Results from Recent High-redshift Type Ia Supernovae Searches

K. Schahmaneche; G. Aldering; R. Amanullah; P. Antilogus; P. Astier; C. Balland; G. Blanc; M. S. Burns; A. Conley; S. Deustua; M. Doi; R. Ellis; S. Fabbro; G. Folatelli; A. Fruchter; G. Garavini; R. Gibbons; G. Goldhaber; A. Goobar; D. E. Groom; D. Hardin; I. M. Hook; D. A. Howell; M. Irwin; D. Kasen; A. Kim; M. Kim; R. A. Knop; J. C. Lee; J. -M. Levy; C. Lidman; R. McMahon; M. Mouchet; S. Nobili; P. Nugent; R. Pain; N. Panagia; E. Pécontal; C. R. Pennypacker; S. Perlmutter; R. Quimby; J. Raux; N. Regnault; P. Ruiz-Lapuente; B. Schaefer; A. L. Spadafora; N. Walton; L. Wang; W. M. Wood-Vasey; N. Yasuda; Supernova Cosmology Project Collaboration

Results from Recent High-redshift Type Ia Supernovae Searches

K. Schahmaneche, G. Aldering, R. Amanullah, P. Antilogus, P. Astier, C. Balland, G. Blanc, M. S. Burns, A. Conley, S. Deustua, M. Doi, R. Ellis, S. Fabbro, G. Folatelli, A. Fruchter, G. Garavini, R. Gibbons, G. Goldhaber, A. Goobar, D. E. GroomD. Hardin, I. M. Hook, D. A. Howell, M. Irwin, D. Kasen, A. Kim, M. Kim, R. A. Knop, J. C. Lee, J. -M. Levy, C. Lidman, R. McMahon, M. Mouchet, S. Nobili, P. Nugent, R. Pain, N. Panagia, E. Pécontal, C. R. Pennypacker, S. Perlmutter, R. Quimby, J. Raux, N. Regnault, P. Ruiz-Lapuente, B. Schaefer, A. L. Spadafora, N. Walton, L. Wang, W. M. Wood-Vasey, N. Yasuda, Supernova Cosmology Project Collaboration

Research School of Astronomy & Astrophysics

Research output: Contribution to conference › Paper

Abstract

Distant type Ia supernovae have been used as calibrated standard candles out to z=0.8 (\bar{z} ~= 0.55) to measure the combination ~ Ω M - Ω _Λ using the classical magnitude-redshift relation. Extending the redshift range will reduce and eventually break the (Ω M,Ω _{Λ )} degeneracy, and also discriminate between a non-zero cosmological constant and models of hypothetical intergalactic grey dust. We present here preliminary results from the most recent very high-redshift (z ~ 1) Type Ia supernova searches of the Supernova Cosmology Project. The supernovae were discovered at the CFHT 3.6-m telescope using the CFH12k camera (run in queue mode), the CTIO 4-m telescope using the MOSAIC camera and the Subaru 8.2-m telescope using SuprimeCam. The observations were coordinated with spectroscopic follow-up at Keck, VLT, and Subaru. The optical photometric follow-up was obtained at WIYN, WHT, and TNG for the brighter supernovae, and at HST for the faintest supernovae. The VLT and Gemini made possible the near-IR photometric follow up. This work was supported in part by the NASA Space Telescope Science Institute.

Original language	English
Pages	16.12
Publication status	Published - 1 Dec 2001

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https://ui.adsabs.harvard.edu/abs/2001AAS...199.1612S

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Schahmaneche, K., Aldering, G., Amanullah, R., Antilogus, P., Astier, P., Balland, C., Blanc, G., Burns, M. S., Conley, A., Deustua, S., Doi, M., Ellis, R., Fabbro, S., Folatelli, G., Fruchter, A., Garavini, G., Gibbons, R., Goldhaber, G., Goobar, A., ... Collaboration, S. C. P. (2001). Results from Recent High-redshift Type Ia Supernovae Searches. 16.12. https://ui.adsabs.harvard.edu/abs/2001AAS...199.1612S

@conference{9c3f383394ed40a99ae533c9fd6db3f8,

title = "Results from Recent High-redshift Type Ia Supernovae Searches",

abstract = "Distant type Ia supernovae have been used as calibrated standard candles out to z=0.8 (\bar{z} ~= 0.55) to measure the combination ~ Ω M - Ω Λ using the classical magnitude-redshift relation. Extending the redshift range will reduce and eventually break the (Ω M,Ω Λ ) degeneracy, and also discriminate between a non-zero cosmological constant and models of hypothetical intergalactic grey dust. We present here preliminary results from the most recent very high-redshift (z ~ 1) Type Ia supernova searches of the Supernova Cosmology Project. The supernovae were discovered at the CFHT 3.6-m telescope using the CFH12k camera (run in queue mode), the CTIO 4-m telescope using the MOSAIC camera and the Subaru 8.2-m telescope using SuprimeCam. The observations were coordinated with spectroscopic follow-up at Keck, VLT, and Subaru. The optical photometric follow-up was obtained at WIYN, WHT, and TNG for the brighter supernovae, and at HST for the faintest supernovae. The VLT and Gemini made possible the near-IR photometric follow up. This work was supported in part by the NASA Space Telescope Science Institute.",

