VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020)

M. Smith; M. Sullivan; P. Wiseman; R. Kessler; D. Scolnic; D. Brout; C. B. D'Andrea; T. M. Davis; R. J. Foley; C. Frohmaier; L. Galbany; R. R. Gupta; C. P. Gutierrez; S. R. Hinton; L. Kelsey; C. Lidman; E. Macaulay; A. Moller; R. C. Nichol; P. Nugent; A. Palmese; M. Pursiainen; M. Sako; E. Swann; R. C. Thomas; B. E. Tucker; M. Vincenzi; D. Carollo; G. F. Lewis; N. E. Sommer; T. M. C. Abbott; M. Aguena; S. Allam; S. Avila; E. Bertin; S. Bhargava; D. Brooks; E. Buckley-Geer; D. L. Burke; A. Carnero Rosell; M. Carrasco Kind; M. Costanzi; L. N. da Costa; Vicente J. de; S. Desai; H. T. Diehl; P. Doel; T. F. Eifler; S. Everett; B. Flaugher; P. Fosalba; J. Frieman; J. Garcia-Bellido; E. Gaztanaga; K. Glazebrook; D. Gruen; R. A. Gruendl; J. Gschwend; G. Gutierrez; W. G. Hartley; D. L. Hollowood; K. Honscheid; D. J. James; E. Krause; K. Kuehn; N. Kuropatkin; M. Lima; N. Maccrann; M. A. G. Maia; J. L. Marshall; P. Martini; P. Melchior; F. Menanteau; R. Miquel; F. Paz-Chinchon; A. A. Plazas; A. K. Romer; A. Roodman; E. S. Rykoff; E. Sanchez; V. Scarpine; M. Schubnell; S. Serrano; I. Sevilla-Noarbe; E. Suchyta; M. E. C. Swanson; G. Tarle; D. Thomas; D. L. Tucker; T. N. Varga; A. R. Walker

VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020)

M. Smith, M. Sullivan, P. Wiseman, R. Kessler, D. Scolnic, D. Brout, C. B. D'Andrea, T. M. Davis, R. J. Foley, C. Frohmaier, L. Galbany, R. R. Gupta, C. P. Gutierrez, S. R. Hinton, L. Kelsey, C. Lidman, E. Macaulay, A. Moller, R. C. Nichol, P. NugentA. Palmese, M. Pursiainen, M. Sako, E. Swann, R. C. Thomas, B. E. Tucker, M. Vincenzi, D. Carollo, G. F. Lewis, N. E. Sommer, T. M. C. Abbott, M. Aguena, S. Allam, S. Avila, E. Bertin, S. Bhargava, D. Brooks, E. Buckley-Geer, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, M. Costanzi, L. N. da Costa, Vicente J. de, S. Desai, H. T. Diehl, P. Doel, T. F. Eifler, S. Everett, B. Flaugher, P. Fosalba, J. Frieman, J. Garcia-Bellido, E. Gaztanaga, K. Glazebrook, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, W. G. Hartley, D. L. Hollowood, K. Honscheid, D. J. James, E. Krause, K. Kuehn, N. Kuropatkin, M. Lima, N. Maccrann, M. A. G. Maia, J. L. Marshall, P. Martini, P. Melchior, F. Menanteau, R. Miquel, F. Paz-Chinchon, A. A. Plazas, A. K. Romer, A. Roodman, E. S. Rykoff, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, D. L. Tucker, T. N. Varga, A. R. Walker

Research School of Astronomy & Astrophysics

Research output: Other contribution

Abstract

The DES-SN Program was a 5yr rolling search using the 570 Megapixel Dark Energy Camera (DECam; Flaugher et al. 2015AJ....150..150F) on the 4-m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO), giving a 2.7deg² field of view. DES-SN observed two 'deep' fields and eight 'shallow' fields in griz filters approximately every 7d, to single-visit depths of ~24.5 and ~23.5mag, respectively.

