Supernova/Acceleration Probe: Science with Wide Deep Fields

E. Linder; C. Akerlof; G. Aldering; D. Amidei; P. Astier; A. Baden; C. Bebek; L. Bergstrom; G. Bernstein; M. Campbell; W. Carithers; E. Commins; D. Curtis; S. Deustua; W. Edwards; R. Ellis; A. Fruchter; B. Frye; J. F. Genat; G. Goldhaber; A. Goobar; J. Goodman; J. Graham; D. Hardin; S. Harris; P. Harvey; H. Heetderks; S. Holland; I. Hook; D. Huterer; D. Kasen; A. Kim; R. Knop; R. Lafever; M. Lampton; M. Levi; D. Levin; J. -M. Levy; C. Lidman; R. Lin; S. Loken; T. McKay; S. McKee; M. Metzger; R. Miquel; A. Mourao; P. Nugent; R. Pain; D. Pankow; C. Pennypacker; S. Perlmutter; A. Refregier; J. Rich; K. Robinson; K. Schahmaneche; M. Schubnell; A. Spadafora; G. Smoot; G. Sullivan; G. Tarle; A. Tomasch; SNAP Collaboration

Supernova/Acceleration Probe: Science with Wide Deep Fields

E. Linder, C. Akerlof, G. Aldering, D. Amidei, P. Astier, A. Baden, C. Bebek, L. Bergstrom, G. Bernstein, M. Campbell, W. Carithers, E. Commins, D. Curtis, S. Deustua, W. Edwards, R. Ellis, A. Fruchter, B. Frye, J. F. Genat, G. GoldhaberA. Goobar, J. Goodman, J. Graham, D. Hardin, S. Harris, P. Harvey, H. Heetderks, S. Holland, I. Hook, D. Huterer, D. Kasen, A. Kim, R. Knop, R. Lafever, M. Lampton, M. Levi, D. Levin, J. -M. Levy, C. Lidman, R. Lin, S. Loken, T. McKay, S. McKee, M. Metzger, R. Miquel, A. Mourao, P. Nugent, R. Pain, D. Pankow, C. Pennypacker, S. Perlmutter, A. Refregier, J. Rich, K. Robinson, K. Schahmaneche, M. Schubnell, A. Spadafora, G. Smoot, G. Sullivan, G. Tarle, A. Tomasch, SNAP Collaboration

Research School of Astronomy & Astrophysics

Research output: Contribution to conference › Paper

Abstract

The SNAP satellite will survey 20 square degrees down to magnitude R=30.4 with coadded images to m(AB)=32. This is 13000 times the area of the HDF and 6300 times the area of the ACS, to about the same depth and resolution. Like the Hubble Deep Field, SNAP survey data will be eminently combinable with other observations and analyses. It can act as a feeder for NGST in galaxy structure and evolution, weak and strong lensing, rare objects, and other studies that benefit from an ultra deep 11 band survey. Its time domain capabilities probe gamma ray burst afterglows, proper motions, supernova phenomenology, and outer solar system objects. This project is supported by the US Department of Energy/Office of High Energy Physics.

Original language	English
Pages	64.04
Publication status	Published - 1 Dec 2001

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https://ui.adsabs.harvard.edu/abs/2001AAS...199.6404L

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Linder, E., Akerlof, C., Aldering, G., Amidei, D., Astier, P., Baden, A., Bebek, C., Bergstrom, L., Bernstein, G., Campbell, M., Carithers, W., Commins, E., Curtis, D., Deustua, S., Edwards, W., Ellis, R., Fruchter, A., Frye, B., Genat, J. F., ... Collaboration, SNAP. (2001). Supernova/Acceleration Probe: Science with Wide Deep Fields. 64.04. https://ui.adsabs.harvard.edu/abs/2001AAS...199.6404L

@conference{956f34cb09924e3d8b2b1232859a76dd,

title = "Supernova/Acceleration Probe: Science with Wide Deep Fields",

abstract = "The SNAP satellite will survey 20 square degrees down to magnitude R=30.4 with coadded images to m(AB)=32. This is 13000 times the area of the HDF and 6300 times the area of the ACS, to about the same depth and resolution. Like the Hubble Deep Field, SNAP survey data will be eminently combinable with other observations and analyses. It can act as a feeder for NGST in galaxy structure and evolution, weak and strong lensing, rare objects, and other studies that benefit from an ultra deep 11 band survey. Its time domain capabilities probe gamma ray burst afterglows, proper motions, supernova phenomenology, and outer solar system objects. This project is supported by the US Department of Energy/Office of High Energy Physics.",

author = "E. Linder and C. Akerlof and G. Aldering and D. Amidei and P. Astier and A. Baden and C. Bebek and L. Bergstrom and G. Bernstein and M. Campbell and W. Carithers and E. Commins and D. Curtis and S. Deustua and W. Edwards and R. Ellis and A. Fruchter and B. Frye and Genat, {J. F.} and G. Goldhaber and A. Goobar and J. Goodman and J. Graham and D. Hardin and S. Harris and P. Harvey and H. Heetderks and S. Holland and I. Hook and D. Huterer and D. Kasen and A. Kim and R. Knop and R. Lafever and M. Lampton and M. Levi and D. Levin and Levy, {J. -M.} and C. Lidman and R. Lin and S. Loken and T. McKay and S. McKee and M. Metzger and R. Miquel and A. Mourao and P. Nugent and R. Pain and D. Pankow and C. Pennypacker and S. Perlmutter and A. Refregier and J. Rich and K. Robinson and K. Schahmaneche and M. Schubnell and A. Spadafora and G. Smoot and G. Sullivan and G. Tarle and A. Tomasch and SNAP Collaboration",

