Stabilized dispersive focal plane systems for space

As the costs of space missions continue to rise, the demand for compact, low mass, low-cost technologies that maintain high reliability and facilitate high performance is increasing. One such technology is the stabilized dispersive focal plane system (SDFPS). This technology provides image stabilization while simultaneously delivering spectroscopic or direct imaging functionality using only a single optical path and detector. Typical systems require multiple expensive optical trains and/or detectors, sometimes at the expense of photon throughput. The SDFPS is ideal for performing wide-field low-resolution space-based spectroscopic and direct-imaging surveys. In preparation for a suborbital flight, we have built and ground tested a prototype SDFPS that will concurrently eliminate unwanted image blurring due to the lack of adequate platform stability, while producing images in both spectroscopic and direct-imaging modes. We present the overall design, testing results, and potential scientific applications.

[1]  O. Fèvre,et al.  The Canada-France Redshift Survey: The Luminosity Density and Star Formation History of the Universe to z ~ 1 , 1996, astro-ph/9601050.

[2]  Sven G. Bilen,et al.  Joint astrophysics nascent universe satellite: Utilizing GRBs as high redshift probes , 2012 .

[3]  D. E. Trilling,et al.  The Substellar Mass Function: A Bayesian Approach , 2005, astro-ph/0502189.

[4]  Daniel J. Eisenstein,et al.  Luminosity Function Constraints on the Evolution of Massive Red Galaxies since z ~ 0.9 , 2008, 0804.4516.

[5]  Derek B. Fox,et al.  The Joint Astrophysics Nascent Universe Satellite , 2008 .

[6]  R. L. Smart,et al.  THE PHYSICAL PROPERTIES OF FOUR ∼600 K T DWARFS , 2009, 0901.4093.

[7]  A. Szalay,et al.  The Sloan Digital Sky Survey Quasar Survey: Quasar Luminosity Function from Data Release 3 , 2006, astro-ph/0601434.

[8]  David A. Golimowski,et al.  A Unified Near-Infrared Spectral Classification Scheme for T Dwarfs , 2006 .

[9]  Arjun Dey,et al.  The 1 < z < 5 Infrared Luminosity Function of Type I Quasars , 2005, astro-ph/0510504.

[10]  P. Capak,et al.  The Evolution of the Ultraluminous Infrared Galaxy Population from Redshift 0 to 1.5 , 2004 .

[11]  I. Neill Reid M dwarfs, L dwarfs, T dwarfs and subdwarfs: Psi(Mu) at and below the hydrogen-burning limit , 1999 .

[12]  A. Fruchter,et al.  HIGH-REDSHIFT GALAXIES IN THE HUBBLE DEEP FIELD : COLOUR SELECTION AND STAR FORMATION HISTORY TO Z 4 , 1996, astro-ph/9607172.

[13]  Lennox L. Cowie,et al.  The Evolution of the Distribution of Star Formation Rates in Galaxies , 1997, astro-ph/9702235.

[14]  UK,et al.  TIDALLY INDUCED BROWN DWARF AND PLANET FORMATION IN CIRCUMSTELLAR DISKS , 2010, 1005.3017.

[15]  I. Smail,et al.  The 2df SDSS LRG and QSO survey: evolution of the luminosity function of luminous red galaxies to z= 0.6 , 2006, astro-ph/0607629.

[16]  A. Szalay,et al.  Galaxy Luminosity Functions to z~1 from DEEP2 and COMBO-17: Implications for Red Galaxy Formation , 2005, astro-ph/0506044.

[17]  Stewart Sharpless,et al.  The Infrared Spectral Classification of M-Type Stars. , 1956 .