Course Objectives:
The aim of this course is to introduce you, the students, to seminal papers
and more recent developments in mid-infrared astronomical research —
in particular the wealth of discoveries resulting from the Spitzer
Space Telescope, the last of NASA's four Great Observatories, launched in
2003. We will do so through presentations followed by discussion with active
participation by all students, and determine what are the active areas of
mid-IR research. Textbooks, by their nature, are out of date at the time of
their publication. In this course we aim to bridge the gap between passive
acquisition of knowledge and active PhD research by reading and discussing
papers from the professional literature. The emphasis will lie on the
development and uncertainties of current scientific theory and method.
Oral reports on the papers selected will be presented in class at the rate
of one ~45 minute presentation per week (assuming the number of students is
13 or less). Oral reports by senior graduate students, postdocs and/or
talks by visiting scientists would be on a voluntary and as-time-permits
basis only. Each report should consist of a general introduction covering
the scope of the paper and where it fits within the larger field of research
of which the paper is part, followed by a more detailed summary of the
original research presented in the paper and a discussion of its impact.
Each presentation is followed by time for questions and answers, and
discussion by the students, using questions e-mailed to me in advance
of each class as a guide. At the end of each class, you will be asked to
evaluate the student speaker. Please fill out the evaluation form, and
return it to the instructor at the end of the class. Like in the refereeing
process in publishing scientific papers, you may remain anonymous. But
please be polite in your comments, because you too one day will be judged
by your peers!
Dates for the presentations(s) by each student will be assigned within the
first week of the first class — first come, first serve (see the
Seminar Schedule below). The choice of paper to discuss will be up to the
student, but certain restrictions and requirements will apply
(see also Tips.., below). I'll be happy
to discuss that choice.
Requirements and Course Grades:
70% of the final grade
will be based on the presentation, where the emphasis lies more on content
and clarity than on how fancy the presentation looks. Each student is
responsible for providing me no later than one week
before their scheduled presentation the full bibliographic
reference to a paper of their choice (i.e., the last
possible moment will be in class the week before). I will place a link on
the class web-page to an electronic version of this paper (PDF/Postscript),
so all students can download and read it, and formulate questions. Non-timely submission of a reference will result in a
reduction of your grade. Also, after class, each student must send me
their electronic presentation exported as a PDF
file with all fonts included (if the PDF file size is larger than
~3 Mb when exporting from PowerPoint or similar presentation software,
then first remove any background images and try again). I will create a link
to it into the following table (see Seminar Schedule below), so it
can be viewed and consulted later.
30% of the final grade
will be based on the participation by each student in the discussion of each
paper, as demonstrated by the posing of non-trivial questions and reasoning
demonstrating the use of the scientific method. Each student, except the
student giving the presentation, must prepare and e-mail me
at least two non-trivial questions regarding
the paper no later than 5:00PM of the Thursday before
each class (except if that class is a Special Seminar by a visiting
scientist).
Note that failure to submit questions for at least 50% of the presentations
means that even if you give a perfect presentation, your final grade
can be no better than a C+. Also note that, whereas a question can
be trivial, confused or poorly posed, the only stupid question is a question
not asked.
A full bibliographic reference includes
at the very least (1) the name of the lead author, (2) publication year, (3)
name or abbreviation of the journal, (4) volume number, and (5) page number.
Do not send me just a web-link to a PDF file or just a PDF file. It
is OK to send me a link in addition to the full bibliographic
reference, but in that case please specify the relevant ADS abstract page
(for example:
http://adsabs.harvard.edu/abs/1962ApJ...136..748E ).
Presentations:
For the computer-based presentations (i.e., HTML, PDF, Power Point, etc..),
an old laptop computer running Redhat 9 Linux (with Mozilla 1.4.2
browser, Acrobat Reader 5.0 [PDF], and OpenOffice 1.1 [PPT]) will
be available in the classroom, but students are encouraged to and will likely
prefer to bring and use their own Windows, Linux or Macintosh laptop. If
you use a Macintosh, remember to bring a DVI-to-VGA adaptor to connect to
the LCD projector. Note, that the projector provides a 1024×768 pixel
standard field of view, and has a 60 Hz refresh rate, so you need to
adjust your display settings if you have a wide-screen laptop. Practice
doing so in advance of your presentation.
If you prepare a PowerPoint presentation and do not plan to use your
own laptop, send your presentation no later than
Thursday afternoon preceding class to me by e-mail as an attachment,
so I can check that it displays properly: proprietary fonts from Microsoft,
Adobe, and other commercial founderies (e.g., math and greek symbols, fancy
fonts) often don't display or are substituted by unreadable characters on
Open Source machines!
Tips for finding a suitable paper:
For a 45 min presentation, single 4 or 5-page Letters are not
suitable (but three related ones might well be). Typically, papers
should be the equivalent of 15–20 pages in a main journal (multi-page
tables or atlasses of figures, and the list of references don't count toward
this number; manuscripts in pre-print format should be at least 3× as
many pages).
