Exoplanet HAT-P-37b (Dra)

Discovery and References:

HAT-P-34b -- HAT-P-37b: Four Transiting Planets More Massive Than Jupiter Orbiting Moderately Bright Stars

... report the discovery of four transiting extrasolar planets (HAT-P-34b–HAT-P-37b) with masses ranging from 1.05 to 3.33MJ and periods from 1.33 to 5.45 days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33MJ), has a high eccentricity of e = 0.441±0.032 at P = 5.452654±0.000016 d period, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.

BASIC DATA FROM: Exoplanets Data Explorer
Reference CCD frame with the callibration stars
Downloading, please wait ...
© Velimir Popov & Emil Ivanov 2013


Date: 2013-04-14

Submission to: ETD - Exoplanet Transit Database

Differential Photometry and Light Curve with FOTODIFF

Optic(s): RC 12" with Astro-Physics corrector @ f/5 (RC)
Mount: ASA DDM85 Premium
Camera: ATIK 4000 M
Filters: Astronomik Tri G filter - very symilar to V (Jonson)
Dates/Times: 2013-04-14 from UTC 21:14:34 to 2013-04-15 UTC 00:26:11
Location: IRIDA Observatory, BG, longitude: E 24 44' 18", latitude: N 41 41' 42"
Exp. Details: Tri G filter: 166 frames 60 sec each, Bin 1
More details: Dark and flat frames reduction
Processing: Reduction and Differential Photometry
Copyright: Velimir Popov and Emil Ivanov 2013. All Rights Reserved
e-mail: info@irida-observatory.org
click tracking