Program of the Sessions New Orleans, Louisiana, January 6–9, 2011
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Mothers in Science
The aim of this book is to illustrate, graphically, that it is perfectly possible to combine a successful and fulfilling career in research science with motherhood, and that there are no rules about how to do this. On each page you will find a timeline showing on one side, the career path of a research group leader in academic science, and on the other side, important events in her family life. Each contributor has also provided a brief text about their research and about how they have combined their career and family commitments. This project was funded by a Rosalind Franklin Award from the Royal Society 1 Foreword It is well known that women are under-represented in careers in These rules are part of a much wider mythology among scientists of science. In academia, considerable attention has been focused on the both genders at the PhD and post-doctoral stages in their careers. paucity of women at lecturer level, and the even more lamentable The myths bubble up from the combination of two aspects of the state of affairs at more senior levels. The academic career path has academic science environment. First, a quick look at the numbers a long apprenticeship. Typically there is an undergraduate degree, immediately shows that there are far fewer lectureship positions followed by a PhD, then some post-doctoral research contracts and than qualified candidates to fill them. Second, the mentors of early research fellowships, and then finally a more stable lectureship or career researchers are academic scientists who have successfully permanent research leader position, with promotion on up the made the transition to lectureships and beyond. -
[email protected]
SIMON GRITSCHACHER April 2021 Department of Mathematical Sciences University of Copenhagen Universitetsparken 5 2100 Copenhagen, Denmark [email protected] NATIONALITY Austrian EMPLOYMENT 10/2017 - present University of Copenhagen Postdoctoral fellow Marie-Curie fellow since 9/2019 EDUCATION 10/2013 - 05/2017 University of Oxford, Lincoln College 05/2017 DPhil in Mathematics Commutative K-theory (Advisor: Prof. Ulrike Tillmann) 10/2011 - 09/2013 Ludwig-Maximilians-University, Munich 09/2013 MSc in Mathematics (distinction) 07/2010 - 08/2011 Max Planck Institute for Physics, Munich Diploma student 10/2008 - 06/2012 Technical University, Munich 06/2012 BSc in Mathematics (distinction) 08/2011 Diploma in Physics (5 years degree, distinction) 04/2007 - 07/2008 Technical University, Graz BSc in Technical Physics and Technical Mathematics (not completed) AWARDS, PRIZES AND SCHOLARSHIPS Marie Curie Individual Fellowship 2018, European Union (¿ 207.312) 150th Anniversary Postdoctoral Mobility Grant 2017, London Mathematical Society (£ 8.000) EPSRC Scholarship, 10/2013 - 04/2017 Carathéodory Prize for my Master thesis, LMU Munich, 09/2014 Best Study Award for Bachelor Mathematics for the best overall grade, TU Munich, 06/2013 Scholar of the Cusanuswerk 04/2009 - 09/2013 37th International Physics Olympiad, Singapore, Honourable mention 07/2006 1 PUBLICATIONS AND PREPRINTS Preprints On families of nilpotent subgroups and associated coset posets (with B. Villarreal) Preprint (2021) 1–14, arXiv:2104.06869 On the second homotopy group of spaces of commuting elements in Lie groups (with A. Adem and J. M. Gómez) Preprint (2020) 1–52, submitted, arXiv:2009.09045 A remark on the group-completion theorem Preprint (2017) 1–9, arXiv:1709.02036 Published articles Higher generation by abelian subgroups in Lie groups (with O. -
CRATER MORPHOMETRY on VENUS. C. G. Cochrane, Imperial College, London ([email protected])
