Discovery of two gravitationally lensed quasars in the Dark Energy Survey

A. Agnello; T. Treu; F. Ostrovski; P. L. Schechter; E. J. Buckley-Geer; H. Lin; M. W. Auger; F. Courbin; C. D. Fassnacht; J. Frieman; N. Kuropatkin; P. J. Marshall; R. G. McMahon; G. Meylan; A. More; S. H. Suyu; C. E. Rusu; D. Finley; T. Abbott; F. B. Abdalla; S. Allam; J. Annis; M. Banerji; A. Benoit-Lévy; E. Bertin; D. Brooks; D. L. Burke; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; C. E. Cunha; C. B. D'Andrea; L. N. da Costa; S. Desai; H. T. Diehl; J. P. Dietrich; P. Doel; T. F. Eifler; J. Estrada; A. Fausti Neto; B. Flaugher; P. Fosalba; D. W. Gerdes; D. Gruen; G. Gutierrez; K. Honscheid; D. J. James; K. Kuehn; O. Lahav; M. Lima; M. A.G. Maia; M. March; J. L. Marshall; P. Martini; P. Melchior; C. J. Miller; R. Miquel; R. C. Nichol; R. Ogando; A. A. Plazas; K. Reil; A. K. Romer; A. Roodman; M. Sako; E. Sanchez; B. Santiago; V. Scarpine; M. Schubnell; I. Sevilla-Noarbe; R. C. Smith; M. Soares-Santos; F. Sobreira; E. Suchyta; M. E.C. Swanson; G. Tarle; J. Thaler; D. Tucker; A. R. Walker; R. H. Wechsler; Y. Zhang

doi:10.1093/mnras/stv2171

Discovery of two gravitationally lensed quasars in the Dark Energy Survey

A. Agnello
, T. Treu
, F. Ostrovski
, P. L. Schechter
, E. J. Buckley-Geer
, H. Lin
, M. W. Auger
, F. Courbin
, C. D. Fassnacht
, J. Frieman
, N. Kuropatkin
, P. J. Marshall
, R. G. McMahon
, G. Meylan
, A. More
, S. H. Suyu
, C. E. Rusu
, D. Finley
, T. Abbott
, F. B. Abdalla

S. Allam, J. Annis, M. Banerji, A. Benoit-Lévy, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, C. E. Cunha, C. B. D'Andrea, L. N. da Costa, S. Desai, H. T. Diehl, J. P. Dietrich, P. Doel, T. F. Eifler, J. Estrada, A. Fausti Neto, B. Flaugher, P. Fosalba, D. W. Gerdes, D. Gruen, G. Gutierrez, K. Honscheid, D. J. James, K. Kuehn, O. Lahav, M. Lima, M. A.G. Maia, M. March, J. L. Marshall, P. Martini, P. Melchior, C. J. Miller, R. Miquel, R. C. Nichol, R. Ogando, A. A. Plazas, K. Reil, A. K. Romer, A. Roodman, M. Sako, E. Sanchez, B. Santiago, V. Scarpine, M. Schubnell, I. Sevilla-Noarbe, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E.C. Swanson, G. Tarle, J. Thaler, D. Tucker, A. R. Walker, R. H. Wechsler, Y. Zhang

University of California at Los Angeles
Institute of Astronomy
University of Cambridge
Ministry of Education of Brazil
MIT Kavli Institute for Astrophysics and Space Research
Fermi National Accelerator Laboratory
École Polytechnique Fédérale de Lausanne (EPFL)
University of California, Davis
Stanford University
University of Tokyo
Academia Sinica, Institute of Astronomy and Astrophysics
National Optical Astronomy Observatory
University College London
Institut d'Astrophysique de Paris
Centre de Recherche Institut du Cerveau et de la Moelle
Laboratório Interinstitucional de e-Astronomia
Observatório Nacional
University of Illinois
CSIC/UPC
Universitat Autònoma de Barcelona (UAB)
University of Portsmouth
Cluster of Excellence E-conversion
Ludwig-Maximilians-Universität München
University of Pennsylvania
Jet Propulsion Laboratory
University of Michigan, Ann Arbor
Max-Planck-Institut
Ohio State University
Australian Astronomical Observatory
University of São Paulo
Texas A and M University
Technology Department
University of Sussex
CIEMAT Energy Department
UFRGS

