Accurate Spitzer infrared radius measurement for the hot Neptune GJ 436b (Astronomy and Astrophysics (2007) 471 (L51-L54) DOI: 10.1051/0004-6361: 20078283)

M. Gillon; B. O. Demory; T. Barman; X. Bonfils; T. Mazeh; S. Udry; M. Mayor; D. Queloz

doi:10.1051/0004-6361:20078283e

Accurate Spitzer infrared radius measurement for the hot Neptune GJ 436b (Astronomy and Astrophysics (2007) 471 (L51-L54) DOI: 10.1051/0004-6361: 20078283)

M. Gillon^*, B. O. Demory, T. Barman, X. Bonfils, T. Mazeh, S. Udry, M. Mayor, D. Queloz

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Comment/debate

Original language	English
Pages (from-to)	L1
Journal	Astronomy and Astrophysics
Volume	490
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361:20078283e
State	Published - Oct 2008

Keywords

Eclipses
Errata, addenda
Infrared: general
Planetary systems
Stars: individual: GJ 436
Techniques: photometric

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10.1051/0004-6361:20078283e

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@article{49951b1e96064b8eba3eeb7bc55a6800,

title = "Accurate Spitzer infrared radius measurement for the hot Neptune GJ 436b (Astronomy and Astrophysics (2007) 471 (L51-L54) DOI: 10.1051/0004-6361: 20078283)",

keywords = "Eclipses, Errata, addenda, Infrared: general, Planetary systems, Stars: individual: GJ 436, Techniques: photometric",

author = "M. Gillon and Demory, {B. O.} and T. Barman and X. Bonfils and T. Mazeh and S. Udry and M. Mayor and D. Queloz",

note = "Funding Information: The author would like to thank the Editor and three anonymous reviewers for their insightful comments and constructive suggestions that have contributed to improve this manuscript. This work was jointly supported by National Key Research and Development Plan of China (2016YFC1302602), Shanghai Sailing Program (17YF1404100), the Science and Technology Commission of Shanghai Municipality (15dz1207805), Shanghai Municipal Commission of Health and Family Planning (15GWZK0201), and USDA NIFA (2015-34263-24070). The merged ground-based total ozone data set was obtained freely from the World Ozone and Ultraviolet Data Center (http://woudc.org/archive/Projects-Campaigns/ZonalMeans/) and the SBUV MOD v8.6 was acquired from the NASA Goddard Space Flight Center (http://acd-ext.gsfc.nasa.gov/Data_services/merged/), while the ERA-Interim ozone reanalysis was obtained from ECMWF (http://apps.ecmwf.int/datasets/data/interim-full-moda/levtype=sfc/) and the MSR-2 total ozone was provided by the Tropospheric Emission Monitoring Internet Service (http://www.temis.nl/protocols/O3global.html). Additionally, the solar flux used as a proxy of solar cycle was provided by the NOAA National Centers for Environmental Information (https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-radio/noontime-flux/penticton/penticton_averaged/). QBO and NINO 3.4 data were obtained from the NOAA Climate Prediction Center (www.cpc.ncep.noaa.gov/data/indices/). AOD and EESC data were acquired from the NASA Goddard Institute for Space Studies (http://data.giss.nasa.gov/modelforce/strataer/tau.line_2012.12.txt) and Atmospheric Chemistry and Dynamics Laboratory (http://acdb-ext.gsfc.nasa.gov/Data_services/automailer/index.html), respectively.",

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T1 - Accurate Spitzer infrared radius measurement for the hot Neptune GJ 436b (Astronomy and Astrophysics (2007) 471 (L51-L54) DOI: 10.1051/0004-6361: 20078283)

AU - Gillon, M.

AU - Demory, B. O.

AU - Barman, T.

AU - Bonfils, X.

AU - Mazeh, T.

AU - Udry, S.

AU - Mayor, M.

AU - Queloz, D.

N1 - Funding Information: The author would like to thank the Editor and three anonymous reviewers for their insightful comments and constructive suggestions that have contributed to improve this manuscript. This work was jointly supported by National Key Research and Development Plan of China (2016YFC1302602), Shanghai Sailing Program (17YF1404100), the Science and Technology Commission of Shanghai Municipality (15dz1207805), Shanghai Municipal Commission of Health and Family Planning (15GWZK0201), and USDA NIFA (2015-34263-24070). The merged ground-based total ozone data set was obtained freely from the World Ozone and Ultraviolet Data Center (http://woudc.org/archive/Projects-Campaigns/ZonalMeans/) and the SBUV MOD v8.6 was acquired from the NASA Goddard Space Flight Center (http://acd-ext.gsfc.nasa.gov/Data_services/merged/), while the ERA-Interim ozone reanalysis was obtained from ECMWF (http://apps.ecmwf.int/datasets/data/interim-full-moda/levtype=sfc/) and the MSR-2 total ozone was provided by the Tropospheric Emission Monitoring Internet Service (http://www.temis.nl/protocols/O3global.html). Additionally, the solar flux used as a proxy of solar cycle was provided by the NOAA National Centers for Environmental Information (https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-radio/noontime-flux/penticton/penticton_averaged/). QBO and NINO 3.4 data were obtained from the NOAA Climate Prediction Center (www.cpc.ncep.noaa.gov/data/indices/). AOD and EESC data were acquired from the NASA Goddard Institute for Space Studies (http://data.giss.nasa.gov/modelforce/strataer/tau.line_2012.12.txt) and Atmospheric Chemistry and Dynamics Laboratory (http://acdb-ext.gsfc.nasa.gov/Data_services/automailer/index.html), respectively.

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KW - Eclipses

KW - Errata, addenda

KW - Infrared: general

KW - Planetary systems

KW - Stars: individual: GJ 436

KW - Techniques: photometric

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Accurate Spitzer infrared radius measurement for the hot Neptune GJ 436b (Astronomy and Astrophysics (2007) 471 (L51-L54) DOI: 10.1051/0004-6361: 20078283)

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