VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019)

D. Brout; D. Scolnic; R. Kessler; C. B. D'Andrea; T. M. Davis; R. R. Gupta; S. R. Hinton; A. G. Kim; J. Lasker; C. Lidman; E. Macaulay; A. Moller; R. C. Nichol; M. Sako; M. Smith; M. Sullivan; B. Zhang; P. Andersen; J. Asorey; A. Avelino; B. A. Bassett; P. Brown; J. Calcino; D. Carollo; P. Challis; M. Childress; A. Clocchiatti; A. V. Filippenko; R. J. Foley; L. Galbany; K. Glazebrook; J. K. Hoormann; E. Kasai; R. P. Kirshner; K. Kuehn; S. Kuhlmann; G. F. Lewis; K. S. Mandel; M. March; V. Miranda; E. Morganson; D. Muthukrishna; P. Nugent; A. Palmese; Y. -C. Pan; R. Sharp; N. E. Sommer; E. Swann; R. C. Thomas; B. E. Tucker; S. A. Uddin; W. Wester; T. M. C. Abbott; S. Allam; J. Annis; S. Avila; K. Bechtol; G. M. Bernstein; E. Bertin; D. Brooks; D. L. Burke; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; F. J. Castander; C. E. Cunha; L. N. da Costa; C. Davis; Vicente J. de; D. L. Depoy; S. Desai; H. T. Diehl; P. Doel; A. Drlica-Wagner; T. F. Eifler; J. Estrada; E. Fernandez; B. Flaugher; P. Fosalba; J. ! Frieman; J. Garcia-Bellido; D. Gruen; R. A. Gruendl; G. Gutierrez; W. G. Hartley; D. L. Hollowood; K. Honscheid; B. Hoyle; D. J. James; M. Jarvis; T. Jeltema; E. Krause; O. Lahav; T. S. Li; M. Lima; M. A. G. Maia; J. Marriner; J. L. Marshall; P. Martini; F. Menanteau; C. J. Miller; R. Miquel; R. L. C. Ogando; A. A. Plazas; A. K. Romer; A. Roodman; E. S. Rykoff; E. Sanchez; B. Santiago; V. Scarpine; M. Schubnell; S. Serrano; I. Sevilla-Noarbe; R. C. Smith; M. Soares-Santos; F. Sobreira; E. Suchyta; M. E. C. Swanson; G. Tarle; D. Thomas; M. A. Troxel; D. L. Tucker; V. Vikram; A. R. Walker; Y. Zhang

doi:10.26093/cds/vizier.18740150

VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019)

D. Brout, D. Scolnic, R. Kessler, C. B. D'Andrea, T. M. Davis, R. R. Gupta, S. R. Hinton, A. G. Kim, J. Lasker, C. Lidman, E. Macaulay, A. Moller, R. C. Nichol, M. Sako, M. Smith, M. Sullivan, B. Zhang, P. Andersen, J. Asorey, A. AvelinoB. A. Bassett, P. Brown, J. Calcino, D. Carollo, P. Challis, M. Childress, A. Clocchiatti, A. V. Filippenko, R. J. Foley, L. Galbany, K. Glazebrook, J. K. Hoormann, E. Kasai, R. P. Kirshner, K. Kuehn, S. Kuhlmann, G. F. Lewis, K. S. Mandel, M. March, V. Miranda, E. Morganson, D. Muthukrishna, P. Nugent, A. Palmese, Y. -C. Pan, R. Sharp, N. E. Sommer, E. Swann, R. C. Thomas, B. E. Tucker, S. A. Uddin, W. Wester, T. M. C. Abbott, S. Allam, J. Annis, S. Avila, K. Bechtol, G. M. Bernstein, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, C. E. Cunha, L. N. da Costa, C. Davis, Vicente J. de, D. L. Depoy, S. Desai, H. T. Diehl, P. Doel, A. Drlica-Wagner, T. F. Eifler, J. Estrada, E. Fernandez, B. Flaugher, P. Fosalba, J. ! Frieman, J. Garcia-Bellido, D. Gruen, R. A. Gruendl, G. Gutierrez, W. G. Hartley, D. L. Hollowood, K. Honscheid, B. Hoyle, D. J. James, M. Jarvis, T. Jeltema, E. Krause, O. Lahav, T. S. Li, M. Lima, M. A. G. Maia, J. Marriner, J. L. Marshall, P. Martini, F. Menanteau, C. J. Miller, R. Miquel, R. L. C. Ogando, A. A. Plazas, A. K. Romer, A. Roodman, E. S. Rykoff, E. Sanchez, B. Santiago, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, M. A. Troxel, D. L. Tucker, V. Vikram, A. R. Walker, Y. Zhang

