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A Guide to the Graduate Academic Program
Beginning the Graduate Program
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Upon arrival, new
students should meet with the Graduate Program Advisor, who will help
them plan their first year of graduate study. All students should
check with the computer support group to open an individual account
on the observatory's computer network. Most departmental memos are
sent by e-mail, and most students and faculty use the computers for
computations, word processing, etc. For office supplies such as
pens, pencils, and pads of paper, see Michelle Cournoyer or Erin
Carlson in the Departmental Office. For general advice be sure to
ask the other graduate students.
Students normally register for classes by
using the WebReg on-line computer
registration system. Tuition and fees must generally be paid about
one week before classes start. Graduate Teaching Assistants (GTAs) and Research Associates (RAs) do not have
to pay out-of-state tuition, but you will have to pay Registration
Fees (about $2000). All students are encouraged to apply for
fellowships and scholarships.
All graduate students who have teaching
assistantships must have completed the GTA Training Programs
administered by the Graduate
College and University Teaching Center. Only students who have
attended the required two sessions will receive paychecks from the University.
The sessions generally occur during the week before the first day
of classes.
After the semester is well underway, it may
be a good idea for the new student to assess how much time he/she
is spending on various professional activities. We feel that the
major, long-term emphasis here is on research, with lesser amounts
of time devoted to one's own course work and teaching duties.
For a first-year student taking nine hours of
courses, the situation is somewhat different, and the student might
well be spending 50% of his/her work time on course work (both in
class and out). That would
leave 40% for research and 10% on miscellany such as attending
colloquia, journal club, etc. Of course, this is just a rough guide,
and exceptions will certainly be the rule here. It is not a requirement for first
year graduate students to teach.
About grades in course work: Although one
must maintain a 3.0 GPA, the real purpose of any course should be
to foster the student's comprehension. Grades per se are
secondary, but we realize that there is some correlation between
grades and understanding. Certainly, a grade below "B" on
a graduate course may indicate serious problems.
Please note that all Graduate Teaching and
Research Assistants must register for at least six units of
graduate credit per semester. These can include Dissertation (920),
when appropriate.
All students have an obligation to teach for
a total of two semesters at some point in their graduate
careers. The department
recommends that students get involved in research as early as
possible. As a result, some students choose to postpone their
teaching until their second year or later. Other students
compromise by teaching the first semester of their first year and
by concentrating on research during the second semester after
they've had time to identify a research advisor. These students
then complete their second required semester of teaching at a
future date. The department is quite flexible on this issue.
Students who wish to hold a research
assistantship (RA) during their first semester must notify us by
mid July that they plan to do an RA (or to do research using their
NSF, NASA, Steward or Graduate College Fellowship, if they've been
offered one), although they do not need to know then who their supervisor
will be.
Students who decided to do an RA their first
semester (and who are not on a Fellowship) must tell us by
mid-September who their advisor will be for that semester. If for
some reason a student does not have an advisor at that point, he or
she will be assigned one.
Sometimes a student will be unable to obtain
a research assistantship with their first choice of advisor because
that person does not have the time or funding resources.
(Fellowship students can work with anyone as long as the advisor
has the time.) In such cases, we can remind the students that they
are encouraged to pursue several different research projects during
their graduate careers, and that a faculty member who is initially
unavailable may later become a collaborator or supervisor. In
addition, there are ample opportunities for research projects as
independent study projects (without salary) or with faculty, staff
or postdocs who are not their research
supervisors.
During their first two years, students are encouraged
to work with at least two different faculty members. We recommend
changing research advisors at the beginning of the second year.
Research advisors can be chosen from the ranks of research or
teaching faculty at Steward
Observatory. Members of the faculty of the Lunar and Planetary
Laboratory, Planetary Sciences, Physics, Optical Science, and staff
members at the National Optical Astronomy Observatory may also
serve as student research advisors.
When the student has chosen a research
advisor, he/she should check with the Graduate Program Advisor
(currently Ann Zabludoff) to see about selecting two or three more
faculty members to serve with the research advisor on the student's
mentoring committee. This committee meets every term and guides the
student up to the prelim exam. After passing the exam, the student
then forms a thesis committee, which may or may not include
mentoring committee members. The thesis committee meets every term
until completion of the Ph.D. and makes sure the student remains on
track through his/her career at Steward.
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Summary
of Requirements
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All Ph.D. students
are required to teach at least two discussion or laboratory
sections of an undergraduate astronomy course (e.g., Natural
Sciences 102 or Astronomy 201, 202, 203, and 204) before they
graduate.
