Snap telescope

M. Sholl; M. Lampton; G. Aldering; W. Althouse; R. Amanullah; J. Annis; P. Astier; C. Baltay; E. Barrelet; S. Basa; C. Bebek; L. Bergström; G. Bernstein; M. Bester; B. Bigelow; R. Blandford; R. Bohlin; A. Bonissent; C. Bower; M. Brown; M. Campbell; W. Carithers; E. Commins; W. Craig; C. Day; F. DeJongh; S. Deustua; T. Diehl; S. Dodelson; A. Ealet; R. Ellis; W. Emmet; D. Fouchez; J. Frieman; A. Fruchter; D. Gerdes; L. Gladney; G. Goldhaber; A. Goobar; D. Groom; H. Heetderks; M. Hoff; S. Holland; M. Huffer; L. Hui; D. Huterer; B. Jain; P. Jelinsky; A. Karcher; S. Kahn; S. Kent; A. Kim; W. Kolbe; B. Krieger; G. Kushner; N. Kuznetsova; R. Lafever; J. Lamoureux; O. Le Fèvre; M. Levi; P. Limon; H. Lin; E. Linder; S. Loken; W. Lorenzon; R. Malina; J. Marriner; P. Marshall; R. Massey; A. Mazure; T. McKay; S. McKee; R. Miquel; N. Morgan; E. Mörtsell; N. Mostek; S. Mufson; J. Musser; P. Nugent; H. Oluşeyi; R. Pain; N. Palaio; D. Pankow; J. Peoples; S. Perlmutter; E. Prieto; D. Rabinowitz; A. Refregier; J. Rhodes; N. Roe; D. Rusin; V. Scarpine; M. Schubnell; G. Smadja; R. M. Smith; G. Smoot; J. Snyder; A. Spadafora; A. Stebbins; C. Stoughton; A. Szymkowiak; G. Tarlé; K. Taylor; A. Tilquin; A. Tomasch; D. Tucker; D. Vincent; H. von der Lippe; J. P. Walder; G. Wang; W. Wester

doi:10.1117/12.552081

Snap telescope

M. Sholl^*
, M. Lampton
, G. Aldering
, W. Althouse
, R. Amanullah
, J. Annis
, P. Astier
, C. Baltay
, E. Barrelet
, S. Basa
, C. Bebek
, L. Bergström
, G. Bernstein
, M. Bester
, B. Bigelow
, R. Blandford
, R. Bohlin
, A. Bonissent
, C. Bower
, M. Brown

M. Campbell, W. Carithers, E. Commins, W. Craig, C. Day, F. DeJongh, S. Deustua, T. Diehl, S. Dodelson, A. Ealet, R. Ellis, W. Emmet, D. Fouchez, J. Frieman, A. Fruchter, D. Gerdes, L. Gladney, G. Goldhaber, A. Goobar, D. Groom, H. Heetderks, M. Hoff, S. Holland, M. Huffer, L. Hui, D. Huterer, B. Jain, P. Jelinsky, A. Karcher, S. Kahn, S. Kent, A. Kim, W. Kolbe, B. Krieger, G. Kushner, N. Kuznetsova, R. Lafever, J. Lamoureux, O. Le Fèvre, M. Levi, P. Limon, H. Lin, E. Linder, S. Loken, W. Lorenzon, R. Malina, J. Marriner, P. Marshall, R. Massey, A. Mazure, T. McKay, S. McKee, R. Miquel, N. Morgan, E. Mörtsell, N. Mostek, S. Mufson, J. Musser, P. Nugent, H. Oluşeyi, R. Pain, N. Palaio, D. Pankow, J. Peoples, S. Perlmutter, E. Prieto, D. Rabinowitz, A. Refregier, J. Rhodes, N. Roe, D. Rusin, V. Scarpine, M. Schubnell, G. Smadja, R. M. Smith, G. Smoot, J. Snyder, A. Spadafora, A. Stebbins, C. Stoughton, A. Szymkowiak, G. Tarlé, K. Taylor, A. Tilquin, A. Tomasch, D. Tucker, D. Vincent, H. von der Lippe, J. P. Walder, G. Wang, W. Wester

^*Corresponding author for this work

Research output: Contribution to journal › Conference article published in journal › peer-review