Lunar and Planetary Science XXXIV (2003) 1173.pdf CRATER MORPHOMETRY ON VENUS. C. G. Cochrane, Imperial College, London ([email protected]). Introduction: Most impact craters on Venus are propagating east and north/south. Can be minimised if pristine, and provide probably the best available ana- framelets have good texture on the left-hand side. logs for craters on Earth soon after impact; hence the Prominence extension – features extend down value of measuring their 3-D shape to known accuracy. range into a ridge, eg central peak linked to the rim. The USGS list 967 craters: from the largest, Mead at Probably due to radar shadowing differences, these are 270 km diameter, to the smallest, unnamed at 1.3 km. easily recognised and avoided during analysis. Initially, research focussed on the larger craters. Araration (from Latin: Arare to plough) consists of Schaber et al [1] (11 craters >50 km) and Ivanov et al parallel furrows some 50 pixels apart, oriented north- [2] (31 craters >70 km) took crater depth from Magel- south, and at least tens of metres deep. Fig 2, a lan altimetry. Sharpton [3] (94 craters >18 km) used floor-offsets in Synthetic Aperture Radar (SAR) F- MIDR pairs, as did Herrick & Phillips [4]. They list many parameters but not depth for 891 craters. The LPI database1 now numbers 941. Herrick & Sharpton [5] made Digital Elevation Models (DEMs) of all cra- ters at least partially imaged twice down to 12 km, and 20 smaller craters down to 3.6 km. Using FMAP im- ages and the Magellan Stereo Toolkit (MST) v.1, they automated matches every 900m but then manually ed- ited the resultant data. -
Microwave Properties and the 1-Micron Emissivity of Crater-Related Radar- Dark Parabolas and Other Surface Features in Five Areas of Venus
46th Lunar and Planetary Science Conference (2015) 1135.pdf MICROWAVE PROPERTIES AND THE 1-MICRON EMISSIVITY OF CRATER-RELATED RADAR- DARK PARABOLAS AND OTHER SURFACE FEATURES IN FIVE AREAS OF VENUS. N.V. Bondarenko 1,2 , A.T. Basilevsky 3,4 , E.V. Shalygin 3, W.J. Markiewicz 3; 1University of California – Santa Cruz, 95064 Santa Cruz, USA; 2Institute of Radiophysics and Electronics, National Academy of Sciences of Ukraine, 61085 Kharkiv, Ukraine; 3 Max-Planck-Institut für Sonnensystemforschung, 37077 Göttingen, Germany; 4Vernadsky Institute RAS, 119991 Moscow, Russia; [email protected]. Introduction: This work presents a comparative study dark haloes are considered to be associated with craters older of the Magellan-based microwave properties and the 1- than those having the radar-dark parabolas [e.g., 5, 6, 7]. micron emissivity of the surface for five crater-associated radar-dark parabolas, the neighboring plains and some other geologic units. The 1-micron emissivity was derived from the measurements done by the Venus Monitoring Camera on board the Venus Express spacecraft. The craters under study are Adivar, Bassi, Batsheba, du Chatelet (plus located nearby crater Caccini with non-parabolic radar-dark halo) and Sit- well. All these craters are located in the latitude belt from 25 oS to 25 oN where the geometry and other conditions for the VMC mapping are optimal. Data description and approach: Used for our analysis microwave properties include microwave emissivity, Fresnel reflectivity, surface roughness presented as root-mean-square slopes, and radar cross-section. These parameters depend on surface dielectric permittivity and surface roughness at dif- ferent spatial scales. -
Respicite Astra: a Historic Journey in Astronomy Through Books
