Academic literature on the topic 'Spitzer'

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Journal articles on the topic "Spitzer"

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Spitzer, Judy, A. "Ethanol and LPS modulate NF-KappaB activation, inducible no synthase and Cox-2 gene expression in rat liver cells in vivo." Frontiers in Bioscience 7, no. 1-3 (2002): a99. http://dx.doi.org/10.2741/spitzer.

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Snyder, Alison. "Robert L Spitzer." Lancet 387, no. 10017 (January 2016): 428. http://dx.doi.org/10.1016/s0140-6736(16)00182-3.

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Spitzer, TR. "Dr Spitzer Replies." Bone Marrow Transplantation 22, no. 10 (November 1998): 1028. http://dx.doi.org/10.1038/sj.bmt.1700619.

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Spitzer, Michael. "Michael Spitzer Writes." Music Analysis 16, no. 3 (October 1997): 420. http://dx.doi.org/10.2307/854411.

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SPITZER, ROBERT L. "Dr. Spitzer Replies." American Journal of Psychiatry 150, no. 8 (August 1993): 1277—a—1278. http://dx.doi.org/10.1176/ajp.150.8.1277-a.

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Bahcall, John N., and Jeremiah P. Ostriker. "Lyman Spitzer Jr." Physics Today 50, no. 10 (October 1997): 123–24. http://dx.doi.org/10.1063/1.881941.

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Kerschhofer, Richard. "Mit spitzer Feder." e & i Elektrotechnik und Informationstechnik 115, no. 7-8 (July 1998): 431–32. http://dx.doi.org/10.1007/bf03159619.

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Alves, João, and Virginia Trimble. "Star Formation from Spitzer (Lyman) to Spitzer (Space Telescope) and Beyond1." Publications of the Astronomical Society of the Pacific 121, no. 878 (April 2009): 433–35. http://dx.doi.org/10.1086/598789.

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Menocal, Maria Rosa, Alban K. Forcione, Herbert Lindenberger, and Madeline Sutherland. "Leo Spitzer, Representative Essays." Hispanic Review 59, no. 2 (1991): 207. http://dx.doi.org/10.2307/473724.

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Spitzer, Sarabeth A., Kristan L. Staudenmayer, and Thomas G. Weiser. "Spitzer et al. Respond." American Journal of Public Health 107, no. 8 (August 2017): e25-e25. http://dx.doi.org/10.2105/ajph.2017.303870.

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Dissertations / Theses on the topic "Spitzer"

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Pechmann, Maximilian [Verfasser], Wolfgang [Akademischer Betreuer] Spitzer, Wolfgang [Gutachter] Spitzer, and Robert [Gutachter] Seiringer. "Bose-Einstein Condensation in Random Potentials / Maximilian Pechmann ; Gutachter: Wolfgang Spitzer, Robert Seiringer ; Betreuer: Wolfgang Spitzer." Hagen : FernUniversität in Hagen, 2019. http://d-nb.info/1192512251/34.

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Heinzelmann, Mirjam [Verfasser], Carsten [Akademischer Betreuer] Spitzer, Carsten [Gutachter] Spitzer, and Dirk [Gutachter] Wedekind. "Psychometrische Evaluation des Fragebogens zum Therapeutenverhalten / Mirjam Heinzelmann ; Gutachter: Carsten Spitzer, Dirk Wedekind ; Betreuer: Carsten Spitzer." Göttingen : Niedersächsische Staats- und Universitätsbibliothek Göttingen, 2018. http://d-nb.info/1162697725/34.

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Timlin, John D., Nicholas P. Ross, Gordon T. Richards, Mark Lacy, Erin L. Ryan, Robert B. Stone, Franz E. Bauer, et al. "SpIES: THE SPITZER IRAC EQUATORIAL SURVEY." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621506.

