VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020)

P. Wiseman; M. Pursiainen; M. Childress; E. Swann; M. Smith; L. Galbany; C. Lidman; T. M. Davis; C. P. Gutierrez; A. Moller; B. P. Thomas; C. Frohmaier; R. J. Foley; S. R. Hinton; L. Kelsey; R. Kessler; G. F. Lewis; M. Sako; D. Scolnic; M. Sullivan; M. Vincenzi; T. M. C. Abbott; M. Aguena; S. Allam; J. Annis; E. Bertin; S. Bhargava; D. Brooks; D. L. Burke; A. Carnero Rosell; D. Carollo; M. Carrasco Kind; J. Carretero; M. Costanzi; L. N. da Costa; H. T. Diehl; P. Doel; S. Everett; P. Fosalba; J. Frieman; J. Garcia-Bellido; E. Gaztanaga; K. Glazebrook; D. Gruen; R. A. Gruendl; J. Gschwend; G. Gutierrez; D. L. Hollowood; K. Honscheid; D. J. James; K. Kuehn; N. Kuropatkin; M. Lima; M. A. G. Maia; J. L. Marshall; P. Martini; F. Menanteau; R. Miquel; A. Palmese; F. Paz-Chinchon; A. A. Plazas; A. K. Romer; E. Sanchez; V. Scarpine; M. Schubnell; S. Serrano; I. Sevilla-Noarbe; N. E. Sommer; E. Suchyta; M. E. C. Swanson; G. Tarle; B. E. Tucker; D. L. Tucker; T. N. Varga; A. R. Walker

VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020)

P. Wiseman, M. Pursiainen, M. Childress, E. Swann, M. Smith, L. Galbany, C. Lidman, T. M. Davis, C. P. Gutierrez, A. Moller, B. P. Thomas, C. Frohmaier, R. J. Foley, S. R. Hinton, L. Kelsey, R. Kessler, G. F. Lewis, M. Sako, D. Scolnic, M. SullivanM. Vincenzi, T. M. C. Abbott, M. Aguena, S. Allam, J. Annis, E. Bertin, S. Bhargava, D. Brooks, D. L. Burke, A. Carnero Rosell, D. Carollo, M. Carrasco Kind, J. Carretero, M. Costanzi, L. N. da Costa, H. T. Diehl, P. Doel, S. Everett, P. Fosalba, J. Frieman, J. Garcia-Bellido, E. Gaztanaga, K. Glazebrook, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, N. Kuropatkin, M. Lima, M. A. G. Maia, J. L. Marshall, P. Martini, F. Menanteau, R. Miquel, A. Palmese, F. Paz-Chinchon, A. A. Plazas, A. K. Romer, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, N. E. Sommer, E. Suchyta, M. E. C. Swanson, G. Tarle, B. E. Tucker, D. L. Tucker, T. N. Varga, A. R. Walker

Research School of Astronomy & Astrophysics

Research output: Other contribution

Abstract

Our sample of RETs comprises 106 events discovered in the 5-yr DES-SN transient survey. This number expands upon the 72 of Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) (P18). The first reason for the increased sample size is the use of the fifth year of DES-SN, as Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) were only able to make use of the first 4yr. By imposing the P18 selection criteria on season 5, the sample is increased to 92 objects. The second reason is an update to the sample selection technique, which adds a further 14 transients.

Of the 106 objects in the sample, 96 have a host galaxy detected in deep host galaxy photometry of Wiseman et al. (2020MNRAS.495.4040W) when using the directional light radius method (Sullivan et al. 2006ApJ...648..868S) to associate hosts as per Wiseman et al. (2020MNRAS.495.4040W). Of these, 49 have a host galaxy spectroscopic redshift which we access through an internal release of the OzDES Global Redshift Catalog (GRC; v.2020₀₁04). The full OzDES redshift catalogue will be available alongside the public data release detailed in Lidman et al. (2020MNRAS.496...19L).

We also obtained redshifts for some transient hosts serendipitously as part of the Looking at the Distant Universe with the MeerKAT Array (LADUMA) survey (http://www.laduma.uct.ac.za). Objects for which the host already had a publicly available redshift were not observed with OzDES, but merged into the GRC none the less. In total we analyse 45 spectra, with a mean continuum SNR of 2.56/pixel.

(3 data files).

