GravityCam: Wide-field high-resolution high-cadence imaging surveys in the visible from the ground
GravityCam: Wide-field high-resolution high-cadence imaging surveys in the visible from the ground
 
  GravityCam is a new concept of ground-based imaging instrument capable of delivering significantly sharper images from the ground than is normally possible without adaptive optics. Advances in optical and near-infrared imaging technologies allow images to be acquired at high speed without significant noise penalty. Aligning these images before they are combined can yield a 2.5–3-fold improvement in image resolution. By using arrays of such detectors, survey fields may be as wide as the telescope optics allows. Consequently, GravityCam enables both wide-field high-resolution imaging and high-speed photometry. We describe the instrument and detail its application to provide demographics of planets and satellites down to Lunar mass (or even below) across the Milky Way. GravityCam is also suited to improve the quality of weak shear studies of dark matter distribution in distant clusters of galaxies and multiwavelength follow-ups of background sources that are strongly lensed by galaxy clusters. The photometric data arising from an extensive microlensing survey will also be useful for asteroseismology studies, while GravityCam can be used to monitor fast multiwavelength flaring in accreting compact objects and promises to generate a unique data set on the population of the Kuiper belt and possibly the Oort cloud.
  
  
  
    
      Mackay, C.
      
        b7bc8866-cfd1-4e97-8fe4-d9e90c3446bd
      
     
  
    
      Dominik, M.
      
        511df084-2aed-4be1-8f2b-6f1a11aa2e6a
      
     
  
    
      Steele, I. A.
      
        f1e6f218-4a2b-4a00-a8f9-93a8ce35c797
      
     
  
    
      Snodgrass, C.
      
        df71f691-52e9-46d7-9ac4-3652a94ba770
      
     
  
    
      Jørgensen, U. G.
      
        29f05d39-ebe1-4eaa-972b-d001363d89ac
      
     
  
    
      Skottfelt, J.
      
        8f42cacd-0261-4caa-9877-2219c8e47033
      
     
  
    
      Stefanov, K.
      
        39d95914-dbb7-450b-9b9a-fbe6cfa6a16d
      
     
  
    
      Carry, B.
      
        d4cdf027-07ed-4e2a-9e6c-2625fa42bca4
      
     
  
    
      Braga-ribas, F.
      
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      Doressoundiram, A.
      
        adeac4e8-69a5-4cc8-9c2e-e8b045fb219f
      
     
  
    
      Ivanov, V. D.
      
        3d83ff7c-b4ce-4abd-8ffc-db071c17fecd
      
     
  
    
      Gandhi, P.
      
        5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
      
     
  
    
      Evans, D. F.
      
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      Hundertmark, M.
      
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      Serjeant, S.
      
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      Ortolani, S.
      
        91b3ef88-3a14-434e-8074-374fa74f8c90
      
     
  
  
   
  
  
    
    
  
    
      27 December 2018
    
    
  
  
    
      Mackay, C.
      
        b7bc8866-cfd1-4e97-8fe4-d9e90c3446bd
      
     
  
    
      Dominik, M.
      
        511df084-2aed-4be1-8f2b-6f1a11aa2e6a
      
     
  
    
      Steele, I. A.
      
        f1e6f218-4a2b-4a00-a8f9-93a8ce35c797
      
     
  
    
      Snodgrass, C.
      
        df71f691-52e9-46d7-9ac4-3652a94ba770
      
     
  
    
      Jørgensen, U. G.
      
        29f05d39-ebe1-4eaa-972b-d001363d89ac
      
     
  
    
      Skottfelt, J.
      
        8f42cacd-0261-4caa-9877-2219c8e47033
      
     
  
    
      Stefanov, K.
      
        39d95914-dbb7-450b-9b9a-fbe6cfa6a16d
      
     
  
    
      Carry, B.
      
        d4cdf027-07ed-4e2a-9e6c-2625fa42bca4
      
     
  
    
      Braga-ribas, F.
      
        d033f603-3513-4334-beee-2297a402f274
      
     
  
    
      Doressoundiram, A.
      
        adeac4e8-69a5-4cc8-9c2e-e8b045fb219f
      
     
  
    
      Ivanov, V. D.
      
