'Detail of the Milky Way galactic core. The light is from millions of stars near the center, at which there is a super massive b - Home Page Slideshow - Northern California Council Of Camera Clubs

Northern California Council Of Camera Clubs View More Photos Skip to Main Content

You are invited to become a member in a local camera club near you to take your photography to the next level.

First Place, Best in Division and Best of Show Winners from the N4C 2025 August/September Competition

In response to the on-going Covid-19 virus, N4C Board meetings will be hybrid as clubs are gradually returning to print competitions.

The Northern California Council of Camera Clubs (N4C) is the umbrella organization for sixteen San Francisco Bay Area camera clubs, whose members comprise photography enthusiasts—beginners, amateurs and professionals.

N4C provides an opportunity to grow photographically and compete at an interclub level. Most individual member clubs hold their own local monthly judged competitions in two photographic mediums, Prints and Projected Images, and in various subject matter.

Join in the fun with N4C and their local camera clubs. Participate in field trips, seminars, and workshops, share learning experiences and camaraderie among fellow photographers in your area!


To see all winning photos submitted for the month and for additional information, please visit the N4C’s PhotoClubServices Website.

SIMPLE = T / file does conform to FITS standard<br />BITPIX = -32 / number of bits per data pixel<br />NAXIS = 3 / number of data axes<br />NAXIS1 = 7906 / length of data axis 1<br />NAXIS2 = 5469 / length of data axis 2<br />NAXIS3 = 3 / length of data axis 3<br />EXTEND = T / FITS dataset may contain extensions<br />COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy<br />COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&amp;A...376..359H<br />BZERO = 0. / Offset data range to that of unsigned short<br />BSCALE = 1. / Default scaling factor<br />MIPS-HI = 64704 / Lower visualization cutoff<br />MIPS-LO = 390 / Upper visualization cutoff<br />PROGRAM = 'Siril 1.4.0-beta3' / Software that created this HDU<br />DATE = '2025-08-01T01:27:45' / UTC date that FITS file was created<br />ROWORDER= 'TOP-DOWN' / Order of the rows in image array<br />FILTER = 'mixed ' / Active filter name<br />XBINNING= 1 / Camera binning mode<br />YBINNING= 1 / Camera binning mode<br />STACKCNT= 1 / Stack frames<br />END
Sonoma,Coast,MW
'Detail of the Milky Way galactic core. The light is from millions of stars near the center, at which there is a super massive b - Home Page Slideshow - Northern California Council Of Camera Clubs
SIMPLE = T / file does conform to FITS standard<br />BITPIX = -32 / number of bits per data pixel<br />NAXIS = 3 / number of data axes<br />NAXIS1 = 7906 / length of data axis 1<br />NAXIS2 = 5469 / length of data axis 2<br />NAXIS3 = 3 / length of data axis 3<br />EXTEND = T / FITS dataset may contain extensions<br />COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy<br />COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&amp;A...376..359H<br />BZERO = 0. / Offset data range to that of unsigned short<br />BSCALE = 1. / Default scaling factor<br />MIPS-HI = 64704 / Lower visualization cutoff<br />MIPS-LO = 390 / Upper visualization cutoff<br />PROGRAM = 'Siril 1.4.0-beta3' / Software that created this HDU<br />DATE = '2025-08-01T01:27:45' / UTC date that FITS file was created<br />ROWORDER= 'TOP-DOWN' / Order of the rows in image array<br />FILTER = 'mixed ' / Active filter name<br />XBINNING= 1 / Camera binning mode<br />YBINNING= 1 / Camera binning mode<br />STACKCNT= 1 / Stack frames<br />END