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Washington Double Star Supplemental Catalog (WDSS) - formats


Format for the summary lines are as follows:
----------------------------------------------------------------------------------------------------
01  001-014  a14                     WDSS identifier
02  016-018  a3                      Component identifier
03  025-028  i4                      dates of first/last observation
04  030-032  i3                      Number of astrometric observations
05  034-036  i3           deg        First/last position angle 
06  038-043  f6.2         arcsec     First/last separation (arcseconds or as noted)
07  044-044  a1                      Flag for separation units 
					m = mas
					M = arcminutes
					D = degrees
08  046-050  f5.2         mag        Primary/secondary visual magnitudes
09  051-051  a1                      Flag for filter: 
					blank = Gaia DR2 584/436 nm G filter (default)
					b = blue
					r = red
					g = SDSS g (477/280 nm)  
10  053-057  f5.2         mag        Primary/secondary infrared magnitudes 
11  058-058  a1                      Flag for filter:
					blank = K-band (default)
					h = H-band
					j = J-band   
12  060-064  a5                      Spectral type of primary/secondary
13  066-081  2f8.2        mas/y      Proper motion (RA and DEC) of primary/secondary
14  083-089  f7.2         mas        Parallax of primary/secondary
15  091-114  a24                     Alternate name for primary/secondary. Default is the Gaia Second
					Data Release, or DR2 designation, which constituted 99.2% of 
					all alternte designations as of Nov 2021. Next most common is 
					the Gaia Early Third Data Release, or ER3 designation (0.3%).
16  116-117  2a1                     Note flags:
					C = pair has both orbit and linear solutions, uncertain which 
					    is correct
					L = pair has rectilinear solution in Linear Elements Catalog
					N = see note in notes file
					O = pair has orbital solution in the Sixth Orbit Catalog
					U = pair is optical, based on parallax, proper motion, or 
					    other factors
					V = pair is physical, based on parallax, proper motion, or 
					    other factors
					X = pair is bogus (due to error in published coordinates, 
					    plate flaw identified as star, or other problem)
17  119-136                          Coordinates (J2000) of primary/secondary
             2i2,f5.2     hhmmss.ss	Right ascension  
             a1,2i2,f4.1  +ddmmss.s	Declination  
18  138-147  a10                     Designation in main WDS of component matching object in that catalog
19  149-155  a7                      Discoverer designation in main WDS catalog
20  156-160  a5                      Component designation in main WDS catalog

====================================================================================================

Format for measurement lines are as follows:
----------------------------------------------------------------------------------------------------
01  001-014  a14                     WDSS identifier
02  017-023  a7                      Component pair identifier
03  025-034  f10.5                   Date of observation (Julian epoch)           
04  036-036  a1                      Position angle flag              
					: = value is uncertain/estimated
					L = originally published as nf, sp, etc. 
					q = quadrant has been flipped 180deg from published value
					V = measure is a vector separation along this angle vector 
05  037-043  f7.3         deg        Position angle
06  045-050  f6.3         deg        Position angle error
07  052-052  a1                      Separation flag
					: = value is uncertain/estimated
					< = separation is less than quoted value 
					E = pair elongated 
					U = pair unresolved/single 
					G,O,S,V,X = Hipparcos non-component double star solutions or 
					            suspected non-single 
					R = pair resolved but no separation give 
					D = separation is in degrees
					M = separation is in arcminutes
					m = separation is in milliarcseconds
08  053-061  f9.5         arcsec     Separation (arcseconds or as noted by separation flag)
09  063-063  a1                      Separation error flag
					P, F, G, V = quality flags (poor, fair, etc.)
					> = error is lower limit to true value
					< = error is upper limit to true value
10  064-070  f7.5         arcsec     Separation error (same units as separation)
11  072-072  a1                      Primary magnitude flag
					> = magnitude is lower limit to true value
					v = primary is variable
12  073-078  f6.3         mag        Primary magnitude
13  079-079  a1                      Primary magnitude error flag
					> = error is lower limit to true value
					< = error is upper limit to true value
14  080-084  f5.3         mag        Primary magnitude error
15  086-086  a1                      Secondary magnitude flag 
					> = magnitude is lower limit to true value
					s = magnitude rather than magnitude difference (only used if 
					    primary magnitude field is blank)
					f = star is too faint
					v = secondary is variable
16  087-092  f6.3         mag        Secondary magnitude, or magnitude difference if primary 
					magnitude field is blank
17  093-093  a1                      Secondary magnitude error flag 
					> = error is lower limit to true value
					< = error is upper limit to true value
18  094-098  f5.3         mag        Secondary magnitude error
19  100-107  2i4          nm         Filter effective wavelength and FWHM
             or 2f4.1
20  108-108  a1                      Filter flag
					a = value is average of multiple filters
					u = wavelength is in microns
					m = wavelength is in mm
					c = wavelength is in cm
					M = wavelength is in meters
					B = blue filter (effective wavelength/FWHM values unknown)
					K = IR filter (effective wavelength/FWHM values unknown)  
					R = red filter (effective wavelength/FWHM values unknown)    
					X = X-ray band (effective wavelength/FWHM values unknown)    
					n = no filter used   
					? = filter information is uncertain
					: =filter information is approximate