Course Requirements: Students are required to
complete successfully the 8 "core" courses in astronomy,
3 graduate level physics courses, and 2 elective graduate courses
which can be in astronomy, physics, mathematics, optical sciences,
engineering, etc., for a total of 13 graduate courses. The
"core" courses are 515
, 518,
522,
535,
540,
541,
545,
and 582.
Other courses which are cross-listed with Astronomy and Physics may
be used to fulfill the physics requirement, as may Astronomy 571
and 589.
Astronomy 589 may be taken twice for credit if the instructor and
course material change. The second credit may be applied to the
elective requirement. Students may also fulfill one elective
requirement by combing 1 or 2 credit electives to total one 3 credit
elective. For example, a student may take Journal Club (1 credit)
for credit up to two times and combine that with another 1 credit
course. In addition, by the end of the second year, students should
have taken six units of research credits (i.e., Astronomy 900). A
typical study plan is listed below. Variations from this will
sometimes occur. Courses below the 500 level are not acceptable for
graduate credit.
By the end of the second year, the student
should have completed the basic Ph.D. qualification requirement,
which consists of eight graduate astronomy courses and three
graduate physics courses (possibly including Astronomy 571
and/or 589),
with a grade of C or better in each course. One's overall GPA has
to stay above 3.0 to hold an assistantship, either teaching or
research. The 3.0 is also a graduation requirement for either a
Masters or Ph.D.
The Prelim Exams
The preliminary exams
generally take place in the grad student's third year, after the 8
core courses have been completed in the first two years. The exam now consists of two parts:
(1) a written, comprehensive examination in September of the fifth
semester, and (2) an oral examination on the student's research
paper to be taken by the end of the fifth semester.
The written exam is authored,
administered and graded by a committee of several faculty members,
and is given simultaneously to all in the third year class, in
September at the start of their third academic year. This exam will
be eight hours long, in one or two days. The first four hours are
"closed book" questions, answered in a classroom. Typical questions of general
knowledge of astronomy and astrophysics might be to write one or
two sentences about the meaning of the Tully-Fisher relation, or
the nature of brown dwarfs.
In the remaining four hours, the exam is "open
book," actually an "open everything" exam. The
student may use any and all resources within the building except
for the resource of talking to other people about the test. The philosophy of the exam is to
test how well the student can synthesize essential concepts from
core courses by posing actual research-type questions which require
across-the-board knowledge such as theoretical motivation and
observational solution. A folder containing exams from past years
is available in the department academic office. If a student fails the written
exam, one more attempt is allowed no more than four months
later. If the student fails
a second time, he/she will not be allowed candidacy to pursue a
PhD, but may take an oral exam based on a research paper for a
possible Masters Degree. So
far, 16 students in three different years of entry have taken the
written exam, and 16 have passed since 2002.
The written exam is followed
no more than three months later with the successful student taking
an oral exam. It is
encouraged that this exam be taken before the written exam if the
student's research paper is completed earlier. While the ultimate goal for
student is to finish a paper that would qualify for submission to a
publication like the Astrophysical Journal, the bar for passing the
oral exam is lower. While
student should get as close as possible to a submission-worthy
paper before the oral exam (and many do in fact defend submitted or
even published papers), the focus of the exam is on the student's
research paper (and what it still requires to be
publication-grade), the talk given by the student, and the general
area(s) of research the paper covers. The format of the exam will
begins with a 25-30 minute talk on the research paper by the
student. This is followed by
the first round of questions.
The focus should be on the content of the paper, and the
student's understanding of and ability to defend this
research. After a short
break, there follows a second round of questioning in the area(s)
of astronomy and astrophysics in which the student's paper and
research fit. A pass will
require a good performance on both parts of the oral exam. A requirement of the Graduate
College is that the exam should be no longer than three hours. If the student fails the oral
exam, a second try will generally be allowed up to six months
later. If the exam is failed
the second time, the student is dropped from qualification for a
PhD, although at the discretion of the committee, a Masters Degree
may be awarded.
The Graduate College has
dropped the requirement that there be an external representative
appointed by them in attendance at the exam. This representative has been
replaced by an internal member called the "recorder." This should be an astronomy
faculty person not associated with the student in research,
mentoring or advising. The
recorder will be the official chair of the committee and will also
be a voting member who asks questions. This person is empowered to make
sure that correct procedures are followed, and that the rights of
the student are protected.
