxy pilot survey

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