Research output: Other contribution

Abstract

The Dark Energy Survey Supernova Program (DES-SN) performed a deep, time-domain survey in four optical bands (g, r, i, z) covering ~27deg² over five seasons (2013-2018) using the DECam mounted on the 4m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO).

A detailed overview of the spectroscopic follow-up program as well as a general overview of the DES-SN program and observing strategy can be found in D'Andrea et al. (2018, arXiv:1811.09565).

Over the first 3 years of DES-SN, from 2013 September to 2016 February, we discovered roughly ~12000 candidates of which ~2000 are likely SNe Ia. In this first analysis we analyze only the spectroscopically confirmed SN Ia subset of the data. The majority of spectra come from the Anglo-Australian Telescope (AAT) as part of the OzDES program (Yuan+ 2015MNRAS.452.3047Y & Childress+ 2017, J/MNRAS/472/273).

We also utilize four publicly available low-redshift surveys ("LOWz" subset): CfA3S (CfA3 Shooter), CfA3K (CfA3 KeplerCam), CfA4, and CSP-1 (Jha+ 2006, J/AJ/131/527; Hicken+ 2009, J/ApJ/700/1097 and 2012, J/ApJS/200/12; Contreras+ 2010, J/AJ/139/519), consisting of 303 spectroscopically confirmed SNe Ia in the redshift range 0.01(2 data files).

Original language	English
Publisher	American Astronomical Society
DOIs	https://doi.org/10.26093/cds/vizier.18740150
Publication status	Published - 1 Aug 2020

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10.26093/cds/vizier.18740150

https://ui.adsabs.harvard.edu/abs/2020yCat..18740150B

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Brout, D., Scolnic, D., Kessler, R., D'Andrea, C. B., Davis, T. M., Gupta, R. R., Hinton, S. R., Kim, A. G., Lasker, J., Lidman, C., Macaulay, E., Moller, A., Nichol, R. C., Sako, M., Smith, M., Sullivan, M., Zhang, B., Andersen, P., Asorey, J., ... Zhang, Y. (2020, Aug 1). VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019). American Astronomical Society. https://doi.org/10.26093/cds/vizier.18740150

@misc{52409aee57ef4ab3a0d4eb13d46cff26,

title = "VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019)",

abstract = "The Dark Energy Survey Supernova Program (DES-SN) performed a deep, time-domain survey in four optical bands (g, r, i, z) covering ~27deg2 over five seasons (2013-2018) using the DECam mounted on the 4m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO). A detailed overview of the spectroscopic follow-up program as well as a general overview of the DES-SN program and observing strategy can be found in D'Andrea et al. (2018, arXiv:1811.09565). Over the first 3 years of DES-SN, from 2013 September to 2016 February, we discovered roughly ~12000 candidates of which ~2000 are likely SNe Ia. In this first analysis we analyze only the spectroscopically confirmed SN Ia subset of the data. The majority of spectra come from the Anglo-Australian Telescope (AAT) as part of the OzDES program (Yuan+ 2015MNRAS.452.3047Y & Childress+ 2017, J/MNRAS/472/273). We also utilize four publicly available low-redshift surveys ({"}LOWz{"} subset): CfA3S (CfA3 Shooter), CfA3K (CfA3 KeplerCam), CfA4, and CSP-1 (Jha+ 2006, J/AJ/131/527; Hicken+ 2009, J/ApJ/700/1097 and 2012, J/ApJS/200/12; Contreras+ 2010, J/AJ/139/519), consisting of 303 spectroscopically confirmed SNe Ia in the redshift range 0.01(2 data files).",

