We present sky-SB measurements on all images in the SKYSURF database. For an overview on the project, refer to Windhorst et al. (2022). For a description of sky-SB measurement algorithms and a summary of sky-SB results, refer to O'Brien et al. (2022).
There is 1 csv file corresponding to each Hubble Space Telscope (HST) filter. Each csv file contains 1 sky-SB measurement per detector (i.e. 1 sky measurement for each WFC3/IR image and 2 sky measurements for each WFC3/UVIS and ACS/WFC image).
Column Name | Description |
---|---|
File | File name that sky-SB was measured on |
Root | Root name of file that sky-SB was measured on |
Extension | FITS file extension that sky-SB was measured on |
Sky_e or Sky_e/s | Measured sky-SB, in units of electrons or electrons/sec |
RMS_e or RMS_e/s | Measured sky-SB RMS, in units of electrons or electrons/sec |
Error_e or Error_e/s | Uncertainty in sky-SB, in units of electrons or electrons/sec |
Flag | Flag associated with measurement (see Table 2 below) |
N_bad_regions | Number of bad sub-regions in sky-SB measurement (not including bad pixel sub-regions) |
N_bad_pixel_regions | Number of bad pixel sub-regions in sky-SB measurement |
N_good_regions | Number of good sub-regions in sky-SB measurement |
N_total_regions | Total number of sub-regions in sky-SB measurement |
Mean_x_px or Mean_y_px | Mean x or y pixel position of good sub-regions used in sky-SB measurement |
Std_x_px or Std_y_px | Std of x or y pixels of good sub-regions used in sky-SB measurement |
Q1_Sky_e/s or Q1_RMS_e/s | Sky-SB or sky-SB RMS in WFC3/IR Quadrant 1 (top left) |
Q2_Sky_e/s or Q2_RMS_e/s | Sky-SB or sky-SB RMS in WFC3/IR Quadrant 2 (bottom left) |
Q3_Sky_e/s or Q3_RMS_e/s | Sky-SB or sky-SB RMS in WFC3/IR Quadrant 3 (bottom right) |
Q4_Sky_e/s or Q4_RMS_e/s | Sky-SB or sky-SB RMS in WFC3/IR Quadrant 4 (top right) |
Quad_Left_Sky_e or Quad_Left_RMS_e | Sky-SB or sky-SB RMS in left half of ACS/WFC or WFC3/UVIS chip |
Quad_Right_Sky_e or Quad_Right_RMS_e | Sky-SB or sky-SB RMS in right half of ACS/WFC or WFC3/UVIS chip |
Expected_RMS_e or Expected_RMS_e/s | Expected RMS based on Poisson and Gaussian noise |
RA_J2000 | RA of image |
DEC_J2000 | DEC of image |
Target_Name | Target name associated with image |
Start_JD | Start Modified Julian Date associated with image |
Start_Time | Start time associated with image |
Average_Earth_Limb_Angle | Average Earth Limb Angle during the exposure |
Ecliptic_Latitude | Ecliptic Latitude of exposure |
Ecliptic_Longitude | Ecliptic Longitude of exposure |
Galactic_Latitude | Galactic Latitude of exposure |
Galactic_Longitude | Galactic Longitude of exposure |
Exp_Time | Exposure Time |
Moon_Angle | Moon Angle |
Sun_Altitude | Sun Altitude |
Sun_Angle | Sun Angle |
CAL_VER | calwf3 version used to reduce file |
Sensitivity_Jy/(e/s) | Inverse sensitivity in units of Jy/(e/s) |
Sensitivity_SCI1_Jy/(e/s) | Inverse sensitivity of the first science extension (Chip 2) in units of Jy/(e/s) |
Sensitivity_SCI2_Jy/(e/s) | Inverse sensitivity of the second science extension (Chip 1) in units of Jy/(e/s) |
Sensitivity_Err_Jy/(e/s) | Error in zeropoint from Calamida et al. (2022) |
Sky_MJy/sr | Measured sky-SB, in units of MJy/sr |
Sky_rms_MJy/sr | Measured sky-SB rms, in units of MJy/sr |
Error_MJy/sr | Uncertainty in sky-SB, in units of MJy/sr |
Sky_MJy/sr_thermcorr | Measured sky-SB, in units of MJy/sr, with Thermal Dark signal subtracted |
Sky_MJy/sr_no_thermcorr | Measured sky-SB, in units of MJy/sr, with Thermal Dark signal NOT subtracted |
Therm_Corr_MJy/sr | Thermal Dark signal in units of MJy/sr |
Therm_Corr_e/s | Thermal Dark signal in units of e/s |
Flag | Flag Description |
---|---|
0 | No flag |
1 | More than 30% of sub-regions are flagged as bad |
2 | The sky-SB rms is higher than 2.5 times the expected rms |
4 | Image flagged via manual inspections |
8 | Exposure within 20 degrees of the galactic plane |
16 | Exposure with an Earth Limb Angle less than 40 deg |
32 | Exposure with a Sun Altitude greater than 0 deg |
64 | Exposure with Sun Angle less than 80 deg |
128 | Exposure with Moon Angle less than 50 deg |
256 | Image taken close to large, nearby galaxy |
512 | Exposure affected by persistence |