        3d83ff7c-b4ce-4abd-8ffc-db071c17fecd
      
     
  
    
      Gandhi, P.
      
        5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
      
     
  
    
      Evans, D. F.
      
        dfeb0026-de4d-482c-a3c6-df64357e90b0
      
     
  
    
      Hundertmark, M.
      
        bcdee73a-d510-413c-98ab-aec4609b1079
      
     
  
    
      Serjeant, S.
      
        694633e3-bd1f-42f1-b04d-2b5d6cc186b9
      
     
  
    
      Ortolani, S.
      
        91b3ef88-3a14-434e-8074-374fa74f8c90
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Mackay, C., Dominik, M., Steele, I. A., Snodgrass, C., Jørgensen, U. G., Skottfelt, J., Stefanov, K., Carry, B., Braga-ribas, F., Doressoundiram, A., Ivanov, V. D., Gandhi, P., Evans, D. F., Hundertmark, M., Serjeant, S. and Ortolani, S.
  
  
  
  
   
    (2018)
  
  
    
    GravityCam: Wide-field high-resolution high-cadence imaging surveys in the visible from the ground.
  
  
  
  
    Publications of the Astronomical Society of Australia, 35, [e047].
  
   (doi:10.1017/pasa.2018.43). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          GravityCam is a new concept of ground-based imaging instrument capable of delivering significantly sharper images from the ground than is normally possible without adaptive optics. Advances in optical and near-infrared imaging technologies allow images to be acquired at high speed without significant noise penalty. Aligning these images before they are combined can yield a 2.5–3-fold improvement in image resolution. By using arrays of such detectors, survey fields may be as wide as the telescope optics allows. Consequently, GravityCam enables both wide-field high-resolution imaging and high-speed photometry. We describe the instrument and detail its application to provide demographics of planets and satellites down to Lunar mass (or even below) across the Milky Way. GravityCam is also suited to improve the quality of weak shear studies of dark matter distribution in distant clusters of galaxies and multiwavelength follow-ups of background sources that are strongly lensed by galaxy clusters. The photometric data arising from an extensive microlensing survey will also be useful for asteroseismology studies, while GravityCam can be used to monitor fast multiwavelength flaring in accreting compact objects and promises to generate a unique data set on the population of the Kuiper belt and possibly the Oort cloud.
         
      
      
        
          
            
  
    Text
 GravityCam- Wide Field High Resolution
     - Accepted Manuscript
   
  
  
    
  
 
          
            
          
            
           
            
           
        
        
       
    
   
  
  
  More information
  
    
      Accepted/In Press date: 25 September 2018
 
    
      Published date: 27 December 2018
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 427939
        URI: http://eprints.soton.ac.uk/id/eprint/427939
        
          
        
        
        
          ISSN: 1323-3580
        
        
          PURE UUID: 2a4fc7ac-cdf1-4e6a-898b-e5f68eb0528e
        
  
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
  
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  Date deposited: 05 Feb 2019 17:30
  Last modified: 16 Mar 2024 04:20
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      Contributors
      
          
          Author:
          
            
            
              C. Mackay
            
          
        
      
          
          Author:
          
            
            
              M. Dominik
            
          
        
      
          
          Author:
          
            
            
              I. A. Steele
            
          
        
      
          
          Author:
          
            
            
              C. Snodgrass
            
          
        
      
          
          Author:
          
            
            
              U. G. Jørgensen
            
          
        
      
          
          Author:
          
            
            
              J. Skottfelt
            
          
        
      
          
          Author:
          
            
            
              K. Stefanov
            
          
        
      
          
          Author:
          
            
            
              B. Carry
            
          
        
      
          
          Author:
          
            
            
              F. Braga-ribas
            
          
        
      
          
          Author:
          
            
            
              A. Doressoundiram
            
          
        
      
          
          Author:
          
            
            
              V. D. Ivanov
            
          
        
      
        
      
          
          Author:
          
            
            
              D. F. Evans
            
          
        
      
          
          Author:
          
            
            
              M. Hundertmark
            
          
        
      
          
          Author:
          
            
            
              S. Serjeant
            
          
        
      
          
          Author:
          
            
            
              S. Ortolani
            
          
        
      
      
      
    
  
   
  
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