author = "K. Schahmaneche and G. Aldering and R. Amanullah and P. Antilogus and P. Astier and C. Balland and G. Blanc and Burns, {M. S.} and A. Conley and S. Deustua and M. Doi and R. Ellis and S. Fabbro and G. Folatelli and A. Fruchter and G. Garavini and R. Gibbons and G. Goldhaber and A. Goobar and Groom, {D. E.} and D. Hardin and Hook, {I. M.} and Howell, {D. A.} and M. Irwin and D. Kasen and A. Kim and M. Kim and Knop, {R. A.} and Lee, {J. C.} and Levy, {J. -M.} and C. Lidman and R. McMahon and M. Mouchet and S. Nobili and P. Nugent and R. Pain and N. Panagia and E. P{\'e}contal and Pennypacker, {C. R.} and S. Perlmutter and R. Quimby and J. Raux and N. Regnault and P. Ruiz-Lapuente and B. Schaefer and Spadafora, {A. L.} and N. Walton and L. Wang and Wood-Vasey, {W. M.} and N. Yasuda and Collaboration, {Supernova Cosmology Project}",

year = "2001",

month = dec,

day = "1",

language = "English",

pages = "16.12",

}

Schahmaneche, K, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Balland, C, Blanc, G, Burns, MS, Conley, A, Deustua, S, Doi, M, Ellis, R, Fabbro, S, Folatelli, G, Fruchter, A, Garavini, G, Gibbons, R, Goldhaber, G, Goobar, A, Groom, DE, Hardin, D, Hook, IM, Howell, DA, Irwin, M, Kasen, D, Kim, A, Kim, M, Knop, RA, Lee, JC, Levy, J-M, Lidman, C, McMahon, R, Mouchet, M, Nobili, S, Nugent, P, Pain, R, Panagia, N, Pécontal, E, Pennypacker, CR, Perlmutter, S, Quimby, R, Raux, J, Regnault, N, Ruiz-Lapuente, P, Schaefer, B, Spadafora, AL, Walton, N, Wang, L, Wood-Vasey, WM, Yasuda, N & Collaboration, SCP 2001, 'Results from Recent High-redshift Type Ia Supernovae Searches', pp. 16.12. <https://ui.adsabs.harvard.edu/abs/2001AAS...199.1612S>

TY - CONF

T1 - Results from Recent High-redshift Type Ia Supernovae Searches

AU - Schahmaneche, K.

AU - Aldering, G.

AU - Amanullah, R.

AU - Antilogus, P.

AU - Astier, P.

AU - Balland, C.

AU - Blanc, G.

AU - Burns, M. S.

AU - Conley, A.

AU - Deustua, S.

AU - Doi, M.

AU - Ellis, R.

AU - Fabbro, S.

AU - Folatelli, G.

AU - Fruchter, A.

AU - Garavini, G.

AU - Gibbons, R.

AU - Goldhaber, G.

AU - Goobar, A.

AU - Groom, D. E.

AU - Hardin, D.

AU - Hook, I. M.

AU - Howell, D. A.

AU - Irwin, M.

AU - Kasen, D.

AU - Kim, A.

AU - Kim, M.

AU - Knop, R. A.

AU - Lee, J. C.

AU - Levy, J. -M.

AU - Lidman, C.

AU - McMahon, R.

AU - Mouchet, M.

AU - Nobili, S.

AU - Nugent, P.

AU - Pain, R.

AU - Panagia, N.

AU - Pécontal, E.

AU - Pennypacker, C. R.

AU - Perlmutter, S.

AU - Quimby, R.

AU - Raux, J.

AU - Regnault, N.

AU - Ruiz-Lapuente, P.

AU - Schaefer, B.

AU - Spadafora, A. L.

AU - Walton, N.

AU - Wang, L.

AU - Wood-Vasey, W. M.

AU - Yasuda, N.

AU - Collaboration, Supernova Cosmology Project

PY - 2001/12/1

Y1 - 2001/12/1

N2 - Distant type Ia supernovae have been used as calibrated standard candles out to z=0.8 (\bar{z} ~= 0.55) to measure the combination ~ Ω M - Ω Λ using the classical magnitude-redshift relation. Extending the redshift range will reduce and eventually break the (Ω M,Ω Λ ) degeneracy, and also discriminate between a non-zero cosmological constant and models of hypothetical intergalactic grey dust. We present here preliminary results from the most recent very high-redshift (z ~ 1) Type Ia supernova searches of the Supernova Cosmology Project. The supernovae were discovered at the CFHT 3.6-m telescope using the CFH12k camera (run in queue mode), the CTIO 4-m telescope using the MOSAIC camera and the Subaru 8.2-m telescope using SuprimeCam. The observations were coordinated with spectroscopic follow-up at Keck, VLT, and Subaru. The optical photometric follow-up was obtained at WIYN, WHT, and TNG for the brighter supernovae, and at HST for the faintest supernovae. The VLT and Gemini made possible the near-IR photometric follow up. This work was supported in part by the NASA Space Telescope Science Institute.

AB - Distant type Ia supernovae have been used as calibrated standard candles out to z=0.8 (\bar{z} ~= 0.55) to measure the combination ~ Ω M - Ω Λ using the classical magnitude-redshift relation. Extending the redshift range will reduce and eventually break the (Ω M,Ω Λ ) degeneracy, and also discriminate between a non-zero cosmological constant and models of hypothetical intergalactic grey dust. We present here preliminary results from the most recent very high-redshift (z ~ 1) Type Ia supernova searches of the Supernova Cosmology Project. The supernovae were discovered at the CFHT 3.6-m telescope using the CFH12k camera (run in queue mode), the CTIO 4-m telescope using the MOSAIC camera and the Subaru 8.2-m telescope using SuprimeCam. The observations were coordinated with spectroscopic follow-up at Keck, VLT, and Subaru. The optical photometric follow-up was obtained at WIYN, WHT, and TNG for the brighter supernovae, and at HST for the faintest supernovae. The VLT and Gemini made possible the near-IR photometric follow up. This work was supported in part by the NASA Space Telescope Science Institute.

M3 - Paper

SP - 16.12

ER -

Results from Recent High-redshift Type Ia Supernovae Searches

Abstract

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