Original language	English
Publication status	Published - 1 Aug 2023

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https://ui.adsabs.harvard.edu/abs/2023yCat..74982575W

Cite this

Wiseman, P., Pursiainen, M., Childress, M., Swann, E., Smith, M., Galbany, L., Lidman, C., Davis, T. M., Gutierrez, C. P., Moller, A., Thomas, B. P., Frohmaier, C., Foley, R. J., Hinton, S. R., Kelsey, L., Kessler, R., Lewis, G. F., Sako, M., Scolnic, D., ... Walker, A. R. (2023, Aug 1). VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020). https://ui.adsabs.harvard.edu/abs/2023yCat..74982575W

@misc{40f37b5ba7814f23be70740695a36d6d,

title = "VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020)",

abstract = "Our sample of RETs comprises 106 events discovered in the 5-yr DES-SN transient survey. This number expands upon the 72 of Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) (P18). The first reason for the increased sample size is the use of the fifth year of DES-SN, as Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) were only able to make use of the first 4yr. By imposing the P18 selection criteria on season 5, the sample is increased to 92 objects. The second reason is an update to the sample selection technique, which adds a further 14 transients. Of the 106 objects in the sample, 96 have a host galaxy detected in deep host galaxy photometry of Wiseman et al. (2020MNRAS.495.4040W) when using the directional light radius method (Sullivan et al. 2006ApJ...648..868S) to associate hosts as per Wiseman et al. (2020MNRAS.495.4040W). Of these, 49 have a host galaxy spectroscopic redshift which we access through an internal release of the OzDES Global Redshift Catalog (GRC; v.20200104). The full OzDES redshift catalogue will be available alongside the public data release detailed in Lidman et al. (2020MNRAS.496...19L). We also obtained redshifts for some transient hosts serendipitously as part of the Looking at the Distant Universe with the MeerKAT Array (LADUMA) survey (http://www.laduma.uct.ac.za). Objects for which the host already had a publicly available redshift were not observed with OzDES, but merged into the GRC none the less. In total we analyse 45 spectra, with a mean continuum SNR of 2.56/pixel. (3 data files).",

keywords = "Transient, Galaxies, Positional data, Redshifts, Abundances: peculiar, Spectra: optical",

author = "P. Wiseman and M. Pursiainen and M. Childress and E. Swann and M. Smith and L. Galbany and C. Lidman and Davis, \{T. M.\} and Gutierrez, \{C. P.\} and A. Moller and Thomas, \{B. P.\} and C. Frohmaier and Foley, \{R. J.\} and Hinton, \{S. R.\} and L. Kelsey and R. Kessler and Lewis, \{G. F.\} and M. Sako and D. Scolnic and M. Sullivan and M. Vincenzi and Abbott, \{T. M. C.\} and M. Aguena and S. Allam and J. Annis and E. Bertin and S. Bhargava and D. Brooks and Burke, \{D. L.\} and \{Carnero Rosell\}, A. and D. Carollo and \{Carrasco Kind\}, M. and J. Carretero and M. Costanzi and \{da Costa\}, \{L. N.\} and Diehl, \{H. T.\} and P. Doel and S. Everett and P. Fosalba and J. Frieman and J. Garcia-Bellido and E. Gaztanaga and K. Glazebrook and D. Gruen and Gruendl, \{R. A.\} and J. Gschwend and G. Gutierrez and Hollowood, \{D. L.\} and K. Honscheid and James, \{D. J.\} and K. Kuehn and N. Kuropatkin and M. Lima and Maia, \{M. A. G.\} and Marshall, \{J. L.\} and P. Martini and F. Menanteau and R. Miquel and A. Palmese and F. Paz-Chinchon and Plazas, \{A. A.\} and Romer, \{A. K.\} and E. Sanchez and V. Scarpine and M. Schubnell and S. Serrano and I. Sevilla-Noarbe and Sommer, \{N. E.\} and E. Suchyta and Swanson, \{M. E. C.\} and G. Tarle and Tucker, \{B. E.\} and Tucker, \{D. L.\} and Varga, \{T. N.\} and Walker, \{A. R.\}",

year = "2023",

month = aug,

day = "1",

language = "English",

type = "Other",

}

Wiseman, P, Pursiainen, M, Childress, M, Swann, E, Smith, M, Galbany, L, Lidman, C, Davis, TM, Gutierrez, CP, Moller, A, Thomas, BP, Frohmaier, C, Foley, RJ, Hinton, SR, Kelsey, L, Kessler, R, Lewis, GF, Sako, M, Scolnic, D, Sullivan, M, Vincenzi, M, Abbott, TMC, Aguena, M, Allam, S, Annis, J, Bertin, E, Bhargava, S, Brooks, D, Burke, DL, Carnero Rosell, A, Carollo, D, Carrasco Kind, M, Carretero, J, Costanzi, M, da Costa, LN, Diehl, HT, Doel, P, Everett, S, Fosalba, P, Frieman, J, Garcia-Bellido, J, Gaztanaga, E, Glazebrook, K, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hollowood, DL, Honscheid, K, James, DJ, Kuehn, K, Kuropatkin, N, Lima, M, Maia, MAG, Marshall, JL, Martini, P, Menanteau, F, Miquel, R, Palmese, A, Paz-Chinchon, F, Plazas, AA, Romer, AK, Sanchez, E, Scarpine, V, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Sommer, NE, Suchyta, E, Swanson, MEC, Tarle, G, Tucker, BE, Tucker, DL, Varga, TN & Walker, AR 2023, VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020).. <https://ui.adsabs.harvard.edu/abs/2023yCat..74982575W>

TY - GEN

T1 - VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020)

AU - Wiseman, P.