0 Respicite Astra: A Historic Journey in Astronomy through Books RReessppiicciittee AAssttrraa A Historic Journey in Astronomy through Books The Astronomiicall Sociiety of Mallta The Natiionall Liibrary of Mallta The Astronomical Society of Malta The National Library of Malta 1 Respicite Astra: A Historic Journey in Astronomy through Books Respicite Astra A Historic Journey in Astronomy through Books Exhibition held between 25 September – 18 October 2010-09-21 at the National Library, Valletta, Malta on the occasion of Notte Bianca 2010 Introductory Text Mr Victor Farrugia Captions Mr Leonard Ellul Mercer – Pgs 23-24, 57 Mr Alexander Pace – Pgs 25-26, 58, 63, 70 Prof Frank Ventura – Pgs 4, 6-13, 15-18, 21, 27-31, 33, 35-38, 40, 42- 43, 45-48, 50-56, 60-62, 65-69, 72-76, 80, 85, 87, 93 Acknowledgements The Committee of the Astronomical Society of Malta would like to acknowledge the following persons for their kind and generous help in setting up this Exhibition at the Main Hall of the National Library starting on 25th September 2010 during the Notte Bianca event: Mr Fabio Agius (MaltaPost Philatelic Archives) Ms C Michelle Buhagiar (National Library of Malta) Ms Maroma Camilleri National Library of Malta) Mr Leonard Ellul Mercer (Personal capacity) Victor Farrugia (Astronomical Society of Malta) Mr Alexander Pace (Astronomical Society of Malta) Arch Alexei Pace (Astronomical Society of Malta) Ms Joanne Sciberras (National Library of Malta) Mr Tony Tanti (Astronomical Society of Malta) Prof Frank Ventura (University of Malta) Staff of the National Library of Malta Front Image Great Orion Nebula by Mr Leonard Ellul Mercer Production The Astronomical Society of Malta P.O. -
Program of the Sessions San Diego, California, January 9–12, 2013
Program of the Sessions San Diego, California, January 9–12, 2013 AMS Short Course on Random Matrices, Part Monday, January 7 I MAA Short Course on Conceptual Climate Models, Part I 9:00 AM –3:45PM Room 4, Upper Level, San Diego Convention Center 8:30 AM –5:30PM Room 5B, Upper Level, San Diego Convention Center Organizer: Van Vu,YaleUniversity Organizers: Esther Widiasih,University of Arizona 8:00AM Registration outside Room 5A, SDCC Mary Lou Zeeman,Bowdoin upper level. College 9:00AM Random Matrices: The Universality James Walsh, Oberlin (5) phenomenon for Wigner ensemble. College Preliminary report. 7:30AM Registration outside Room 5A, SDCC Terence Tao, University of California Los upper level. Angles 8:30AM Zero-dimensional energy balance models. 10:45AM Universality of random matrices and (1) Hans Kaper, Georgetown University (6) Dyson Brownian Motion. Preliminary 10:30AM Hands-on Session: Dynamics of energy report. (2) balance models, I. Laszlo Erdos, LMU, Munich Anna Barry*, Institute for Math and Its Applications, and Samantha 2:30PM Free probability and Random matrices. Oestreicher*, University of Minnesota (7) Preliminary report. Alice Guionnet, Massachusetts Institute 2:00PM One-dimensional energy balance models. of Technology (3) Hans Kaper, Georgetown University 4:00PM Hands-on Session: Dynamics of energy NSF-EHR Grant Proposal Writing Workshop (4) balance models, II. Anna Barry*, Institute for Math and Its Applications, and Samantha 3:00 PM –6:00PM Marina Ballroom Oestreicher*, University of Minnesota F, 3rd Floor, Marriott The time limit for each AMS contributed paper in the sessions meeting will be found in Volume 34, Issue 1 of Abstracts is ten minutes. -
February 2007
THE LONDON MATHEMATICAL SOCIETY NEWSLETTER No. 356 February 2007 Forthcoming NEXT STEPS a problem with any transfer- ence of the existing two such Society INITIATIVE grades within the IMA (Fellow Meetings The second meeting of the and Member) into a new Joint Planning Group to body. This problem needs to 2007 develop the framework for a be resolved and it was agreed Friday 9 February possible unification of the to ask two individuals to draft London IMA and LMS took place on opposing papers as a basis for P. Maini 6 December 2006. Verbal further and fuller discussion. A. Stevens reports from Council meet- The Group went on to con- (Mary Cartwright ings of both bodies were sider proposals for a Lecture) given. The LMS Council had Constitution. Good