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We describe the first data release from the Spitzer-IRAC Equatorial Survey (SpIES); a large-area survey of similar to 115 deg(2) in the Equatorial SDSS Stripe 82 field using Spitzer during its "warm" mission phase. SpIES was designed to probe sufficient volume to perform measurements of quasar clustering and the luminosity function at z >= 3 to test various models for "feedback" from active galactic nuclei (AGNs). Additionally, the wide range of available multi-wavelength, multi-epoch ancillary data enables SpIES to identify both high-redshift (z >= 5) quasars as well as obscured quasars missed by optical surveys. SpIES achieves 5 sigma depths of 6.13 mu Jy (21.93 AB magnitude) and 5.75 mu Jy (22.0 AB magnitude) at 3.6 and 4.5 mu m, respectively-depths significantly fainter than the Wide-field Infrared Survey Explorer (WISE). We show that the SpIES survey recovers a much larger fraction of spectroscopically confirmed quasars (similar to 98%) in Stripe 82 than are recovered by WISE (similar to 55%). This depth is especially powerful at high-redshift (z >= 3.5), where SpIES recovers 94% of confirmed quasars, whereas WISE only recovers 25%. Here we define the SpIES survey parameters and describe the image processing, source extraction, and catalog production methods used to analyze the SpIES data. In addition to this survey paper, we release 234 images created by the SpIES team and three detection catalogs: a 3.6 mu m. only detection catalog containing similar to 6.1 million sources, a 4.5 mu m. only detection catalog containing similar to 6.5 million sources, and a dual-band detection catalog containing similar to 5.4 million sources.
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Scheunert, Mathias [Verfasser], Klaus [Akademischer Betreuer] Spitzer, Klaus [Gutachter] Spitzer, and Esben [Gutachter] Auken. "3-D inversion of helicopter-borne electromagnetic data / Mathias Scheunert ; Gutachter: Klaus Spitzer, Esben Auken ; Betreuer: Klaus Spitzer." Freiberg : Technische Universitaet Bergakademie Freiberg Universitaetsbibliothek "Georgius Agricola", 2016. http://d-nb.info/1220912379/34.

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Kasliwal, Mansi M., John Bally, Frank Masci, Ann Marie Cody, Howard E. Bond, Jacob E. Jencson, Samaporn Tinyanont, et al. "SPIRITS: Uncovering Unusual Infrared Transients with Spitzer." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624045.

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We present an ongoing, five-year systematic search for extragalactic infrared transients, dubbed SPIRITS-SPitzer InfraRed Intensive Transients Survey. In the first year, using Spitzer/IRAC, we searched 190 nearby galaxies with cadence baselines of one month and six months. We discovered over 1958 variables and 43 transients. Here, we describe the survey design and highlight 14 unusual infrared transients with no optical counterparts to deep limits, which we refer to as SPRITEs (eSPecially Red Intermediate-luminosity Transient Events). SPRITEs are in the infrared luminosity gap between novae and supernovae, with [4.5] absolute magnitudes between -11 and -14 (Vega-mag) and [3.6]-[4.5] colors between 0.3 mag and 1.6 mag. The photometric evolution of SPRITEs is diverse, ranging from < 0.1 mag yr(-1) to > 7 mag yr(-1). SPRITEs occur in star-forming galaxies. We present an indepth study of one of them, SPIRITS 14ajc in Messier 83, which shows shock-excited molecular hydrogen emission. This shock may have been triggered by the dynamic decay of a non-hierarchical system of massive stars that led to either the formation of a binary or a protostellar merger.
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Mahtani, Deepak Prakash. "Spitzer Space Telescope observations of hot Jupiters." Thesis, Keele University, 2015. http://eprints.keele.ac.uk/2341/.