21 Citations (Scopus)

Abstract

Mission requirements, the baseline design, and optical systems budgets for the SuperNova/Acceleration Probe (SNAP) telescope are presented. SNAP is a proposed space-based experiment designed to study dark energy and alternate explanations of the acceleration of the universe's expansion by performing a series of complementary systematics-controlled astrophysical measurements. The goals of the mission are a Type la supernova Hubble diagram and a wide-field weak gravitational lensing survey. A 2m widefield three-mirror telescope feeds a focal plane consisting of 36 CCDs and 36 HgCdTe detectors and a high-efficiency, low resolution integral field spectrograph. Details of the maturing optical system, with emphasis on structural stability during terrestrial testing as well as expected environments during operations at L2 are discussed. The overall stray light mitigation system, including illuminated surfaces and visible objects are also presented.

Original language	English
Pages (from-to)	1473-1483
Number of pages	11
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	5487
Issue number	PART 3
DOIs	https://doi.org/10.1117/12.552081
Publication status	Published - 2004
Externally published	Yes
Event	Optical, Infrared, and Millimeter Space Telecopes - Glasgow, United Kingdom Duration: 21 Jun 2004 → 25 Jun 2004

Keywords

Dark energy
Space astronomy
Three-mirror telescopes
Wide-field imaging

Access to Document

10.1117/12.552081

Cite this

Sholl, M., Lampton, M., Aldering, G., Althouse, W., Amanullah, R., Annis, J., Astier, P., Baltay, C., Barrelet, E., Basa, S., Bebek, C., Bergström, L., Bernstein, G., Bester, M., Bigelow, B., Blandford, R., Bohlin, R., Bonissent, A., Bower, C., ... Wester, W. (2004). Snap telescope. Proceedings of SPIE - The International Society for Optical Engineering, 5487(PART 3), 1473-1483. https://doi.org/10.1117/12.552081

@article{cbd048fe9d8d4cc88d3edb0e47ce54a3,

title = "Snap telescope",

abstract = "Mission requirements, the baseline design, and optical systems budgets for the SuperNova/Acceleration Probe (SNAP) telescope are presented. SNAP is a proposed space-based experiment designed to study dark energy and alternate explanations of the acceleration of the universe's expansion by performing a series of complementary systematics-controlled astrophysical measurements. The goals of the mission are a Type la supernova Hubble diagram and a wide-field weak gravitational lensing survey. A 2m widefield three-mirror telescope feeds a focal plane consisting of 36 CCDs and 36 HgCdTe detectors and a high-efficiency, low resolution integral field spectrograph. Details of the maturing optical system, with emphasis on structural stability during terrestrial testing as well as expected environments during operations at L2 are discussed. The overall stray light mitigation system, including illuminated surfaces and visible objects are also presented.",

keywords = "Dark energy, Space astronomy, Three-mirror telescopes, Wide-field imaging",

author = "M. Sholl and M. Lampton and G. Aldering and W. Althouse and R. Amanullah and J. Annis and P. Astier and C. Baltay and E. Barrelet and S. Basa and C. Bebek and L. Bergstr{\"o}m and G. Bernstein and M. Bester and B. Bigelow and R. Blandford and R. Bohlin and A. Bonissent and C. Bower and M. Brown and M. Campbell and W. Carithers and E. Commins and W. Craig and C. Day and F. DeJongh and S. Deustua and T. Diehl and S. Dodelson and A. Ealet and R. Ellis and W. Emmet and D. Fouchez and J. Frieman and A. Fruchter and D. Gerdes and L. Gladney and G. Goldhaber and A. Goobar and D. Groom and H. Heetderks and M. Hoff and S. Holland and M. Huffer and L. Hui and D. Huterer and B. Jain and P. Jelinsky and A. Karcher and S. Kahn and S. Kent and A. Kim and W. Kolbe and B. Krieger and G. Kushner and N. Kuznetsova and R. Lafever and J. Lamoureux and \{Le F{\`e}vre\}, O. and M. Levi and P. Limon and H. Lin and E. Linder and S. Loken and W. Lorenzon and R. Malina and J. Marriner and P. Marshall and R. Massey and A. Mazure and T. McKay and S. McKee and R. Miquel and N. Morgan and E. M{\"o}rtsell and N. Mostek and S. Mufson and J. Musser and P. Nugent and H. Olu{\c s}eyi and R. Pain and N. Palaio and D. Pankow and J. Peoples and S. Perlmutter and E. Prieto and D. Rabinowitz and A. Refregier and J. Rhodes and N. Roe and D. Rusin and V. Scarpine and M. Schubnell and G. Smadja and Smith, \{R. M.\} and G. Smoot and J. Snyder and A. Spadafora and A. Stebbins and C. Stoughton and A. Szymkowiak and G. Tarl{\'e} and K. Taylor and A. Tilquin and A. Tomasch and D. Tucker and D. Vincent and \{von der Lippe\}, H. and Walder, \{J. P.\} and G. Wang and W. Wester",

