 
 
 
 
 
 
 
 
 
 
(Above) Latest solar images, from various telescopes and spacecraft.
Click on them for more detail.
| PHYS 151 Observational Astronomy MW 6-7:15 (lecture) in McLane 167.
 M or Tu or W 7:30-9:20 (lab),
 in the Campus Obsevatory.
 2018 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: MW 12:00-12:50 p.m., Tu 4:00-7:15 p.m.
 and other times too, by appointment.
 
 |  | 
Course description: (4 credits) Prerequisite: PHYS 4C.  Celestial 
coordinates, time, stellar motions, constellations, star charts, catalogs, 
astronomical sources, observational limits, telescopes, detectors, 
atmospheric effects, digital image processing, photometry, and 
spectroscopy.  (3 lecture, 3 lab hours)
Required Course Texts:
(1) The Stars, by H. A. Rey.  This is where to start, for learning 
constellations.  There should be extras on the PSci 21 (Elementary 
Astronomy) shelf.
(2) An Introduction to Observational Astrophysics, by Mark Gallaway.
(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). There 
should be copies of both editions in the Campus Observatory and in McLane 
220. I will also lend out copies of the first edition in class, to be 
returned during the Final Exam.
(4) Phys 151 Class Notes, edited by F. Ringwald.  These will be available 
in loose-leaf binders, and will be distributed in class.
Recommended Course Equipment:
 
(1) A 16-GB or larger USB flash drive (also called a thumb drive or a 
memory stick), for you to take digital images home from the 
observatory. (As of 2018, these cost less than $10.) 
(2) A flashlight, with a red light for night vision, although there are 
many of them in the Campus Observatory.
Recommended Course Texts (copies of all are in the Campus 
Observatory and in McLane 220):
(1) A second edition of The Handbook of Astronomical Image Processing, by 
Richard Berry and James Burnell. This course will use the first 
edition (from 2000), but if you want a second edition, you may purchase a 
copy directly from the publisher (http://www.willbell.com/aip/index.htm). 
(The campus bookstore has difficulty getting them.) 
(2) The New CCD 
Astronomy, by Ron Wodaski.
 This has lots of practical advice, 
especially on using Photoshop. 
(3) CCDSoft Version 5 
User Guide,
 which is available free online; a printed copy can 
also be obtained from this site, for $25.
Recommended for participating in research:
 
Cataclysmic Variable Stars, by Coel Hellier (2001).
If you want to be a professional astronomer, or a research 
scientist in any field, read this entire book:
A Ph.D. is Not Enough, by Peter J. Feibelman (1993, or the new 
2011 edition).
TENTATIVE list of topics to be covered (updated 
2018 November 14):
| Week | Date | Topic | Date | Topic | Read by Wednesday of next week | 
| 2 | 8/27 | Introduction; Astronomical Computer Resources
 | 8/29 | Position and Time | 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).
 | 
 
| 3 | 9/03 | Holiday | 9/05 | Position and Time | Section B of the Class Notes (the Friendly Manuals). | 
| 4 | 9/10 | Position and Time | 9/12 | Using the Telescope | Chapter 6 of Gallaway (Names, catalogs, and databases). | 
| 5 | 9/17 | Constellations, star charts, and star catalogs | 9/19 | Astronomical coordinate systems | Chapters 2 and 13 of Gallaway (Light and spectra); Chapter 9 of Berry & Burnell (Spectroscopy).
 | 
| 6 | 9/24 | Spectroscopy | 9/26 | Spectroscopy | Section C of the Class Notes (Astronomical Sources). | 
| 7 | 10/01 | Astronomical Sources: line radiation (the H atom); thermal (blackbody) radiation
 | 10/03 | Astronomical Sources: planets, stars, nebulae, and galaxies
 | Chapter 3 of Gallaway (Optics and telescopes) | 
| 8 | 10/08 | Telescopes and Optics | 10/10 | Telescopes and Optics | Section D of the Class Notes (Telescopes); Section E of the Class Notes (Seeing and Weather).
 | 
| 9 | 10/15 | Telescope mounts | 10/17 | 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).
 | 
| 10 | 10/22 | Mid-Term Exam 1 | 10/24 | CCDs | 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).
 | 
| 11 | 10/29 | CCDs | 10/31 | CCDs | Chapter 9 of Gallaway (Digital image processing); Chapter 4 of Berry & Burnell (Image Calibration);
 Chapter 5 of Berry & Burnell (Image Analyis software).
 | 
 
