UCSC Astronomy & Astrophysics
Unofficial Orientation Guide
Scott Seagroves, Lynne Raschke
last update: Apr 11, 2002
Important: much of the information in
here about room numbers, phone numbers, and other where-things-are
will be going out of date this summer as the astro dept moves from
Kerr Hall into a new building, the ISB. I will try to keep this
updated as I learn new stuff, but bear with me. And certainly
don't keep old copies of this document around; check in the
summer/fall for new ones.
Contents
1 Introduction
2 What to do in your first days
2.1 Upon your arrival at the Astronomy & Astrophysics Dept.
2.2 Within your first couple of weeks
2.3 Find housing!
3 The Astronomy & Astrophysics Dept.
3.1 Who's who
3.2 Projects/Acronyms
3.3 The graduate curriculum
3.4 Classes
3.5 Advising
3.6 Department events
3.7 Your dept. responsibilities; Czars
3.8 Computing
3.9 Funding/Support
3.10 Miscellany
4 The University
4.1 What's where; campus facilities
4.2 Structure
4.3 Transportation and parking
4.4 Housing
5 Santa Cruz and environs
5.1 Geography
5.2 Housing
5.3 Transportation
5.4 Businesses and other miscellany
A Useful websites
1 Introduction
This document isn't really endorsed in any official way, it's just a
place where we hope you find the answers to some of your questions.
If you find that we're wrong, please let us know and we'll update
this.
This guide is a bit crammed full of information. It's pretty dense,
and probably not fun to read in one sitting. What we hope is that the
answers to most (or maybe all) of your questions are in here, and we
hope you come here first to look for them. When the answers aren't
here, or the stated answers are wrong, let us know.
First there is a section on what to do when you first arrive. Then
the guide is organized from smallest to largest, from the Dept.,
to the University, then the city of Santa Cruz and environs.
This document lives on the web at
http://www.ucolick.org/~
board/grad/orientation/orientation.html, so check there for updates
(or just start at http://www.astro.ucsc.edu/grads.xml).
Important: much of the information in
here about room numbers, phone numbers, and other where-things-are
will be going out of date this summer as the astro dept moves from
Kerr Hall into a new building, the ISB. I will try to keep this
updated as I learn new stuff, but bear with me. And certainly
don't keep old copies of this document around; check in the
summer/fall for new ones.
2 What to do in your first days
There are a few things you should do pretty quickly upon arriving in
the area. Some will be covered in more detail later.
2.1 Upon your arrival at the Astronomy & Astrophysics Dept.
Unless you already have housing (by some miracle of miracles), you
have no place from which to base operations, so you ought to head to
the Dept. Things to do immediately (order not necessarily important):
- Go to the Dept. office (Kerr 477) and introduce yourself to
Mary Kiegelis, the department manager, if she's around.
She can probably help you through all the rest of this.
- Get a key to Kerr hall and a ``grad'' key. Mary will help you
contact the Lick Observatory Business Office (LOBO), and you go up
there (they're in the Natural Sciences II Annex) to get your keys.
- Mary will give you some paperwork to get a computer account.
Then, go downstairs to NICS, the computer system administrators, and
set it all up. They're located in several offices around
Kerr 13. Your new account may only work on one machine,
bigdog, for a day or so.
- Get on the payroll. There are a couple of aspects here. If you
will ever TA, which of course you will, then you need to get on the
Natural Sciences Division payroll. They're located in Baskin
Engineering, a.k.a. Applied Sciences. Mary can help you get in touch
with them. For doing research as opposed to teaching, you will need
to get on the payroll with LOBO, which you can probably do when you go
get your keys. You can set up direct deposit to your bank accounts at
the two payroll offices. If you will be on a fellowship, then you will be paid
no matter what. Not sure how to set up direct deposit for a
fellowship, but it is possible.
- Introduce yourself to Kurtis Williams, a grad student whose
office is Kerr 231. He is in charge of office space and will show you
where your desk and such is.
- You already have a mailbox in the UCO/Lick mailroom, Kerr 9.
Check for mail.
2.2 Within your first couple of weeks
Other things that are not incredibly urgent but that you ought to take
care of include:
- Get a UCSC ID card. These are available at ID Card Services,
located adjacent to the Bay Tree Bookstore. (Ok, it turns out you
can't get your ID until mid-September anyway, so if you're here early
you can ignore this.)
- Register for fall classes early, so there won't be any surprises
if you have missing paperwork or something. (For instance, if you
just graduated, you may have to have an updated transcript sent to
UCSC to prove you got your degree.)
- Get a CA driver's license or ID, and register your vehicle with
the DMV. Even if you do not own the vehicle (like it's your
parents'), technically you must register it anyway within 10 days.
- Besides getting your CA driver's license, do other things that establish
your California residency, like open a bank account, register to vote,
etc. Of course the best way to establish residency is with a
lease/rental agreement.
The DMV, some banks, etc., are discussed in §5.
2.3 Find housing!
Your real job during your first few weeks is to find housing, but you
didn't need us to tell you that, did you? For details on housing,
check out §4.4 (on-campus resources),
§5 (Santa Cruz-wide info), and the list of housing
links in §A.
3 The Astronomy & Astrophysics Dept.
Welcome to grad school at the UCSC Astro Dept. There's a lot to cover
here, and we'll probably miss a lot, but here goes.
3.1 Who's who
Grads
Table 1 has the current graduate student
population, including you, as of 1 August 2001.
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Table 1: Current Astronomy & Astrophysics graduate students
as of January 2002.
| Name | Email1
| Year2
| Previous Education | Current Advisor(s) |
Phil Choi | pchoi | AC | Wesleyan | Guhathakurta |
Ian Dobbs-Dixon | iandd | 1 | UC-Santa Cruz | ... |
Shawfeng Dong | dong | AC | U. of Science & Tech. (China) | Lin |
Marla Geha | mgeha | AC | Cornell, NMSU | Guhathakurta |
Justin Harker | jharker | 1 | U. of Wisconsin-Madison | ... |
Justin Howell | jhhowell | ~ 4 | Caltech, Columbia | Guhathakurta |
Patrik Jonsson | patrik | AC | Uppsala (Sweden) | Primack, Faber |
Michael Kuhlen | mqk | 2 | Caltech | Woosley, Madau |
David Lai | david | 1 | Reed | ... |
Laura Langland-Shula | laura | 1 | ... | ... |
Sarah Martell | martell | 1 | U. of Washington | ... |
Alex McDaniel | alexm | 2 | Princeton | Laughlin |
Jason Melbourne | jmel | 1 | Wesleyan | ... |
Anne Metevier | anne | AC | Northwestern | Koo |
Greg Novak | novak | 1 | Harvard | Lin |
Lynne Raschke | lynne | 4 | Haverford | Faber |
Tami Rogers | tami | 3 | U. of Arizona | Woosley |
Linda Schroder | linda | AC | Arizona State | Brodie |
Scott Seagroves | scott | 3 | UNC-Chapel Hill | Thorsett |
Andrew Sheinis | sheinis | AC | UMass-Amherst, Worcester | Miller |
Kim-Vy Tran | vy | AC | U. of Arizona | Illingworth |
Kurtis Williams | williams | 5 | Penn State | Bolte |
Weiqun Zhang | zhang | AC | U. of Science & Tech. (China) | Woosley |
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Faculty and other researchers
What follows is a very concise, definitely non-exhaustive
summary of the faculty's research interests. Listed in the ``Notes''
field are current projects or collaborations that person is affiliated
with; see §3.2 for descriptions of these projects.
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GEORGE BLUMENTHAL
Office: 439B Kerr Phone: 459-2005
Email: george@ucolick.org
Notes:
Issues in theoretical cosmology, including: the role of dark matter;
the origin of structure in the universe; galaxy evolution; voids;
inflation; perturbations in the CMB. Also: AGNs; accretion
disks; GRBs.