year = "2004",

doi = "10.1117/12.552081",

language = "English",

volume = "5487",

pages = "1473--1483",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "SPIE",

number = "PART 3",

note = "Optical, Infrared, and Millimeter Space Telecopes ; Conference date: 21-06-2004 Through 25-06-2004",

}

Sholl, M, Lampton, M, Aldering, G, Althouse, W, Amanullah, R, Annis, J, Astier, P, Baltay, C, Barrelet, E, Basa, S, Bebek, C, Bergström, L, Bernstein, G, Bester, M, Bigelow, B, Blandford, R, Bohlin, R, Bonissent, A, Bower, C, Brown, M, Campbell, M, Carithers, W, Commins, E, Craig, W, Day, C, DeJongh, F, Deustua, S, Diehl, T, Dodelson, S, Ealet, A, Ellis, R, Emmet, W, Fouchez, D, Frieman, J, Fruchter, A, Gerdes, D, Gladney, L, Goldhaber, G, Goobar, A, Groom, D, Heetderks, H, Hoff, M, Holland, S, Huffer, M, Hui, L, Huterer, D, Jain, B, Jelinsky, P, Karcher, A, Kahn, S, Kent, S, Kim, A, Kolbe, W, Krieger, B, Kushner, G, Kuznetsova, N, Lafever, R, Lamoureux, J, Le Fèvre, O, Levi, M, Limon, P, Lin, H, Linder, E, Loken, S, Lorenzon, W, Malina, R, Marriner, J, Marshall, P, Massey, R, Mazure, A, McKay, T, McKee, S, Miquel, R, Morgan, N, Mörtsell, E, Mostek, N, Mufson, S, Musser, J, Nugent, P, Oluşeyi, H, Pain, R, Palaio, N, Pankow, D, Peoples, J, Perlmutter, S, Prieto, E, Rabinowitz, D, Refregier, A, Rhodes, J, Roe, N, Rusin, D, Scarpine, V, Schubnell, M, Smadja, G, Smith, RM, Smoot, G, Snyder, J, Spadafora, A, Stebbins, A, Stoughton, C, Szymkowiak, A, Tarlé, G, Taylor, K, Tilquin, A, Tomasch, A, Tucker, D, Vincent, D, von der Lippe, H, Walder, JP, Wang, G & Wester, W 2004, 'Snap telescope', Proceedings of SPIE - The International Society for Optical Engineering, vol. 5487, no. PART 3, pp. 1473-1483. https://doi.org/10.1117/12.552081

TY - JOUR

T1 - Snap telescope

AU - Sholl, M.

AU - Lampton, M.

AU - Aldering, G.

AU - Althouse, W.

AU - Amanullah, R.

AU - Annis, J.

AU - Astier, P.

AU - Baltay, C.

AU - Barrelet, E.

AU - Basa, S.

AU - Bebek, C.

AU - Bergström, L.

AU - Bernstein, G.

AU - Bester, M.

AU - Bigelow, B.

AU - Blandford, R.

AU - Bohlin, R.

AU - Bonissent, A.

AU - Bower, C.

AU - Brown, M.

AU - Campbell, M.

AU - Carithers, W.

AU - Commins, E.

AU - Craig, W.

AU - Day, C.

AU - DeJongh, F.

AU - Deustua, S.

AU - Diehl, T.

AU - Dodelson, S.

AU - Ealet, A.

AU - Ellis, R.

AU - Emmet, W.

AU - Fouchez, D.

AU - Frieman, J.

AU - Fruchter, A.

AU - Gerdes, D.

AU - Gladney, L.