keywords = "Supernovae, Surveys, Redshifts, Photometry: RI",

author = "D. Brout and D. Scolnic and R. Kessler and D'Andrea, {C. B.} and Davis, {T. M.} and Gupta, {R. R.} and Hinton, {S. R.} and Kim, {A. G.} and J. Lasker and C. Lidman and E. Macaulay and A. Moller and Nichol, {R. C.} and M. Sako and M. Smith and M. Sullivan and B. Zhang and P. Andersen and J. Asorey and A. Avelino and Bassett, {B. A.} and P. Brown and J. Calcino and D. Carollo and P. Challis and M. Childress and A. Clocchiatti and Filippenko, {A. V.} and Foley, {R. J.} and L. Galbany and K. Glazebrook and Hoormann, {J. K.} and E. Kasai and Kirshner, {R. P.} and K. Kuehn and S. Kuhlmann and Lewis, {G. F.} and Mandel, {K. S.} and M. March and V. Miranda and E. Morganson and D. Muthukrishna and P. Nugent and A. Palmese and Pan, {Y. -C.} and R. Sharp and Sommer, {N. E.} and E. Swann and Thomas, {R. C.} and Tucker, {B. E.} and Uddin, {S. A.} and W. Wester and Abbott, {T. M. C.} and S. Allam and J. Annis and S. Avila and K. Bechtol and Bernstein, {G. M.} and E. Bertin and D. Brooks and Burke, {D. L.} and {Carnero Rosell}, A. and {Carrasco Kind}, M. and J. Carretero and Castander, {F. J.} and Cunha, {C. E.} and {da Costa}, {L. N.} and C. Davis and de, {Vicente J.} and Depoy, {D. L.} and S. Desai and Diehl, {H. T.} and P. Doel and A. Drlica-Wagner and Eifler, {T. F.} and J. Estrada and E. Fernandez and B. Flaugher and P. Fosalba and {! Frieman}, J. and J. Garcia-Bellido and D. Gruen and Gruendl, {R. A.} and G. Gutierrez and Hartley, {W. G.} and Hollowood, {D. L.} and K. Honscheid and B. Hoyle and James, {D. J.} and M. Jarvis and T. Jeltema and E. Krause and O. Lahav and Li, {T. S.} and M. Lima and Maia, {M. A. G.} and J. Marriner and Marshall, {J. L.} and P. Martini and F. Menanteau and Miller, {C. J.} and R. Miquel and Ogando, {R. L. C.} and Plazas, {A. A.} and Romer, {A. K.} and A. Roodman and Rykoff, {E. S.} and E. Sanchez and B. Santiago and V. Scarpine and M. Schubnell and S. Serrano 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 D. Thomas and Troxel, {M. A.} and Tucker, {D. L.} and V. Vikram and Walker, {A. R.} and Y. Zhang",

