number: Calculate number from image series.
In nandb: Number and Brightness Image Analysis

Description Usage Arguments Value References Examples

Given a time stack of images, number() performs a calculation of the number for each pixel.

number(
  img,
  def,
  thresh = NULL,
  detrend = FALSE,
  quick = FALSE,
  filt = NULL,
  s = 1,
  offset = 0,
  readout_noise = 0,
  gamma = 1,
  parallel = FALSE
)

`img`	A 4-dimensional array of images indexed by `img[y, x, channel, frame]` (an object of class ijtiff::ijtiff_img). The image to perform the calculation on. To perform this on a file that has not yet been read in, set this argument to the path to that file (a string).
`def`	A character. Which definition of number do you want to use, `"n"` or `"N"`?
`thresh`	The threshold or thresholding method (see `autothresholdr::mean_stack_thresh()`) to use on the image prior to detrending and number calculations. If there are many channels, this may be specified as a vector or list, one element for each channel.
`detrend`	Detrend your data with `detrendr::img_detrend_rh()`. This is the best known detrending method for brightness analysis. For more fine-grained control over your detrending, use the `detrendr` package. If there are many channels, this may be specified as a vector, one element for each channel.
`quick`	`FALSE` repeats the detrending procedure (which has some inherent randomness) a few times to hone in on the best detrend. `TRUE` is quicker, performing the routine only once. `FALSE` is better.
`filt`	Do you want to smooth (`filt = 'mean'`) or median (`filt = 'median'`) filter the number image using `smooth_filter()` or `median_filter()` respectively? If selected, these are invoked here with a filter radius of 1 (with corners included, so each median is the median of 9 elements) and with the option `na_count = TRUE`. If you want to smooth/median filter the number image in a different way, first calculate the numbers without filtering (`filt = NULL`) using this function and then perform your desired filtering routine on the result. If there are many channels, this may be specified as a vector, one element for each channel.
`s`	A positive number. The S-factor of microscope acquisition.
`offset, readout_noise`	Microscope acquisition parameters. See reference Dalal et al.
`gamma`	Factor for correction of number n due to the illumination profile. The default (`gamma = 1`) has no effect. Changing gamma will have the effect of dividing the result by `gamma`, so the result with `gamma = 0.5` is two times the result with `gamma = 1`. For a Gaussian illumination profile, use `gamma = 0.3536`; for a Gaussian-Lorentzian illumination profile, use `gamma = 0.0760`.
`parallel`	Would you like to use multiple cores to speed up this function? If so, set the number of cores here, or to use all available cores, use `parallel = TRUE`.

A matrix, the number image.

Digman MA, Dalal R, Horwitz AF, Gratton E. Mapping the Number of Molecules and Brightness in the Laser Scanning Microscope. Biophysical Journal. 2008;94(6):2320-2332. doi: 10.1529/biophysj.107.114645.

Dalal, RB, Digman, MA, Horwitz, AF, Vetri, V, Gratton, E (2008). Determination of particle number and brightness using a laser scanning confocal microscope operating in the analog mode. Microsc. Res. Tech., 71, 1:69-81. doi: 10.1002/jemt.20526.

Hur K-H, Macdonald PJ, Berk S, Angert CI, Chen Y, Mueller JD (2014) Quantitative Measurement of Brightness from Living Cells in the Presence of Photodepletion. PLoS ONE 9(5): e97440. doi: 10.1371/journal.pone.0097440.

img <- ijtiff::read_tif(system.file("extdata", "50.tif", package = "nandb"))
ijtiff::display(img[, , 1, 1])
num <- number(img, "N", thresh = "Huang")
num <- number(img, "n", thresh = "tri")