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Astrophysical Sciences and Technology MS
There has never been a more exciting time to study the universe beyond the confines of the Earth. A new generation of advanced ground-based and space-borne telescopes and enormous increases in computing power are enabling a golden age of astrophysics. The MS program in astrophysical sciences and technology focuses on the underlying physics of phenomena beyond the Earth, and on the development of the technologies, instruments, data analysis, and modeling techniques that will enable the next major strides in the field. The multidisciplinary emphasis of this program sets it apart from conventional astrophysics graduate programs at traditional research universities.
The MS program comprises a minimum of 32 semester credit hours of study. The curriculum consists of 4 core courses, 4 elective courses, two semesters of graduate seminar, and a research project culminating in a thesis.
Typically following the first year, but sometimes initiated during the first year for well-prepared students, candidates begin a research project under the guidance of a faculty research adviser. A thesis committee is appointed by the program director, consisting of the student's adviser and at least two additional members, one of whom must be a program faculty member. The final examination of the thesis consists of a public oral presentation by the student, followed by questions from the audience. The thesis committee will privately question the candidate following the presentation. The committee will caucus immediately following the examination and thereafter notify the candidate and the program director of the results.
Astrophysical sciences and technology, MS degree, typical course sequence (semesters), effective fall 2013
|Course||Sem. Cr. Hrs.|
|ASTP-613||Astronomical Observational Techniques and Instrumentation||3|
|ASTP-760||Introduction to Relativity and Gravitation||3|
|ASTP-601||Graduate Seminar I||1|
|ASTP-615||Radiative Processes for Astrophysical Sciences||3|
|Choose one of the following:||3|
|ASTP-610||Mathematical Methods for the Astrophysical Sciences|
|ASTP-611||Statistical Methods for Astrophysics|
|ASTP-730||Stellar Structure and Atmospheres||3|
|ASTP-602||Graduate Seminar II||1|
|ASTP-790||Research and Thesis||3|
|ASTP-790||Research and Thesis||3|
|Total Semester Credit Hours||32|
To be considered for admission to the MS program in astrophysical sciences and technology, a candidate must fulfill the following requirements:
- Hold a baccalaureate degree in physical science, mathematics, computer science, or engineering at an accredited college or university,
- Have a minimum undergraduate GPA of 3.2/4.0 in course work in mathematical, science, engineering, and computer subject areas,
- Submit official transcripts (in English) for all previously completed undergraduate and graduate course work,
- Submit two letters of recommendation,
- Submit scores from the Graduate Record Exam (GRE), and
- Complete a graduate application.
- International applicants whose native language is not English must submit scores from the Test of English as a Foreign Language (TOEFL). A minimum score of 550 (paper-based) or 79 (Internet-based) is required. International English Language Testing System (IELTS) scores will be accepted in place of the TOEFL exam. Minimum scores will vary; however, the absolute minimum score required for unconditional acceptance is 6.5. For additional information about the IELTS, please visit www.ielts.org.
For candidates lacking adequate academic preparation or for those who hold a bachelor's degree in an area other than those listed above, bridge and foundation course work may be necessary prior to full admission.
MS to Ph.D. transfer
Depending on each student's progress in their course work and the research project, students may be allowed to attempt the Ph.D. Qualifying Examination. Upon successfully passing the exam, students may choose to proceed to Ph.D. candidacy rather than accepting a terminal master of science degree. This is contingent on the availability of an adviser and research funding.