Final published version
Licence: CC BY: Creative Commons Attribution 4.0 International License
Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
}
TY - JOUR
T1 - The Dark Energy Survey Supernova Program
T2 - Light Curves and 5 Yr Data Release
AU - Sánchez, B. O.
AU - Brout, D.
AU - Vincenzi, M.
AU - Sako, M.
AU - Herner, K.
AU - Kessler, R.
AU - Davis, T. M.
AU - Scolnic, D.
AU - Acevedo, M.
AU - Lee, J.
AU - Möller, A.
AU - Qu, H.
AU - Kelsey, L.
AU - Wiseman, P.
AU - Armstrong, P.
AU - Rose, B.
AU - Camilleri, R.
AU - Chen, R.
AU - Galbany, L.
AU - Kovacs, E.
AU - Lidman, C.
AU - Popovic, B.
AU - Smith, M.
AU - Shah, P.
AU - Sullivan, M.
AU - Toy, M.
AU - Abbott, T. M. C.
AU - Aguena, M.
AU - Allam, S.
AU - Alves, O.
AU - Annis, J.
AU - Asorey, J.
AU - Avila, S.
AU - Bacon, D.
AU - Brooks, D.
AU - Burke, D. L.
AU - Carnero Rosell, A.
AU - Carollo, D.
AU - Carretero, J.
AU - da Costa, L. N.
AU - Castander, F. J.
AU - Desai, S.
AU - Diehl, H. T.
AU - Duarte, J.
AU - Everett, S.
AU - Ferrero, I.
AU - Flaugher, B.
AU - Frieman, J.
AU - García-Bellido, J.
AU - Gatti, M.
AU - Gaztanaga, E.
AU - Giannini, G.
AU - Glazebrook, K.
AU - González-Gaitán, S.
AU - Gruendl, R. A.
AU - Gutierrez, G.
AU - Hinton, S. R.
AU - Hollowood, D. L.
AU - Honscheid, K.
AU - James, D. J.
AU - Kuehn, K.
AU - Lahav, O.
AU - Lee, S.
AU - Lewis, G. F.
AU - Lin, H.
AU - Marshall, J. L.
AU - Mena-Fernández, J.
AU - Miquel, R.
AU - Myles, J.
AU - Nichol, R. C.
AU - Ogando, R. L. C.
AU - Palmese, A.
AU - Pereira, M. E. S.
AU - Pieres, A.
AU - Malagón, A. A. Plazas
AU - Porredon, A.
AU - Romer, A. K.
AU - Sanchez, E.
AU - Sanchez Cid, D.
AU - Sevilla-Noarbe, I.
AU - Suchyta, E.
AU - Swanson, M. E. C.
AU - Tarle, G.
AU - Tucker, B. E.
AU - Tucker, D. L.
AU - Vikram, V.
AU - Walker, A. R.
AU - Weaverdyck, N.
PY - 2024/11/1
Y1 - 2024/11/1
N2 - We present griz photometric light curves for the full 5 yr of the Dark Energy Survey Supernova (DES-SN) program, obtained with both forced point-spread function photometry on difference images (DiffImg) performed during survey operations, and scene modelling photometry (SMP) on search images processed after the survey. This release contains 31,636 DiffImg and 19,706 high-quality SMP light curves, the latter of which contain 1635 photometrically classified SNe that pass cosmology quality cuts. This sample spans the largest redshift (z) range ever covered by a single SN survey (0.1 < z < 1.13) and is the largest single sample from a single instrument of SNe ever used for cosmological constraints. We describe in detail the improvements made to obtain the final DES-SN photometry and provide a comparison to what was used in the 3 yr DES-SN spectroscopically confirmed Type Ia SN sample. We also include a comparative analysis of the performance of the SMP photometry with respect to the real-time DiffImg forced photometry and find that SMP photometry is more precise, more accurate, and less sensitive to the host-galaxy surface brightness anomaly. The public release of the light curves and ancillary data can be found at github.com/des-science/DES-SN5YR and doi:10.5281/zenodo.12720777.
AB - We present griz photometric light curves for the full 5 yr of the Dark Energy Survey Supernova (DES-SN) program, obtained with both forced point-spread function photometry on difference images (DiffImg) performed during survey operations, and scene modelling photometry (SMP) on search images processed after the survey. This release contains 31,636 DiffImg and 19,706 high-quality SMP light curves, the latter of which contain 1635 photometrically classified SNe that pass cosmology quality cuts. This sample spans the largest redshift (z) range ever covered by a single SN survey (0.1 < z < 1.13) and is the largest single sample from a single instrument of SNe ever used for cosmological constraints. We describe in detail the improvements made to obtain the final DES-SN photometry and provide a comparison to what was used in the 3 yr DES-SN spectroscopically confirmed Type Ia SN sample. We also include a comparative analysis of the performance of the SMP photometry with respect to the real-time DiffImg forced photometry and find that SMP photometry is more precise, more accurate, and less sensitive to the host-galaxy surface brightness anomaly. The public release of the light curves and ancillary data can be found at github.com/des-science/DES-SN5YR and doi:10.5281/zenodo.12720777.
KW - Cosmology
KW - Type Ia supernovae
KW - Dark energy
U2 - 10.3847/1538-4357/ad739a
DO - 10.3847/1538-4357/ad739a
M3 - Journal article
VL - 975
JO - The Astrophysical Journal
JF - The Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 5
ER -