Papers that had/have a large impact will be cited by many other authors.
Papers with few or no citations, or mostly self-citations by the authors,
may not be suitable for discussion. Papers are required to (1)
have been published in a peer reviewed journal or been accepted for
publication in a peer reviewed journal and (2) have at least 1
non-trivial citation by researchers other than the authors of that
paper. Discussion of a paper that recently appeared on 'astro-ph' may be OK
if the above conditions are met, and the "Comments" give a specific
volume/issue of the peer-reviewed journal where such paper is scheduled to
appear.
Although not a complete depository of all scientific literature in astronomy
and astrophysics, none the less, astronomy as a science is blessed in having
a very large, full-text digital library: the NASA Astrophysics Data System
(ADS) (http://adsabs.harvard.edu/abstract_service.html).
For example, a search for a paper that I discussed a while back returned:
A full text, printable version of this paper may be obtained by clicking
on the "F" link (or by clicking on the full
reference link or "A" link, and following the
links on the abstract page that it opens). Often,
there is also a "G" that points to GIF-format
scans of each page of the paper or an "E" that
points to an HTML version (both may come handy to extract/retrieve a digital
version of a figure, table or equation to insert in your presentation).
To check the number of citations, one can click the link marked
"C".
Full resolution Postscript versions of figures can often be found on the
LANL (arXiv.org) preprint server:
(http://xxx.lanl.gov/find/astro-ph) by searching for the lead
author(s) and selecting [..., other] as the
download format and then Source (this will allow you to download a
tar-ball, which includes the originally submitted figures). Note, that the
preprint can be of an earlier year than the actual year of publication.
The following is the schedule of presentations:
Spring 2009 Seminar Schedule
Date |
Person |
Paper |
Title + link to presentation |
1/23
| Rolf Jansen
|
| Introduction to the Class
|
1/30
| Rolf Jansen
|
HTML/PDF,
HTML/PDF,
HTML/PDF,
HTML/PDF
|
The Spitzer Space Telescope: Last of the Great Observatories
Werner, M.W., et al. 2004, ApJS 154, 1;
Fazio, G.G., et al. 2004, ApJS 154, 10;
Houck, J.R., et al. 2004, ApJS 154, 18; and
Rieke, G.H., et al. 2004, ApJS 154, 25.
|
2/06
| Michael Pagano
|
HTML/PDF
|
Multiwavelength Constraints of the Day-Night Circulation Patterns
of HD 189733b,
Knutson, H.A., Charbonneau, D., Cowan, N.B., et al. 2009, ApJ 690, 822
|
2/09
| Dante Lauretta (UofA/LPL)
|
| SESE Astronomy Seminar
(PSF-566 2:00–3:00PM)
The Diversity of Extrasolar Terrestrial Planets
|
2/11
| Deborah Padgett (IPAC/Caltech)
|
| SESE Astronomy Seminar
(PSF-226 1:00–2:00PM)
WISE – The Wide-field Infrared Survey Explorer
|
2/11
| Deborah Padgett (IPAC/Caltech)
|
| SESE Colloquium
(PSH-153 4:10–5:10PM)
The Taurus Spitzer Legacy Survey
|
2/13
| Teresa Ashcraft
|
HTML/PDF
|
Hubble+Spitzer Survey for Gravitationally Lensed Galaxies: low-L
galaxies beyond z=7,
Richard, J., Stark, D.P., Ellis, R.S., et al. 2008, ApJ 685, 705
|
2/20
| Matthijs Smith
|
HTML/PDF
|
An Evolutionary Model For Submillimeter Galaxies,
Chakrabarti, S., Fenner, Y., Cox, T.J., et al. 2008, ApJ 688, 972
|
2/23
| Don Neill (Caltech)
|
| SESE Astronomy Seminar
(PSF-566 2:00–3:00PM)
Unraveling Mira's Mysterious Tail
|
2/25
| Brian Fields (U.Illinois)
|
| SESE Astronomy Seminar
(PSF-226 1:00–2:00PM)
Primordial Nucleosynthesis and Particle Dark Matter:
Beyond the Standard Model
|
2/25
| Brian Fields (U.Illinois)
|
| SESE Colloquium
(PSH-153 4:10–5:10PM)
When Supernovae Attack!
