The shear catalogs are provided in three bands: g/r/z, among which the g band results are least reliable. We recommend users to use only the r and z band results. Different from the catalogs in DECALS_shear_220214, the current ones include slight corrections from time-dependent superflat images each of which is achieved through stacking at least a few hundred exposures taken within a certain period of time. Each file include the following columns: "# RA Dec mag_g mag_r mag_z zp_Zou z_err zs zm CCDNUM ig x y sig nstar imax jmax Half_L_F Half_L_A flag PSF_FWHM SNR_F ra2 dec2 gf1 gf2 g1 g2 de h1 h2 cos2 sin2 parity dist RA3 Dec3 zp_Rongpu zs_Rongpu " The meanings of the items are given below: RA, Dec: the position of the source provided in Zou Hu's catalog; mag_g, mag_r, mag_z: the g/r/z band magnitude of the source in Zou Hu's catalog; zp_Zou, z_err: the photo-z and its error in Zou Hu's catalog; zs, zm: the spectral zs and the median zm (photo-z) of Zou; CCDNUM: the id of the CCD in which the image is located; ig: the index of galaxy in the whole catalog; x, y: the position of the galaxy in the CCD; sig: the rms of the background; nstar: the number of bright stars used for PSF reconstruction in the CCD of the galaxy; imax, jmax: the maximum number of bad pixels along the x and y direction in the source stamp; Half_L_F: half-light-flux, normalized by the rms of the background; Half_L_A: half-light-area; flag: a parameter indicating the distance (in unit of pixel size) of the source to its nearest neighbor; PSF_FWHM: the FWHM (in arcsec) of the PSF at the position of the galaxy; SNR_F: the signal-to-noise-ratio defined in Fourier space (see Hekun's paper); ra2, dec2: the positions calculated by the Fourier_Quad pipeline (for the purpose of cross-check only); gf1,gf2: the two components of the field distortion at the galaxy position; g1, g2: the G_1 and G_2 components of the Fourier_Quad shear estimator; de: the "N" of the Fourier_Quad shear estimator; h1, h2: they are essentially (U, V) defined in the original PDF-SYM paper, but with negative signs; cos2, sin2: cos(2\phi) and sin(2\phi), where \phi is the angle between the CCD x-y coordinate and the RA-Dec coordinate; parity: the parity of the CCD x-y coordinate with respect to the RA-Dec coordinate; dist: the distance (in arcsec) between (RA, Dec) and (RA3, Dec3); RA3, Dec3: the source position from Rongpu's catalog; zp_Rongpu: the photo-z from Zhou Rongpu; zs_Rongpu: spec-z from Rongpu's catalog. To use the catalogs, we recommend applying the following cuts: 1. General cuts: 1) If CCDNUM=16, please require x>1025; 2) If CCDNUM=9, please require x<1025; 3) If CCDNUM=2, please require x<1025; 4) If CCDNUM=57, please require x>1025; 5) Try NOT to use the data from the chips with CCDNUM=25, 31, 32, 38. 2. For z-band data: SNR_F > 2-4; 3. For r-band data: SNR_F > 4-6, and NOT use the data with -5e-4