progress [page 3] been the less satisfied of the was made on matters of rep- 1 two with the three papers – resentation: the future Friday 20 April Vision and Mission, Council, elections to it, co- Midlands Regional Constitution and Membership option, constituencies, its Meeting – that the Group had pro- Boards, Committees and serv- Loughborough duced for them. They asked ice areas. There was general Y. Colin de Verdière for improvements to the agreement on the principles F. Kirwan Vision and Mission paper and that would underlie the draft- O. Viro expressed concerns over the ing of a Charter, By-Laws and proposed membership struc- Regulations and on the ring- Tuesday 24 April ture. By contrast the IMA fencing and protection of the David Crighton Council was reported to LMS research funds. -
Lick Observatory Records: Photographs UA.036.Ser.07
http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory. -
Curriculum Vitae
Curriculum Vitae 25. Mai 2021 Name: Dr. Fabian Hebestreit Address: Mathematisches Institut Universit¨at Bonn Endenicher Allee 60 53115 Bonn, Germany Office: 3.023 E-mail: [email protected] Phone: +49 228 73 62239 Web: http://www.math.uni-bonn.de/people/fhebestr Date of Birth: 14.08.1989 Education and theses 07/2006 Abitur, Ratsgymnasium Osnabruck¨ 10/2006 - 12/2010 Studies of Mathematics and Computer Science Universit¨at Osnabruck¨ 12/2010 Diploma in Mathematics, Universt¨at Osnabruck¨ Advisors: Oliver R¨ondigs, Manfred Stelzer. On topological realisation at odd primes 01/2011 - 07/2014 Graduate studies in Mathematics, WWU Munster¨ research group `Topology' 07/2014 Doctorate in Mathematics, WWU Munster¨ Advisor: Michael Joachim. Twisted Spin Cobordism in progress Habilitation in Mathematics, RFWU Bonn (expected to complete 10/2021) Supervisor: Wolfgang Luck.¨ Cobordism categories in topology and algebra 1 Employment 10/2007 - 09/2010 Student assistant (Studentische Hilfskraft), Universit¨at Osnabruck¨ 01/2011 - 08/2014 Research assistant (Wissenschaftlicher Mitarbeiter), WWU Munster¨ 09/2014 - 08/2015 Research visitor, University of Notre Dame 10/2015 - 03/2017 Postdoctoral research fellow, RFWU Bonn 04/2017 - 04/2024 Lecturer (akademischer Rat auf Zeit, non-tenure track), RFWU Bonn 09/2017 - 03/2018 Visiting associate professor (Vertretung von W. Steim- le, W2), Universit¨at Augsburg, on leave from Bonn Research Interests Homotopical Algebra, Algebraic Topology, Geometric Topology more specifically: the homotopy theory of diffeomor- -
VENUS Corona M N R S a Ak O Ons D M L YN a G Okosha IB E .RITA N Axw E a I O
N N 80° 80° 80° 80° L Dennitsa D. S Yu O Bachue N Szé K my U Corona EG V-1 lan L n- H V-1 Anahit UR IA ya D E U I OCHK LANIT o N dy ME Corona A P rsa O r TI Pomona VA D S R T or EG Corona E s enpet IO Feronia TH L a R s A u DE on U .TÜN M Corona .IV Fr S Earhart k L allo K e R a s 60° V-6 M A y R 60° 60° E e Th 60° N es ja V G Corona u Mon O E Otau nt R Allat -3 IO l m k i p .MARGIT M o E Dors -3 Vacuna Melia o e t a M .WANDA M T a V a D o V-6 OS Corona na I S H TA R VENUS Corona M n r s a Ak o ons D M L YN A g okosha IB E .RITA n axw e A I o U RE t M l RA R T Fakahotu r Mons e l D GI SSE I s V S L D a O s E A M T E K A N Corona o SHM CLEOPATRA TUN U WENUS N I V R P o i N L I FO A A ght r P n A MOIRA e LA L in s C g M N N t K a a TESSERA s U . P or le P Hemera Dorsa IT t M 11 km e am A VÉNUSZ w VENERA w VENUE on Iris DorsaBARSOVA E I a E a A s RM A a a OLO A R KOIDULA n V-7 s ri V VA SSE e -4 d E t V-2 Hiei Chu R Demeter Beiwe n Skadi Mons e D V-5 S T R o a o r LI s I o R M r Patera A I u u s s V Corona p Dan o a s Corona F e A o A s e N A i P T s t G yr A A i U alk 1 : 45 000 000 K L r V E A L D DEKEN t Baba-Jaga D T N T A a PIONEER or E Aspasia A o M e s S a (1 MM= 45 KM) S r U R a ER s o CLOTHO a A N u s Corona a n 40° p Neago VENUS s s 40° s 40° o TESSERA r 40° e I F et s o COCHRAN ZVEREVA Fluctus NORTH 0 500 1000 1500 2000 2500 KM A Izumi T Sekhm n I D . -