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Currently the Spitzer Space Telescope is the most reliable telescope for conducting secondary eclipse observations of exoplanets. The depth and the time of mid-eclipse are two important parameters that come from a secondary eclipse analysis. The eclipse depth gives information on the temperature of the atmosphere, and can provide evidence for the presence of molecules in the atmosphere of the planet. If multiple wavelengths have secondary eclipse depths measured then it is possible to constrain the spectral energy distribution (SED) of the atmosphere given some assumptions on, for example, the metallicity of the planet's atmosphere. The time of mid-eclipse gives e cos which, with an analysis including transit, radial velocity and secondary eclipse data, can strongly constrain the eccentricity of the planet's orbit. To fully understand the conclusions drawn from these two parameters realistic error bars must be quoted on the measurement of these parameters. It is generally understood that error bars that come from MCMC analyses of secondary eclipse observations are underestimated because the correlated noise in the data is not accounted for in the analysis. The goal of this thesis was to find a method to improve the estimates of the uncertainties on these two parameters as derived from Spitzer secondary eclipse lightcurves at 3.6 um and 4.5 um. This work was conducted through the generation and fitting of semi-synthetic Spitzer secondary eclipse light curves. I estimate the amount the uncertainties on these parameters need to be inflated by and show how my results compare with other similar work in the field. I show that the amount of inflation does affect the conclusions drawn when fitting these data with model atmospheres. This could also mean that for systems where complex chemistry is invoked to explain the observed data, simpler model can now fit the data due to the increase in the error bars. I also find that when multiple realisations of the same, simulated, secondary eclipse lightcurve are fit with the standard MCMC code, the amplitude and time of mid-eclipse can be recovered and found to be more than 3 away from the true value of the injected signal. This can mean that, because usually only 1 lightcurve is obtained per observation of the secondary eclipse, some detections of eccentricity and molecules may not be real detections but simply a result of noise in the data.
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Olofsson, Johan. "La formation planétaire vue par Spitzer et le VLTI." Phd thesis, Grenoble 1, 2009. http://tel.archives-ouvertes.fr/tel-00534116.

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Cette thèse se découpe en deux volets complémentaires, orientés sur la formation planétaire dans les disques autour d'étoiles jeunes. Dans une première partie je présente les résultats obtenus avec des données spectroscopiques du satellite Spitzer. Ces spectres (5-35 µm) montrent un grand nombre de raies en émission, attribuées à des poussière silicatées, amorphes ou cristallines. Sur un large échantillon, j'ai mené deux analyses statistiques complémentaires sur la minéralogie des grains de poussière. Je montre tout d'abord que les silicates cristallins sont très présents dans les disques proto-planétaires, et je mets en évidence un paradoxe de cristallinité sur la distribution radiale de ces cristallins, avec moins de cristaux dans les régions internes (lieu de leur formation préférentiel) que dans les régions externes. Des processus d'amorphisation peuvent être responsables de cet écart. Par la suite, j'ai montré qu'un applatissement des distributions en taille de grain a lieu dans les disques (ce qui était souvent interprété comme un grossissement de grains). Cela peut s'expliquer soit par un changement d'équilibre entre les processus de fragmentation et de coagulation, soit par une évacuation des petits grains par la pression de radiation ou les vents stellaires. Dans une seconde partie, je présente les résultats d'observations pionières, par la méthode d'interférométrie dans le proche infrarouge, avec l'instrument AMBER, pour deux étoiles TTauri. Ces observations ont permis de confirmer deux modèles existants dans la litérature : i) la présence d'un sillon dans un disque en transition, avec un disque interne proche de l'étoile, ii) l'importance de la lumière diffusée dans l'interprétation de données interférométriques. Ces travaux permettent de mieux connaître les régions de formation planétaire.
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Flynn, Stephen. "AzTEC and Spitzer investigations of high redshift submillimetre galaxies." Thesis, Cardiff University, 2011. http://orca.cf.ac.uk/12383/.

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Submillimetre galaxies are an important element in the history of the universe. There have been great advances in technology in the last ten years that have enabled deeper and more detailed investigations of these distant objects. In thisthesis I describe investigations of the properties of high redshift submillimetre galaxies made using data from multiple surveys and multiple instruments. Firstly I describe the process involved in reducing AzTEC data to produce images. I then present the reduced maps and compare them, along with a source catalogue, to those produced by the AzTEC instrument team. I found both reductions produce broadly similar results with some differences that can be explained by slightly different sets of input maps. I then present an analysis of the fainter objects in one of the AzTEC fields using a stacking technique. This analysis determines the contribution Spitzer detected galaxies make to the background at 1.1mm, the redshift dependence of this contribution and the average dust mass that can be associated with it. I also describe an analysis of the ux ratios Eales et al. (2003)found using the available AzTEC data and Spitzer IRAC imaging. In the the penultimate chapter I describe the frequentist identification technique I used to determine counterparts to SCUBA submillimetre sources in the CUDSS three hour field using Spitzer infrared data.
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Schwarzbach, Christoph [Verfasser], Klaus [Akademischer Betreuer] Spitzer, Klaus [Gutachter] Spitzer, Peter [Gutachter] Weidelt, and Eldad [Gutachter] Haber. "Stability of finite element solutions to Maxwell's equations in frequency domain / Christoph Schwarzbach ; Gutachter: Klaus Spitzer, Peter Weidelt, Eldad Haber ; Betreuer: Klaus Spitzer." Freiberg : TU Bergakademie Freiberg, 2009. http://d-nb.info/1220836885/34.