The recorder will also be responsible for filing the signed
papers reporting the exam's outcome with the Graduate College. The
recorder has the right in extreme circumstances to report directly
to the Chairman of the Department afterwards, if she/he feels an
exam was conducted improperly and/or with the result not justified.
The Graduate
College requires that the examining committee consist of a minimum
of four faculty (including the recorder), and four is what this
faculty has decided is appropriate.
The policy in appointing these committees is to have no more
than two members who are associated with the student in research,
mentoring, or advising. Two
additional members not associated with the student, including the
recorder, will be appointed.
At least one of these two should work in a markedly
different field than that of the candidate. In rare cases there may be reason
for three mentors of the student to be appointed to the committee,
but then two non-associated committee members must be appointed, so
that the committee would have five people. (Note that, regardless of
committee size, two negative votes are sufficient for the exam to
be failed, as has always been the policy). So far, everyone
completing the written exam has completed the oral exam
successfully.
The Mentoring and
Thesis Committees
It is required that each student, in consultation with
the principal advisor, form a mentoring committee with 2-3 more
faculty, senior postdocs, faculty members
from other departments, or other astronomical institutions,
interested in the student's likely research. After passing the prelim, the
student forms a thesis committee, which may have a different membership,
to replace the mentoring committee. The mentoring/thesis committee
meets with the student every term and discuss the student's
progress and general wellbeing.
The student can also convey any suggestions for improving the
program to the committee, which the committee should then
communicate to the Academic Program Committee. The student needs to inform the
department office (currently Erin Carlson) that
the meeting has taken place.
After each meeting, a form is filled out by the committee
members describing the research progress made by the student. In those rare cases where the
student is past the prelim and has made no research progress in the
two subsequent semesters, the student is placed on academic probation.
Two additional semesters of no progress without a medical excuse
will result in dismissal from the program.
Final Dissertation
Defense
A five-person committee, which may be
different from the student's thesis committee, is appointed when
the student's dissertation is completed. (The Grad College requires only
four, but the faculty agreed to have five members: this gives us
insurance if some committee member gets stuck in an airport the day
before the exam.) All five
should read the thesis at least three weeks in advance -- or some
other length of time agreed to by the committee and student -- and
forward questions/comments to the student in advance of the exam.
The oral exam consists of a 30-minute talk by
the student, to which the "public" are invited. In the private session following,
questions are asked by each committee member on the thesis work and
associated topics in the subject area.
The
possible outcomes are (1) pass with no
reservations, (2) pass conditional upon changes made to the
dissertation recommended by members of the committee, or (3)
fail. In case (2) the
committee may grant discretion to the principal advisor to enforce
the changes to be made to the thesis recommended by the committee. The members would sign the
paperwork certifying completion of a satisfactory thesis, but the
advisor would withhold the paperwork until satisfactory changes are
made in the opinion of the advisor.
All requirements for the degree of
Doctor of Philosophy must be completed within 5 years of passing
the Comprehensive Exam. Should a student not finish within that
time period, he or she may be allowed to re-take the Comprehensive
Exam with permission of the program, and then proceed to complete
other requirements, e.g., the dissertation.
Important Forms Required by the Graduate College
Graduate
College Forms & Publications
The Minor
Formally, all PhD students in our
program select both a major and a minor subject. For most, both are
astronomy. However, it is
possible for the minor to be in one of the other sciences,
including biological and optical.
The course requirement is set by the minor department, but
usually four of the five elective courses should be in acceptable
graduate courses in the minor department. At least one representative from
the minor department should participate on the preliminary and
final oral (thesis defense) exams.
The astronomy department allows
graduate students whose PhD major is one of the other sciences to
minor in astronomy. We
require that they pass four courses the department considers
acceptable for this purpose, preferably from the "core"
courses listed below, and that one astronomy faculty member
participate in the preliminary and final oral exams.
See the Graduate
Catalogue and the "Handbook for Completing the Steps to
Your Degree" for more information. These publications also
contain requirements involving the dissertation, as does also the Manual for
Theses and Dissertations.