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PETER BODENHEIMER
Office: 415F Kerr Phone: 459-2064
Email: peter@ucolick.org
Notes: CODEP
Theoretical studies of star and planet formation, including:
calculation of protostellar collapse; multiple-star
system formation; evolution of protostellar disks and the formation
of planets within them; giant planets; solar system formation.
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MICHAEL BOLTE
Office: 401 Kerr Phone: 459-3896
Email: bolte@ucolick.org
Notes: CELT
Primarily observational studies of globular clusters as tests of
theories about stellar structure & evolution, star formation, and for
constraining the age of the universe. Also: stellar populations;
dwarf galaxies; effects of environment on galaxies; instrumentation.
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JEAN BRODIE
Office: 141B Kerr Phone: 459-2987
Email: brodie@ucolick.org
Notes:
Observational studies of Galactic and extragalactic globular
clusters; galactic dynamics and chemical evolution;
instrumentation.
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HARLAND EPPS
Office: 133A Kerr Phone: 459-3454
Email: epps@ucolick.org
Notes: HST NICMOS
Astronomical instrumentation: optical design, fabrication, and
testing.
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SANDY FABER
Office: 470 Kerr Phone: 459-2944
Email: faber@ucolick.org
Notes: DEEP, DEIMOS, CfAO, HST WFC
Observational and theoretical studies of the formation
and evolution of galaxies, including: stellar populations; black
holes in galactic nuclei; dark matter; velocity
fields; high-z galaxies. Also: adaptive optics and
astronomical instrumentation.
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JOHN FAULKNER
Office: 403 Kerr Phone: 459-2815
Email: johnf@ucolick.org
Notes:
Theory of stellar evolution, including: red giants and horizontal
branch stars; solar models; dwarf novae; nucleosynthesis.
Also: cosmology; mathematics; history of science.
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RAJA GUHATHAKURTA
Office: 481 Kerr Phone: 459-5169
Email: raja@ucolick.org
Notes: DEEP, CfAO, CELT
Observational studies of globular clusters, galaxies, and
galaxy evolution, including: interacting galaxies; dwarf
galaxies; faint blue galaxies;
Tully-Fisher relation; dust and reddening; stellar populations;
gravitational lensing; dark matter. Also: adaptive optics.
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GARTH ILLINGWORTH
Office: 467 Kerr Phone: 459-2843
Email: gdi@ucolick.org
Notes: DEEP, HST ACS, NGST
Observational studies of high-z galaxies; galaxy formation
and evolution, including: structure; kinematics;
stellar populations. Also: space telescopes.
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BURT JONES
Office: 473A Kerr Phone: 459-2384
Email: jones@ucolick.org
Notes:
Observational studies of stellar dynamics and stellar evolution,
including: astrometry and proper motion studies; spectroscopy
of young and low-mass stars; the rotation, lithium abundance, age,
and chromospheric activity of solar-type stars.
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DAVID KOO
Office: 435 Kerr Phone: 459-2130
Email: koo@ucolick.org
Notes: DEEP, DEIMOS, CfAO
Observational cosmology: angular and redshift distributions of
galaxies, quasars, and gas; clustering; stellar populations;
galaxy evolution. Also: adaptive optics and astronomical
instrumentation.
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GREG LAUGHLIN
Office: 464 Kerr Phone: 459-3208
Email: laugh@ucolick.org
Notes: CODEP
Theoretical astrophysics, including topics in planet formation
and evolution; extrasolar planet searches;
multiple-planet systems; dynamical interactions; evolution of
the universe into the distant future.
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DOUG LIN
Office: 461 Kerr Phone: 459-2732
Email: lin@ucolick.org
Notes: CODEP
Theoretical astrophysics: star and planet formation; dynamical
evolution of planetary, stellar, and galactic
systems; galaxy formation; galactic structure; globular clusters
and dwarf galaxies; interacting galaxies; astrophysical fluid
dynamics; AGNs; accretion.
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PIERO MADAU
Office: 473 Kerr Phone: 459-3839
Email: pmadau@ucolick.org
Notes:
Theoretical astrophysics, including: early structure
formation; reionization; the intergalactic medium;
universe at high-z; radiative transfer; high-energy
astrophysics.
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BILL MATHEWS
Office: 421 Kerr Phone: 459-2074
Email: mathews@ucolick.org
Notes:
Theoretical studies of astrophysical gas dynamics, including:
galactic winds; cooling flows; elliptical galaxies;
instabilities and dynamics in cores of quasars and AGNs.
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CLAIRE MAX
Office: 14 Kerr Phone: 459-2049
Email: max@ucolick.org
Notes: CfAO
Adaptive optics instrumentation; science with adaptive optics;
solar system science.
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JOSEPH MILLER
Office: Nat. Sci. II Annex Phone: 459-2991
Email: miller@ucolick.org
Notes: Director of UC Observatories, CELT
Observational studies of AGNs.
Also: astronomical instrumentation and telescopes.
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JERRY NELSON
Office: 463 Kerr Phone: 459-5132
Email: jnelson@ucolick.org
Notes: CfAO (Director), CELT
Design of giant telescopes; astronomical instrumentation; adaptive
optics.
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JOEL PRIMACK
Office: 209 Kerr Phone: 459-2580
Email: joel@ucolick.org
Notes: UCSC Physics Dept., SCIPP, DEEP
Theoretical cosmology, including: nature and composition of
dark matter; galaxy formation and evolution by analytic and
semi-analytic methods; N-body and hydrodynamical simulations
of structure formation and galaxy interactions.
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JASON X. PROCHASKA NEW FACULTY MEMBER,
ARRIVING SUMMER 2002
Office: Phone:
Email: @ucolick.org
Notes:
Observational cosmology and galaxy formation, including:
quasar absorption line systems, chemical abundances at
high-z and in the Galaxy, missing baryons, high-z galaxy
dynamics, star formation. Also: ISM, cosmological
simulations, metal-poor stars.
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GRAEME SMITH
Office: 149 Kerr Phone: 459-2907
Email: graeme@ucolick.org
Notes:
Observational studies of old stellar populations; stellar evolution;
Galactic chemical evolution; red giants; comets.
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STEVE THORSETT
Office: 439A Kerr Phone: 459-5170
Email: thorsett@ucolick.org
Notes: HETE, GLAST
Observational studies of compact objects, including:
pulsar timing, dynamics, & ages; neutron stars; GRBs & GRB
afterglows. Also: radio observations & instrumentation;
high-precision VLBI; GRB host galaxy observations; high-energy
astrophysics.
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STEVE VOGT
Office: 129 Kerr Phone: 459-2151
Email: vogt@ucolick.org
Notes: CODEP, CELT
Design and use of high-resolution spectrometers; extrasolar planets;
quasar spectra.
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STAN WOOSLEY
Office: 433A Kerr Phone: 459-2976
Email: woosley@ucolick.org
Notes: Department Chair, CODEP, HETE
Theoretical high-energy astrophysics, including supernovae and
gamma-ray bursts. Also: stellar evolution, particularly of high-mass
stars; hydrodynamics; nucleosynthesis; nuclear astrophysics.
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Besides the faculty, there are some other relatively permanent
researchers, valuable resources you should know about:
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JULIAN CHRISTOU
Office: 59 Kerr Phone: 459-5775
Email: christou@ucolick.org
Notes: CfAO
Adaptive optics, especially characterization of PSFs and
deconvolution; science with AO.
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RACHEL DEWEY
Office: 415G Kerr Phone: 459-3081
Email: dewey@ucolick.org
Notes:
Radio pulsars; astronomy education and outreach.
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TERRY MAST
Office: 229 Kerr Phone: 459-3807
Email: mast@ucolick.org
Notes: CfAO, CELT
Design of giant telescopes; astronomical instrumentation;
adaptive optics and its applications.
