Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS
Abstract
We present the results of the first test plates of the extended Baryon Oscillation Spectroscopic Survey. This paper focuses on the emission line galaxies (ELG) population targetted from the Dark Energy Survey (DES) photometry. We analyse the success rate, efficiency, redshift distribution, and clustering properties of the targets. From the 9000 spectroscopic redshifts targetted, 4600 have been selected from the DES photometry. The total success rate for redshifts between 0.6 and 1.2 is 71\% and 68\% respectively for a bright and faint, on average more distant, samples including redshifts measured from a single strong emission line. We find a mean redshift of 0.8 and 0.87, with 15 and 13\% of unknown redshifts respectively for the bright and faint samples. In the redshift range 0.6<1.2, for the most secure spectroscopic redshifts, the mean redshift for the bright and faint sample is 0.85 and 0.9 respectively. Star contamination is lower than 2\%. We measure a galaxy bias averaged on scales of 1 and 10~Mpc/h of 1.72 \pm 0.1 for the bright sample and of 1.78 \pm 0.12 for the faint sample. The error on the galaxy bias have been obtained propagating the errors in the correlation function to the fitted parameters. Thismore »
- Authors:
- more »
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- National Science Foundation (NSF); USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- DES Collaboration; DES; BOSS
- OSTI Identifier:
- 1390286
- Alternate Identifier(s):
- OSTI ID: 1253006
- Report Number(s):
- FERMILAB-PUB-15-451-AE; arXiv:1509.07121
Journal ID: ISSN 0035-8711; TRN: US1702480
- Grant/Contract Number:
- AC02-76SF00515; AST1138766; AYA201239559; ESP2013- 48274; FPA2013-47986; AC02-07CH11359
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 469; Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; surveys; cosmology; observations
Citation Formats
Jouvel, S., Delubac, T., Comparat, J., Camacho, H., Carnero, A., Abdalla, F. B., Kneib, J. -P., Merson, A., Lima, M., Sobreira, F., da Costa, Luiz, Prada, F., Zhu, G. B., Benoit-Levy, A., Macora, A. De La, Kuropatkin, N., Lin, H., Abbott, T. M. C., Allam, S., Banerji, M., Bertin, E., Brooks, D., Capozzi, D., Kind, M. Carrasco, Carretero, J., Castander, F. J., Cunha, C. E., Desai, S., Doel, P., Eifler, T. F., Estrada, J., Neto, A. Fausti, Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Li, T. S., Maia, M. A. G., March, M., Marshall, J. L., Miquel, R., Ogando, R., Percival, W. J., Plazas, A. A., Reil, K., Romer, A. K., Roodman, A., Rykoff, E. S., Sako, M., Sanchez, E., Santiago, B., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., Thaler, J., Thomas, D., Walker, A., Zhang, Y., and Brownstein, J. Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS. United States: N. p., 2017.
Web. doi:10.1093/mnras/stx163.
Jouvel, S., Delubac, T., Comparat, J., Camacho, H., Carnero, A., Abdalla, F. B., Kneib, J. -P., Merson, A., Lima, M., Sobreira, F., da Costa, Luiz, Prada, F., Zhu, G. B., Benoit-Levy, A., Macora, A. De La, Kuropatkin, N., Lin, H., Abbott, T. M. C., Allam, S., Banerji, M., Bertin, E., Brooks, D., Capozzi, D., Kind, M. Carrasco, Carretero, J., Castander, F. J., Cunha, C. E., Desai, S., Doel, P., Eifler, T. F., Estrada, J., Neto, A. Fausti, Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Li, T. S., Maia, M. A. G., March, M., Marshall, J. L., Miquel, R., Ogando, R., Percival, W. J., Plazas, A. A., Reil, K., Romer, A. K., Roodman, A., Rykoff, E. S., Sako, M., Sanchez, E., Santiago, B., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., Thaler, J., Thomas, D., Walker, A., Zhang, Y., & Brownstein, J. Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS. United States. https://doi.org/10.1093/mnras/stx163
Jouvel, S., Delubac, T., Comparat, J., Camacho, H., Carnero, A., Abdalla, F. B., Kneib, J. -P., Merson, A., Lima, M., Sobreira, F., da Costa, Luiz, Prada, F., Zhu, G. B., Benoit-Levy, A., Macora, A. De La, Kuropatkin, N., Lin, H., Abbott, T. M. C., Allam, S., Banerji, M., Bertin, E., Brooks, D., Capozzi, D., Kind, M. Carrasco, Carretero, J., Castander, F. J., Cunha, C. E., Desai, S., Doel, P., Eifler, T. F., Estrada, J., Neto, A. Fausti, Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Li, T. S., Maia, M. A. G., March, M., Marshall, J. L., Miquel, R., Ogando, R., Percival, W. J., Plazas, A. A., Reil, K., Romer, A. K., Roodman, A., Rykoff, E. S., Sako, M., Sanchez, E., Santiago, B., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., Thaler, J., Thomas, D., Walker, A., Zhang, Y., and Brownstein, J. Fri .
"Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS". United States. https://doi.org/10.1093/mnras/stx163. https://www.osti.gov/servlets/purl/1390286.
@article{osti_1390286,
title = {Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS},
author = {Jouvel, S. and Delubac, T. and Comparat, J. and Camacho, H. and Carnero, A. and Abdalla, F. B. and Kneib, J. -P. and Merson, A. and Lima, M. and Sobreira, F. and da Costa, Luiz and Prada, F. and Zhu, G. B. and Benoit-Levy, A. and Macora, A. De La and Kuropatkin, N. and Lin, H. and Abbott, T. M. C. and Allam, S. and Banerji, M. and Bertin, E. and Brooks, D. and Capozzi, D. and Kind, M. Carrasco and Carretero, J. and Castander, F. J. and Cunha, C. E. and Desai, S. and Doel, P. and Eifler, T. F. and Estrada, J. and Neto, A. Fausti and Flaugher, B. and Fosalba, P. and Frieman, J. and Gaztanaga, E. and Gerdes, D. W. and Gruen, D. and Gruendl, R. A. and Gutierrez, G. and Honscheid, K. and James, D. J. and Kuehn, K. and Lahav, O. and Li, T. S. and Maia, M. A. G. and March, M. and Marshall, J. L. and Miquel, R. and Ogando, R. and Percival, W. J. and Plazas, A. A. and Reil, K. and Romer, A. K. and Roodman, A. and Rykoff, E. S. and Sako, M. and Sanchez, E. and Santiago, B. and Scarpine, V. and Sevilla-Noarbe, I. and Soares-Santos, M. and Suchyta, E. and Tarle, G. and Thaler, J. and Thomas, D. and Walker, A. and Zhang, Y. and Brownstein, J.},
abstractNote = {We present the results of the first test plates of the extended Baryon Oscillation Spectroscopic Survey. This paper focuses on the emission line galaxies (ELG) population targetted from the Dark Energy Survey (DES) photometry. We analyse the success rate, efficiency, redshift distribution, and clustering properties of the targets. From the 9000 spectroscopic redshifts targetted, 4600 have been selected from the DES photometry. The total success rate for redshifts between 0.6 and 1.2 is 71\% and 68\% respectively for a bright and faint, on average more distant, samples including redshifts measured from a single strong emission line. We find a mean redshift of 0.8 and 0.87, with 15 and 13\% of unknown redshifts respectively for the bright and faint samples. In the redshift range 0.6<1.2, for the most secure spectroscopic redshifts, the mean redshift for the bright and faint sample is 0.85 and 0.9 respectively. Star contamination is lower than 2\%. We measure a galaxy bias averaged on scales of 1 and 10~Mpc/h of 1.72 \pm 0.1 for the bright sample and of 1.78 \pm 0.12 for the faint sample. The error on the galaxy bias have been obtained propagating the errors in the correlation function to the fitted parameters. This redshift evolution for the galaxy bias is in agreement with theoretical expectations for a galaxy population with MB-5\log h < -21.0. We note that biasing is derived from the galaxy clustering relative to a model for the mass fluctuations. We investigate the quality of the DES photometric redshifts and find that the outlier fraction can be reduced using a comparison between template fitting and neural network, or using a random forest algorithm.},
doi = {10.1093/mnras/stx163},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 469,
place = {United States},
year = {Fri Mar 24 00:00:00 EDT 2017},
month = {Fri Mar 24 00:00:00 EDT 2017}
}
Web of Science
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