Abstract:
The invention disclosed here teaches methods to fabricate and utilize a non-dispersive holographic wavelength blocker. The invention enables the observation of the Raman signal near the excitation wavelength (˜9 cm −1 ) with the compactness of standard thin film/holographic notch filter. The novelty is contacting several individual volume holographic blocking notch filter (VHBF) to form one high optical density blocking filter without creating spurious multiple diffractions that degrade the filter performance. Such ultra-narrow-band VHBF can be used in existing compact Raman instruments and thus will help bring high-end research to a greater number of users at a lower cost.

Description:
RELATED APPLICATION 
       [0001]    The present patent application is a continuation and claims the priority benefit of U.S. patent application Ser. No. 12/315,470 filed Dec. 3, 2008, which claims the priority benefit of U.S. provisional patent application No. 61/137,871 filed on Aug. 4, 2008, the disclosures of which are incorporated by reference herein in their entirety. 
     
    
     BACKGROUND OF THE INVENTION 
       [0002]    1. Field of the Invention 
         [0003]    The present invention relates to a method and apparatus for fabricating and using volume holographic wavelength blockers of high optical density and narrow bandwidth. Wavelength blockers are used to attenuate the signal of a pump source such as lasers while letting a scattering signal such as but not limited to fluorescence or Raman to go through. Thick reflective volume holographic elements (&gt;typ. 0.1 mm thickness) have narrow rejection band but have limited attenuation of the order of optical density of 1 to 2. It is desirable to have a narrow spectral band rejection in conjunction with high attenuation reaching at least an optical density 6 for Raman spectroscopy for example. 
         [0004]    Portions of the disclosure of this patent document contain material that is subject to copyright protection. The copyright owner has no objection to the facsimile reproduction by anyone of the patent document or the patent disclosure as it appears in the Patent and Trademark Office file or records, but otherwise reserves all copyright rights whatsoever. 
         [0005]    2. Background Art 
         [0006]    Wavelength blockers, also called notch rejection filters, are an essential component in Raman and fluorescence instruments. The purpose of the wavelength blocker is to greatly attenuate the backscattered light from the laser illuminating a sample under test, while letting the faint Raman spectrally shifted signature pass through. Two non-dispersive filter technologies are currently used for the wavelength blocker: holographic and thin film. Commercial holographic notch filter technology uses holographic recording in a thin film of dichromated gelatin to produce a notch filter with 3 dB bandwidth of 350 cm −1  and optical density of 6. Commercial thin film technology uses deposition of many layers to obtain a 3 dB bandwidth of approximately 600 cm −1  and optical density of 6. Both technologies provide a compact size wavelength blocker element with a 10 mm aperture diameter and several millimeters thickness. However both notch filter technologies are limited to observing Raman spectral shift above approximately 350 cm −1 . 
         [0007]    The Raman signal in the low frequency shift region, i.e near the frequency of the excitation laser, contains critical information about the molecular structure. For example carbon nanotubes exhibit vibration modes in the range of 150 cm −1  to 200 cm −1  depending on their size. Relaxation in liquids, solutions and biological samples exhibit Raman shift in the range between 0 and 400 cm −1 . U.S. Pat. Nos. 5,684,611 and 5,691,989 describe the use of reflective volume holographic filters (VHG) with millimeters thickness as filters producing 3 dB bandwidth of the order of 10 cm −1 . VHGs produced in a glass material are now commercially available and show long lifetime, high efficiency and excellent transmission in the red and near infrared. The photosensitive glass can contain for example silicon oxide, aluminum oxide and zinc oxide, fluorine, silver, chlorine, bromine and iodine, cerium oxide. Composition and processes for manufacturing the photosensitive glass are described in U.S. Pat. No. 4,057,408, the disclosure of which is incorporated herein by reference. Large area (30×30 mm) reflective VHGs are restricted to the millimeter range thickness due to the material absorption. The optical density (O.D) achievable is therefore limited to O.D near unity (i.e ˜90% efficiency) with thickness of 1.5 mm and transmission of 97 to 98% away from the notch in the near infrared. 
         [0008]    By carefully individually aligning a cascade of VHGs, researchers have shown that the optical density can be added up: a cascade of 4 VHGs with each exhibiting an optical density of one yields a compounded notch with an optical density of 4. Commercial instruments comprising individual alignment fixtures for each VHG exhibit an optical density ranging from 4 to 6 with bandwidth of 10 cm −1 . However, there are several drawbacks to this approach: 
         [0009]    1. The alignment procedure is complicated and required for each VHG separately. 
         [0010]    2. The footprint is large (˜100 cm 3 ) and as such not suitable to replace standard notch filters in existing Raman instruments. 
         [0011]    3. The surface of each VHG contributes to Fresnel reflection loss. 
         [0012]    4. Upon rotation of the assembly, the individual VHGs spectrally shift at different rates, thus reducing severely the optical density and broadening the overall blocker bandwidth. 
         [0013]    The technology utilized to observe the Raman signal close to the laser excitation (&gt;9 cm −1 ) is based on cascading dispersive spectrometers. The cascaded spectrometers are bulky (˜1 m 2 ), expensive (˜$100K) and of moderate transmission (˜50%). 
       SUMMARY OF THE INVENTION 
       [0014]    The invention disclosed here teaches methods to fabricate and utilize a non-dispersive holographic wavelength blocker to overcome all the limitations outlined above. The invention enables the observation of the Raman signal near the excitation wavelength (˜9 cm −1 ) with the compactness of standard thin film/holographic notch filter. The novelty is contacting several individual volume holographic blocking notch filter (VHBF) to form one high optical density blocking filter without creating the spurious multiple diffractions that yield unacceptable rejection ratios. Such ultra-narrow-band VHBF can be used in existing compact Raman instruments and thus will help bring high-end research to a greater number of users at a lower cost. 
     