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RUTH PETERSON
Office: 17 Kerr Phone: 459-3559
Email: peterson@ucolick.org
Notes:
Spectroscopy of stellar populations.
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DREW PHILLIPS
Office: 499 Kerr Phone: 459-3841
Email: phillips@ucolick.org
Notes: CfAO, DEEP, DEIMOS
High-z galaxies and galaxy evolution; instrumentation;
adaptive optics.
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SCOTT SEVERSON
Office: 241 Nat. Sci. II Phone: 459-5149
Email: severson@ucolick.org
Notes:
IR instrumentation, adaptive optics, science with AO.
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And of course, like any healthy department, we have lots of top-notch
postdocs. It is quite likely you will work closely with some, but
they're an even more transient population than graduate students, and
hence hard to list here.
Astronomers vs. professors?
This is a confusing aspect you shouldn't worry about:
Some of our faculty are entirely affiliated with the Astronomy & Astrophysics Department; others are only 20% with the department, and 80%
with the U. of California Observatories/Lick Observatory (UCO/Lick).
This does affect who teaches more classes
(the ones with entirely Dept. appointments), but otherwise this is
not a concern for graduate students. In all respects all faculty
members are well-integrated in the department, and students may work
with whomever they wish.
3.2 Projects/Acronyms
Members of UCSC Astronomy & Astrophysics are affiliated with large
collaborations and other major projects. Here is a brief summary of
some of them, along with a few other acronyms you've seen floating
around:
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· CfAO: http://www.ucolick.org/~cfao/
Astronomical images taken from ground-based observatories suffer blurring
from turbulence in the atmosphere. `Adaptive optics' is a set of
technologies and techniques for correcting these aberrations in
real-time, resulting in images as sharp as those taken from space.
The Center for Adaptive Optics is a major NSF-funded center based in
Santa Cruz, but with member institutions from other campuses of UC and from
across the nation. Jerry Nelson is director of the CfAO; other Center
faculty include Sandy Faber, David Koo, and Raja Guhathakurta. In addition,
further researchers (Julian Christou, Drew Phillips), a
great host of postdocs, and several grad students are affiliated with the
Center.
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· CELT: http://www.ucolick.org/~celt/
The University of California and Caltech are exploring the idea
of a 30-meter telescope, and have dubbed this project the California Extremely
Large Telescope. (If this seems giant to you, note that the Europeans have
begun planning OWL - the Overwhelmingly Large telescope - which will have
a 100-meter primary!) CELT and the CfAO are somewhat related, because CELT
is being designed for AO from the start.
Jerry Nelson and Terry Mast (who were `instrumental' in the design and
construction of the Keck telescopes) are working on this project.
Other faculty affiliates include Mike Bolte, Raja Guhathakurta,
Joe Miller, and Steve Vogt.
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· CODEP: http://natsci.ucsc.edu/codep/
CODEP is the Center for the Origin, Dynamics, and Evolution of Planets,
and that pretty well explains what they're about. Over the next four
years, CODEP will coordinate the hiring of seven new faculty members,
some in Astronomy & Astrophysics, some in other departments.
CODEP affiliates in the Dept. include Peter Bodenheimer, Doug Lin, Steve
Vogt, and Stan Woosley. Astrophysics grads also enjoy the valuable resources
of some other CODEP faculty, including Gary Glatzmaier of the Earth
Sciences Dept. (who is an expert on magnetohydrodynamics and dynamos) and
Erik Asphaug of the Institute of Tectonics (who is an expert on impacts
within the solar system and other aspects of planetary science).
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· DEEP: http://www.ucolick.org/~deep/
The Deep Extragalactic Evolutionary Probe, composed of researchers at UCSC
in collaboration with researchers at Berkeley, Caltech, U. of Chicago,
Hawaii, and Johns Hopkins, is a long-term Keck and HST project. The broad
goals of this large-scale survey of distant, faint field galaxies include
studying galaxy formation and evolution, the origin of large-scale
structure, the nature and role of dark matter, and the overall geometry
of the universe. Phase I of DEEP, already under way, involves Keck
observations with the current suite of instruments, and HST observations.
The next phase of DEEP will employ DEIMOS, a new spectrograph for Keck
being constructed at Santa Cruz, and SIRTF, NASA's next great space
telescope.
Members of the DEEP team at Santa Cruz include Sandy Faber, Raja Guhathakurta,
Garth Illingworth, David Koo, and several postdocs.
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· DEIMOS: http://www.ucolick.org/~loen/Deimos/deimos.html
The Deep Extragalactic Imaging Multi-Object Spectrograph is an
impressive Keck instrument being built at Santa Cruz. Sandy Faber is the
PI of the project; other Santa Cruz researchers affiliated with DEIMOS
include Terry Mast, Garth Illingworth, Drew Phillips, and other DEEP team
members.
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· GLAST: http://glast.gsfc.nasa.gov
The Gamma-ray Large Area Space Telescope is a future
NASA mission that may launch as early as 2005. It will study high-energy
astrophysical phenomena, including but not limited to neutron stars
and GRBs.
Steve Thorsett is an interdisciplinary scientist on the GLAST team.
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· HETE: http://space.mit.edu/HETE/
The High Energy Transient Explorer mission recently launched, and the
commissioning of its instruments is under way. HETE's goal is to
provide precise localizations of gamma-ray bursts. This will
facilitate follow-up observations of the afterglows, and further our
understanding of GRBs a great deal.
Stan Woosley and Steve Thorsett are affiliated with the project.
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· HST: http://www.stsci.edu/
Of course, one of the premier instruments of astronomy
today is the Hubble Space Telescope. Harland Epps was involved in the
optical design of the NICMOS instrument; Sandy Faber is on the WFC team.
Garth Illingworth is affiliated with the Advanced Camera, an instrument
slated to be installed on HST as a testbed for NGST technologies. Many
(if not most) researchers at UCSC work with HST data regularly.
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· NGST: http://ngst.gsfc.nasa.gov/
A high priority in major astronomy funding over the
next decade, the proposed Next Generation Space Telescope will be an orbiting
8-meter class telescope. It is intended to pick up where HST leaves off ...
Garth Illingworth has some affiliations with the project.
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· SCIPP: http://scipp.ucsc.edu
The Santa Cruz Institute for Particle Physics, primarily concerned
with accelerator experiments at SLAC and CERN, is also involved in
particle and high-energy astrophysics. Current interests include
the Milagro cosmic ray airshower detector and the GLAST mission. In
addition, SCIPP supports the work of theoretical cosmology.
Joel Primack, George Blumenthal, and several members of the Physics
Dept. faculty are affiliated with SCIPP.
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· UCO/Lick: http://www.ucolick.org
The University of California Observatories/Lick Observatory is an
organized research unit of the UC system. Lick Observatory, located
atop Mt. Hamilton near San Jose, harbors 3-m and 1-m `workhorse'
telescopes that are extensively used by faculty and graduate students.
In addition, UCO/Lick administers the UC portion of access to Keck
Observatory atop Mauna Kea, which is shared with Caltech. The twin
Keck telescopes (10-m) are the largest in the world, and UCSC
researchers make extensive use of this facility.
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3.3 The graduate curriculum
In roughly chronological order, here's how you get from where you are
now to a PhD:
Classes
Table 2 lists the classes usually taught
in our curriculum. In approximately your first two
years (that's 6 quarters, not 4 semesters),
you will take 12 ``real'' classes, plus 2 others. Let me
get the ``others'' out of the way first: one (Intro. to Research)
is simply a course where each faculty member comes by to chat with your
class of first-years about his or her research; the other is
Independent Study, which you must take in connection with your
Research Project. Read more about that below.
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Table 2: Astronomy & Astrophysics courses.