21  110-114  f5.1         m          Telescope aperture
22  115-115  a1                      Telescope aperture flag
					a = average of multiple telescopes
					k = multiple aperture telescope, baseline in km
23  117-118  i2                      Number of nights averaged into mean measure
24  120-127  a7                      Reference code (see file wdsref.memo)
25  129-130  a2                      Technique code (see table below)                       

====================================================================================================

Technique codes for measurement lines:

(Note: a plus sign (+) in the technique columns of wdsref.memo indicates the paper contains measures 
made by more than one similar method. For example, H+ means the paper includes measures from more 
than one space-based technique.)

A  = adaptive optics
Aa = adaptive optics with apodizing phase plate
Ac = CHARA adaptive optics
Ad = adaptive optics spectral deconvolution technique
Ag = laser-guided AO
Al = adaptive optics imaging, keeping only selected images ("lucky imaging")
Am = adaptive optics with aperture mask
Ao = adaptive optics coronagraph
As = AO + dark speckle coronagraph
Aw = adaptive optics with coronagraph and "well-corrected subaperture"

C  = CCD or other two-dimensional electronic imaging
Ca = area scanner                             
Cc = IR coronagraph
Ce = electronographic camera                  
Cg = imaging using Gaussian aperture pupil mask
Ci = IR direct imaging
Cl = short-exposure CCD imaging, keeping only selected images ("lucky imaging")
Cp = IR imaging polarimetry
Cs = IR one-dimensional slit scanning
Cu = USNO CCD imaging (speckle-style reduction)     

D  = Heliometer                               

E  = Wide-field CCD or other two-dimensional electronic imaging
E2 = 2MASS (Two Micron All-Sky Survey)
Ed = DENIS (Deep Near-Infrared Survey)
Ek = UKIDSS (UKIRT Infrared Deep Sky Survey)
Ep = PPMX, PPMXL
Er = USNO URAT
Es = SDSS (Sloan Digital Sky Survey)
Eu = UCAC                               
Ey = Yale SPM (Southern Proper Motion) Survey

H  = Hipparcos/Tycho, HST, Spitzer, or other space-based technique
Ha = HST + ACS
Hc = Chandra
He = Einstein
Hf = HST + Fine Guidance Sensor
Hg = Gaia
Hh = Hipparcos
Hi = Spitzer Space Telescope + IRAC (Infrared Array Camera)
Hk = Kepler
Hm = Spitzer Space Telescope + MIPS (Multiband Imaging Photometer for Spitzer)
Hn = HST + NICMOS IR direct imaging
Ho = HST + Faint Object Camera
Hp = HST + WFPC2 Planetary Camera
Hs = HST + STIS
Ht = Tycho
Hw = WISE (Wide-field Infrared Survey Explorer) satellite (IR imaging)
Hx = Spitzer Space Telescope + SpeX spectrometer and slit-viewing camera
Hz = XMM Newton satellite

I  = interferometric technique
Ig = phase grating interferometer  
Im = Michelson interferometer

J  = visual interferometer 
     [aperture value indicates the longest baseline on the monolithic mirror  
     (e.g., 0.7m for Finsen's eyepiece interferometer or 6.1m for the 20-foot 
     beam used on the Mount Wilson 100inch)]
Jm = Mount Wilson 100inch telescope rotating interferometer (Anderson, Merrill)
Jp = Mount Wilson 20-foot beam interferometer (Pease)