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Beichman, Charles, John Livingston, Michael Werner, Varoujan Gorjian, Jessica Krick, Katherine Deck, Heather Knutson, et al. "SPITZER OBSERVATIONS OF EXOPLANETS DISCOVERED WITH THE KEPLER K2 MISSION." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621243.

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We have used the Spitzer Space Telescope to observe two transiting planetary systems orbiting low-mass stars discovered in the Kepler K2 mission. The system K2-3 (EPIC 201367065) hosts three planets, while K2-26 (EPIC 202083828) hosts a single planet. Observations of all four objects in these two systems confirm and refine the orbital and physical parameters of the planets. The refined orbital information and more precise planet radii possible with Spitzer will be critical for future observations of these and other K2 targets. For K2-3b we find marginally significant evidence for a transit timing variation between the K2 and Spitzer epochs.
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Books on the topic "Spitzer"

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Chatham, George. Spitzer descendants of Hans Bartholomeaus Spitzer. 2nd ed. Fort Wayne, Ind. (3534 Montagne Dr., 46816): G. Chatham, 2008.

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Spitzer, W. Walter Spitzer. Paris, France: Fragments Editions, 2002.

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Spitzer, Serge. Serge Spitzer: Round the corner. [New York]: Nyehaus, 2006.

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Franklin, Leallah. Johann Heinrich Spitzer: Ancestors and descendants. Baltimore, MD: Otter Bay Books, 2012.

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Wilhelm Busch: Philosoph mit spitzer Feder. München: W. Heyne, 1993.

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Spitzer, Serge. Serge Spitzer: Hannover Relevator : 1990/1991. Ostfildern-Ruit bei Stuttgart: Edition Cantz, 1991.

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Spitzer, Federica. Theresienstadt: Aufzeichnungen von Federica Spitzer und Ruth Weisz. Berlin: Metropol, 1997.

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Breitschwerdt, Dieter, Michael Freyberg, and Joachim Trümper, eds. The Local Bubble and Beyond Lyman-Spitzer-Colloquium. Berlin, Heidelberg: Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/bfb0104684.

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Catano, James V. Language, history, style: Leo Spitzer and the critical tradition. Urbana: University of Illinois Press, 1988.

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The twentieth-century humanist critics: From Spitzer to Frye. Toronto: University of Toronto Press, 2007.

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Book chapters on the topic "Spitzer"

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Viso, Michel. "Spitzer Space Telescope." In Encyclopedia of Astrobiology, 1561–64. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_1492.

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Viso, Michel. "Spitzer Space Telescope." In Encyclopedia of Astrobiology, 1–5. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_1492-3.

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Viso, Michel. "Spitzer Space Telescope." In Encyclopedia of Astrobiology, 2325–29. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_1492.

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Ikeuchi, Satoru. "Spitzer, Lyman, Jr." In Biographical Encyclopedia of Astronomers, 2041–43. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4419-9917-7_1306.

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Mumford, George S., Glen M. Cooper, Thomas R. Williams, Roser Puig, Yatendra P. Varshni, Lutz Richter‐Bernburg, Katherine Haramundanis, et al. "Spitzer, Lyman, Jr." In The Biographical Encyclopedia of Astronomers, 1078–79. New York, NY: Springer New York, 2007. http://dx.doi.org/10.1007/978-0-387-30400-7_1306.

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deJong-Lambert, William. "The “Spitzer Affair”." In The Cold War Politics of Genetic Research, 111–40. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-94-007-2840-0_5.

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Alves, João, and Virginia Trimble. "Star Formation from Spitzer (Lyman) to Spitzer (Space Telescope) and Beyond." In Reviews in Modern Astronomy, 141–46. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2010. http://dx.doi.org/10.1002/9783527629190.ch7.