(Boldface indicates a required class; 14 total required.)
| Physics (3)3 | Stars (3) | Galaxies (3) | Other (2) |
E&M/Plasmas | Stellar Structure
| Galaxies A | Intro. to Research |
General Relativity | Star Formation | Galaxies B | Ind. Study |
Physics of Astrophysics A | Star Death | Galaxies C | Observation Techniques |
Physics of Astrophysics B | Accretion | Cosmology | Radio/Sub-mm |
Gas Dynamics | Compact Objects | Low-Density | Instrumentation |
QM sequence4
| Atmospheres | Stellar Dynamics | Planetary Science |
Classical Mechanics | | | Numerical Techniques |
Magnetohydrodynamics | | | |
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As for the 12 ``real'' classes: You will be required to take 3 classes in
particular. One is an E&M class on radiation and plasma physics;
one is a standard course in stellar structure & evolution; one is a standard
course on galaxies. After that, you must take at least 2 more classes from
the ``physics'' column, 2 more from the ``stars'' column, 2 more from the
``galaxies'' column, and then take whatever you like until you have 12.
Read more about classes in §3.4.
TA
At least one quarter you must be a Teaching Assistant.
Typically students do this early, when they don't necessarily have a regular
research advisor for financial support anyway. You become a TA by
signing up to TA for a particular class or by consultation with Mary
(the Dept. Manager). There may be some paperwork to fill out and you
have to be on the appropriate payroll. TAs at UCSC are unionized;
this can have arbitrarily small or large impact here in the Astronomy & Astrophysics Dept. where TAs have usually not been particularly abused. TAing
involves teaching sections, holding office hours, and grading papers.
You may need to guest lecture for the professor when s/he's out of town.
Research Project
Ideally during the summer between your 1st and 2nd year,
you will work on a roughly Master's-thesis-size project. (This is
sometimes referred to as the Second-Year Project.) A good thing
to do is to use the
Independent Study course in the spring before or
the fall after that summer, either to prepare for your project or to
finish it up. Your first summer is coming sooner than you think, so
start thinking about this!
When you're done, if you can get a publication out of it,
that's great; if not you must submit a journal-style writeup to the
Dept. to help fulfill this requirement. You must also give a talk
(in the form of a FLASH, see below) on your Research Project.
It is certainly allowed (sometimes even encouraged) to change topics
completely between your Research Project and your thesis. So don't
worry that in your first year you are choosing the field you will
spend the rest of your life on. Of course, if you find that you
do want to continue in a certain specialty beyond the
Research Project requirements, and into a thesis, well that's fine too.
FLASH
FLASH (the Friday Lunch Astronomy Seminar Hour) is a weekly
talk given by visitors, faculty, postdocs, or grads.
In connection with the Research Project, you must give
a FLASH by the end of your 2nd year to finish the completion of this
requirement.
Prelims
The prelims are two 3-hour written examinations: one is on basic physics and
the other is on graduate-level astronomy & astrophysics. The department offers the
prelims every June. You may pass either
or both exams in your first attempt. You really should pass both
sections by the summer after your 2nd year, i.e., after your second
attempt. However, see the Dept. Review.
You should get your hands on prelims from previous years; that's the
best way to grasp what level the exams are at. But basically, the
physics exam is intended to test your use of basic physics and
physical intuition. In principle there is no need to have taken the
grad astro classes for this exam. You are expected to answer/attempt
all questions on the physics exam. The astro exam, on the other hand,
is usually formatted as a question or two from every class that has
been offered in our dept. over the previous two years. (In addition,
sometimes classes from outside the dept. are included if it is known
that astro students took the class or it otherwise seems relevant.)
You are then usually asked to answer/attempt a portion of the
questions, of your choosing.
Dept. Review
Typically just before your 3rd year the faculty review your progress.
By the time of the Dept. Review, you should have completed your
classes, your Research Project and its FLASH, and passed the prelims.
``Passing'' the Dept. Review typically means being granted a Master's
and being encouraged toward thesis work. In other instances
you may be provisionally passed with the
opportunity to re-take the prelims or an extension on your FLASH. In
principle, the faculty could choose not to pass you.
Qual
After completing classes, prelims, and all
Research Project requirements, it's time to start thinking about a thesis.
The Qualifying Exam is the place to propose and defend a thesis topic; that
means you don't necessarily have to complete lots of the thesis work before
this exam. The Qual is a defense-style exam: you give some presentation but
also face comments, objections, and suggestions from your committee.
Students are encouraged to complete their Qual by the end of their
3rd year, and are required to do so before the end of their 4th.
Upon passing the Qual, one has ``Advanced to Candidacy''.
More FLASHes
You need to give a couple more FLASHes as you
progress on your dissertation work; this is good practice for your thesis
defense and all the talks you'll have to give as you apply for postdocs.
Defense
Finally, of course, you must write a thesis and defend
it in front of your committee. Hopefully your thesis is composed of
several publications you've written while you worked; that will help with
your postdoc applications. Then you're done!
3.4 Classes
A little more about classes: To fulfill your class requirements,
there will be quarters in which you will have to take 3 classes. Our
advice is to be careful when you do this. Ask around about the
relative workloads of various classes, and factor in whether you'll be
TAing or whether you expect to get any research done. It is nearly
impossible (or dangerously stressful) to TA or GSR while taking 3
relatively serious classes.
The current mode of class scheduling in the dept. works like this:
one year is a ``stars'' year - 220A (Stellar Structure &
Evolution), 220B (Star & Planet Formation), and 220C (Late Stellar
Evolution/Death/Supernovae) are taught in succession in such years.
The next year, then, is a ``galaxies'' year, with an analogous
sequence of courses taught. In any year there are other courses
taught from any and all columns as well.
It is not always the case that the same person teaches the same course
every time, but often it is. Here's a quick list of the courses and
who you might want to chat with about them, along with a pithy
statement and the textbook used if there is a consistent one. Be
warned that there's been some tinkering with what goes in what
classes, and that continues to go on, so don't take this as cast in stone:
- AY202: E&M/Plasma Physics
- George Blumenthal. Basically a
course on the second half of Jackson - classical radiation
processes. A required class for astro grads (the required class of
the ``physics'' column); often cross-listed as PH213,
the second half of the physics grads' E&M sequence.
- AY204A: Physics of Astrophysics A
- Doug Lin. What material goes
in what order in the PoA series is in flux. In the past this has been
a course on dynamics and statistical mechanics. Not sure what it will
be in the future.
- AY204B: Physics of Astrophysics B
- George Blumenthal. Ditto
the previous PoA disclaimer. In the past the course has been on the
disparate topics of quantum radiation processes and MHD.
- AY205: Intro to Astro Research
- Graeme Smith. Graeme organizes
a seminar series, basically, wherein each faculty member comes and
describes her/his research with your class of 1st-years. In some
sense not a ``real'' class, but required.
- AY210: Stellar Atmospheres
- ??. Not offered in anyone's
memory.
- AY220A: Stellar Structure & Evolution
- Peter Bodenheimer. The
standard course in stellar structure. Peter uses Kippenhahn &
Weigert as the text. Pencil-and-paper as well as stellar model coding
is involved. This class is the required course in the ``stars'' column.
- AY220B: Star & Planet Formation
- Peter Bodenheimer. Much like
220A in form; assumes 220A as prerequisite.
- AY220C: Advanced Stages of Stellar Evolution &
Nucleosynthesis
- Stan Woosley. ``Star Death'' or ``Supernovae'' -
no one calls it by the catalog name. Assumes 220A as prerequisite.
- AY222: Planetary Science
- Doug Lin. Not taught recently, but
will be this year, so tell us how it goes.
- AY225: Compact Objects
- Steve Thorsett. Not taught recently.
- AY226: General Relativity
- George Blumenthal. When last taught,
George used Weinberg's text.
- AY230: Low-Density Astrophysics
- Bill Mathews. Sort of a course
on the ISM.