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Typical
Graduate Plan
Fall
Semester
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Spring
Semester
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First Year
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ASTR
522: Atomic & Molecular Astrophysics
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ASTR
515: Interstellar Medium & Star Formation
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ASTR 540: Structure & Dynamics of
Galaxies
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ASTR
541: Extragalactic Astronomy & Cosmology
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One Elective*
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One Elective
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Second Year
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ASTR
545: Stellar Atmospheres
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ASTR
535: Stellar Structure
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ASTR
518: Instrumentation & Techniques
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ASTR
582: High Energy Astrophysics
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ASTR 900: Research
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ASTR 900: Research
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One Elective
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One Elective
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Third Year
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ASTR 920: Dissertation
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ASTR 920: Dissertation
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One Elective
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Fourth Year
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ASTR 920: Dissertation
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ASTR 920: Dissertation
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*General Relativity and Cosmology (571)
is recommended as a preliminary to 541, although it is not a formal
prerequisite.
Course
Descriptions
502. Astronomical
Instrumentation Project (3) II 2001-02 Design,
construction and testing of an astronomical instrument chosen by each
student under the guidance and supervision of the instructor. Regular
class sessions are devoted to discussing techniques and reporting
progress and problems.
503. Physics of the Solar System (3)
I 2001-02 (Identical with PTYS 503) May be convened with 403.
515. Interstellar Medium and Star Formation (3)
II 2000-01 Derivation of physical conditions from spectral data.
Ionized, atomic and molecular clouds, interstellar dust and magnetic
fields. Ionization equilibrium, heating and cooling, supernova
shocks, dust and protostellar evolution.
518. Modern Astronomical Instrumentation and
Techniques (3) I 2001-02 For a description of course
topics, see 418. Graduate-level requirements include an in-depth
research paper. (Identical with PTYS 518) May be convened with 418.
522. Atomic and Molecular Astrophysics (3)
I 2000-01 Interpretation of astronomical spectra: basic aspects of
atomic and molecular spectra and processes that enable one to infer
physical conditions in astronomical environments from analysis of
their electromagnetic spectra. Familiarity with basic quantum
mechanics is assumed.
523. Statistical Mechanical Problems in the
Space Sciences (3) I 2000-01 (Identical with PTYS 523)
535. Stellar Structure (3) II 2001-02
Equations of stellar structure, virial
theorem, energy transport, equations of state, opacities, nuclear
reactions, stellar models, evolution of low and high mass stars,
observational tests, rotation and magnetic fields, binary evolution.
540. Structure and Dynamics of
Galaxies
(3) I 2000-01 Observational properties of galaxies; structure,
kinematics, star and gas content. Structure of our own galaxy.
Dynamics of stellar systems: equilibria,
instabilities, internally and externally driven evolution.
541. Extragalactic
Astronomy and Cosmology (3) II 2000-01 The structure, origin and
evolution of the physical universe from theory and observations of
systems outside our own galaxy. Relativistic cosmology; galaxy
evolution and clustering; active galaxies and quasars; the microwave
background; galaxy formation; the hot big bang; and physics of the
early universe. P, 540.
545. Stellar Atmospheres (3) I 2001-02 Radiative transfer, gray atmosphere, opacity,
line formation, non-LTE, curves of growth,
stellar hydrodynamics, and planetary applications. (Identical with
PTYS 545)
553. Solar System Dynamics (3)
I 2001-02 (Identical with PTYS 553)
555. Remote Sensing of
Planetary Surfaces (3) II 2001-02 (Identical with PTYS 555)
556. Electrodynamics of Conducting Fluids and
Plasmas (3) 2000-01 (Identical with PTYS 556)
571. General Relativity and Cosmology (3)
II 2000-01 General relativity with application to celestial
mechanics, stellar structure, gravitational radiation, black holes,
gravitational lensing and cosmology.
582. High Energy
Astrophysics (3) Radiation mechanisms, synchrotron radiation,
charged particle acceleration, pulsars, black holes, accretion disks,
X-ray binaries, gamma-ray sources, radio galaxies, active galactic
nuclei. (Identical with PHYS 582 and PTYS 582)
589. Topics in
Theoretical Astrophysics (3) [Rpt.] I (Identical with PHYS 589)
596B. Methods in Computational
Astrophysics
Astronomy Electives
·
Instrumentation Projects (502)
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General Relativity and Cosmology (571)
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Topics in Theoretical Astrophysics (589)
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Computational Astrophysics (596)
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Galaxy Evolution (596x)
Faculty
of the Department of Astronomy and Steward Observatory
Contact
Information:
Prospective Students: Dr. Laird Close, 2007-2008
Graduate Admissions Chair
Academic Program Questions: Dr. Ann Zabludoff,
Graduate Advisor
Other questions: Erin Carlson, Graduate
Admissions Coordinator
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