J/ApJ/689/L149  Parameter variations of Gliese 436b transits   (Coughlin+, 2008)

New observations and a possible detection of parameter variations in the transits of Gliese 436b. Coughlin J.L., Stringfellow G.S., Becker A.C., Lopez-Morales M., Mezzalira F., Krajci T. <Astrophys. J., 689, L149-L152 (2008)> =2008ApJ...689L.149C 2008ApJ...689L.149C
ADC_Keywords: Planets ; Stars, diameters ; Stars, variable Keywords: planetary systems - stars: individual (Gliese 436) Abstract: We present ground-based observations of the transiting Neptune-mass planet Gl 436b obtained with the 3.5m telescope at Apache Point Observatory and other supporting telescopes. Included in this is an observed transit in early 2005, over 2 years before the earliest reported transit detection. We have compiled all available transit data to date and perform a uniform modeling using the JKTEBOP code. We do not detect any transit timing variations of amplitude greater than ∼1 minute over the ∼3.3 year baseline. We do however find possible evidence for a self-consistent trend of increasing orbital inclination, transit width, and transit depth, which supports the supposition that Gl 436b is being perturbed by another planet of ≲12M{earth} in a nonresonant orbit. Description: We observed Gl 436 (J114211+264224) in the V filter on the nights of 2008 April 7, April 28, and May 6 UT with the 3.5m telescope at Apache Point Observatory (APO). Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 11 42 11.1 +26 42 24 Gliese 436b = GJ 436 b ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 125 58 Parameters derived from using the JKTEBOP code with 1σ errors -------------------------------------------------------------------------------- See also: J/A+A/471/L51 : Spitzer observations of the hot Neptune GJ 436b (Gillon+, 2007) J/A+A/475/1125 : Characterization of the hot Neptune GJ 436b (Demory+, 2007) J/A+A/507/481 : GJ 436b and XO-1b transits (Caceres+, 2009) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Mod Model type (1) 3- 6 I4 --- E ? Epoch of observation (2) 8- 25 A18 --- Source Source of Data (telescope or author) 27- 45 A19 --- BibCode Bibcode of author if relevent 47 A1 --- f_Source [ab] Precision on source (3) 49- 52 A4 --- Filt Filter (8um, B, H, I, R, V, None); Johnson-Cousins system 54- 63 F10.5 d t0 ? HJD-2450000 (Heliocentric Julian Date) of minimum 65- 71 F7.5 d e_t0 ? 1σ uncertainty in Tmin 73- 77 F5.2 deg i Orbital inclination 79- 82 F4.2 deg e_i 1σ uncertainty in i 84- 88 F5.3 Rsun R* Stellar radius (in solar radius) 90- 94 F5.3 Rsun e_R* 1σ uncertainty in R* 96- 99 F4.2 --- Rp Planetary radius in Earth radii (6371km) 101-104 F4.2 --- e_Rp 1σ uncertainty in Rp 106-110 F5.2 mmag Depth Depth of eclipse 112-115 F4.2 mmag e_Depth 1σ uncertainty in Depth 117-120 F4.1 min Width Width of eclipse 122-125 F4.1 min e_Width 1σ uncertainty in Width -------------------------------------------------------------------------------- Note (1): Model type as follows: V = Ratio of radii k=Rp/Rs allowed to vary. F = Star and Planet radii fixed by fixing k. Note (2): Epoch with E=0 the initial transit discovery of Gillon et al. (2007A&A...472L..13G 2007A&A...472L..13G). Note (3): Data source as follows: a = Amateur Observer with data obtained from Bruce Gary. http://brucegary.net/AXA/GJ436/gj436.htm. b = Data were digitized from published plot. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 20-Jan-2011
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