Transient events were detected using a difference-imaging pipeline (Kessler et al. 2015AJ....150..172K), with machine-learning algorithms used to remove spurious candidates (Goldstein et al. 2015AJ....150...82G). During the first 3yr, 251 SNe Ia were spectroscopically classified. Quality cuts, based on the light-curve coverage, are applied to the sample (see Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150 for details), which removes 45 SNe Ia. This leaves 206 SNe Ia in the fiducial DES sample.

Photometric data for the host galaxies of the DES3YR cosmology analysis (Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150) were determined from the DES SVA1-GOLD catalogue. This catalogue has 10σ limiting magnitudes of (g, r, i, z) = (24.0, 23.8, 23.0, 22.3). It was constructed from DES Science Verification data collected prior to the DES-SN data used in the DES3YR sample. In this paper, we upgrade from the DES SVA1-GOLD catalogue and instead determine photometric properties of the DES SNe Ia host galaxies from DES deep stack photometry (Wiseman et al. 2020MNRAS.495.4040W) utilizing images from all 5yr of DES-SN.

(1 data file).

Original language	English
Publication status	Published - 1 Jun 2023

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https://ui.adsabs.harvard.edu/abs/2023yCat..74944426S

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Smith, M., Sullivan, M., Wiseman, P., Kessler, R., Scolnic, D., Brout, D., D'Andrea, C. B., Davis, T. M., Foley, R. J., Frohmaier, C., Galbany, L., Gupta, R. R., Gutierrez, C. P., Hinton, S. R., Kelsey, L., Lidman, C., Macaulay, E., Moller, A., Nichol, R. C., ... Walker, A. R. (2023, Jun 1). VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020). https://ui.adsabs.harvard.edu/abs/2023yCat..74944426S

@misc{da66ec7ba8f3454289bdcc24f36c5ad8,

title = "VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020)",

abstract = "The DES-SN Program was a 5yr rolling search using the 570 Megapixel Dark Energy Camera (DECam; Flaugher et al. 2015AJ....150..150F) on the 4-m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO), giving a 2.7deg2 field of view. DES-SN observed two 'deep' fields and eight 'shallow' fields in griz filters approximately every 7d, to single-visit depths of ~24.5 and ~23.5mag, respectively. Transient events were detected using a difference-imaging pipeline (Kessler et al. 2015AJ....150..172K), with machine-learning algorithms used to remove spurious candidates (Goldstein et al. 2015AJ....150...82G). During the first 3yr, 251 SNe Ia were spectroscopically classified. Quality cuts, based on the light-curve coverage, are applied to the sample (see Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150 for details), which removes 45 SNe Ia. This leaves 206 SNe Ia in the fiducial DES sample. Photometric data for the host galaxies of the DES3YR cosmology analysis (Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150) were determined from the DES SVA1-GOLD catalogue. This catalogue has 10σ limiting magnitudes of (g, r, i, z) = (24.0, 23.8, 23.0, 22.3). It was constructed from DES Science Verification data collected prior to the DES-SN data used in the DES3YR sample. In this paper, we upgrade from the DES SVA1-GOLD catalogue and instead determine photometric properties of the DES SNe Ia host galaxies from DES deep stack photometry (Wiseman et al. 2020MNRAS.495.4040W) utilizing images from all 5yr of DES-SN. (1 data file).",

