The SDSS-IV eBOSS emission-line galaxy pilot survey

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

doi:10.1051/0004-6361/201527377

The SDSS-IV eBOSS emission-line galaxy pilot survey

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

Institute of Cosmology & Gravitation

New Mexico State University

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Abstract

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 standard ruler (BAO) at redshift 0.9. To test different ELG selection algorithms, based on data from several imaging surveys, 9,000 spectra were observed with the SDSS spectrograph as a pilot survey. First, using visual inspection and redshift quality flags, we find that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a robust BAO measurement. Also, we 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 tested and compare them with the requirements of the eBOSS experiment. As a result, we provide robust redshift distributions for the different target selection schemes tested. Finally, we infer two optimal target selection algorithms to be applied on DECam photometry that fulfill the eBOSS survey efficiency requirements.

Original language	English
Article number	A121
Number of pages	18
Journal	Astronomy and Astrophysics
Volume	592
Early online date	9 Aug 2016
DOIs	https://doi.org/10.1051/0004-6361/201527377
Publication status	Published - Aug 2016

Keywords

astro-ph.CO
astro-ph.GA
cosmology
survey
spectroscopy
galaxy
emission lines
RCUK
STFC
large-scale structure of Universe
galaxies: general
methods: observational

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10.1051/0004-6361/201527377

1509.05045v3Accepted author manuscript (Post-print), 2.31 MB

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Comparat, J., Delubac, T., Jouvel, S., Raichoor, A., Kneib, J-P., Yeche, C., Abdalla, F. B., Cras, C. L., Maraston, C., Wilkinson, D. M., Zhu, G., Jullo, E., Prada, F., Schlegel, D., Xu, Z., Zou, H., Bautista, J., Bizyaev, D., Bolton, A., ... Zhang, Y. (2016). The SDSS-IV eBOSS emission-line galaxy pilot survey. Astronomy and Astrophysics, 592, [A121]. https://doi.org/10.1051/0004-6361/201527377

@article{f7a3900c8c12418caf6634c22b3dda02,

title = "The SDSS-IV eBOSS emission-line galaxy pilot survey",

abstract = "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 standard ruler (BAO) at redshift 0.9. To test different ELG selection algorithms, based on data from several imaging surveys, 9,000 spectra were observed with the SDSS spectrograph as a pilot survey. First, using visual inspection and redshift quality flags, we find that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a robust BAO measurement. Also, we 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 tested and compare them with the requirements of the eBOSS experiment. As a result, we provide robust redshift distributions for the different target selection schemes tested. Finally, we infer two optimal target selection algorithms to be applied on DECam photometry that fulfill the eBOSS survey efficiency requirements.",

keywords = "astro-ph.CO, astro-ph.GA, cosmology, survey, spectroscopy, galaxy, emission lines, RCUK, STFC, large-scale structure of Universe, galaxies: general, methods: observational",

author = "J. Comparat and T. Delubac and S. Jouvel and A. Raichoor and J-P Kneib and C. Yeche and Abdalla, {F. B.} and Cras, {C. Le} and C. Maraston and Wilkinson, {D. M.} and G. Zhu and E. Jullo and F. Prada and D. Schlegel and Z. Xu and H. Zou and J. Bautista and D. Bizyaev and A. Bolton and Brownstein, {J. R.} and Dawson, {K. S.} and Stephanie Escoffier and P. Gualme and K. Kinemuchi and E. Malanushenko and V. Malanushenko and V. Mariappan and Newman, {J. A.} and D. Oravetz and K. Pan and Percival, {W. J.} and A. Prakash and Schneider, {D. P.} and A. Simmons and Abbott, {T. M. C.} and S. Allam and M. Banerji and A. Benoit-L{\'e}vy and E. Bertin and D. Brooks and D. Capozzi and Rosell, {A. Carnero} and Kind, {M. Carrasco} and J. Carretero and Castander, {F. J.} and Cunha, {C. E.} and Costa, {L. N. da} and S. Desai and P. Doel and Eifler, {T. F.} and J. Estrada and B. Flaugher and P. Fosalba and J. Frieman and E. Gaztanaga and Gerdes, {D. W.} and D. Gruen and Gruendl, {R. A.} and G. Gutierrez and K. Honscheid and James, {D. J.} and K. Kuehn and N. Kuropatkin and O. Lahav and M. Lima and Maia, {M. A. G.} and M. March and Marshall, {J. L.} and R. Miquel and Plazas, {A. A.} and K. Reil and N. Roe and Romer, {A. K.} and A. Roodman and Rykoff, {E. S.} and M. Sako and E. Sanchez and V. Scarpine and I. Sevilla-Noarbe and M. Soares-Santos and F. Sobreira and E. Suchyta and Swanson, {M. E. C.} and G. Tarle and J. Thaler and D. Thomas and Walker, {A. R.} and Y. Zhang",

