scholarly journals Retrieving the transmission spectrum of HD 209458b using CHOCOLATE: a new chromatic Doppler tomography technique

Author(s):  
E. Esparza-Borges ◽  
M. Oshagh ◽  
N. Casasayas-Barris ◽  
E. Palle ◽  
G. Chen ◽  
...  
2021 ◽  
Author(s):  
Emma Esparza-Borges ◽  
Mahmoud Oshagh ◽  
Nuria Casasayas-Barris ◽  
Enric Pallé

<p>Multi-band photometric transit observations or low resolution spectroscopy (spectro-photometry) are normally used to retrieve the broadband transmission spectra of transiting exoplanets in order to assess the chemical composition of their atmospheres. In this work, we present an alternative approach for recovering the broadband transmission spectra using chromatic Doppler Tomography. To validate the method and examine its performance, we used new observational data obtained with the ESPRESSO instruments to retrieve the  transmission spectra of the archetypal hot Jupiter HD209458b. Our findings indicate that the recovered transmission spectrum is in good agreement with the results presented in previous studies, which used different methodologies to extract the spectrum.</p>


2014 ◽  
Vol 134 (9) ◽  
pp. 523-524
Author(s):  
Hideya Koike ◽  
Masanobu Annoura ◽  
Kento Nishida ◽  
Hiroshi Tanabe ◽  
Michiaki Inomoto ◽  
...  

Author(s):  
Shijia Sun ◽  
Qi Wei ◽  
Bing-Xuan Li ◽  
Xingjun Shi ◽  
feifei yuan ◽  
...  

The pure and Nd3+-doped YMgB5O10 (YMB, Nd:YMB) crystals were grown successfully by the top-seeded solution growth method with composite fluxes Li2O-B2O3-LiF. The systematic investigation of crystal structure, transmission spectrum, band...


2010 ◽  
Author(s):  
Huasong Liu ◽  
Dandan Liu ◽  
Yiqin Ji ◽  
Zhanshan Wang ◽  
Deying Chen ◽  
...  

2011 ◽  
Vol 7 (S282) ◽  
pp. 201-202 ◽  
Author(s):  
O. I. Sharova ◽  
M. I. Agafonov ◽  
E. A. Karitskaya ◽  
N. G. Bochkarev ◽  
S. V. Zharikov ◽  
...  

AbstractThe 2D and 3D Doppler tomograms of X-ray binary system Cyg X-1 (V1357 Cyg) were reconstructed from spectral data for the line HeII 4686Å obtained with 2-m telescope of the Peak Terskol Observatory (Russia) and 2.1-m telescope of the Mexican National Observatory in June, 2007. Information about gas motions outside the orbital plane, using all of the three velocity components Vx, Vy, Vz, was obtained for the first time. The tomographic reconstruction was carried out for the system inclination angle of 45°. The equal resolution (50 × 50 × 50 km/s) is realized in this case, in the orbital plane (Vx, Vy) and also in the perpendicular direction Vz. The checkout tomograms were realized also for the inclination angle of 40° because of the angle uncertainty. Two versions of the result showed no qualitative discrepancy. Details of the structures revealed by the 3D Doppler tomogram were analyzed.


2016 ◽  
Vol 832 (2) ◽  
pp. 202 ◽  
Author(s):  
A. Tsiaras ◽  
I. P. Waldmann ◽  
M. Rocchetto ◽  
R. Varley ◽  
G. Morello ◽  
...  

2006 ◽  
Vol 31 (6) ◽  
pp. 778 ◽  
Author(s):  
Jeehyun Kim ◽  
Junghwan Oh ◽  
Thomas E. Milner ◽  
J. Stuart Nelson

1983 ◽  
Vol 71 (2) ◽  
pp. 254-261 ◽  
Author(s):  
D.L. Mensa ◽  
S. Halevy ◽  
G. Wade

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