| 12 | 11/05 | Digital Image Processing | 11/07 | Digital Image Processing | Chapter 10 of Gallaway (Photometry); Chapter 8 of Berry & Burnell (Photometry).
 | 
| 13 | 11/12 | Holiday | 11/14 | Digital image processing | Chapters 17 and 18 of Berry & Burnell (Color and Advanced Imaging). | 
| 14 | 11/19 | Imaging and Photometry | 11/21 | Holiday | - | 
| 15 | 11/26 | Imaging and Photometry | 11/28 | Imaging and Photometry | - | 
| 16 | 12/03 | Advanced imaging | 12/05 | Advanced imaging; Take-Home Mid-Term Exam 2 due
 | - | 
| 17 | 12/10 | Advanced imaging | 12/12 | Advanced imaging; Projects and printed recipes due on last day of 
instruction, Wednesday, December 12. | - | 
 
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.
Course grades will be awarded for the following final
percentages:
 
85.0-100% = A; 70.0-84.9% = B;  55.0-69.9% = C;  40.0-54.9% = D;  0-39.9%
= F.
These percentages will be computed with the following weights:
 
| 10% | Homework.  (Sorry, but no late assignments will be accepted.) | 
 
| 40% | Four projects and printed recipes, at 10% each (see below), due 
Wednesday, December 12, the last day of instruction. | 
| 15% | Mid-Term Exam 1 (in class, closed book and closed notes). | 
| 15% | Mid-Term Exam 2 (take-home). | 
| 20% | Final Exam: in class, open book & notes, 8-10 p.m. Wednesday, December 19 
in McLane 167. | 
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 hands 
in by the end of the time the exam is given. If any questions or answers 
are missing from the copy the student has handed in, no credit will be 
given for the items on any missing pages.
Course web age: 
http://zimmer.csufresno.edu/~fringwal/phys151.html
Central Valley 
Astronomers meetings (public welcome) will be at 7-9 p.m. in East 
Engineering 191, on:
 September 22, October 27, November 24, and 
December 15.
Star Parties: Phys 151 students are encouraged to get as much 
observing experience as they can, with the Campus Observatory, and under 
a dark sky with the Central Valley 
Astronomers:
- Dark-Sky Star Parties (weather permitting, public welcome) with the 
Central Valley Astronomers, at 
Eastman Lake, are scheduled for after 7 p.m. on September 8, October 6, 
November 10, and December 8.
 
 
- Public-Centered Sidewalk Astroonomy (weather permitting, public 
welcome) with the Central Valley 
Astronomers, under a bright sky in town at the River Park shopping 
center, are scheduled for after 7 p.m. on September 15, October 13, and 
November 17.
 
 
DO NOT EVER observe the Sun, with the Campus 
Observatory or any other equipment belonging to Fresno State, unless 
under Professor Ringwald's direct supervision.
Observatory Scheduling: Students registered in Phys 151 
(Observational Astronomy) have priority with the Campus Observatory on 
every night of the week, except on the Friday nights following public 
planetarium shows, the Saturday nights immediately following Central Valley 
Astronomers meetings, and the nights of other public observing events 
(which will be announced in class). We can schedule blocks of telescope 
time in advance for any observers, whether or not in Phys 151.
Public Nights: 
The Downing Planetarium sometimes has public shows on Friday nights, from 
7 p.m. to 9:30 p.m. If Professor Ringwald is not present, Phys 151 
students may elect to open the Campus Observatory to the public during 
this time.  However, Phys 151 students are not required to open 
the observatory for anyone at any time, except other students registered 
in Phys 151 and Professor Ringwald.  In this case, Professor Ringwald 
recommends that Phys 151 students be courteous but firm with the public: 
for example, tell the public "Sorry, we're closed, because we're doing 
work with instruments for a class."  Don't be rude to anyone.
 Please remember: observing labs are the bare minimum of 
what will be needed for students to learn to use a telescope and a camera.  
You should plan on spending a lot more time at the telescope, 
to gain the proficiency you'll need to do astronomy professionally.
If this doesn't seem like fun to you, something is wrong. 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.
Projects and recipes:
Forty percent of the course grade will be for up to four projects. These 
projects can be any combination of the following, each of which may be used 
for more than one of the four projects:
-  Five black-and-white CCD images (in FITS format) of separate 
astronomical objects.  
 
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, e.g. 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 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, printed 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 printed recipes will cause "A" images to be recorded 
as "B" images.
 