note = "21 pages. Submitted to A and A",

year = "2016",

month = aug,

doi = "10.1051/0004-6361/201527377",

language = "English",

volume = "592",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Comparat, J, Delubac, T, Jouvel, S, Raichoor, A, Kneib, J-P, Yeche, C, Abdalla, FB, Cras, CL, Maraston, C, Wilkinson, DM, Zhu, G, Jullo, E, Prada, F, Schlegel, D, Xu, Z, Zou, H, Bautista, J, Bizyaev, D, Bolton, A, Brownstein, JR, Dawson, KS, Escoffier, S, Gualme, P, Kinemuchi, K, Malanushenko, E, Malanushenko, V, Mariappan, V, Newman, JA, Oravetz, D, Pan, K, Percival, WJ, Prakash, A, Schneider, DP, Simmons, A, Abbott, TMC, Allam, S, Banerji, M, Benoit-Lévy, A, Bertin, E, Brooks, D, Capozzi, D, Rosell, AC, Kind, MC, Carretero, J, Castander, FJ, Cunha, CE, Costa, LND, Desai, S, Doel, P, Eifler, TF, Estrada, J, Flaugher, B, Fosalba, P, Frieman, J, Gaztanaga, E, Gerdes, DW, Gruen, D, Gruendl, RA, Gutierrez, G, Honscheid, K, James, DJ, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Maia, MAG, March, M, Marshall, JL, Miquel, R, Plazas, AA, Reil, K, Roe, N, Romer, AK, Roodman, A, Rykoff, ES, Sako, M, Sanchez, E, Scarpine, V, Sevilla-Noarbe, I, Soares-Santos, M, Sobreira, F, Suchyta, E, Swanson, MEC, Tarle, G, Thaler, J, Thomas, D, Walker, AR & Zhang, Y 2016, 'The SDSS-IV eBOSS emission-line galaxy pilot survey', Astronomy and Astrophysics, vol. 592, A121. https://doi.org/10.1051/0004-6361/201527377

TY - JOUR

T1 - The SDSS-IV eBOSS emission-line galaxy pilot survey

AU - Comparat, J.

AU - Delubac, T.

AU - Jouvel, S.

AU - Raichoor, A.

AU - Kneib, J-P

AU - Yeche, C.

AU - Abdalla, F. B.

AU - Cras, C. Le

AU - Maraston, C.

AU - Wilkinson, D. M.

AU - Zhu, G.

AU - Jullo, E.

AU - Prada, F.

AU - Schlegel, D.

AU - Xu, Z.

AU - Zou, H.

AU - Bautista, J.

AU - Bizyaev, D.

AU - Bolton, A.

AU - Brownstein, J. R.

AU - Dawson, K. S.

AU - Escoffier, Stephanie

AU - Gualme, P.

AU - Kinemuchi, K.

AU - Malanushenko, E.

AU - Malanushenko, V.

AU - Mariappan, V.

AU - Newman, J. A.

AU - Oravetz, D.

AU - Pan, K.

AU - Percival, W. J.

AU - Prakash, A.

AU - Schneider, D. P.

AU - Simmons, A.

AU - Abbott, T. M. C.

AU - Allam, S.

AU - Banerji, M.

AU - Benoit-Lévy, A.

AU - Bertin, E.

AU - Brooks, D.

AU - Capozzi, D.

AU - Rosell, A. Carnero

AU - Kind, M. Carrasco

AU - Carretero, J.

AU - Castander, F. J.

AU - Cunha, C. E.

AU - Costa, L. N. da

AU - Desai, S.

AU - Doel, P.

AU - Eifler, T. F.

AU - Estrada, J.

AU - Flaugher, B.

AU - Fosalba, P.

AU - Frieman, J.

AU - Gaztanaga, E.

AU - Gerdes, D. W.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gutierrez, G.

AU - Honscheid, K.

AU - James, D. J.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Lima, M.

AU - Maia, M. A. G.

AU - March, M.

AU - Marshall, J. L.

AU - Miquel, R.

AU - Plazas, A. A.

AU - Reil, K.

AU - Roe, N.

AU - Romer, A. K.

AU - Roodman, A.

AU - Rykoff, E. S.

AU - Sako, M.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Sevilla-Noarbe, I.

AU - Soares-Santos, M.

AU - Sobreira, F.

AU - Suchyta, E.

AU - Swanson, M. E. C.

AU - Tarle, G.

AU - Thaler, J.

AU - Thomas, D.

AU - Walker, A. R.

AU - Zhang, Y.

N1 - 21 pages. Submitted to A and A

PY - 2016/8

Y1 - 2016/8

N2 - 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 standard ruler (BAO) at redshift 0.9. To test different ELG selection algorithms, based on data from several imaging surveys, 9,000 spectra were observed with the SDSS spectrograph as a pilot survey. First, using visual inspection and redshift quality flags, we find that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a robust BAO measurement. Also, we 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 tested and compare them with the requirements of the eBOSS experiment. As a result, we provide robust redshift distributions for the different target selection schemes tested. Finally, we infer two optimal target selection algorithms to be applied on DECam photometry that fulfill the eBOSS survey efficiency requirements.

AB - 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 standard ruler (BAO) at redshift 0.9. To test different ELG selection algorithms, based on data from several imaging surveys, 9,000 spectra were observed with the SDSS spectrograph as a pilot survey. First, using visual inspection and redshift quality flags, we find that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a robust BAO measurement. Also, we 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 tested and compare them with the requirements of the eBOSS experiment. As a result, we provide robust redshift distributions for the different target selection schemes tested. Finally, we infer two optimal target selection algorithms to be applied on DECam photometry that fulfill the eBOSS survey efficiency requirements.

KW - astro-ph.CO

KW - astro-ph.GA

KW - cosmology

KW - survey

KW - spectroscopy

KW - galaxy

KW - emission lines

KW - RCUK

KW - STFC

KW - large-scale structure of Universe

KW - galaxies: general

KW - methods: observational

U2 - 10.1051/0004-6361/201527377

DO - 10.1051/0004-6361/201527377

M3 - Article

VL - 592

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - A121

ER -

The SDSS-IV eBOSS emission-line galaxy pilot survey

Abstract

Keywords

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