eso metis hires · M4-M6 [Rsunl 1.00 0.49 0.19 1.00 0.49 0.19 awz 1.000 0.203 0.058 Prob 0.47 1.12...

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The technique of highdispersion spectroscopy First successes using CRIRES@VLT Unique ELT Science in the JWST era Ignas Snellen, Leiden Observatory

Transcript of eso metis hires · M4-M6 [Rsunl 1.00 0.49 0.19 1.00 0.49 0.19 awz 1.000 0.203 0.058 Prob 0.47 1.12...

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  The  technique  of  high-­‐dispersion  spectroscopy  

  First  successes  using  CRIRES@VLT  

  Unique  ELT  Science  in  the  JWST  era  

Ignas  Snellen,  Leiden  Observatory  

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transmission  spectroscopy  

eclipse    spectroscopy  

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• At  R=100,000  molecular  bands  are  resolved  in  tens  of  individual  lines  

• Strong  doppler  effects    due  the  orbital  motion  of  the  planet  (up  to    >150  km/s).  

• Moving  planet  lines  can  be  distinguished  from  stationary  telluric  +  stellar  lines    

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Observing  philosophy:  no  external  calibration    removal  of  telluric  features  by  “self  calibration”  Retrieve  signal  by  combining  lines  through  cross-­‐correlation    

CRIRES    

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•  Reveals  planet  orbital  velocity  •  Solves  for  masses  of  both  planet  and  star  (model  independent)  •  Evidence  for  blueshift  (high  altitude  winds?)  

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~2  km/s  (2σ)  blueshift  wrt  the  systemic  velocity  

Winds  from  day-­‐  to  nightside  

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Brogi  et  al.,  Nature  2012  

First  detection  of  non-­‐transiting  planet  inclination,  mass  

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But,  no  detection  in  third  night    weather  or  instrumental  issue??  

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Seager  &  Deming  

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Showman  et  al.  2012  

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Cho  et  al.  2003  

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12C16O  

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SNR  for  ELT  in  1  transit    Brightest  expected  systems  

Snellen  et  al.  2013  

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Read  more  about  the  high-­‐res  oxygen  science  case:  

Snellen  et  al.,  ApJ  764,  182  (ArXiv:1302.3251)