 
 
-  Five separate 16-bit color images (in PNG-format) made from video 
(AVI-format files) that were taken with a planetary imager such as the 
Philips ToUcam or the Lumenera SKYnyx2-2, and processed with Registax 
software, of different fields of the Moon, Mercury, Venus, Mars, Jupiter, 
or Saturn, bright stars, colorful stars, or binary or multiple star 
systems.
 
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.
 
 
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 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, printed 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 printed recipes will cause "A" images to be recorded 
as "B" images.
 
 
 
-  One full-color CCD image of any deep-sky object (including M3, M15, 
M31, M34, M45, M92, NGC 891, or NGC 7008), or of a comet, Uranus, 
Neptune, Pluto, Eris, or any other Trans-Neptunian object, taken with a 
deep-sky CCD camera such as the STF-8300M or the ST-9.  In addition to 
the above considerations concerning image quality and image descriptions, 
the color should look natural, unless you can explain convincingly why an 
alternative color scheme helps one better understand the nature of the 
target. 
 
Color images from the CCD camera should be turned 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 recorded 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, 
printed 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 printed recipes will cause "A" images to be recorded 
as "B" images.
 
 
 
-  Eight hours of time-resolved, differential CCD photometry, of a 
variable star such as any of the stars currently being observed by the 
Center for Backyard Astrophysics, especially any of the other DQ Her 
stars currently being monitored.  The timing should be accurate to within 
0.1 seconds, calibrated by using the "Nistime" software on the 
observatory's computer. These data shoul be of the quality to be useful 
for participating in campaigns for the Center for Backyard Astrophysics 
(see http://cba.phys.columbia.edu/), American Association of Variable 
Star Observers (http://www.aavso.org), or other professionally 
coordinated campaigns.  This photometry must be correctly reduced and 
given in a three-column table, listing Julian Date (not heliocentrically 
corrected), V-C magnitudes, and C-K magnitudes.  (For more on this, see 
the chapter on photometry of Berry & Burnell.) This three-column table 
must be recorded in either a plain-text or Excel-format file on a CD, 
DVD, or USB drive (which will be returned to the student after the Phys 
151 Final Exam), and turned in to Professor Ringwald.
 
 
-  For any of the above projects, one-quarter credit will be given for 
students who process images that were taken by someone else, including 
any of the images provided by Professor Ringwald.  This may be useful if 
anyone has poor luck with weather, and is unable to get as many of the 
above observing projects completed as they would like. These must be 
accompanied by short printed recipes, as described above. 
Not including the printed recipes will cause "A" spectra to be 
recorded as "B" spectra.
 