keywords = "Supernovae, Surveys, Redshifts, Galaxies: photometry, Optical",

author = "M. Smith and M. Sullivan and P. Wiseman and R. Kessler and D. Scolnic and D. Brout and D'Andrea, {C. B.} and Davis, {T. M.} and Foley, {R. J.} and C. Frohmaier and L. Galbany and Gupta, {R. R.} and Gutierrez, {C. P.} and Hinton, {S. R.} and L. Kelsey and C. Lidman and E. Macaulay and A. Moller and Nichol, {R. C.} and P. Nugent and A. Palmese and M. Pursiainen and M. Sako and E. Swann and Thomas, {R. C.} and Tucker, {B. E.} and M. Vincenzi and D. Carollo and Lewis, {G. F.} and Sommer, {N. E.} and Abbott, {T. M. C.} and M. Aguena and S. Allam and S. Avila and E. Bertin and S. Bhargava and D. Brooks and E. Buckley-Geer and Burke, {D. L.} and {Carnero Rosell}, A. and {Carrasco Kind}, M. and M. Costanzi and {da Costa}, {L. N.} and de, {Vicente J.} and S. Desai and Diehl, {H. T.} and P. Doel and Eifler, {T. F.} and S. Everett and B. Flaugher 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 Hartley, {W. G.} and Hollowood, {D. L.} and K. Honscheid and James, {D. J.} and E. Krause and K. Kuehn and N. Kuropatkin and M. Lima and N. Maccrann and Maia, {M. A. G.} and Marshall, {J. L.} and P. Martini and P. Melchior and F. Menanteau and R. Miquel and F. Paz-Chinchon and Plazas, {A. A.} and Romer, {A. K.} and A. Roodman and Rykoff, {E. S.} and E. Sanchez and V. Scarpine and M. Schubnell and S. Serrano and I. Sevilla-Noarbe and E. Suchyta and Swanson, {M. E. C.} and G. Tarle and D. Thomas and Tucker, {D. L.} and Varga, {T. N.} and Walker, {A. R.}",

year = "2023",

month = jun,

day = "1",

language = "English",

type = "Other",

}

Smith, M, Sullivan, M, Wiseman, P, Kessler, R, Scolnic, D, Brout, D, D'Andrea, CB, Davis, TM, Foley, RJ, Frohmaier, C, Galbany, L, Gupta, RR, Gutierrez, CP, Hinton, SR, Kelsey, L, Lidman, C, Macaulay, E, Moller, A, Nichol, RC, Nugent, P, Palmese, A, Pursiainen, M, Sako, M, Swann, E, Thomas, RC, Tucker, BE, Vincenzi, M, Carollo, D, Lewis, GF, Sommer, NE, Abbott, TMC, Aguena, M, Allam, S, Avila, S, Bertin, E, Bhargava, S, Brooks, D, Buckley-Geer, E, Burke, DL, Carnero Rosell, A, Carrasco Kind, M, Costanzi, M, da Costa, LN, de, VJ, Desai, S, Diehl, HT, Doel, P, Eifler, TF, Everett, S, Flaugher, B, Fosalba, P, Frieman, J, Garcia-Bellido, J, Gaztanaga, E, Glazebrook, K, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hartley, WG, Hollowood, DL, Honscheid, K, James, DJ, Krause, E, Kuehn, K, Kuropatkin, N, Lima, M, Maccrann, N, Maia, MAG, Marshall, JL, Martini, P, Melchior, P, Menanteau, F, Miquel, R, Paz-Chinchon, F, Plazas, AA, Romer, AK, Roodman, A, Rykoff, ES, Sanchez, E, Scarpine, V, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Suchyta, E, Swanson, MEC, Tarle, G, Thomas, D, Tucker, DL, Varga, TN & Walker, AR 2023, VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020).. <https://ui.adsabs.harvard.edu/abs/2023yCat..74944426S>

TY - GEN

T1 - VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020)

AU - Smith, M.

AU - Sullivan, M.

AU - Wiseman, P.

AU - Kessler, R.

AU - Scolnic, D.

AU - Brout, D.

AU - D'Andrea, C. B.

AU - Davis, T. M.

AU - Foley, R. J.

AU - Frohmaier, C.

AU - Galbany, L.

AU - Gupta, R. R.

AU - Gutierrez, C. P.

AU - Hinton, S. R.

AU - Kelsey, L.

AU - Lidman, C.

AU - Macaulay, E.

AU - Moller, A.

AU - Nichol, R. C.

AU - Nugent, P.

AU - Palmese, A.

AU - Pursiainen, M.

AU - Sako, M.

AU - Swann, E.

AU - Thomas, R. C.

AU - Tucker, B. E.

AU - Vincenzi, M.

AU - Carollo, D.

AU - Lewis, G. F.

AU - Sommer, N. E.

AU - Abbott, T. M. C.

AU - Aguena, M.

AU - Allam, S.

AU - Avila, S.

AU - Bertin, E.

AU - Bhargava, S.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Costanzi, M.

AU - da Costa, L. N.

AU - de, Vicente J.

AU - Desai, S.

AU - Diehl, H. T.

AU - Doel, P.

AU - Eifler, T. F.