- AY231: Astrophysical Gas Dynamics
- Bill Mathews. Also sort of a
course on the ISM.
- AY233: Physical Cosmology
- George Blumenthal. Regarded as
complementary, but perhaps prerequisite to, Joel's class PHYS224.
- AY235: Numerical Techniques
- Greg Laughlin. A new class.
- AY237: Accretion
- Doug Lin. Don't know very much about this
class, sorry.
- AY240A: Galactic & Extragalactic Systems
- Sandy Faber.
The required class from the ``galaxies'' column. Binney &
Merrifield with some from Binney & Tremaine.
- AY240B: ditto?
- Garth Illingworth. Not sure what the
``official'' name of this is, but like AY240A but with more emphasis
on high-z galaxies.
- AY240C: ditto?
- Piero Madau. Very high redshift cosmology.
- AY253: Stellar Dynamics
- Doug Lin. A standard course out of
Binney & Tremaine.
- AY257: Modern Observational Techniques
- Mike Bolte. Data
reduction techniques, etc.
- AY260: Instrumentation
- Jerry Nelson & Terry Mast. Jerry and
Terry organize a series of lectures by themselves and many others on topics
in instrumentation.
- AY275: Radio/Sub-mm
- Steve Thorsett. Last time Steve suggested
Rohlfs & Wilson, and Burke & Graham-Smith.
- PH224: Cosmology/Early Universe
- Joel Primack. A course with a
heavy emphasis on current research.
- PH215-218: QM/QFT sequence
- Various instructors. Standard
non-relativistic quantum mechanics (215 & 216) followed by quantum
field theory (217 & 218). A sequence, each class a prerequisite for
the later courses.
- EMS275: Magnetohydrodynamics
- Gary Glatzmaier. Offered in the
Earth & Marine Sciences Dept. Gary also teaches courses in fluid
dynamics that parallel the astro dept's.
- EMS290: Topics in Planetary Science
- Erik Asphaug. A seminar.
- ENG206: Bayesian Statistics
- David Draper. A new course in the
Applied Mathematics dept.
- AY292: Seminar
- The astro colloquium.
- AY297: Independent Study
- What you sign up for to get
credit-hours for non-thesis research, like your 2nd-year Research
Project. Mary can give you the codes to sign up with your particular
advisor.
- AY299: Thesis Research
- What you sign up for to get credit-hours
(and thus make you a student) after classes are done and you are
working on your thesis.
- AY301: Teaching
- What you sign up for so that TAing appears on
your transcript.
If you take classes outside the department, keep in touch with Steve
Thorsett or Stan Woosley (Dept. Chair) about what requirements they
might fulfill. We have in mind here some courses in the Physics Dept. or in Earth & Marine Sciences.
You register for classes via the Schedule of Classes and Teleslug.
The SoC is at http://reg.ucsc.edu/soc/ while Teleslug is
http://teleslug.ucsc.edu/. All that is explained in §4.
In principle you have the option to take classes for a grade, rather
than Pass/Fail (or, we guess, Satisfactory/Unsatisfactory is what your
grade record actually says). The consensus opinion is that there is
no reason to opt for grades, and we aren't aware of grads who do
or have. You will receive ``narrative evaluations'' of your
performance, once the professor gets around to writing them. These
can either be essentially just a grade (``Student X performed in the
middle third of the class''), or, in the best of situations, a
highly-detailed account of your strengths and weaknesses. This can
alert you to what you might want to work on.
3.5 Advising
A logical question you might ask at this point is, ``Who's my
advisor?'' In some sense, you don't have (or really need) one, until
you are doing research. Then whomever you work for is your advisor.
Before you are doing research, if you feel you need advising, in some
sense any faculty member will do. More strictly, though, Steve
Thorsett is the Associate Chair in charge of the grad program. So
probably, you should start with him on whatever advising questions you
have.
Once you start research, your research advisor is your advisor. (You
should still feel free to shop around for opinions, however.) Upon
passing the Dept. Review, you will need to form a committee of advisors
to serve as your Qualifying Exam Committee. This same committee will
likely become all or most of your Thesis Exam Committee when you do
your defense.
3.6 Department events
There is an extremely informal coffee/tea/cookie break at 3:30pm
nearly every day. It takes place at the table and chairs in front of
the elevators on the 4th floor of Kerr Hall.
The Astronomy & Astrophysics colloquium is on Wednesday afternoons. Cookies and
coffee start at around 3:30pm, usually in Kerr 283 but sometimes in
the 2nd floor lobby. Then, eventually, people wander up to Nat. Sci. Annex room 101, where the colloquium talk is actually held. The talk
typically starts around 4:00. See 3.7 for
important info about colloquium cookies.
The FLASH - Friday Lunch Astronomy Seminar Hour - is held on
Fridays at 12:30 in Kerr 283. Bring your lunch and see a talk.
Sometimes there are FLASH-like talks on other days, given cute names
like MLASH, THLASH, etc.
The talk schedule for a week is usually emailed out on Monday.
Repeated reminders of the talk may come from the speaker's host(s).
In addition, the current talk schedule is available at
http://www.astro.ucsc.edu/talks.xml.
Some other talks in other departments: The Physics Dept. colloquium
is on Thursday afternoons, with a similar 3:30 cookies and 4:00 talk
schedule. The colloquium schedule is at
http://maxwell.ucsc.edu/events/colloquia.html. The CODEP
seminars are always moving around, but the schedule is at
http://www.es.ucsc.edu/~asphaug/taps.html.
GAS, the Grad Astro Seminar, is something
like a journal club. Grads give short informal talks on a rotating
schedule. Check it out at
http://www.ucolick.org/~novak/Gas/.
Subject to the whims of the Beer Czar, we usually have Beer Hour on
Friday evenings.
Other less frequent department events include:
- The annual Lick Picnic, at the Observatory on Mt. Hamilton.
This year it's on September 22.
- A welcoming reception for you, the incoming grad students,
sometime in the fall. Be warned, you will probably be asked to supply
some story about yourself or something.
- Cake and champagne for grads completing their defenses; goodbye
festivities for departing postdocs, grads, etc., the occasional wild
party at a faculty member's house, ...
- Prospective season: hosting prospective graduate students,
answering questions, taking them out to dinner, etc., as was done for
you when you were a prospective.
3.7 Your dept. responsibilities; Czars
You should sign up for ASTR292, which is labeled ``seminar'' in the
Schedule of Classes. It's actually the Dept. colloquium, it isn't
really a class at all. It's just necessary
that people sign up so that the department can reserve the room.
Every grad student who has not yet passed his/her Qual is needed to
prepare cookies & coffee for colloquium. Each week, it becomes the
next student's turn. When it's your turn, you should go buy about
$20 worth of cookies and other goodies. You prepare the coffee,
cookies, and set up the room where the refreshments will be served.
You clean up after the colloquium, turn in your receipt to the office
to get reimbursed, and you're done. The Cookie Czar will explain all
this to you as well. Or you can check out the instructions at the
current cookie czar's website:
http://www.ucolick.org/~laura/cookies/.
You may wonder why this is our job - the
origins are lost to unrecorded history.
Various other responsibilities are delegated through
czarships. In principle, czars are elected democratically by
the grads; in practice, czars often choose their successors and the
voting is a formality. As the name suggests, czars typically have
complete reign over their domain. Czars are determined in a meeting
held in the fall, long enough after you get here that you'll have
figured most of this out. Here's some of the current czars:
- Czar Czar
- The `czar of czars' is our graduate student
representative in Dept. faculty meetings - our way of providing input
into many department decisions. Also, the czar czar is in charge of
grad office space (so is sometimes also known as Space Czar). This
position can entail a lot of work. Currently the position is in flux,
with some of the duties being filled by Patrik Jonsson.