year = "2020",

month = aug,

day = "1",

doi = "10.26093/cds/vizier.18740150",

language = "English",

publisher = "American Astronomical Society",

address = "United States",

type = "Other",

}

Brout, D, Scolnic, D, Kessler, R, D'Andrea, CB, Davis, TM, Gupta, RR, Hinton, SR, Kim, AG, Lasker, J, Lidman, C, Macaulay, E, Moller, A, Nichol, RC, Sako, M, Smith, M, Sullivan, M, Zhang, B, Andersen, P, Asorey, J, Avelino, A, Bassett, BA, Brown, P, Calcino, J, Carollo, D, Challis, P, Childress, M, Clocchiatti, A, Filippenko, AV, Foley, RJ, Galbany, L, Glazebrook, K, Hoormann, JK, Kasai, E, Kirshner, RP, Kuehn, K, Kuhlmann, S, Lewis, GF, Mandel, KS, March, M, Miranda, V, Morganson, E, Muthukrishna, D, Nugent, P, Palmese, A, Pan, Y-C, Sharp, R, Sommer, NE, Swann, E, Thomas, RC, Tucker, BE, Uddin, SA, Wester, W, Abbott, TMC, Allam, S, Annis, J, Avila, S, Bechtol, K, Bernstein, GM, Bertin, E, Brooks, D, Burke, DL, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, FJ, Cunha, CE, da Costa, LN, Davis, C, de, VJ, Depoy, DL, Desai, S, Diehl, HT, Doel, P, Drlica-Wagner, A, Eifler, TF, Estrada, J, Fernandez, E, Flaugher, B, Fosalba, P, ! Frieman, J, Garcia-Bellido, J, Gruen, D, Gruendl, RA, Gutierrez, G, Hartley, WG, Hollowood, DL, Honscheid, K, Hoyle, B, James, DJ, Jarvis, M, Jeltema, T, Krause, E, Lahav, O, Li, TS, Lima, M, Maia, MAG, Marriner, J, Marshall, JL, Martini, P, Menanteau, F, Miller, CJ, Miquel, R, Ogando, RLC, Plazas, AA, Romer, AK, Roodman, A, Rykoff, ES, Sanchez, E, Santiago, B, Scarpine, V, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Smith, RC, Soares-Santos, M, Sobreira, F, Suchyta, E, Swanson, MEC, Tarle, G, Thomas, D, Troxel, MA, Tucker, DL, Vikram, V, Walker, AR & Zhang, Y 2020, VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019). American Astronomical Society. https://doi.org/10.26093/cds/vizier.18740150

TY - GEN

T1 - VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019)

AU - Brout, D.

AU - Scolnic, D.

AU - Kessler, R.

AU - D'Andrea, C. B.

AU - Davis, T. M.

AU - Gupta, R. R.

AU - Hinton, S. R.

AU - Kim, A. G.

AU - Lasker, J.

AU - Lidman, C.

AU - Macaulay, E.

AU - Moller, A.

AU - Nichol, R. C.

AU - Sako, M.

AU - Smith, M.

AU - Sullivan, M.

AU - Zhang, B.

AU - Andersen, P.

AU - Asorey, J.

AU - Avelino, A.

AU - Bassett, B. A.

AU - Brown, P.

AU - Calcino, J.

AU - Carollo, D.

AU - Challis, P.

AU - Childress, M.

AU - Clocchiatti, A.

AU - Filippenko, A. V.

AU - Foley, R. J.

AU - Galbany, L.

AU - Glazebrook, K.

AU - Hoormann, J. K.

AU - Kasai, E.

AU - Kirshner, R. P.

AU - Kuehn, K.

AU - Kuhlmann, S.

AU - Lewis, G. F.

AU - Mandel, K. S.

AU - March, M.

AU - Miranda, V.

AU - Morganson, E.

AU - Muthukrishna, D.

AU - Nugent, P.

AU - Palmese, A.

AU - Pan, Y. -C.

AU - Sharp, R.

AU - Sommer, N. E.

AU - Swann, E.

AU - Thomas, R. C.

AU - Tucker, B. E.

AU - Uddin, S. A.

AU - Wester, W.

AU - Abbott, T. M. C.

AU - Allam, S.

AU - Annis, J.

AU - Avila, S.

AU - Bechtol, K.

AU - Bernstein, G. M.

AU - Bertin, E.

AU - Brooks, D.

AU - Burke, D. L.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Castander, F. J.

AU - Cunha, C. E.

AU - da Costa, L. N.

AU - Davis, C.

AU - de, Vicente J.

AU - Depoy, D. L.

AU - Desai, S.

AU - Diehl, H. T.

AU - Doel, P.

AU - Drlica-Wagner, A.

AU - Eifler, T. F.

AU - Estrada, J.

AU - Fernandez, E.

AU - Flaugher, B.

AU - Fosalba, P.