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

42 Scopus citations

Abstract

We present spectroscopic confirmation of two new gravitationally lensed quasars, discovered in the Dark Energy Survey (DES) and Wide-field Infrared Survey Explorer (WISE) based on their multiband photometry and extended morphology in DES images. Images of DES J0115-5244 show a red galaxy with two blue point sources at either side, which are images of the same quasar at z_s = 1.64 as obtained by our long-slit spectroscopic data. The Einstein radius estimated from the DES images is 0.51 arcsec. DES J2146-0047 is in the area of overlap between DES and the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fibre spectrum shows a quasar component at z_s = 2.38 and absorption by Mg II and Fe II at z_l = 0.799, which we tentatively associate with the foreground lens galaxy. Our long-slit spectra show that the blue components are resolved images of the same quasar. The Einstein radius is 0.68 arcsec, corresponding to an enclosed mass of 1.6 × 10¹¹M_⊙. Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data mining and model-based selection that is being applied to the entire DES data set.

Original language	English
Pages (from-to)	1260-1265
Number of pages	6
Journal	Monthly Notices of the Royal Astronomical Society
Volume	454
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stv2171
State	Published - 2015
Externally published	Yes

Keywords

Quasars: emission lines
gravitational lensing: strong -methods: observational -methods: statistical

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10.1093/mnras/stv2171

Cite this

Agnello, A., Treu, T., Ostrovski, F., Schechter, P. L., Buckley-Geer, E. J., Lin, H., Auger, M. W., Courbin, F., Fassnacht, C. D., Frieman, J., Kuropatkin, N., Marshall, P. J., McMahon, R. G., Meylan, G., More, A., Suyu, S. H., Rusu, C. E., Finley, D., Abbott, T., ... Zhang, Y. (2015). Discovery of two gravitationally lensed quasars in the Dark Energy Survey. Monthly Notices of the Royal Astronomical Society, 454(2), 1260-1265. https://doi.org/10.1093/mnras/stv2171

@article{35b588a5d3de44b8b91b87657a54963d,

title = "Discovery of two gravitationally lensed quasars in the Dark Energy Survey",

abstract = "We present spectroscopic confirmation of two new gravitationally lensed quasars, discovered in the Dark Energy Survey (DES) and Wide-field Infrared Survey Explorer (WISE) based on their multiband photometry and extended morphology in DES images. Images of DES J0115-5244 show a red galaxy with two blue point sources at either side, which are images of the same quasar at zs = 1.64 as obtained by our long-slit spectroscopic data. The Einstein radius estimated from the DES images is 0.51 arcsec. DES J2146-0047 is in the area of overlap between DES and the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fibre spectrum shows a quasar component at zs = 2.38 and absorption by Mg II and Fe II at zl = 0.799, which we tentatively associate with the foreground lens galaxy. Our long-slit spectra show that the blue components are resolved images of the same quasar. The Einstein radius is 0.68 arcsec, corresponding to an enclosed mass of 1.6 × 1011M⊙. Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data mining and model-based selection that is being applied to the entire DES data set.",

keywords = "Quasars: emission lines, gravitational lensing: strong -methods: observational -methods: statistical",