    
     
       BRIEF DESCRIPTION OF THE DRAWINGS 
         [0015]    These and other features, aspects and advantages of the present invention will become better understood with regard to the following description, appended claims and accompanying drawings where: 
           [0016]      FIG. 1 : Grating wave vector representation of four slanted reflective VHBF diffracting the same wavelength. 
           [0017]      FIG. 2A ,  2 B: Illustration of stacked reflective VHBF assembly. 
           [0018]      FIG. 3 : Illustration for tuning the Bragg wavelength of each VHG in the VHBF assembly. 
           [0019]      FIG. 4 : Plot of a typical angular selectivity of one VHG in the VHBF stack. 
           [0020]      FIG. 5A ,  5 B: Spectral response of a VHBF assembly showing addition of optical densities. 
           [0021]      FIG. 6A ,  6 B: Plot showing wavelength tuning of the VHBF assembly and spectral transmission between 700 and 1000 nm. 
           [0022]      FIG. 7A ,  7 B: Illustration of an ASE filtered laser source and a plot of an ASE suppressed laser diode spectrum. 
           [0023]      FIG. 8 : Plot showing the optical density of 6 achieved with a VHBF assembly of 6 VHGs. 
           [0024]      FIG. 9 : Illustration of a feedback loop for the keep the VHBF assembly aligned to the laser frequency for maintaining maximum optical density. 
           [0025]      FIG. 10 : Illustration of a Raman apparatus using a VHBF assembly and an ASE suppressed laser excitation source. 
           [0026]      FIG. 11 : Illustration of a Raman spectrometer incorporating the ASE function, the blocker function, the dichroic filter function in one glass holographic wafer. 
           [0027]      FIG. 12 : Same as  FIG. 11 , except that the laser is incorporated in the doped holographic wafer. 
       
    
    
     DETAILED DESCRIPTION OF THE INVENTION 
       [0028]    In the following description of the present invention, reference is made to the accompanying drawings which form a part hereof, and in which is shown by way of illustration a specific embodiment in which the invention may be practiced. It is to be understood that other embodiments may be utilized and structural changes may be made without departing from the scope of the present invention. 
         [0029]    The notch wavelength λ B  of a reflective VHG is characterized by the grating period Λ and the angle of incidence Θ of the collimated illumination on the grating planes: 
         [0000]      λ B =λ o ·cos(Θ),  (1)
 