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Buldygin, Valeriĭ V., Karl-Heinz Indlekofer, Oleg I. Klesov, and Josef G. Steinebach. "Spitzer Series and Regularly Varying Functions." In Probability Theory and Stochastic Modelling, 419–38. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-99537-3_11.

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Busby, Robert. "Spitzer: The Downfall of a Governor." In Scandal and American Politics in the 21st Century, 75–105. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-91638-1_4.

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Beichman, Charles A., and Drake Deming. "Observing Exoplanets with the Spitzer Space Telescope." In Handbook of Exoplanets, 1–25. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-30648-3_78-1.

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Conference papers on the topic "Spitzer"

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Wu, Xiuqin, Trey Roby, and Loi Ly. "Spitzer Heritage Archive." In SPIE Astronomical Telescopes + Instrumentation, edited by David R. Silva, Alison B. Peck, and B. Thomas Soifer. SPIE, 2010. http://dx.doi.org/10.1117/12.857728.

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Pesenson, M., W. Roby, J. Fowler, R. Laher, J. Chavez, X. Wu, L. Ly, S. Wheelock, and D. Henderson. "SPITZER bandmerge GUI." In SPIE Astronomical Telescopes + Instrumentation, edited by Martin J. Cullum and George Z. Angeli. SPIE, 2006. http://dx.doi.org/10.1117/12.669860.

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Chavez, Joe. "Spitzer science archive interface." In SPIE Astronomical Telescopes + Instrumentation, edited by David R. Silva and Rodger E. Doxsey. SPIE, 2006. http://dx.doi.org/10.1117/12.671893.

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Rieke, G. H. "Spitzer and Other Planetary Systems." In Frontiers in Optics. Washington, D.C.: OSA, 2008. http://dx.doi.org/10.1364/fio.2008.stuc2.

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Kwok, Johnny H., Mark D. Garcia, Eugene Bonfiglio, and Stacia M. Long. "Spitzer Space Telescope mission design." In SPIE Astronomical Telescopes + Instrumentation, edited by John C. Mather. SPIE, 2004. http://dx.doi.org/10.1117/12.551598.

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Rieke, G. H. "Spitzer and Other Planetary Systems." In Laser Science. Washington, D.C.: OSA, 2008. http://dx.doi.org/10.1364/ls.2008.stuc2.

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Storrie-Lombardi, Lisa J., Sean Carey, Lisa J. Storrie-Lombardi, and Nancy A. Silbermann. "Spitzer Warm Mission Workshop Introduction." In THE SCIENCE OPPORTUNITIES OF THE WARM SPITZER MISSION WORKSHOP. AIP, 2007. http://dx.doi.org/10.1063/1.2806785.

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Laine, S., N. A. Silbermann, L. M. Rebull, and L. J. Storrie-Lombardi. "Spitzer Space Telescope proposal process." In SPIE Astronomical Telescopes + Instrumentation, edited by David R. Silva and Rodger E. Doxsey. SPIE, 2006. http://dx.doi.org/10.1117/12.669087.

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Scire, Elena, Ben Hiu Pan Chan, Nancy Silbermann, and Aomawa Shields. "The Spitzer Bibliography Database: bibliographic statistics." In SPIE Astronomical Telescopes + Instrumentation, edited by David R. Silva, Alison B. Peck, and B. Thomas Soifer. SPIE, 2010. http://dx.doi.org/10.1117/12.857735.

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Mahoney, William A., Lisa J. Garcia, Joseph Hunt, Jr., Douglas B. McElroy, Vince G. Mannings, David S. Mittman, JoAnn C. O'Linger, Marc Sarrel, and Elena Scire. "Spitzer warm mission transition and operations." In SPIE Astronomical Telescopes + Instrumentation, edited by David R. Silva, Alison B. Peck, and B. Thomas Soifer. SPIE, 2010. http://dx.doi.org/10.1117/12.857814.

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Reports on the topic "Spitzer"

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Najita, Joan R., John S. Carr, Stephen E. Strom, Dan M. Watson, Ilaria Pascucci, David Hollenbach, Uma Gorti, and Luke Keller. Spitzer Spectroscopy of the Transition Object TW Hya. Fort Belvoir, VA: Defense Technical Information Center, February 2010. http://dx.doi.org/10.21236/ada522664.