AU - ! Frieman, J.

AU - Garcia-Bellido, J.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gutierrez, G.

AU - Hartley, W. G.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - Hoyle, B.

AU - James, D. J.

AU - Jarvis, M.

AU - Jeltema, T.

AU - Krause, E.

AU - Lahav, O.

AU - Li, T. S.

AU - Lima, M.

AU - Maia, M. A. G.

AU - Marriner, J.

AU - Marshall, J. L.

AU - Martini, P.

AU - Menanteau, F.

AU - Miller, C. J.

AU - Miquel, R.

AU - Ogando, R. L. C.

AU - Plazas, A. A.

AU - Romer, A. K.

AU - Roodman, A.

AU - Rykoff, E. S.

AU - Sanchez, E.

AU - Santiago, B.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Serrano, S.

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 - Thomas, D.

AU - Troxel, M. A.

AU - Tucker, D. L.

AU - Vikram, V.

AU - Walker, A. R.

AU - Zhang, Y.

PY - 2020/8/1

Y1 - 2020/8/1

N2 - The Dark Energy Survey Supernova Program (DES-SN) performed a deep, time-domain survey in four optical bands (g, r, i, z) covering ~27deg2 over five seasons (2013-2018) using the DECam mounted on the 4m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO). A detailed overview of the spectroscopic follow-up program as well as a general overview of the DES-SN program and observing strategy can be found in D'Andrea et al. (2018, arXiv:1811.09565). Over the first 3 years of DES-SN, from 2013 September to 2016 February, we discovered roughly ~12000 candidates of which ~2000 are likely SNe Ia. In this first analysis we analyze only the spectroscopically confirmed SN Ia subset of the data. The majority of spectra come from the Anglo-Australian Telescope (AAT) as part of the OzDES program (Yuan+ 2015MNRAS.452.3047Y & Childress+ 2017, J/MNRAS/472/273). We also utilize four publicly available low-redshift surveys ("LOWz" subset): CfA3S (CfA3 Shooter), CfA3K (CfA3 KeplerCam), CfA4, and CSP-1 (Jha+ 2006, J/AJ/131/527; Hicken+ 2009, J/ApJ/700/1097 and 2012, J/ApJS/200/12; Contreras+ 2010, J/AJ/139/519), consisting of 303 spectroscopically confirmed SNe Ia in the redshift range 0.01(2 data files).

AB - The Dark Energy Survey Supernova Program (DES-SN) performed a deep, time-domain survey in four optical bands (g, r, i, z) covering ~27deg2 over five seasons (2013-2018) using the DECam mounted on the 4m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO). A detailed overview of the spectroscopic follow-up program as well as a general overview of the DES-SN program and observing strategy can be found in D'Andrea et al. (2018, arXiv:1811.09565). Over the first 3 years of DES-SN, from 2013 September to 2016 February, we discovered roughly ~12000 candidates of which ~2000 are likely SNe Ia. In this first analysis we analyze only the spectroscopically confirmed SN Ia subset of the data. The majority of spectra come from the Anglo-Australian Telescope (AAT) as part of the OzDES program (Yuan+ 2015MNRAS.452.3047Y & Childress+ 2017, J/MNRAS/472/273). We also utilize four publicly available low-redshift surveys ("LOWz" subset): CfA3S (CfA3 Shooter), CfA3K (CfA3 KeplerCam), CfA4, and CSP-1 (Jha+ 2006, J/AJ/131/527; Hicken+ 2009, J/ApJ/700/1097 and 2012, J/ApJS/200/12; Contreras+ 2010, J/AJ/139/519), consisting of 303 spectroscopically confirmed SNe Ia in the redshift range 0.01(2 data files).

KW - Supernovae

KW - Surveys

KW - Redshifts

KW - Photometry: RI

U2 - 10.26093/cds/vizier.18740150

DO - 10.26093/cds/vizier.18740150

M3 - Other contribution

PB - American Astronomical Society

ER -

VizieR Online Data Catalog: The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019)

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