AU - Goldhaber, G.

AU - Goobar, A.

AU - Groom, D.

AU - Heetderks, H.

AU - Hoff, M.

AU - Holland, S.

AU - Huffer, M.

AU - Hui, L.

AU - Huterer, D.

AU - Jain, B.

AU - Jelinsky, P.

AU - Karcher, A.

AU - Kahn, S.

AU - Kent, S.

AU - Kim, A.

AU - Kolbe, W.

AU - Krieger, B.

AU - Kushner, G.

AU - Kuznetsova, N.

AU - Lafever, R.

AU - Lamoureux, J.

AU - Le Fèvre, O.

AU - Levi, M.

AU - Limon, P.

AU - Lin, H.

AU - Linder, E.

AU - Loken, S.

AU - Lorenzon, W.

AU - Malina, R.

AU - Marriner, J.

AU - Marshall, P.

AU - Massey, R.

AU - Mazure, A.

AU - McKay, T.

AU - McKee, S.

AU - Miquel, R.

AU - Morgan, N.

AU - Mörtsell, E.

AU - Mostek, N.

AU - Mufson, S.

AU - Musser, J.

AU - Nugent, P.

AU - Oluşeyi, H.

AU - Pain, R.

AU - Palaio, N.

AU - Pankow, D.

AU - Peoples, J.

AU - Perlmutter, S.

AU - Prieto, E.

AU - Rabinowitz, D.

AU - Refregier, A.

AU - Rhodes, J.

AU - Roe, N.

AU - Rusin, D.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Smadja, G.

AU - Smith, R. M.

AU - Smoot, G.

AU - Snyder, J.

AU - Spadafora, A.

AU - Stebbins, A.

AU - Stoughton, C.

AU - Szymkowiak, A.

AU - Tarlé, G.

AU - Taylor, K.

AU - Tilquin, A.

AU - Tomasch, A.

AU - Tucker, D.

AU - Vincent, D.

AU - von der Lippe, H.

AU - Walder, J. P.

AU - Wang, G.

AU - Wester, W.

PY - 2004

Y1 - 2004

N2 - Mission requirements, the baseline design, and optical systems budgets for the SuperNova/Acceleration Probe (SNAP) telescope are presented. SNAP is a proposed space-based experiment designed to study dark energy and alternate explanations of the acceleration of the universe's expansion by performing a series of complementary systematics-controlled astrophysical measurements. The goals of the mission are a Type la supernova Hubble diagram and a wide-field weak gravitational lensing survey. A 2m widefield three-mirror telescope feeds a focal plane consisting of 36 CCDs and 36 HgCdTe detectors and a high-efficiency, low resolution integral field spectrograph. Details of the maturing optical system, with emphasis on structural stability during terrestrial testing as well as expected environments during operations at L2 are discussed. The overall stray light mitigation system, including illuminated surfaces and visible objects are also presented.

AB - Mission requirements, the baseline design, and optical systems budgets for the SuperNova/Acceleration Probe (SNAP) telescope are presented. SNAP is a proposed space-based experiment designed to study dark energy and alternate explanations of the acceleration of the universe's expansion by performing a series of complementary systematics-controlled astrophysical measurements. The goals of the mission are a Type la supernova Hubble diagram and a wide-field weak gravitational lensing survey. A 2m widefield three-mirror telescope feeds a focal plane consisting of 36 CCDs and 36 HgCdTe detectors and a high-efficiency, low resolution integral field spectrograph. Details of the maturing optical system, with emphasis on structural stability during terrestrial testing as well as expected environments during operations at L2 are discussed. The overall stray light mitigation system, including illuminated surfaces and visible objects are also presented.

KW - Dark energy

KW - Space astronomy

KW - Three-mirror telescopes

KW - Wide-field imaging

UR - https://www.webofscience.com/wos/woscc/full-record/WOS:000225098600145

UR - https://openalex.org/W4234694014

U2 - 10.1117/12.552081

DO - 10.1117/12.552081

M3 - Conference article published in journal

SN - 0277-786X

VL - 5487

SP - 1473

EP - 1483

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

IS - PART 3

T2 - Optical, Infrared, and Millimeter Space Telecopes

Y2 - 21 June 2004 through 25 June 2004

ER -

Snap telescope

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this