author = "A. Agnello and T. Treu and F. Ostrovski and Schechter, \{P. L.\} and Buckley-Geer, \{E. J.\} and H. Lin and Auger, \{M. W.\} and F. Courbin and Fassnacht, \{C. D.\} and J. Frieman and N. Kuropatkin and Marshall, \{P. J.\} and McMahon, \{R. G.\} and G. Meylan and A. More and Suyu, \{S. H.\} and Rusu, \{C. E.\} and D. Finley and T. Abbott and Abdalla, \{F. B.\} and S. Allam and J. Annis and M. Banerji and A. Benoit-L{\'e}vy and E. Bertin and D. Brooks and Burke, \{D. L.\} and \{Carnero Rosell\}, A. and \{Carrasco Kind\}, M. and J. Carretero and Cunha, \{C. E.\} and D'Andrea, \{C. B.\} and \{da Costa\}, \{L. N.\} and S. Desai and Diehl, \{H. T.\} and Dietrich, \{J. P.\} and P. Doel and Eifler, \{T. F.\} and J. Estrada and \{Fausti Neto\}, A. and B. Flaugher and P. Fosalba and Gerdes, \{D. W.\} and D. Gruen and G. Gutierrez and K. Honscheid and James, \{D. J.\} and K. Kuehn and O. Lahav and M. Lima and Maia, \{M. A.G.\} and M. March and Marshall, \{J. L.\} and P. Martini and P. Melchior and Miller, \{C. J.\} and R. Miquel and Nichol, \{R. C.\} and R. Ogando and Plazas, \{A. A.\} and K. Reil and Romer, \{A. K.\} and A. Roodman and M. Sako and E. Sanchez and B. Santiago and V. Scarpine and M. Schubnell and I. Sevilla-Noarbe and Smith, \{R. C.\} and M. Soares-Santos and F. Sobreira and E. Suchyta and Swanson, \{M. E.C.\} and G. Tarle and J. Thaler and D. Tucker and Walker, \{A. R.\} and Wechsler, \{R. H.\} and Y. Zhang",

note = "Publisher Copyright: {\textcopyright} 2015 The Authors.",

year = "2015",

doi = "10.1093/mnras/stv2171",

language = "English",

volume = "454",

pages = "1260--1265",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

}

Agnello, A, Treu, T, Ostrovski, F, Schechter, PL, Buckley-Geer, EJ, Lin, H, Auger, MW, Courbin, F, Fassnacht, CD, Frieman, J, Kuropatkin, N, Marshall, PJ, McMahon, RG, Meylan, G, More, A, Suyu, SH, Rusu, CE, Finley, D, Abbott, T, Abdalla, FB, Allam, S, Annis, J, Banerji, M, Benoit-Lévy, A, Bertin, E, Brooks, D, Burke, DL, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Cunha, CE, D'Andrea, CB, da Costa, LN, Desai, S, Diehl, HT, Dietrich, JP, Doel, P, Eifler, TF, Estrada, J, Fausti Neto, A, Flaugher, B, Fosalba, P, Gerdes, DW, Gruen, D, Gutierrez, G, Honscheid, K, James, DJ, Kuehn, K, Lahav, O, Lima, M, Maia, MAG, March, M, Marshall, JL, Martini, P, Melchior, P, Miller, CJ, Miquel, R, Nichol, RC, Ogando, R, Plazas, AA, Reil, K, Romer, AK, Roodman, A, Sako, M, Sanchez, E, Santiago, B, Scarpine, V, Schubnell, M, Sevilla-Noarbe, I, Smith, RC, Soares-Santos, M, Sobreira, F, Suchyta, E, Swanson, MEC, Tarle, G, Thaler, J, Tucker, D, Walker, AR, Wechsler, RH & Zhang, Y 2015, 'Discovery of two gravitationally lensed quasars in the Dark Energy Survey', Monthly Notices of the Royal Astronomical Society, vol. 454, no. 2, pp. 1260-1265. https://doi.org/10.1093/mnras/stv2171

TY - JOUR

T1 - Discovery of two gravitationally lensed quasars in the Dark Energy Survey

AU - Agnello, A.

AU - Treu, T.

AU - Ostrovski, F.

AU - Schechter, P. L.

AU - Buckley-Geer, E. J.

AU - Lin, H.

AU - Auger, M. W.

AU - Courbin, F.

AU - Fassnacht, C. D.

AU - Frieman, J.

AU - Kuropatkin, N.

AU - Marshall, P. J.

AU - McMahon, R. G.

AU - Meylan, G.

AU - More, A.

AU - Suyu, S. H.

AU - Rusu, C. E.

AU - Finley, D.

AU - Abbott, T.