Fourth SIAM Conference on Applications of Dynamical Systems
Utah State University DigitalCommons@USU All U.S. Government Documents (Utah Regional U.S. Government Documents (Utah Regional Depository) Depository) 5-1997 Fourth SIAM Conference on Applications of Dynamical Systems SIAM Activity Group on Dynamical Systems Follow this and additional works at: https://digitalcommons.usu.edu/govdocs Part of the Physical Sciences and Mathematics Commons Recommended Citation Final program and abstracts, May 18-22, 1997 This Other is brought to you for free and open access by the U.S. Government Documents (Utah Regional Depository) at DigitalCommons@USU. It has been accepted for inclusion in All U.S. Government Documents (Utah Regional Depository) by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. tI...~ Confers ~'t' '"' \ 1I~c9 ~ 1'-" ~ J' .. c "'. to APPLICAliONS cJ May 18-22, 1997 Snowbird Ski and Summer Resort • Snowbird, Utah Sponsored by SIAM Activity Group on Dynamical Systems Conference Themes The themes of the 1997 conference will include the following topics. Principal Themes: • Dynamics in undergraduate education • Experimental studies of nonlinear phenomena • Hamiltonian systems and transport • Mathematical biology • Noise in dynamical systems • Patterns and spatio-temporal chaos Applications in • Synchronization • Aerospace engineering • Biology • Condensed matter physics • Control • Fluids • Manufacturing • Me;h~~~~nograPhY 19970915 120 • Lasers and o~ • Quantum UldU) • 51a m.@ Society for Industrial and Applied Mathematics http://www.siam.org/meetingslds97/ds97home.htm 2 " DYNAMICAL SYSTEMS Conference Prl Contents A Message from the Conference Chairs ... Get-Togethers 2 Dear Colleagues: Welcoming Message 2 Welcome to Snowbird for the Fourth SIAM Conference on Applications of Dynamica Systems. Organizing Committee 2 This highly interdisciplinary meeting brings together a diverse group of mathematicians Audiovisual Notice 2 scientists, and engineers, all working on dynamical systems and their applications. -
NAMED VENUSIAN CRATERS; Joel F
NAMED VENUSIAN CRATERS; Joel F. Russell and Gerald G. Schaber, U.S. Geological Survey, 2255 N. Gemini Dr. Flagstaff, AZ 86001 Schaber et al. [I] compiled a database of 841 craters on Venus, based on Magellan coverage of 89% of the planet's surface. That database, derived from coverage of approximately 98% of Venus' surface, has been expanded to 912 craters, ranging in diameter from 1.5 to 280 krn [2]. About 150 of the larger craters were previously identified by Pioneer Venus and Soviet Venera projects and subsequently forrnally named by the International Astronomical Union (IAU). A few of the features identified and nanled as impact craters on Pioneer and Venera images have not been recognized on Magellan images, and therefore the IAU is being requested to drop their names. For example, the feature known as Cleopatra is officially named as a patera, although it is now generally accepted that Cleopatra is a crater [I]. Also, the feature Eve, which has been used to define the prime meridian for Venus, was erroneously identified as an impact feature, but its true morphology has not been determined from Magellan images. The Magellan project has requested the IAU to name hundreds of craters identified by Magellan. At its triennial General Assembly in Buenos Aires in 1991, the IAU [3] gave full approval to names for 102 craters (table 1) in addition to those previously named. At its 1992 meeting, the IAU's Working Group for Planetary System Nomenclature, which screens all planetary names prior to formal consideration by the General Assembly, gave provisional approval to names for an additional 239 Venusian craters.