K  = long-baseline visual/IR/radio interferometer 
     (aperture value indicates the longest baseline used)
K2 = CERGA 2-telescope interferometer
Ka = VLTI/AMBER
Kb = BIMA 
Kc = CHARA Array
Ke = European VLBI network
Kf = CHARA Array (separated fringe packet data)
Kg = global VLBI array
Ki = IOTA 
Kk = Keck interferometer
Kl = VLA/VLBA
Km = Mark III 
Kn = NPOI/NOI [Navy (Prototype) Optical Interferometer]
Kp = PTI (Palomar Testbed Interferometer)
Kr = radio/IR aperture synthesis technique
Ks = SUSI (Sydney University Stellar Interferometer)
Ku = Pulkovo Stellar Interferometer

M  = micrometry technique
Ma = micrometer with refractor
Mb = micrometer with reflector
Mc = comparison image micrometer
Md = visual measures with a double-image micrometer
Mg = illuminated-reticle micrometer (e.g. Celestron Micro-Guide)
Mr = RGO use of micrometer plus comparison image micrometer on same star        

O  = occultation 

P  = photographic technique
Pa = photographic, with astrograph
Pb = USNO-B photographic, with multiple astrographs
Pc = Astrographic Catalog 
Pe = ESO Schmidt astrograph
Pk = AGK Catalog
Po = photographic, with medium or long-focus technique or ocular enlargement
Pp = Palomar Observatory Sky Survey  POSS-I:  1948-1958, 48in/1.2m Schmidt
                                     POSS-II: 1985-1999, 48in/1.2m Schmidt
Pu = UK Schmidt Southern Survey               1974-1987, 48in/1.2m Schmidt

S  = speckle interferometric technique
Sa = aperture masking technique (MAPPIT, etc.)
Sb = bispectrum speckle interferometric technique
Sc = CHARA speckle  
Si = IR speckle  
Sp = speckle polarimetry
Ss = shift-and-add technique
St = Tokovinin "hrcam"
Su = USNO speckle  

T  = Transit circle / Meridian circle
Tm = "Eyepiece micrometer" transit/chronometric technique

V  = visual estimate

X  = spectroscopic technique 
Xg = visual estimate made with an objective grating
Xh = high-resolution spectroscopy
Xl = low-resolution spectroscopy
Xr = resolved spectroscopy
Xs = spectrophotometry      

Z  = photometric technique
Z  = photometer
Zc = CCD photometry
Zd = photocell with diaphragm in focal plane
Zp = visual photometry with a double-image or polarizing photometer
Zw = wedge photometer

====================================================================================================