AU - Abdalla, F. B.

AU - Allam, S.

AU - Annis, J.

AU - Banerji, M.

AU - Benoit-Lévy, A.

AU - Bertin, E.

AU - Brooks, D.

AU - Burke, D. L.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Cunha, C. E.

AU - D'Andrea, C. B.

AU - da Costa, L. N.

AU - Desai, S.

AU - Diehl, H. T.

AU - Dietrich, J. P.

AU - Doel, P.

AU - Eifler, T. F.

AU - Estrada, J.

AU - Fausti Neto, A.

AU - Flaugher, B.

AU - Fosalba, P.

AU - Gerdes, D. W.

AU - Gruen, D.

AU - Gutierrez, G.

AU - Honscheid, K.

AU - James, D. J.

AU - Kuehn, K.

AU - Lahav, O.

AU - Lima, M.

AU - Maia, M. A.G.

AU - March, M.

AU - Marshall, J. L.

AU - Martini, P.

AU - Melchior, P.

AU - Miller, C. J.

AU - Miquel, R.

AU - Nichol, R. C.

AU - Ogando, R.

AU - Plazas, A. A.

AU - Reil, K.

AU - Romer, A. K.

AU - Roodman, A.

AU - Sako, M.

AU - Sanchez, E.

AU - Santiago, B.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Sevilla-Noarbe, I.

AU - Smith, R. C.

AU - Soares-Santos, M.

AU - Sobreira, F.

AU - Suchyta, E.

AU - Swanson, M. E.C.

AU - Tarle, G.

AU - Thaler, J.

AU - Tucker, D.

AU - Walker, A. R.

AU - Wechsler, R. H.

AU - Zhang, Y.

PY - 2015

Y1 - 2015

N2 - We present spectroscopic confirmation of two new gravitationally lensed quasars, discovered in the Dark Energy Survey (DES) and Wide-field Infrared Survey Explorer (WISE) based on their multiband photometry and extended morphology in DES images. Images of DES J0115-5244 show a red galaxy with two blue point sources at either side, which are images of the same quasar at zs = 1.64 as obtained by our long-slit spectroscopic data. The Einstein radius estimated from the DES images is 0.51 arcsec. DES J2146-0047 is in the area of overlap between DES and the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fibre spectrum shows a quasar component at zs = 2.38 and absorption by Mg II and Fe II at zl = 0.799, which we tentatively associate with the foreground lens galaxy. Our long-slit spectra show that the blue components are resolved images of the same quasar. The Einstein radius is 0.68 arcsec, corresponding to an enclosed mass of 1.6 × 1011M⊙. Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data mining and model-based selection that is being applied to the entire DES data set.

AB - We present spectroscopic confirmation of two new gravitationally lensed quasars, discovered in the Dark Energy Survey (DES) and Wide-field Infrared Survey Explorer (WISE) based on their multiband photometry and extended morphology in DES images. Images of DES J0115-5244 show a red galaxy with two blue point sources at either side, which are images of the same quasar at zs = 1.64 as obtained by our long-slit spectroscopic data. The Einstein radius estimated from the DES images is 0.51 arcsec. DES J2146-0047 is in the area of overlap between DES and the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fibre spectrum shows a quasar component at zs = 2.38 and absorption by Mg II and Fe II at zl = 0.799, which we tentatively associate with the foreground lens galaxy. Our long-slit spectra show that the blue components are resolved images of the same quasar. The Einstein radius is 0.68 arcsec, corresponding to an enclosed mass of 1.6 × 1011M⊙. Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data mining and model-based selection that is being applied to the entire DES data set.

KW - Quasars: emission lines

KW - gravitational lensing: strong -methods: observational -methods: statistical

UR - https://www.scopus.com/pages/publications/85040225580

U2 - 10.1093/mnras/stv2171

DO - 10.1093/mnras/stv2171

M3 - Article

AN - SCOPUS:85040225580

SN - 0035-8711

VL - 454

SP - 1260

EP - 1265

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

Discovery of two gravitationally lensed quasars in the Dark Energy Survey

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Keywords

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