         [0000]    where λ o =2·n·Λ is the anti-parallel diffraction wavelength where n the index of refraction. 
         [0030]    Identical reflection VHGs, i.e. VHGs characterized by the same grating period Λ and incidence angle Θ cannot simply be stacked since the diffracted beams will fulfill the Bragg condition for other VHGs in the stack. Double diffraction on individual VHGs will cause interference effects and prevent the optical density values to be simply added. 
         [0031]    However, by varying the grating slant (the angle between the grating vector and the VHG surface normal) and the grating spacing, Λ of each individual VHG in such a way that the same wavelength fulfills the Bragg condition for each VHG, the diffracted light from subsequent VHGs does not full fill the Bragg condition on any other grating.  FIG. 1  illustrates an embodiment of the construction for a stack of four VHGs. The incident light beam  100  is represented in grating vector space. The grating vectors  110 ,  120 ,  130  and  140  each have a specific direction and amplitude and are represented in one plane for simplicity of the explanation. The diffracted beams  112 ,  122 ,  132  and  142  corresponding respectively to the four slanted VHGs diffract the same wavelength but propagate in different directions given respectively by the angles  115 ,  125 ,  135  and  145  and thus the diffracted beams do not interfere or re-diffract with the other gratings. 
         [0032]    In one embodiment each VHG may be physically separated for example, but not limited to, spacers as  FIG. 2A  illustrates. In another embodiment each VHG maybe physically contacted for example, but limited to, with an index matching epoxy as  FIG. 2B  illustrates. The invention is not limited to stacking three VHGs but rather the drawing in  FIGS. 2A and 2B  uses three VHBFs for simplicity. The number of VHGs comprising a VHBF is limited by the total transmission achievable. 
         [0033]    For the following analysis, we will assume that the collimated incident beam wave vector outside the material is parallel to the z-axis as  FIG. 3  illustrates. The incident collimated beam  311  propagates in the direction of the z-axis: {right arrow over (k)} air =k air {right arrow over (e)} z . We will allow a grating slant φ (angle between grating vector and surface normal) only in the x-z plane. We assume that the illumination is of single frequency. The laser wavelength is chosen slightly below the normal incidence wavelength of each VHG in the stack. 
         [0034]    Following the illustration in  FIG. 2 , the first VHG is positioned with its grating vector {right arrow over (K)} ( 310 ) in the x-z plane and rotated around the x-axis to fulfill the Bragg condition according to equation (1). the facet normal of the first VHG defines the incidence angle Θ M  of the entire stack with respect to the collimated illumination direction {right arrow over (k)} air . The orientation of the facet normal of subsequent VHGs with respect to the incident beam, i.e. Θ M  are collinear with each other since we assume the VHG in the stack are in mechanical contact. 
         [0035]    For the subsequent VHGs after the first one, fine wavelength tuning is achieved by rotating the VHG around its surface normal, the only degree of freedom left, by an angle ω. 
         [0036]    Using Snell&#39;s law the incident beam wave vector in the material is: 
         [0000]    
       
         
           
             
               
                 
                   
                     
                       k 
                       -&gt; 
                     
                     = 
                     
                       
                         
                           k 
                            
                           
                             ( 
                             
                               
                                 
                                   0 
                                 
                               
                               
                                 
                                   
                                     - 
                                     
                                       sin 
                                       ( 
                                       
                                           
                                       
                                        
                                       
                                         
                                           Θ 
                                           x 
                                         
                                         - 
                                         
                                           Θ 
                                           M 
                                         
                                       
                                       ) 
                                     
                                   
                                 
                               
                               
                                 
                                   
                                     cos 
                                      
                                     
                                       ( 
                                       
                                         
                                           Θ 
                                           x 
                                         
                                         - 
                                         
                                           Θ 
                                           M 
                                         
                                       
                                       ) 
                                     
                                   
                                 
                               
                             
                             ) 
                           
                         
                          
                         
                             
                         
                          
                         with 
                          
                         
                             
                         
                          
                         
                           Θ 
                           M 
                         
                       
                       = 
                       
                         asin 
                          
                         
                           ( 
                           
                             
                               sin 
                                
                               
                                 ( 
                                 
                                   Θ 
                                   x 
                                 
                                 ) 
                               
                             
                             / 
                             n 
                           
                           ) 
                         
                       
                     
                   
                   , 
                 
               
               
                 
                   ( 
                   2 
                   ) 
                 
               
             
           
         
       
     
         [0000]    where Θ x −Θ M  is the angle between z-axis and {right arrow over (k)} and Θ M  the angle between surface normal and {right arrow over (k)} measured inside the medium. After rotation of the VHG around the x-axis by an angle Θ x , and around the surface normal by angle ω, the VHG&#39;s grating vector {right arrow over (K)} is: 
         [0000]    
       
         
           
             
               
                 
                   
                     K 
                     -&gt; 
                   
                   = 
                   
                     
                       K 
                        
                       
                         ( 
                         
                           
                             
                               
                                 
                                   cos 
                                    
                                   
                                     ( 
                                     ω 
                                     ) 
                                   
                                 
                                  
                                 
                                   sin 
                                    
                                   
                                     ( 
                                     φ 
                                     ) 
                                   