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wdss.......... comp.... frst nnn th1 rho1..* vmag1* kmag1* spec1 pm1............. par1... name1................... ** coords1........... wds_old... dd_old.comp.
                        last     th2 rho2..* vmag2* kmag2* spec2 pm2............. par2... name2...................    coords2...........                        
----------------------------------------------------------------------------------------------------------------------------------------------------------------
1234567+123456 Aa1....  1234 123 123 123.45* 12.34* 12.34* A1Iab +1234.56+1234.56 1234.56 123456789012345678901234 XY 123456.78+123456.7 12345+1234 XYZ1234AB,CD
----------------------------------------------------------------------------------------------------------------------------------------------------------------
0000004+054750 A        2008   1  25  13.17  20.87g   .    K7         .       .       .   SLW 0000+0547             V 000000.44+054750.7 
0000004+054750 B        2008      25  13.17  22.08g   .    M1         .       .       .                               000000.82+054802.6                        
0000004+054750  AB      2008.8151    25.      .      13.17      .       26.285 0.449  24.040 0.985  355 120    2.5   1 Dhi2015  Es                        
0000004+054750  AB      2008.8151      .      .        .        .       20.868 0.038  22.083 0.103  477 280    2.5   1 Dhi2015  Es                        
0000004+054750  AB      2008.8151      .      .        .        .       19.479 0.017  20.531 0.038  623 280    2.5   1 Dhi2015  Es                        
0000004+054750  AB      2008.8151      .      .        .        .       18.844 0.017  19.688 0.033  762 300    2.5   1 Dhi2015  Es                        
0000004+054750  AB      2008.8151      .      .        .        .       18.447 0.037  19.120 0.065  913 240    2.5   1 Dhi2015  Es                        
0000010+151505 A        1998   2 211   4.13  20.09g 14.63  M1         .       .       .   SLW 0000+1515             V 000001.06+151505.1                        
0000010+151505 B        2000     212   4.08  16.54g 13.46  K2       28.4    -1.9      .   2MASS J00000091+1515015     000000.92+151501.7                        
0000010+151505  AB      1998.883    211.0     .       4.126     .       14.524  .     13.979  .    1256 245    1.3   1 TMA2003  E2                        
0000010+151505  AB      1998.883       .      .        .        .       14.923 0.170  13.528 0.035 1633 160    1.3   1 TMA2003  E2                        
0000010+151505  AB      1998.883       .      .        .        .       14.627 0.093  13.456 0.046 2210 300    1.3   1 TMA2003  E2                        
0000010+151505  AB      2000.7388   212.      .       4.08      .       22.554 0.255  18.720 0.018  355 120    2.5   1 Dhi2015  Es                        
0000010+151505  AB      2000.7388      .      .        .        .       20.092 0.017  16.539 0.004  477 280    2.5   1 Dhi2015  Es                        
0000010+151505  AB      2000.7388      .      .        .        .       18.271 0.008  15.635 0.005  623 280    2.5   1 Dhi2015  Es                        
0000010+151505  AB      2000.7388      .      .        .        .       17.410 0.007  15.314 0.005  762 300    2.5   1 Dhi2015  Es                        
0000010+151505  AB      2000.7388      .      .        .        .       16.952 0.013  15.147 0.006  913 240    2.5   1 Dhi2015  Es                        
0003431-075506 A        2009   1  61   9.67  21.21g 15.21  M2         .       .       .   SLW 0003-0755             V 000343.16-075506.1                        
0003431-075506 B        2009      61   9.67  21.48g 15.83  M2         .       .       .   2MASS J00034378-0755014     000343.74-075501.5                        
0003431-075506  AB      2009.7897    61.      .       9.67      .       22.374 0.457  22.927 0.731  355 120    2.5   1 Dhi2015  Es                        
0003431-075506  AB      2009.7897      .      .        .        .       21.206 0.048  21.480 0.061  477 280    2.5   1 Dhi2015  Es                        
0003431-075506  AB      2009.7897      .      .        .        .       19.865 0.024  20.040 0.027  623 280    2.5   1 Dhi2015  Es                        
0003431-075506  AB      2009.7897      .      .        .        .       18.648 0.013  18.829 0.014  762 300    2.5   1 Dhi2015  Es                        
0003431-075506  AB      2009.7897      .      .        .        .       18.092 0.028  18.207 0.031  913 240    2.5   1 Dhi2015  Es                        
0003431-075506 A        2009   1  92  10.08  21.21g 15.21  M2         .       .       .   SLW 0003-0755             V 000343.16-075506.1                        
0003431-075506 C        2009      92  10.08  21.52g 15.56  M2         .       .       .   2MASS J00034383-0755065     000343.84-075506.4                        
0003431-075506  AC      2009.7897    92.      .      10.08      .       22.374 0.457  26.031 0.908  355 120    2.5   1 Dhi2015  Es                        
0003431-075506  AC      2009.7897      .      .        .        .       21.206 0.048  21.521 0.063  477 280    2.5   1 Dhi2015  Es                        
0003431-075506  AC      2009.7897      .      .        .        .       19.865 0.024  19.862 0.024  623 280    2.5   1 Dhi2015  Es                        
0003431-075506  AC      2009.7897      .      .        .        .       18.648 0.013  18.667 0.013  762 300    2.5   1 Dhi2015  Es                        
0003431-075506  AC      2009.7897      .      .        .        .       18.092 0.028  18.106 0.028  913 240    2.5   1 Dhi2015  Es                        
0003431-075506 B        2009   1 163   5.16  21.48g 15.83  M2         .       .       .   2MASS J00034378-0755014     000343.74-075501.5                        
0003431-075506 C        2009     163   5.16  21.52g 15.56  M2         .       .       .   2MASS J00034383-0755065     000343.84-075506.4                        
0003431-075506  BC      2009.7897   163.      .       5.16      .       22.927 0.731  26.031 0.908  355 120    2.5   1 Dhi2015  Es                        
0003431-075506  BC      2009.7897      .      .        .        .       21.480 0.061  21.521 0.063  477 280    2.5   1 Dhi2015  Es                        
0003431-075506  BC      2009.7897      .      .        .        .       20.040 0.027  19.862 0.024  623 280    2.5   1 Dhi2015  Es                        
0003431-075506  BC      2009.7897      .      .        .        .       18.829 0.014  18.667 0.013  762 300    2.5   1 Dhi2015  Es                        
0003431-075506  BC      2009.7897      .      .        .        .       18.207 0.031  18.106 0.028  913 240    2.5   1 Dhi2015  Es                        
==========================================================================================================================================================