AU - Everett, S.

AU - Flaugher, B.

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 - Hartley, W. G.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - James, D. J.

AU - Krause, E.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lima, M.

AU - Maccrann, N.

AU - Maia, M. A. G.

AU - Marshall, J. L.

AU - Martini, P.

AU - Melchior, P.

AU - Menanteau, F.

AU - Miquel, R.

AU - Paz-Chinchon, F.

AU - Plazas, A. A.

AU - Romer, A. K.

AU - Roodman, A.

AU - Rykoff, E. S.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Serrano, S.

AU - Sevilla-Noarbe, I.

AU - Suchyta, E.

AU - Swanson, M. E. C.

AU - Tarle, G.

AU - Thomas, D.

AU - Tucker, D. L.

AU - Varga, T. N.

AU - Walker, A. R.

PY - 2023/6/1

Y1 - 2023/6/1

N2 - The DES-SN Program was a 5yr rolling search using the 570 Megapixel Dark Energy Camera (DECam; Flaugher et al. 2015AJ....150..150F) on the 4-m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO), giving a 2.7deg2 field of view. DES-SN observed two 'deep' fields and eight 'shallow' fields in griz filters approximately every 7d, to single-visit depths of ~24.5 and ~23.5mag, respectively. Transient events were detected using a difference-imaging pipeline (Kessler et al. 2015AJ....150..172K), with machine-learning algorithms used to remove spurious candidates (Goldstein et al. 2015AJ....150...82G). During the first 3yr, 251 SNe Ia were spectroscopically classified. Quality cuts, based on the light-curve coverage, are applied to the sample (see Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150 for details), which removes 45 SNe Ia. This leaves 206 SNe Ia in the fiducial DES sample. Photometric data for the host galaxies of the DES3YR cosmology analysis (Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150) were determined from the DES SVA1-GOLD catalogue. This catalogue has 10σ limiting magnitudes of (g, r, i, z) = (24.0, 23.8, 23.0, 22.3). It was constructed from DES Science Verification data collected prior to the DES-SN data used in the DES3YR sample. In this paper, we upgrade from the DES SVA1-GOLD catalogue and instead determine photometric properties of the DES SNe Ia host galaxies from DES deep stack photometry (Wiseman et al. 2020MNRAS.495.4040W) utilizing images from all 5yr of DES-SN. (1 data file).

AB - The DES-SN Program was a 5yr rolling search using the 570 Megapixel Dark Energy Camera (DECam; Flaugher et al. 2015AJ....150..150F) on the 4-m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO), giving a 2.7deg2 field of view. DES-SN observed two 'deep' fields and eight 'shallow' fields in griz filters approximately every 7d, to single-visit depths of ~24.5 and ~23.5mag, respectively. Transient events were detected using a difference-imaging pipeline (Kessler et al. 2015AJ....150..172K), with machine-learning algorithms used to remove spurious candidates (Goldstein et al. 2015AJ....150...82G). During the first 3yr, 251 SNe Ia were spectroscopically classified. Quality cuts, based on the light-curve coverage, are applied to the sample (see Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150 for details), which removes 45 SNe Ia. This leaves 206 SNe Ia in the fiducial DES sample. Photometric data for the host galaxies of the DES3YR cosmology analysis (Brout et al. 2019ApJ...874..150B, Cat. J/ApJ/874/150) were determined from the DES SVA1-GOLD catalogue. This catalogue has 10σ limiting magnitudes of (g, r, i, z) = (24.0, 23.8, 23.0, 22.3). It was constructed from DES Science Verification data collected prior to the DES-SN data used in the DES3YR sample. In this paper, we upgrade from the DES SVA1-GOLD catalogue and instead determine photometric properties of the DES SNe Ia host galaxies from DES deep stack photometry (Wiseman et al. 2020MNRAS.495.4040W) utilizing images from all 5yr of DES-SN. (1 data file).

KW - Supernovae

KW - Surveys

KW - Redshifts

KW - Galaxies: photometry

KW - Optical

M3 - Other contribution

ER -

VizieR Online Data Catalog: Effect of host galaxies on SN luminosity (Smith+, 2020)

Abstract

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