                                 
                               
                             
                           
                           
                             
                               
                                 
                                   
                                     cos 
                                      
                                     
                                       ( 
                                       
                                         Θ 
                                         x 
                                       
                                       ) 
                                     
                                   
                                    
                                   
                                     sin 
                                      
                                     
                                       ( 
                                       ω 
                                       ) 
                                     
                                   
                                    
                                   
                                     sin 
                                      
                                     
                                       ( 
                                       φ 
                                       ) 
                                     
                                   
                                 
                                 - 
                                 
                                   
                                     sin 
                                      
                                     
                                       ( 
                                       
                                         Θ 
                                         x 
                                       
                                       ) 
                                     
                                   
                                    
                                   
                                     cos 
                                      
                                     
                                       ( 
                                       φ 
                                       ) 
                                     
                                   
                                 
                               
                             
                           
                           
                             
                               
                                 
                                   
                                     sin 
                                      
                                     
                                       ( 
                                       
                                         Θ 
                                         x 
                                       
                                       ) 
                                     
                                   
                                    
                                   
                                     sin 
                                      
                                     
                                       ( 
                                       ω 
                                       ) 
                                     
                                   
                                    
                                   
                                     sin 
                                      
                                     
                                       ( 
                                       φ 
                                       ) 
                                     
                                   
                                 
                                 + 
                                 
                                   
                                     cos 
                                      
                                     
                                       ( 
                                       
                                         Θ 
                                         x 
                                       
                                       ) 
                                     
                                   
                                    
                                   
                                     cos 
                                      
                                     
                                       ( 
                                       φ 
                                       ) 
                                     
                                   
                                 
                               
                             
                           
                         
                         ) 
                       
                     
                     . 
                   
                 
               
               
                 
                   ( 
                   3 
                   ) 
                 
               
             
           
         
       
     
         [0037]    Using cos(Θ)={right arrow over (k)}·{right arrow over (K)}/(kK) and equation (3), we find the notch wavelength λ B  as a function of the angles ω and Θ M : 
         [0000]      λ B =λ 0  cos(φ)(cos(Θ M )+sin(Θ M )sin(ω)tan(φ)).  (4)
 
         [0038]    From equation (4), we observe that individual VHGs can be Bragg-matched to the required notch wavelength by adjusting the rotation angles ω i  for each grating i=2, . . . , N. The fine wavelength tuning is only possible when Θ M , φ i &gt;0. 
         [0039]    A typical angular selectivity curve for an individual VHG is given in  FIG. 4 . The angular 3 dB bandwidth is 0.4 degrees. In another embodiment, the slant angle of each VHG is chosen such that the diffracted beams do not satisfy the Bragg condition for all other VHGs. From the measurement shown in  FIG. 4 , a value of at least 1 degree for the slant angle has been selected to satisfy that condition. 
         [0040]    The rejection ratio of the VHBF assembly is the compounded rejection of each VHG in the stack when the alignment procedure outlined in the embodiments above is followed. This is justified because there are no coherent effects between the diffracted beams with the arrangement of the grating wave vector of each VHG described above. An example of spectral response of the notch filter with the VHBF assembly of one and three individual VHBF is shown respectively in  FIGS. 5A and 5B . 
         [0041]    We prepared six individual reflection VHGs with thickness of 1.6 mm and diffraction efficiencies near 90% (corresponding to optical density near unity). Anti-parallel diffraction wavelength and slant angles are given in table 1. 
         [0042]    In one embodiment, each of the successive five VHGs is brought into direct mechanical contact to the previous VHG. After alignment, individual gratings are secured to the stack by an index matching epoxy. This procedure ensures that the internal incident angle Θ M  is the same for every grating in the stack. Only the rotation angle ω i  is used to fine tune the Bragg wavelength. 
         [0043]    The laser used for the alignment is a wavelength locked semi-conductor laser diode at 785.0 nm, which is subsequently ASE filtered by a slanted reflection VHG. Grating #1 is aligned for Bragg diffraction with ω 1 ≈0 and Θ M =2.7 deg. 
         [0000]    
       
         
               
             
               
               
               
               
               
             
           
               
                 TABLE 1 
               
             
             
               
                   
               
               
                 Measured anti-parallel diffraction wavelength λ o,i  , slant angle θ i   
               
               
                 and peak diffraction efficiency η for 6 gratings. Also given 
               
               
                 is the normal incidence wavelength λ o,i  cos(θ i ), which determines the 
               
               
                 tuning range of the final stack. The average normal incidence 
               
               
                 wavelength λ o,i  cos(θ i ) is (785.84 ± 0.069) nm. 
               