year = "2001",

month = dec,

day = "1",

language = "English",

pages = "64.04",

}

Linder, E, Akerlof, C, Aldering, G, Amidei, D, Astier, P, Baden, A, Bebek, C, Bergstrom, L, Bernstein, G, Campbell, M, Carithers, W, Commins, E, Curtis, D, Deustua, S, Edwards, W, Ellis, R, Fruchter, A, Frye, B, Genat, JF, Goldhaber, G, Goobar, A, Goodman, J, Graham, J, Hardin, D, Harris, S, Harvey, P, Heetderks, H, Holland, S, Hook, I, Huterer, D, Kasen, D, Kim, A, Knop, R, Lafever, R, Lampton, M, Levi, M, Levin, D, Levy, J-M, Lidman, C, Lin, R, Loken, S, McKay, T, McKee, S, Metzger, M, Miquel, R, Mourao, A, Nugent, P, Pain, R, Pankow, D, Pennypacker, C, Perlmutter, S, Refregier, A, Rich, J, Robinson, K, Schahmaneche, K, Schubnell, M, Spadafora, A, Smoot, G, Sullivan, G, Tarle, G, Tomasch, A & Collaboration, SNAP 2001, 'Supernova/Acceleration Probe: Science with Wide Deep Fields', pp. 64.04. <https://ui.adsabs.harvard.edu/abs/2001AAS...199.6404L>

TY - CONF

T1 - Supernova/Acceleration Probe: Science with Wide Deep Fields

AU - Linder, E.

AU - Akerlof, C.

AU - Aldering, G.

AU - Amidei, D.

AU - Astier, P.

AU - Baden, A.

AU - Bebek, C.

AU - Bergstrom, L.

AU - Bernstein, G.

AU - Campbell, M.

AU - Carithers, W.

AU - Commins, E.

AU - Curtis, D.

AU - Deustua, S.

AU - Edwards, W.

AU - Ellis, R.

AU - Fruchter, A.

AU - Frye, B.

AU - Genat, J. F.

AU - Goldhaber, G.

AU - Goobar, A.

AU - Goodman, J.

AU - Graham, J.

AU - Hardin, D.

AU - Harris, S.

AU - Harvey, P.

AU - Heetderks, H.

AU - Holland, S.

AU - Hook, I.

AU - Huterer, D.

AU - Kasen, D.

AU - Kim, A.

AU - Knop, R.

AU - Lafever, R.

AU - Lampton, M.

AU - Levi, M.

AU - Levin, D.

AU - Levy, J. -M.

AU - Lidman, C.

AU - Lin, R.

AU - Loken, S.

AU - McKay, T.

AU - McKee, S.

AU - Metzger, M.

AU - Miquel, R.

AU - Mourao, A.

AU - Nugent, P.

AU - Pain, R.

AU - Pankow, D.

AU - Pennypacker, C.

AU - Perlmutter, S.

AU - Refregier, A.

AU - Rich, J.

AU - Robinson, K.

AU - Schahmaneche, K.

AU - Schubnell, M.

AU - Spadafora, A.

AU - Smoot, G.

AU - Sullivan, G.

AU - Tarle, G.

AU - Tomasch, A.

AU - Collaboration, SNAP

PY - 2001/12/1

Y1 - 2001/12/1

N2 - The SNAP satellite will survey 20 square degrees down to magnitude R=30.4 with coadded images to m(AB)=32. This is 13000 times the area of the HDF and 6300 times the area of the ACS, to about the same depth and resolution. Like the Hubble Deep Field, SNAP survey data will be eminently combinable with other observations and analyses. It can act as a feeder for NGST in galaxy structure and evolution, weak and strong lensing, rare objects, and other studies that benefit from an ultra deep 11 band survey. Its time domain capabilities probe gamma ray burst afterglows, proper motions, supernova phenomenology, and outer solar system objects. This project is supported by the US Department of Energy/Office of High Energy Physics.

AB - The SNAP satellite will survey 20 square degrees down to magnitude R=30.4 with coadded images to m(AB)=32. This is 13000 times the area of the HDF and 6300 times the area of the ACS, to about the same depth and resolution. Like the Hubble Deep Field, SNAP survey data will be eminently combinable with other observations and analyses. It can act as a feeder for NGST in galaxy structure and evolution, weak and strong lensing, rare objects, and other studies that benefit from an ultra deep 11 band survey. Its time domain capabilities probe gamma ray burst afterglows, proper motions, supernova phenomenology, and outer solar system objects. This project is supported by the US Department of Energy/Office of High Energy Physics.

M3 - Paper

SP - 64.04

ER -

Supernova/Acceleration Probe: Science with Wide Deep Fields

Abstract

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