|
2/26
| George Fuller (UCSD)
|
| Physics Colloquium
(PSF-173 4:00–5:00PM)
Neutrinos: Stealthy agents of creation and destruction
|
2/27
| William Gray
|
HTML/PDF
|
Remarkable Disk and Off-nuclear Starburst Activity in the Tadpole
Galaxy as Revealed by Spitzer,
Jarret, T.H., Polletta, M., Fournon, I.P., et al. 2006, AJ 131, 261
|
3/06
| Michael Rutkowski
|
HTML/PDF,
HTML/PDF
|
Mid- to Far-IR Emission, Star Formation, and Galaxy
Morphologies,
Young, L.M., et al. 2009, AJ 137, 3053; and
Bendo, G.J., et al. 2007, MNRAS 380, 1313
|
3/13
|
|
| Spring break — no class
|
3/16
| Paul Eskridge (MNSU)
|
| SESE Astronomy Seminar
(PSF-566 2:00–3:00PM)
Galaxy Evolution Up Close — Using Pixel
Mapping to Study the Histories of Nearby Galaxies
|
3/18
| Jim Kasting (PSU)
|
| SESE Colloquium
(PSH-153 4:10–5:10PM)
The Climate of Early Mars
|
3/19
| Glenn Starkman (CWRU)
|
| Physics Colloquium
(PSF-173 4:00–5:00PM)
Is the Universe Out of Tune?
|
3/20
| William Keel (U.Alabama)
|
| Special Seminar
(PSF-226 12:15–1:30PM, i.e., regular time and place)
Dead quasars, Backlit galaxies, and other Gems from the Galaxy Zoo
|
3/27
|
|
| no class
|
4/03
| Stevie Dunn
|
HTML/PDF,
HTML/PDF,
HTML/PDF
|
Spitzer Observations in the Lockman Hole: IRAC Imaging, Extremely
Red Objects, and SCUBA/VLA Sources,
Huang, J.-S., et al. 2004, ApJS 154, 44;
Wilson, G., et al. 2004, ApJS 154, 107; and
Egami, E., et al. 2004, ApJS 154, 130.
|
4/10
| Cynthia Morales
|
HTML/PDF
| Embedded Star Formation in the Eagle Nebula with
Spitzer GLIMPSE, R. Indebetouw, T. Robitaille, B. Whitney,
et al. 2007, ApJ 666, 321
|
4/15
| Daniela Calzetti (UMass)
|
| SESE Colloquium
(PSH-153 4:10–5:10PM)
Lessons Learned from the Infrared, and Future
Prospects for Studies of Nearby Galaxies
|
4/17
| Lisa Prato (Lowell Obs.)
|
| Special Seminar
(PSF-226 12:15–1:30PM, i.e., regular
time and place)
The Youngest Planets and Spots' Tricks
|
4/20
| Stuart Shaklan (NASA/JPL)
|
| Special Seminar
(PSF-226 1:00–2:00PM)
The SIM Lite Instrument: The Culmination of
20 years of Technical Development
|
4/24
| Emily McLinden
|
HTML/PDF,
HTML/PDF,
(HTML/PDF)
|
Spitzer Constraints on the Stellar Populations of
Lyα-emitting Galaxies as z = 3.1 Progenitors of
Present-day L* Galaxies,
K. Lai, et al. 2008, ApJ 674, 70 and
E. Gawiser, et al. 2007, ApJ 671, 278; with
L. Pentericci, et al. 2009, A&A 494, 553 for some nuances
|
4/27
| Angela Cotera (SETI)
|
| SESE Astronomy Seminar
(PSF-566 2:00–3:00PM)
Star Formation in the Galactic Center: New clues from a
HST Paschen α survey
|
5/01
| Cody Raskin
|
HTML/PDF,
HTML/PDF,
HTML/PDF
|
Observations and analysis of the Vega and similar Debris
Disks, K. Su, et al. 2005, ApJ 628, 487;
with G. Bryden, et al. 2006, ApJ 636,
1098 and G. Rieke, et al. 2005, ApJ 620, 1010 for background
|
5/04
| Rychard Bouwens (UCSC)
|
| SESE Astronomy Seminar
(PSF-566 2:00–3:00PM)
Early Galaxy formation: Studying the build-up
and evolution of galaxies during the first 2 Gyr of the Universe
|
5/12
| Karthik Sheth (Caltech)
|
| Cosmology Lunch Seminar
(PSF-226 12:00–1:00PM)
Assembly of Galaxy Disks & Evolution
of Galactic Structures in COSMOS – Reconstructing the Hubble
Sequence
|
5/18
| Margaret Turnbull (DTM/CIW)
|
| SESE Astronomy Seminar
(PSF-566 2:00–3:00PM)
(TBA)
|
Click on the links below for the Astrophysics Seminar schedules and student
presentations of previous semesters:
- Fall 2008
(Windhorst) — The Ultraviolet Universe: Hot is "Cool", for
Young and Old
- Spring 2008 (Jansen) —
The Coma Cluster of Galaxies
- Fall 2007 (Jansen) —
News from the Frontier: z = 5 and Beyond
- Spring 2007 (Jansen) —
Nearby Galaxies: How well do we know our Cosmic Backyard?
- Fall 2006
(Windhorst) — Black Hole Growth & Galaxy Assembly: From
First Light & Reionization to the Present
- Spring 2006 (Jansen) —
Planet Formation and Our Milky Way Galaxy
- Fall 2005 (Jansen) —
Star Formation and Chemical Enrichment: From the First Stars to
Present-day Galaxies
Last update: May 1 2009 [RAJ]
|