             
          
           
               
                 VHG # 
                 λ o,i  [nm] 
                 θ i  [deg] 
                 λ o,i  cos(θ i ) [nm] 
                 η [%] 
               
               
                   
               
               
                 1 
                 785.96 
                 +0.94 
                 785.85 
                 93 
               
               
                 2 
                 786.04 
                 −1.02 
                 785.92 
                 92 
               
               
                 3 
                 786.10 
                 +1.50 
                 785.83 
                 95 
               
               
                 4 
                 786.18 
                 −1.50 
                 785.91 
                 91 
               
               
                 5 
                 786.32 
                 +2.02 
                 785.83 
                 92 
               
               
                 6 
                 786.20 
                 −1.99 
                 785.73 
                 91 
               
               
                   
               
             
          
         
       
     
         [0044]    Now, let&#39;s determine what happens when the stack of bonded VHGs is wavelength tuned. 
         [0045]    In another embodiment, wavelength tuning is performed by varying the incident angle from the initial alignment angle Θ M  to a new incident angle Θ M +ΔΘ M . For all VHGs in the stack, the new notch wavelength will vary according to equation (4) and the difference in wavelength between any two gratings can be computed to be: 
         [0000]    
       
         
           
             
               
                 
                   Δλ 
                   = 
                   
                     
                       ( 
                       
                         
                           
                             λ 
                             
                               o 
                               , 
                               1 
                             
                           
                            
                           
                             cos 
                              
                             
                               ( 
                               
                                 φ 
                                 1 
                               
                               ) 
                             
                           
                         
                         - 
                         
                           
                             λ 
                             
                               o 
                               , 
                               2 
                             
                           
                            
                           
                             cos 
                              
                             
                               ( 
                               
                                 φ 
                                 2 
                               
                               ) 
                             
                           
                         
                       
                       ) 
                     
                      
                     
                       
                         
                           sin 
                            
                           
                             ( 
                             
                               ΔΘ 
                               M 
                             
                             ) 
                           
                         
                         
                           sin 
                            
                           
                             ( 
                             
                               Θ 
                               M 
                             
                             ) 
                           
                         
                       
                       . 
                     
                   
                 
               
               
                 
                   ( 
                   5 
                   ) 
                 
               
             
           
         
       
     