AU - Pursiainen, M.

AU - Childress, M.

AU - Swann, E.

AU - Smith, M.

AU - Galbany, L.

AU - Lidman, C.

AU - Davis, T. M.

AU - Gutierrez, C. P.

AU - Moller, A.

AU - Thomas, B. P.

AU - Frohmaier, C.

AU - Foley, R. J.

AU - Hinton, S. R.

AU - Kelsey, L.

AU - Kessler, R.

AU - Lewis, G. F.

AU - Sako, M.

AU - Scolnic, D.

AU - Sullivan, M.

AU - Vincenzi, M.

AU - Abbott, T. M. C.

AU - Aguena, M.

AU - Allam, S.

AU - Annis, J.

AU - Bertin, E.

AU - Bhargava, S.

AU - Brooks, D.

AU - Burke, D. L.

AU - Carnero Rosell, A.

AU - Carollo, D.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Costanzi, M.

AU - da Costa, L. N.

AU - Diehl, H. T.

AU - Doel, P.

AU - Everett, S.

AU - Fosalba, P.

AU - Frieman, J.

AU - Garcia-Bellido, J.

AU - Gaztanaga, E.

AU - Glazebrook, K.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - James, D. J.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lima, M.

AU - Maia, M. A. G.

AU - Marshall, J. L.

AU - Martini, P.

AU - Menanteau, F.

AU - Miquel, R.

AU - Palmese, A.

AU - Paz-Chinchon, F.

AU - Plazas, A. A.

AU - Romer, A. K.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Serrano, S.

AU - Sevilla-Noarbe, I.

AU - Sommer, N. E.

AU - Suchyta, E.

AU - Swanson, M. E. C.

AU - Tarle, G.

AU - Tucker, B. E.

AU - Tucker, D. L.

AU - Varga, T. N.

AU - Walker, A. R.

PY - 2023/8/1

Y1 - 2023/8/1

N2 - Our sample of RETs comprises 106 events discovered in the 5-yr DES-SN transient survey. This number expands upon the 72 of Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) (P18). The first reason for the increased sample size is the use of the fifth year of DES-SN, as Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) were only able to make use of the first 4yr. By imposing the P18 selection criteria on season 5, the sample is increased to 92 objects. The second reason is an update to the sample selection technique, which adds a further 14 transients. Of the 106 objects in the sample, 96 have a host galaxy detected in deep host galaxy photometry of Wiseman et al. (2020MNRAS.495.4040W) when using the directional light radius method (Sullivan et al. 2006ApJ...648..868S) to associate hosts as per Wiseman et al. (2020MNRAS.495.4040W). Of these, 49 have a host galaxy spectroscopic redshift which we access through an internal release of the OzDES Global Redshift Catalog (GRC; v.20200104). The full OzDES redshift catalogue will be available alongside the public data release detailed in Lidman et al. (2020MNRAS.496...19L). We also obtained redshifts for some transient hosts serendipitously as part of the Looking at the Distant Universe with the MeerKAT Array (LADUMA) survey (http://www.laduma.uct.ac.za). Objects for which the host already had a publicly available redshift were not observed with OzDES, but merged into the GRC none the less. In total we analyse 45 spectra, with a mean continuum SNR of 2.56/pixel. (3 data files).

AB - Our sample of RETs comprises 106 events discovered in the 5-yr DES-SN transient survey. This number expands upon the 72 of Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) (P18). The first reason for the increased sample size is the use of the fifth year of DES-SN, as Pursiainen et al. (2018MNRAS.481..894P, Cat. J/MNRAS/481/894) were only able to make use of the first 4yr. By imposing the P18 selection criteria on season 5, the sample is increased to 92 objects. The second reason is an update to the sample selection technique, which adds a further 14 transients. Of the 106 objects in the sample, 96 have a host galaxy detected in deep host galaxy photometry of Wiseman et al. (2020MNRAS.495.4040W) when using the directional light radius method (Sullivan et al. 2006ApJ...648..868S) to associate hosts as per Wiseman et al. (2020MNRAS.495.4040W). Of these, 49 have a host galaxy spectroscopic redshift which we access through an internal release of the OzDES Global Redshift Catalog (GRC; v.20200104). The full OzDES redshift catalogue will be available alongside the public data release detailed in Lidman et al. (2020MNRAS.496...19L). We also obtained redshifts for some transient hosts serendipitously as part of the Looking at the Distant Universe with the MeerKAT Array (LADUMA) survey (http://www.laduma.uct.ac.za). Objects for which the host already had a publicly available redshift were not observed with OzDES, but merged into the GRC none the less. In total we analyse 45 spectra, with a mean continuum SNR of 2.56/pixel. (3 data files).

KW - Transient

KW - Galaxies

KW - Positional data

KW - Redshifts

KW - Abundances: peculiar

KW - Spectra: optical

M3 - Other contribution

ER -

VizieR Online Data Catalog: Rapidly evolving transients discovered by DES (Wiseman+, 2020)

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