(Above) Solar images, from various telescopes and spacecraft. Click on them for more detail.
PHYS 151 Observational Astronomy TuTh 6:00-7:15 (lecture), in-person in Science 2, Room 310 Tu or Th 7:30-9:20 (lab), in the Campus Observatory. 2024 Fall Course Syllabus: Please read carefully |
Instructor: Professor
Ringwald E-mail: ringwald[at]csufresno.edu and replace [at] with @ Phone: (559) 278-8426 Office: Room 11 in the J wing (Building J) of McLane Hall. Office hours (in-person, between August 22 and December 12): TuTh 2-3 p.m. and We 2-5 p.m. |
Required Course Texts:
(2) An
Introduction to Observational Astrophysics, 2nd edition, by Mark
Gallaway, also available from Kennel Bookstore.
(3) A first
edition of The Handbook of Astronomical Image Processing, by Richard
Berry and James Burnell. This course will use the first edition
(from 2000), not the second edition (from 2005). Don't worry if
your copy doesn't contain the disk with the software: see (4)
immediately below.
(4) Click here to download the the PHYS
151 files, including the AIP4WIN 1.4.25 software. Downloading this
will require 2.4 GB of free disk space.
(5) Phys 151 Class Notes, edited by F. Ringwald. These will be available in loose-leaf binders, and will be distributed in class.
(2) A flashlight, with a red light for night vision, although there
should be plenty of them in the Campus Observatory.
(2) The
New CCD Astronomy, by Ron Wodaski. This book revolutionized "pretty
pictures" in astronomy, and has lots of practical advice, especially on
using Photoshop.
(3) CCDSoft Version 5 User Guide, which is the software with which we
operate the cameras in the Campus Observatory. This is available free
online.
Week | Date | Topic | Date | Topic | Read by Wednesday of next week |
1 | 8/20 | No class | 8/22 | Introduction; Astronomical Computer Resources | Web Power Tools
article and the entire Class Syllabus;
Chapters 4 and 5 of Gallaway (Position and Time); The Stars, by H. A. Rey (the whole book); Section A of the Class Notes (Classical Astronomy). |
2 | 8/27 | Position and Time | 8/29 | Position and Time | Section B of the Class Notes (the Friendly Manuals). |
3 | 9/03 | Using the Telescope | 9/05 | Constellations, star charts, and star catalogs | Chapter 6 of Gallaway (Names, catalogs, and databases). |
4 | 9/10 | Astronomical coordinate systems | 9/12 | Spectroscopy |
Chapters 2 and 13 of Gallaway (Light and spectra); Chapter 9 of Berry & Burnell (Spectroscopy). |
5 | 9/17 | Spectroscopy | 9/19 |
Astronomical Sources: thermal (blackbody) radiation | Section C of the Class Notes (Astronomical Sources). |
6 | 9/24 |
Astronomical Sources: line radiation (the H atom) | 9/26 |
Astronomical Sources: planets, stars, nebulae, and galaxies | Chapter 3 of Gallaway (Optics and telescopes) |
7 | 10/01 | Telescopes and Optics | 10/03 | Mid-Term Exam 1 |
Section D of the Class Notes (Telescopes); Section E of the Class Notes (Seeing and Weather). |
8 | 10/08 | Telescope mounts | 10/10 | Detectors |
Chapter 7 of Gallaway (Detectors); Chapter 11 of Gallaway (Statistics); Chapters 1 and 2 of Berry & Burnell; Section F of the Class Notes (CCDs). |
9 | 10/15 | CCDs/CMOS detectors | 10/17 | CCDs/CMOS detectors |
Chapter 8 of Gallaway (Imaging); Chapter 3 of Berry & Burnell (Imaging Techniques); Section G of the Class Notes (Practical Digital Imaging); Section H of the Class Notes (Detectors). |
10 | 10/22 | CCDs/CMOS detectors | 10/24 | CCDs/CMOS detectors |
Chapter 9 of Gallaway (Digital image processing); Chapter 4 of Berry & Burnell (Image Calibration); Chapter 5 of Berry & Burnell (Image Analyis software). |
11 | 10/29 | CCDs/CMOS detectors | 10/31 | Digital Image Processing | Chapter 10 of Gallaway (Photometry); Chapter 8 of Berry & Burnell (Photometry). |
12 | 11/05 | Digital Image Processing | 11/07 | Digital Image Processing | Chapters 17 and 18 of Berry & Burnell (Color and Advanced Imaging). |
13 | 11/12 | Imaging and Photometry | 11/14 | Imaging and Photometry | |
14 | 11/19 | Imaging and Photometry | 11/21 |
Advanced imaging;
Take-Home Mid-Term Exam 2 due | |
15 | 11/26 | Holiday | 11/28 | Holiday | |
16 | 12/03 | Advanced imaging | 12/05 | Advanced imaging | |
17 | 12/10 | Advanced imaging; Projects and printed recipes due on last day of instruction, Tuesday, December 10. | 12/12 | No class |
Class Objectives (also known as Learning Outcomes):
(1) To introduce physicists and other scientists to interesting
techniques, particularly using telescopes and digital imaging.
(2) To provide teachers with a practical background for their
science classes.
(3) To prepare astronomers for the research problems of the future,
by getting them to the research frontier as quickly as possible.