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Trintchouk, F., M. Yamada, H. Ji, R. M. Kulsrud, and T. A. Carter. Measurement of the Transverse Spitzer Resistivity during Collisional Magnetic Reconnection. Office of Scientific and Technical Information (OSTI), September 2000. http://dx.doi.org/10.2172/809842.

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Uchiyama, Yasunobu, C. M. Urry, C. C. Cheung, S. Jester, J. Van Duyne, P. Coppi, R. M. Sambruna, T. Takahashi, F. Tavecchio, and L. Maraschi. Shedding New Light on the 3C 273 Jet With the Spitzer Space Telescope. Office of Scientific and Technical Information (OSTI), May 2006. http://dx.doi.org/10.2172/882831.

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Kaye, S. M., R. Hatcher, R. Kaita, C. Kessel, B. LeBlanc, D. C. McCune, S. Paul, and F. M. Levinton. Spitzer or neoclassical resistivity: A comparison between measured and model poloidal field profiles on PBX-M. Office of Scientific and Technical Information (OSTI), January 1992. http://dx.doi.org/10.2172/5871797.

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Kaye, S. M., R. Hatcher, R. Kaita, C. Kessel, B. LeBlanc, D. C. McCune, S. Paul, and F. M. Levinton. Spitzer or neoclassical resistivity: A comparison between measured and model poloidal field profiles on PBX-M. Office of Scientific and Technical Information (OSTI), January 1992. http://dx.doi.org/10.2172/10115620.

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Alzaid, A. A., C. R. Rao, and D. N. Shanbhag. An Extension of Spitzer's Integral Representation Theorem with an Application. Fort Belvoir, VA: Defense Technical Information Center, April 1985. http://dx.doi.org/10.21236/ada160184.

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Svensson, Lars E. O. Why Exchange Rate Bands? Monetary Independence in Spite of Fixed Exchange Rates. Cambridge, MA: National Bureau of Economic Research, November 1992. http://dx.doi.org/10.3386/w4207.

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Frothingham, Peter J. Successful Operational Leadership in Spite of the Boss: Look at Generals Sheridan and Grant. Fort Belvoir, VA: Defense Technical Information Center, May 1995. http://dx.doi.org/10.21236/ada299813.

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Pelham, Sarah, Tamara Göth, Jorrit Kamminga, Husnia Alkadri, Manizha Ehsan, and Anna Tonelli. 'Leading the Way': Women driving peace and security in Afghanistan, the Occupied Palestinian Territory and Yemen. Oxfam, January 2021. http://dx.doi.org/10.21201/2021.7222.

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In Afghanistan, the Occupied Palestinian Territory (OPT) and Yemen, women’s rights organizations are leading efforts to realize the Women, Peace and Security (WPS) agenda, in spite of ongoing conflict, insecurity and occupation. But without national duty bearers and international actors stepping up to meet their commitments, implement National Action Plans (NAPs) and provide resources and support, the full potential of the agenda will not be reached. This briefing paper explores challenges, lessons learned and opportunities related to realizing the WPS agenda, and makes recommendations to a range of national and international stakeholders on how to support its implementation in Afghanistan, OPT and Yemen.
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10

Asante, Kofi Takyi. Political Economy of the Oil Palm Value Chain in Ghana. Institute of Development Studies (IDS), March 2021. http://dx.doi.org/10.19088/apra.2021.008.

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Abstract:
Oil palm (Elaeis guineensis) is of strategic importance to the Ghanaian economy. It is the second most important industrial crop after cocoa and is used widely in local food preparation as well as in industrial processing. In spite of its importance, however, oil palm has consistently underperformed since the early twentieth century. This paper conducts a value chain analysis of the crop, foregrounding the political economy factors that shape the performance of the sector. It draws on a combination of in-depth interviews conducted in March 2020 with a variety of value chain actors and a review of the secondary literature. Additionally, between late May and early June 2020, twelve further interviews were conducted as part of a rapid market survey to assess the impact of the COVID-19 pandemic on the value chain.
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