- Telescope Czar
- The telescope czar keeps track of the locations,
state of health, sign-outs, etc., of the several small amateur telescopes the
department owns. The current telescope czar is Jason Melbourne.
- CPMC Czar
- The CPMC is the Computing Policy Management
Committee. This czar is the grad representative to that committee.
Currently Phil Choi.
- Beer Czar
- This extremely important czar is in charge of beer
hour on Friday evenings. In the distant past beer czars arranged for
folks to meet at a bar downtown; the current beer czar has simplified
the process by bringing beer and pizza to the Kerr Hall balcony.
Prices are low; chances for hilarity are high. The current beer czars
are Mike Kuhlen and Ian Dobbs-Dixon.
- Colloquium Cookie Czar
- This czar is in charge of the assignment
of colloquium cookie duties to pre-qual grads, as well as maintaining
all the necessary supplies. The current colloquium cookie czar is
Laura Langland-Shula.
- Prospective Czar
- This czar has the arduous task of coordinating
the visits and recruitment efforts for prospective graduate students.
This position can be quite a lot of work. This year's prospective
czar is Tami Rogers, assisted by Alex McDaniel.
- Ask-an-Astronomer
- OK, it doesn't have ``czar'' in its name.
This team answers questions from our ask-an-astronomer website. The
team is currently Kurtis Williams, Marla Geha, Mike Kuhlen, and Greg Novak.
- GSA rep
- Another without ``czar'' - so sue us. This person is
the Astro department representative to the Graduate Student
Association.
- Mail Czar
- This czar or czars handles paper mail the Observatory
and Dept. receive from the public, often with questions similar to
what Ask-an-Astronomer gets. Currently these are David Lai and Sarah Martell.
- Admissions committee
- The faculty allow a grad to sit on the
admissions committee that decides who enters our grad program. Last
year this representative was Anne Metevier.
- Advising
- The grad who serves as advising point-person is Scott
Seagroves.
- RSI Czar
- This czar is in charge of distributing painful
debilitating injuries - just kidding. Many grad students have
suffered a little or a lot from RSI - repetitive strain injuries -
because we sit around and type all the time. This czarship was
created as a watchdog/activist for various things like ergonomic
furniture, seminars, xwrits software (that reminds you to
take wrist breaks), and other safety concerns. Currently the RSI czar
is Kurtis Williams.
- Phone Czars
- Traditionally (but not without protest) the
inhabitants of Kerr 413 have phone calls from the public directed
toward them. These calls range from ``Hey what's this bright star I
see for an hour or so after sunset in the west?'' to ``Is it true that
we will all die because of the tidal forces during a planetary
alignment?'' and so on. You don't always know the answers - often
you don't even understand the questions - but just do your best and
be nice.
- GAS Czar
- The grad student journal-club like seminar is
maintained by Greg Novak.
Of course, other things come up that need to be done, that don't
necessarily fit into these czarships. For instance, the document you
are reading needed to be written; similarly a FAQ was written for
prospective students in the spring (and some of this is cribbed from
there). Usually we take a czar-like attitude about these things too,
meaning once someone has volunteered to take care of a task it
generally becomes that person's exclusive domain.
3.8 Computing
The Lick and Dept. system administrators are NICS - Network,
Information, and Computing Services. Their email alias is
nics@ucolick.org. Be warned that the information in this
section is more likely to go out-of-date soon, given the nature of
computers and computing.
Hardware
There are NICS-managed and non-NICS-managed computers on the network;
the non-NICS-managed hosts are maintained by their users. Among the
NICS-managed hosts, there are several public machines which everyone
has accounts on. When you first arrive, you will likely have a
computer on your desk; if not you will have an
X terminal from which you login to one of these public
machines. (Some of the public machines are unable to serve up X
sessions, but you may still login to them via ssh once you
have a session running.)
Public machines running SunOS/Solaris include isis and
megatron. Public DECs running Digital UNIX include
bigdog. Public Linux boxes include cobra, mariachi
and zoltar. We have probably missed some public machines.
Your public account will appear as /u/yourusername, which is
usually visible from any NICS-managed machine (public or not) as
/home/public/yourusername.
If you don't have a computer, eventually you will move up from the X
terminal on your desk to a computer of your own, so that you do not
have to share processor time with others. This will mean you will
have both a public account and a separate, private account on that
machine. That machine may be a NICS hand-me-down, or a machine bought
for you by an advisor (which can then be NICS-managed or not).
A quick list of some printers: the main general-use printer on the
4th floor is, naturally enough, floor4. The color
printer next to it is color. You can use the command
printers to see lots of printers around the dept. if you are
curious what a printer's name is.
Software
Usually, though not always, the set of NICS-supported software is
consistent across machines running the same OS. That is to say, a
given program like enscript has been installed on the Solaris
hosts, and is consistent no matter which one you are logged into. It
may happen to not exist on the Linux hosts, however. If that becomes
a problem you could always ask NICS to install something.
Often one can download open-source software and install it privately
on your own account. This is fine. But make sure the software you
want really doesn't exist elsewhere or that it's not worth it
to ask NICS to install/update it, before you go using your own disk
space on it. (An example: I (SS) keep my own set of LATEX packages,
my own set of IDL Astro Library routines, etc., because I keep them
more up-to-date than NICS does.)
OK, this will certainly not be an exhaustive list, but here's some of
the software commonly used around here:
- Network/Internet
- All insecure forms of login are disabled; we
use ssh for remote logins (also slogin)
and remote command-execution.
Print to the printers via lpr and other scripts/variations
thereof; query the print queue with lpq.
netscape is the default browser, but you could try
opera or mozilla. Mail programs used by folks include
pine, elm, mutt, and UNIX mail.
- Document production
- Standard editors like emacs,
pico, vi, etc., are used around here. We have a
fairly standard TEX/LATEX/ AASTEX/ BIBTEX
distribution. Some people use StarOffice (soffice) for
working with documents (and you can make PowerPoint-like
presentations). xfig is a clunky but useful
graphics-production program; for graphics manipulation we also have
gimp.
- Viewers
- For viewing all these sorts of documents, we have
xdvi as part of the standard TEX distribution - and we
forgot to mention dvips and dvipdf for making
PostScript and PDF files from your LATEX dvi output. Various
implementations of GhostScript (gv and gs) are used to
look at PS and PDF files; often more useful for PDF is
acroread. xv is useful for looking at graphics
files in almost any format.
- Science
- Here's where we're most likely incomplete. For
coding, standard f77, f90, cc, etc.,
compilers are around. Also people code in IDL (idl),
perl, other scripting languages, and the standard UNIX shell
scripts plus sed, awk, and derivatives. For producing
graphics/plots there are IDL, SuperMongo (sm), the
pgplot and pgperl routines for producing plots from
within other code, xmgrace, and we're sure more that we're
forgetting. Data reduction with IRAF (plus ximtool and
SAOImage/ds9), IDL, and other standard stuff is, well, standard.
Other, more specialized packages like
DAOPHOT/ALLSTAR/ALLFRAME, GIM2D, SExtractor, and many many more are
usually maintained at the user level (or gotten from the authors)
rather than at the system-wide level.
3.9 Funding/Support
The Dept. guarantees support (in some form or another) for its
graduate students. There is the occasional Dept. Fellowship, often
used to support 1st-year students who take a heavy courseload. You
can be a TA; you can be a GSR (Graduate Student Researcher, what is
often called an RA position at most other institutions). TAing in our
department involves holding discussion sections, office hours, grading
papers, etc. GSRs are paid to do research.
You are, of course, encouraged to apply for funding (grants,
fellowships, etc.) of your own. This frees you from the particular
project an advisor might have a grant for, for instance.
Assuming you don't have external support, you need to secure funding
for the next quarter, every quarter. That is, suppose your Dept. fellowship is up (if you have one at all) after, say, two quarters.