10% | Homework, due in class during the first five minutes of class on dates to be annouinced. Sorry, but no late assignments will be accepted. |
40% | Four projects and recipes at 10% each (see below), due by email Tuesday, December 10. |
15% | Mid-Term Exam 1 (in class, closed book and closed notes) on Thursday, October 3. |
15% | Mid-Term Exam 2 (take-home, due in class on during the first five minutes of class) on Thursday, November 21. |
20% | Final Exam (open paper notes to be prepared by each student and no collaborating), 8:00-10:00 p.m. Thursday, December 19 in Science 2, Room 310. |
Sorry, but I don't give make-up exams. Any student who misses either of the mid-term exams for a valid reason (job interview or illness documented by a physician's note) will have the exam grade voided and the remainder of the grade counted as 100%. Any student who misses the final exam will get a grade of I (Incomplete) for the course, to be made up when the next Final Exam for Phys 151 (Observational Astronomy) will be given.
Concerning exams: it is the student's responsibility to make sure all pages of the exam, as well as the student's answers for all of the questions stated on them, are present in the copy that the student turns in by the end of the time the exam is given. If any questions or answers are missing from the copy the student has turned in, no credit will be given for the missing items.
Course webpage:
http://zimmer.csufresno.edu/~fringwal/phys151.html
Some students treat doing their homework as a dreadful chore. This isn't right. Astronomy is an elective course, and it's a competitive profession. If it isn't fun, you may be happier in an easier, more lucrative field. One can make more money for less work doing just about anything other than astronomy, especially with a physics degree.
These may be taken with a clear filter, or with any of the other filters
we have. Images through an H-alpha filter are especially recommended,
for their high contrast, even during Full Moon, and their "dreamy"
quality, especially of H II regions (also called emission
nebulae).
Grading for all images will depend on their quality. They should not be
underexposed (with visible pixels or graininess), overexposed (with
saturation or blooming), out of focus, noticeably trailed,
over-processed (in a way that makes the image look unnatural, for
example, with rings or halos around star images from overzealous unsharp
masking, or flat white star images from too much smoothing, or a flat
black-and-white look from too much contrast enhancement), or with other
noticeable image processing artifacts. It can help to have a target
centered in the frame, and surrounded by aesthetically pleasing black
sky.
These images must be recorded as FITS-format images and turned in to
Professor Ringwald via email. Use Google Drive or Google Docs, since the
volume of data can be large. Please do NOT send the original, raw image
files!
These images must be accompanied by a short, Word- or
plain-text-format recipe identifying the target and how the
image was made, similar to those below each image on the Campus
Observatory gallery pages. (See http://zimmer.csufresno.edu/~fringwal/gallery.html).
These are important, since Professor Ringwald may post these images to
the Campus Observatory gallery pages, if they are of high quality.
Not including the recipes will cause "A" images to be graded as "B"
images.
Three digital videos of the Sun, taken on the same day with the H~alpha, Ca~K, and
white-light dedicated solar telescopes (and NOT any telescope in the Campus Observatory) and
a planetary imaging camera and wavelet processed into still, PNG-format images, will count
as one project.
Four separate images made from video taken with a planetary imager that
are combined together into a mosaic image of a single subject (such as
the Moon, or of Jupiter and its moons) will count as one full project.
Combining the four images into the one mosaic image can be done with
software such as Photoshop, using the instructions on pages 462-470 of
"The New CCD Astronomy" by Ron Wodaski. (If you don't have Photoshop,
you'll need to do some other project or use the computers in McLane
220.)
Images taken with a digital video planetary camera should record the
dates on which they were taken. Images of the Moon must identify which
particular features are shown: Moon maps are available in the Campus
Observatory.
Grading will depend on the above considerations concerning image quality
and image descriptions. Also, mosaics with clearly visible seams between
individual images will not get grades of A. Mosaics with black space
between images will not get grades of A or B.
These images must be recorded as 16-bit PNG format images and turned in
to Professor Ringwald via email. Use Google Drive or Google Docs, since
the volume of data can be large. Please do NOT send video files!
These images may alternatively be recorded as 16-bit PNG format images
on a CD, DVD, or USB drive (that will be returned to the student after
the Phys 151 Final Exam), and turned in to Professor Ringwald.
These images must be accompanied by a short, Word- or
plain-text-format recipe identifying the target and how the
image was made, similar to those below each image on the Campus
Observatory gallery pages. (See http://zimmer.csufresno.edu/~fringwal/gallery.html).
These are important, since Professor Ringwald may post these images to
the Campus Observatory gallery pages, if they are of high quality.
Not including the recipes will cause "A" images to be graded as "B"
images.
Color images from the CCD camera should be emailed to Professor Ringwald
in as PNG-format images. These color images should be accompanied by
FITS-format images of each of the (three, four, or five) registered and
combined black-and-white images that were used to make this color image,
including the combined red, green, and blue frames and the luminance and
H alpha frames, if used. Please don't include every one of the
raw black-and-white FITS frames.
Grading will depend on the above considerations concerning image quality
and image descriptions. Also, any color images not registered well enough
so that red, green, and blue fringes are clearly visible on the sides of
astronomical objects will not get grades of A or B.
These images must be accompanied by a short, Word- or
plain-text-format recipe identifying the target and how the
image was made, similar to those below each image on the Campus
Observatory gallery pages. (See http://zimmer.csufresno.edu/~fringwal/gallery.html).
These are important, since Professor Ringwald may post these images to
the Campus Observatory gallery pages, if they are of high quality.
Not including the recipes will cause "A" images to be gradeed as "B"
images.
If you do collaborate, it must be genuine collaboration, not one person doing all the work, and the others blindly copying. That's cheating! Therefore, while you may work on homework together, write up the results separately, in your own words. A dead giveaway is when two images are exactly the same: this is very noticeable.
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