 
-  Other observations, of your own devising, of scientific interest: 
Professor Ringwald welcomes consulting with him about these first. If, in 
the course of any of these projects, you produce data that are 
scientifically useful, Professor Ringwald would be glad to help you 
publish it.  If you'd rather contribute your data to one of Professor 
Ringwald's papers, you will be listed as a co-author on the paper, but 
Professor Ringwald will insist that you give the manuscript for the paper 
a good, careful read, in order to spot errors or ways to improve the 
paper, before submitting the paper to the journal.
 Professor Ringwald will allow students to collaborate with each 
other on homework and projects, provided everyone lists their 
"co-investigators."  Scientists often do this, and the ability to 
collaborate well and work as part of a team is a good skill to have, in 
many professions.  For a project, first authorship for any CCD image will 
be for whomever typed the commands into CCDSoft that took that image.  
Second authorship will be worth 1/2 as much as first authorship; third 
authorship will be worth 1/3, etc. If there is any doubt about credit, 
you can make sure you get it by doing one or more additional projects.
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.
Students with Disabilities: The Department of Physics 
cooperates with the Services for Students with Disabilities (SSD) to make 
reasonable accommodations for qualified students with physical, 
perceptual, or learning disabilities (cf. Americans with Disabilities Act 
and Section 504, Rehabilitation Act). Students with disabilities should 
present their written accommodation request to Professor Ringwald within 
the first two weeks of class. Upon identifying themselves to the 
instructor and the university, students with disabilities will receive 
reasonable accommodation for learning and evaluation. For more 
information, contact Services to Students with Disabilities in Madden 
Library 1049 (559-278-2811).
Cheating and plagiarism:
Professor Ringwald will not allow students to take work of any kind from 
the Internet or elsewhere, and turn it in as their own work.  This is now 
easy for professors to detect, with www.plagiarism.org. If Professor 
Ringwald finds anything on web page anywhere that closely resembles any 
student's work, that web page had better have the student's name on it.  
If it doesn't, the student's turning in that work with the student's name 
on it will be interpreted as an attempt to misrepresent someone else's 
work as the student's own, which constitutes plagiarism.  Remember, 
always: you are responsible for anything with your name on it.
If Professor Ringwald finds any plagiarized work, the student will 
receive an F for the entire course.  Professor Ringwald may also send 
the plagiarized work to the Dean and recommend the student be expelled 
from the University. Do NOT plagiarize! Modifying someone 
else's work slightly, or changing the text around, or stringing someone 
else's paragraphs together, even if they're cited, is no better: none of 
these dubious practices make it your work.  For information on the 
University's policy regarding cheating and plagiarism, refer to the 
Schedule of Courses (Legal Notices on Cheating and Plagiarism) or 
the University Catalog (Policies and Regulations).
Cheating is the actual or attempted practice of fraudulent or deceptive 
acts for the purpose of improving one's grade or obtaining course credit; 
such acts also include assisting another student to do so. Typically, such 
acts occur in relation to examinations. However, it is the intent of this 
definition that the term 'cheating' not be limited to examination 
situations only, but that it include any and all actions by a student that 
are intended to gain an unearned academic advantage by fraudulent or 
deceptive means. Plagiarism is a specific form of cheating which consists 
of the misuse of the published and/or unpublished works of others by 
misrepresenting the material (i.e., their intellectual property) so used 
as one's own work." Penalties for cheating and plagiarism range from a 0 
or F on a particular assignment, through an F for the course, to expulsion 
from the university. For more information on the University's policy 
regarding cheating and plagiarism, refer to the Class Schedule 
(Polcy/Legal Statements) or the University Catalog (University policies).
Computers: Students may use the computers in the Campus 
Observatory and McLane 220, which have software useful for this course, 
including AIP4WIN, Photoshop, skycalc, TheSky, CCDsoft, etc.  At 
California State University, Fresno, computers and communications links 
to remote resources are recognized as being integral to the education and 
research experience. Every student is required to have his/her own 
computer or have other personal access to a workstation (including a 
modem and a printer) with all the recommended software. The minimum and 
recommended standards for the workstations and software, which may vary 
by academic major, are updated periodically and are available from 
Information Technology Services or the University Bookstore. In the 
curriculum and class assignments, students are presumed to have 24-hour 
access to a computer workstation and the necessary communication links to 
the University's information resources.
Disruptive Classroom Behavior: The classroom is a special 
environment in which students and faculty come together to promote 
learning and growth. It is essential to this learning environment that 
respect for the rights of others seeking to learn, respect for the 
professionalism of the instructor, and the general goals of academic 
freedom are maintained.  Differences of viewpoint or concerns should be 
expressed in terms which are supportive of the learning process, creating 
an environment in which students and faculty may learn to reason with 
clarity and compassion, to share of themselves without losing their 
identities, and to develop and understanding of the community in which 
they live.  Student conduct which disrupts the learning process shall not 
be tolerated and may lead to disciplinary action and/or removal from 
class.
Copyright policy: Copyright laws and fair use policies protect the 
rights of those who have produced the material. The copy in this course 
has been provided for private study, scholarship, or research.  Other 
uses may require permission from the copyright holder.  The user of this 
work is responsible for adhering to copyright law of the U.S. (Title 17, 
U.S. Code).  To help you familiarize yourself with copyright and fair use 
policies, the University encourages you to visit its copyright web page, 
at: http://www.fresnostate.edu/home/about/copyright.html. Digital Campus 
course web sites contains material protected by copyrights held by the 
instructor, other individuals or institutions. Such material is used for 
educational purposes in accord with copyright law and/or with permission 
given by the owners of the original material.  You may download one copy 
of the materials on any single computer for non-commercial, personal, or 
educational purposes only, provided that you (1) do not modify it, (2) 
use it only for the duration of this course, and (3) include both this 
notice and any copyright notice originally included with the material.  
Beyond this use, no material from the course web site may be copied, 
reproduced, re-published, uploaded, posted, transmitted, or distributed 
in any way without the permission of the original copyright holder.  The 
instructor assumes no responsibility for individuals who improperly use 
copyrighted material placed on the web site.
Other astronomy courses at Fresno State include:
This syllabus and schedule are subject to change in the event of 
extenuating circumstances, such as poor weather.  If you are absent from 
class, it is your responsibility to check on announcements made while you 
were absent.
  
 
 
 
Last updated 2018 December 10. Web page by Professor Ringwald 
(ringwald[at]csufresno.edu and replace [at] with @) 
Go to 
Professor Ringwald's home page 
 Department of Physics,  California State University, 
Fresno.  Please read this disclaimer.