         [0046]    Note that the wavelength shift between any two gratings does not depend on the rotation terms ω i . This is due to the constraint that at the alignment angle Θ M  of the stack, the wavelength shift Δλ is equal to zero. 
         [0047]    Table 1 gives a standard deviation of 0.069 nm for the quantity (λ o,i  cos(φ i )−λ o,j  cos(φ j )). 
         [0048]    The stack of six VHGs was aligned at a value for Θ M  of 2.7 degrees and tuned by ΔΘ M  of 11.4 degrees (these are values inside the material of index n=1.5). According to equation 5, we expect to observe a broadening of the overall bandwidth by 0.29 nm. The experimental result is shown in  FIG. 6A . As expected, the 6-stack wavelength blocker maintains a single transmission notch at all tuning angles. The measured spectral bandwidth broadening is half the computed value (0.14 nm vs. 0.29 nm). 
         [0049]    Light transmission of the six-stack wavelength blocker is measured by a CARY 500 spectrometer. The transmission measurement in  FIG. 6B  shows that the 9.6 mm thick filter stack (6 times 1.6 mm) transmits greater than 80% of the incident light outside the notch. The first and last VHG facets are without anti-reflection (AR) coatings. An additional 8% transmission could be gained by adding an AR coating to the outside facet of the first and last VHG in the stack. 
         [0050]    In another embodiment, the Raman excitation laser light source is a laser whose amplified spontaneous emission is filtered as illustrated in  FIG. 7  A. A laser light source  1000  is collimated by collimating assembly  1010 . A slanted reflective VHG is positioned to receive the collimated beam. The diffracted beam  1030  is the ASE filtered beam. The specularly reflected light beam  1040  is propagating in a different direction. In other embodiments, more than one ASE filter can be used to further reduce the ASE content of the laser. 
         [0051]      FIG. 7B  shows the spectrum of the unfiltered and filtered laser diode measured with an ANDO double spectrometer with 0.05 nm resolution. We observe that the ASE of the original laser diode is drastically reduced. The spectrometer distorts and broadens the actual ASE filtered spectrum due to stray light inside the spectrometer. The optical density of the fabricated stack is measured at 780.7 nm with an ASE filtered single frequency laser light source. 
         [0052]    The collimated light beam of dimension 1 mm×2 mm is incident on the wavelength blocker. The transmitted light is fiber coupled to a multimode fiber and sent to the spectrometer. The result is shown in  FIG. 8 . An attenuation of the laser power of 60 dB, corresponding to an optical density of 6, is achieved. The stack was assembled at a wavelength of 785.1 nm. We have shown that after tuning the stack by 5 nm, an optical density of 6 was maintained. 
         [0053]    Another embodiment in the invention is a means to angularly tune the VHBF assembly so that the Bragg wavelength of the VHBF always tracks the wavelength of the excitation laser in order to obtain maximum optical density (maximum rejection of the excitation light). An example of a tuning mechanism consists of positioning the VHBF on a rotation stage and rotating the stage. A detector is added to receive a portion of the attenuated pump after the VHBF assembly. The signal can be used as feedback to the tuning mechanism.  FIG. 9  illustrates the tuning and feedback mechanism. The VHBF  905  is placed on the rotation stage  910 . The collimated signal  900  is incident on the VHBF  905 . A fraction of the transmitted beam  930  is deflected by the beam-splitter  925  and directed to a photodetector  920 . The electrical signal is processed by a computer or microprocessor  915  and a feedback signal is sent to the rotation stage to minimize to photodetected power. 
         [0054]    Another embodiment is an apparatus that uses the VHBF assembly of the embodiments above as illustrated by  FIG. 10 . A laser source  1003  is collimated and ASE filtered by the assembly  1004 . The ASE filtered beam  1005  is reflected by a dichroic beam-splitter  1010  towards a lens assembly  1000  that focuses the laser beam onto a sample under examination. The dichroic beam-splitter reflects the laser beam and is transparent to other wavelength. In yet another embodiment, the dichroic beam-splitter may be a reflective or transmissive VHG or any other type of narrowband filter. The signal beam generated from the sample as a result of the excitation laser beam (fluorescence, Raman) as well as the backscattering of the laser is recollimated by the same lens assembly  1000 . The signal is transmitted through the dichroic beam-splitter  1010  and incident on the VHBF assembly  1015  that may also include the tuning assembly disclosed in the embodiment above. Further spatial beam filters maybe incorporated in the path of the signal beam to perform a confocal system. After the VHBF assembly, the laser light is rejected and the Raman, fluorescence or any other signal generated by the excitation laser impinges on a dispersive element  1025  such as but not limited to a diffraction grating. The spectrally dispersed signal is then received by an array of photodector  1020 . The array of photodetectors can be one or two dimensional. 
         [0055]    In another embodiment, many of the discrete functions that comprise a standard Raman or fluorescence system, such as laser, ASE filtering, dichroic beam-splitters and wavelength blocker are integrated in a single holographic glass wafer.  FIG. 11  illustrates the embodiment. A laser diode  1100  is collimated to produce collimated beam  1115  which is directed to the entrance facet of a holographic glass wafer  1110 . A grating  1120 , recorded holographically using a transmission geometry, filters the beam  1115  and directs it to an identical grating  1130 , also recorded holographically using a transmission geometry. The role of the grating  1130  is of an ASE filter and dichroic beam-splitter. The ASE filtered beam is then brought to a focus by a lens assembly  1120 . The wavelength blocker is a cascade of VHGs  1140  whose grating vector amplitude and direction are designed to diffract the same wavelength. The VHGs  1140  are recorded holographically with the transmission geometry. The wavelength blocker attenuates the backscattered laser excitation light. The dimension of the holographic wafer is approximately 10 mm by 15 mm and comprises three distinct functions: ASE filtering, dichroic beam-splitter and wavelength blocker. 
         [0056]    After the wavelength blocker a lens assembly  1150  is used in conjunction with an aperture  1160  to perform confocal measurements. The lens assembly  1150  can be, but is not limited to, a cylindrical lens. A compact spectrometer is built in one glass block, which has a cylindrical surface  1161  to collimated the signal to direct it to a dispersive grating  1162 . The spectrally dispersed signal is then capture by an array of photodetectors  1163 . 
         [0057]    In another embodiment illustrated in  FIG. 12 , the laser  1200  is used to pump a doped glass region  1210  (for example but not limited to Neodymium) which is surrounded by two holographically written reflective VHGs that serve as resonators to amplify the doped glass region and provide laser light.