==========================================================================
J/A+A/527/A85 Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011)
The following files can be converted to FITS (extension .fit or fit.gz)
hat14.dat hat3.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/527/A85
==========================================================================
drwxr-xr-x 28 cats archive 4096 Nov 21 2017 [Up]
drwxr-xr-x 4 cats archive 304 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 476 Dec 19 2022 .message
-r--r--r-- 1 cats archive 3310 May 19 2017 ReadMe
-r--r--r-- 1 cats archive 69657 May 19 2017 hat14.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 89342 May 19 2017 hat3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/A+A/527/A85 Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011)
================================================================================
TASTE: The Asiago Search for Transit timing variations of Exoplanets
I. Overview and improved parameters for HAT-P-3b and HAT-P-14b.
Nascimbeni V., Piotto G., Bedin L.R., Damasso M.
<Astron. Astrophys. 527, A85 (2011)>
=2011A&A...527A..85N
================================================================================
ADC_Keywords: Stars, double and multiple ; Planets ; Photometry
Keywords: techniques: photometric - planetary systems -
stars: individual: HAT-P-14, HAT-P-3
Abstract:
A promising method for detecting earth-sized exoplanets is the timing
analysis of a known transit. The technique allows a search for
variations in either the transit duration or the center induced by the
perturbation of a third body, e.g. a second planet or an exomoon. By
applying this method, the TASTE (The Asiago Search for Transit Timing
variations of Exoplanets) project will collect high- precision,
short-cadence light curves for a selected sample of transits by using
imaging differential photometry at the Asiago 1.82m telescope. The
first light curves show that our project can achieve a competitive
timing accuracy, as well as a significant improvement of the orbital
parameters. We derived refined ephemerides for HAT-P-3b and HAT-P-14b
with a timing accuracy of 11 and 25s, respectively.
Objects:
---------------------------------------------------------
RA (2000) DE Designation(s) (Per)
---------------------------------------------------------
13 44 22.6 +48 01 43 HAT-P-3 = TYC 3466-819-1 (2.90)
17 20 27.9 +38 14 32 HAT-P-14 = TYC 3086-152-1 (4.63)
---------------------------------------------------------