Then sometime during the winter quarter you need to find someone to do
research with during the spring, or else sign up to TA in the spring.
The Dept. fellowship given in the first year is the only real
instance of ``free'' money - for the rest of your time you will need
to GSR or TA (barring external support).
The pay scale is confusing, and we will probably get it wrong here.
The gross pay for a GSR in our department before advancing to candidacy
(pre-qual) is ``Step 4'', $1566/month. Immediately upon advancing to
candidacy the pay increases to ``Step 5'', $1670/month. One year
later, the pay increases again to ``Step 6'', $1748/month. There is
a plan which may happen, which would implement a pay decrease
of one ``step'' upon year 7 in grad school - an obvious attempt to
keep time-to-degree short. Here's the confusing part: TAs, we think,
make $1413/month if they are not 1st-years. In your
first year, as some sort of break, the Dept. pays your ``fees'' (a
couple hundred dollars a month), so if you TA your pay is a bit higher
in your 1st year. Confusing? Yes.
TAs and GSRs are paid at the beginning of each month, for the previous
month. This means you may not get paid until November 1, depending on
when you joined the payroll. If you are on a fellowship, you will be
paid once at the beginning of the quarter - make sure the money
lasts! It is possible to take out (rather enormous) federal student
loans while in graduate school. Not necessarily a bad thing, but be careful.
3.10 Miscellany
Little things that didn't fit anywhere else are here.
Your address at the mail room (Kerr 9) is something like:
UCO/Lick Observatory
Astronomy Dept., Kerr Hall, UCSC
Santa Cruz, CA 95064
Other variants that take advantage of the UCSC address (1156 High St.)
will probably also work.
Mary will loan you keys to the supply closet (adjacent to the
stairwell on the basement floor) whenever you need. There you can get
all sorts of office supplies for your desk. She also keeps a
mini-stash in her office.
The copy machines take copy-cards, not real money. When TAing, the
dept. can issue you a copy card for that purpose; similarly your
research advisor can usually get you a copy card that deducts from
his/her grant. For personal use, you need to purchase a copy card
from one of the libraries, and maintain money on it.
You need a sticker from Mary at the beginning of each new quarter,
which goes on the front of your student ID. This indicates that you
are currently enrolled; without the sticker your ID has essentially
expired, meaning you can't ride the bus for free and other inconveniences.
4 The University
The UCSC website is, appropriately enough, http://www.ucsc.edu.
The ``A-Z Index'' is often useful when you don't know where to start.
4.1 What's where; campus facilities
It seems silly, but you might want to keep a campus map with you for a
while, if you plan to be walking those footpaths and trails through
the redwoods. Just getting from Kerr Hall over to seemingly nearby
places like McHenry Library or the Hahn Student Services can be
confusing at first.
Science Hill
The astronomers and physicists are in Kerr Hall (bet you already knew
that), which is at the southern, low-elevation end of ``Science
Hill''. Our new building, the Interdisciplinary Science Building,
will be complete soon (and we'll move) - it's located more in the
heart of Science Hill, adjacent to Natural Sciences II, the Earth &
Marine Sciences building, and the new almost-finished Center for
Adaptive Optics building.
``Union''
The campus doesn't really have a student union in the sense that many
other campuses do, but we didn't know what else to call this section.
There's a region of campus east-northeast of Kerr where the Bay Tree
Bookstore (http://slugstore.ucsc.edu),
Whole Earth Restaurant, and Graduate Student Commons
(http://www2.ucsc.edu/gradcommons/) are located. Incidentally,
ID card services are located adjacent to the bookstore.
Cashier, Registrar, etc.
The campus cashier (http://www2.ucsc.edu/accts-rec/cashier.htm),
registrar
(http://reg.ucsc.edu), and financial aid
(http://www2.ucsc.edu/fin-aid/) offices are all
located in Hahn Student Services, sort of between the bookstore and
McHenry Library.
Libraries
It is surprising how little we need to use the libraries for work, but
you may be curious so here goes. The main university library is
McHenry, located east of Kerr along a couple of footpaths. You can
buy a personal copy card there, among other things. The Science
Library, more likely to be of use, is north of Nat. Sci. II. We
think you can buy copy cards there too.
Mail
Outgoing campus mail and US mail can be dropped in the appropriate
mailbags in the Dept./Lick mailroom, Kerr 9. There is a US Post
Office located in Applied Sciences aka Baskin Engineering, on its west
side, lowest floor.
Restaurants and coffee carts
Aside from the Whole Earth Restaurant located at the Grad Commons
building, there is also a restaurant in Kresge (whose name is always
changing); a co-op at Kresge that sometimes sells good food; a
taqueria in Merrill; a coffeeshop in Cowell.
There are Peabody's Coffee carts/stands all over campus: in the
Theater Arts Center; in Sinsheimer; in Earth & Marine Sciences; and
probably more.
The ``lunch lady'' brings food to the 2nd-floor lobby of Kerr
every weekday at 12:00.
4.2 Structure
The University is organized by Divisions and Colleges. The
undergraduate program revolves around the residential colleges
(Kresge, College Eight, Porter, etc.), while academia for undergrads
and grads involves the divisions. For instance, our department is, as
you might expect, a part of the Natural Sciences Division. If you are
ever asked what college you belong to (on a form or something), just
say you are a grad student. This is confusing because really, we have
no college, but there is a Graduate Division.
So for your purposes, the only relevant levels in the hierarchy are
the Natural Sciences Division, through which you get paid when you TA
(among other things), and the Graduate Division, which sets things
like the deadlines for submitting one's PhD materials, thesis
guidelines, etc.
Many activities, such as registering for classes, changing your
address with the Registrar, and more, can be done online. Most of the
websites mentioned in the text, along with some more, are collected in
§A.
4.3 Transportation and parking
The University runs shuttles around the campus, free of charge. Maps
with the various routes are at
http://www2.ucsc.edu/taps/maps.html. The Santa Cruz bus system
has a series of bus routes numbered between 10 and 19,
which service the University
and town and are free to students during academic quarters. Their
routes and other information are available at
http://www.scmtd.com.
Parking is very expensive. The permits that are available to grads
are listed at
http://www2.ucsc.edu/taps/students01.html#grads; a
B permit will cost you $192/year. A much more cost-effective option
is the carpool permit; a B carpool permit is $108/quarter, and this
can be split among those participating in the carpool. (There are
various requirements - you need to show that you live off-campus,
show your car registration, etc.) If you are concerned that there
might be times when you don't want to carpool, you can also
buy a packet of 50 ``scratch-offs'' (one-time-use permits) for $125,
once per year.
4.4 Housing
There is University housing for graduate students. The rent is
expensive even by Santa Cruz standards: $800/month for 2001-2002 and
going up every year. This buys you a room in a four-bedroom apartment
with other grads. For more, check out
http://www.housing.ucsc.edu/housing/graduate.html.
If you are married, in a domestic partnership, or have children or
other dependents, you are eligible for Family Student Housing. Those
with children are given priority; the rent is $810/month, which buys
you a two-bedroom townhouse. This is a great deal in Santa Cruz.
Check them out at
http://www.housing.ucsc.edu/housing/family.html.
For living off-campus, the University has the Community Rentals Office
where there are many listings. They are physically located in Social
Sciences II, but you can now access the listings online at
https://housingweb.ucsc.edu/cro/welcome.asp.
5 Santa Cruz and environs
5.1 Geography
Basic geography: the greater Santa Cruz area occupies the northern end
of the Monterey Bay. Several towns merge smoothly together to form
this area: from west to east they are Santa Cruz, Live Oak, Capitola,
Soquel, and Aptos, with of course other small places too that we
didn't name. Continuing around the Bay along Hwy 1, one arrives at
Watsonville (important for your purposes because it hosts the local
Target!) after 12-15 minutes' drive. Continuing on you eventually get
to the other ``end'' of the Monterey Bay at Monterey itself.
So, the immediately adjacent towns that you might see, for instance,
in housing listings, are: Santa Cruz, Live Oak, Capitola, Soquel,
Aptos, along the Bay roughly from west to east;
in the hills north of Santa Cruz along Hwy 9
(and the San Lorenzo River) are the towns (from south
to north) of Felton, Ben Lomond, and Boulder Creek; north of the
campus along Empire Grade is Bonny Doon; Davenport is northwest of
Santa Cruz along Hwy 1; north along Hwy 17 is Scotts Valley.
The urban areas of the San Francisco Bay are closest ``over the hill''
at the South Bay - San Jose, Santa Clara, etc. This can be a
30-minute drive over Hwy 17, or much much longer depending on
traffic. All the larger cities from San Jose up to San Francisco (on
the west side of the Bay) or up through Oakland and Berkeley (on the
east side of the Bay) are easily two hours' drive from Santa Cruz, and
often much shorter depending on traffic.
5.2 Housing
OK, you're probably aware that getting housing in Santa Cruz is an
ordeal. There's not much we can say here that will make it
not an ordeal, so we'll just briefly give you some
information.
If access to the University by bus, bike, or easy commute is important
to you (as it is to most), then you probably want to live in
``westside'' Santa Cruz (west of the river), or in ``eastside'' Santa
Cruz or Live Oak. As you move further east to Capitola, Soquel,
Aptos, etc., you will find that you have to transfer bus routes to get
to the University, or that your 12-minute car ride becomes 50 minutes
during rush hour.
It's hard to pin down what a ``typical'' rent is; it of course depends
on how great the place you're renting is. It is possible to pay less
than $500/month, but that is becoming rare. So, expect that you may
need to fork out first and last month's rent plus a deposit in order
to move in to a place - that could be $1500-$2000.
A bunch of places to look for listings are given in §A.
Finding housing is a bit of a game. You are in competition with lots
of other students, but remember that many of them are undergrads. You
stand out if you present yourself differently. Rather than calling
yourself a ``student'', emphasize that you are a ``PhD student'' or
something similar. Don't assume that a potential landlord knows what
a grad student is, or that it differs from an 18-year old college
freshman. Pursue housing actively; passively leaving messages and
waiting for calls back may work eventually but will take much longer
than you'd like. If you need references, Mary in the dept. office,
or perhaps a faculty member if you ask nicely, will lie and claim to
have known you forever. Or if they won't lie, they can at least vouch
for the fact that you are employed and all.
5.3 Transportation
It is possible to live in Santa Cruz without a car. The bus system
(http://www.scmtd.com) is pretty good, and free to enrolled
students during academic quarters. Some service is available directly
from where you might live to the University; from other locations you
might have to transfer routes.
Some public transport is available to get over the hill - via the
Santa Cruz route that goes over 17, or via Greyhound and other bus
services. Once over the hill it is not hard to make one's way to the
Bay area's transit options like BART (http://www.bart.org)
and Caltrain (http://www.caltrain.com/caltrain/index.html).
There is a lot of support for bicyclists: bike racks on buses, a
University van with bike trailer from Mission & Bay to campus each
morning (see the TAPS webpage); bike racks for BART and CalTrain, etc.
Most who have lived in Santa Cruz without a car gave in after a year
or so - it is pretty difficult and time-consuming to go to the city
or go to Target in Watsonville without a car.
5.4 Businesses and other miscellany
The main business districts in the Santa Cruz area are: along Mission
(Hwy 1) from about Chestnut to Western, particularly around Mission &
Bay; ``downtown'' centered around Pacific and extending a block or two
east and west; across the river along Soquel; and many more as you
move further east.
Suppose you need to shop for groceries; this seems like something that
might come up. Your choices include the Safeway on the westside at
Mission and Swift; New Leaf Market or Zanotto's downtown; on the
eastside a Safeway along Soquel or an Albertson's along Water. As we
write this paragraph we realize that there are places to shop
everywhere and it is silly to try to enumerate them so perhaps this
section was a bad idea.
Hey, if you just can't live without the mall, there's one at Capitola
Rd. & 41st Ave. in Capitola.
Something you may need to know relatively soon is the location of the
DMV: they are on Capitola Rd. beyond 41st Avenue (like 42nd or
43rd), in Capitola. It helps if you make an appointment first.
Opinions vary on local banks. Bank of America has the advantage of
omnipresent ATMs and all the disadvantages of a faceless corporate
conglomerate. At the other extreme are the Bay Federal Credit Union
and the Santa Cruz Community Credit Union. Wells-Fargo is also used
by some grads.
A Useful websites
Many websites were mentioned in the text, but here we gather some (and
add some more) for convenience.
Housing Links
Some resources to help you on your housing search:
TRG Property Management: http://www.trgprop.com/
Sherman & Boone Real Estate:
http://www.sb-property.com/property/rental.html
Santa Cruz Property Management:
http://santacruzproperty.com/listings.cfm
Bailey Properties:
http://baileyproperties.com/rental/rentalform.asp?VAR_type=permanent
UCSC Community Rentals:
https://housingweb.ucsc.edu/cro/welcome.asp
Santa Cruz Sentinel listings:
http://www.adquest3D.com/search_new/search.asp?BRD=881& PAG=470
Dept. and UCSC
Dept.: http://www.astro.ucsc.edu
UCO/Lick: http://www.ucolick.org
Astro talk schedule: http://www.astro.ucsc.edu/talks.xml
Physics colloquium schedule:
http://maxwell.ucsc.edu/events/colloquia.html
CODEP seminars:
http://www.es.ucsc.edu/~asphaug/taps.html
Grad Astro Seminar:
http://www.ucolick.org/~scott/seminar/
Colloquium Cookies:
http://www.ucolick.org/~scott/cookies/
Our Ask-An-Astronomer: http://www.ucolick.org/~mountain/AAA/
UCSC: http://www.ucsc.edu
UCSC Schedule of Classes: http://reg.ucsc.edu/soc/
Teleslug: http://teleslug.ucsc.edu
Cashier: http://www2.ucsc.edu/accts-rec/cashier.htm
Financial Aid: http://www2.ucsc.edu/fin-aid/
Registrar: http://reg.ucsc.edu
Registrar change-of-address form:
https://oasas.ucsc.edu/reg/address/
Academic Calendars: http://reg.ucsc.edu/calendar/
Transportation and Parking: http://www2.ucsc.edu/taps
Bay Tree Bookstore: http://slugstore.ucsc.edu
Grad Commons: http://www2.ucsc.edu/gradcommons
GSA: http://www2.ucsc.edu/gsa/
UCSC Arts & Lectures Series: http://events.ucsc.edu/artslecs/
Grad Student Housing:
http://www.housing.ucsc.edu/housing/graduate.html
Family Student Housing:
http://www.housing.ucsc.edu/housing/family.html
Santa Cruz and environs
Santa Cruz Metro Transit (bus system): http://www.scmtd.com
When is the next bus off campus?
http://www.ucolick.org/cgi-bin/Tcl/nextbus.cgi
Bay Area Rapid Transit: http://www.bart.org
CalTrain: http://www.caltrain.com/caltrain/
What movies are playing, when?
http://www.metroactive.com/movies/times-sc.html
Was that an earthquake? Where? How big?
http://quake.usgs.gov/recenteqs/latest.htm
Footnotes:
1all emails are @ucolick.org
2Once a student has successfully proposed
a thesis topic (passed his or her ``Qualifying Exam''), that student
has Advanced to Candidacy (AC). At that point it becomes very easy
to lose track of how long s/he's been here ...
3The minimum number of classes you must
take from each column is listed.
4These courses are taught in other departments.
File translated from
TEX
by
TTH,
version 3.05.
On 11 Apr 2002, 17:12.