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1978A&AS...31...99Haslam+ (Paper 1)
1979A&AS...36..237Waldthausen+ (Paper 2)
1980A&AS...41..339Andernach+ (Paper 3)
1981A&AS...43..155Andernach+ (Paper 4)
1986A&AS...65..561Andernach+ (Paper 5)
1988A&AS...73..265Andernach+ (Paper 6)
1990A&AS...82..279Reuter+ (Paper 7)

VIII/43             Radio survey of clusters of galaxies (Andernach+ 1978)
============================================================================
A radio survey of clusters of galaxies
I. 11.1 cm observations of A 591, A 754, A 1066, A 1314, A 1517, A 2094,
A 2142, A 2255, A 2256, A 2319 and A 2462.
     Haslam C.G.T., Kronberg P.P., Waldthausen H., Wielebinski R., Schallwich D.
    
    =1978A&AS...31...99H  (Paper 1)
                               Abstract
As a part of a programme of studies of clusters of galaxies at centimeter
wavelengths, we have observed eleven Abell clusters at 11.1cm using the
100 m radio telescope. The angular resolution at this wavelength is 4.6 arcmin,
and an r.m.s. noise limit of 5 mK was reached in most of the observations.
This enables us to investigate the distribution of low level emission near
point sources in the clusters.
------------------------------------------------------------------------------
II. 11.1 cm observations of A 85, A 407, A 514, A 568, A 602, A 1361, A 1775,
A 2036, A 2079, A 2224, A 2241, A 2365 and A 2634.
     Waldthausen H., Haslam C.G.T., Wielebinski R., Kronberg P.P.
    
    =1979A&AS...36..237W  (Paper 2)
                               Abstract
As part of a programme of high-frequency observations of clusters of galaxies
we have mapped thirteen Abell clusters at 2695 MHz (11.1cm wavelength) using
the 100-m radio telescope. The angular resolution at this wavelength is 4.4 arcmin,
and a rms noise level of 5 mJy per beam area was reached in most of the observations.
These levels are comparable to the confusion limit of the telescope and enable us
to investigate the distribution of complex low-level emission near point sources 
in the clusters.
------------------------------------------------------------------------------
III. 6.2 cm observations, radio spectra and optical identifications of
sources in 29 Abell clusters.
     Andernach H., Waldthausen H., Wielebinski R.
    
    =1980A&AS...41..339A  (Paper 3)
                               Abstract
 As part of a program of high-frequency observations of clusters of galaxies we
mapped twenty-nine Abell clusters of galaxies at 4850 MHz (6.2cm) using the 100-m
radio telescope. The angular resolution at this wavelength is 2.6 arcmin, and r.m.s.
noise levels of between 0.6 and 7 mJy per beam area were achieved. The radio maps
were superimposed onto the optical fields of the Palomar Observatory Sky Survey red
(E) prints. This revealed a large fraction of empty fields or optical objects 
significantly separated from the radio peak. Radio spectra of most of the detected
sources were obtained by combining our published flux data with those at lower
frequencies. We find a trend for cluster source spectra to become steeper with
decreasing distance from the cluster centre. In a few cases there is an indication
of low-level extended cluster emission. For A2319 the radio halo is clearly 
detected at 4850 MHz.
------------------------------------------------------------------------------
IV. 11.1 cm observations of 19 Abell clusters in total intensity
and polarization.
     Andernach H., Schallwich D., Haslam C.G.T., Wielebinski R.
    
    =1981A&AS...43..155A  (Paper 4)
                               Abstract
Radio continuum maps obtained with the Effelsberg 100-m telescope are  
presented for twelve rich clusters of galaxies. For some of these 
sources linear polarization information is given as well. Radio spectra of the
sources were obtained using published flux values while optical  
identifications are suggested from overlays of radio maps onto the red  
prints of the Palomar Sky Survey. No radio haloes on the order of the  
cluster size have been detected in the presented sample.  Observations 
of further seven cluster fields already published in paper II have been
reanalyzed in linear polarization. 

------------------------------------------------------------------------------
V. 11.1 cm maps of 18 Abell Clusters and observations of selected sources
at 6.3 and 2.8 cm.
     Andernach H., Sievers A., Kus A., Schnaubelt J.
    
    =1986A&AS...65..561A  (Paper 5)
                               Abstract
Thirteen areas containing eighteen rich clusters of galaxies have been mapped
in radio continuum at 11.1 cm wavelength with the 100-m Effelsberg telescope. The
angular resolution is 4.4 arcmin. Linear polarization was also recorded for some 
of the fields, which in most cases extend to the full Abell radius of the clusters.
A few of the more complex sources in these fields have been additionally observed
at 6.3 cm wavelength and, for the first time in this series of papers, also at 2.8 cm
wavelength to study their structure and spectral variations. A total of 142 sources
are reported here and radio spectra for 108 of them have been obtained using literature
data. Optical identifications are proposed for nearly half of the detected sources.
The mean spectral index of sources out to a projected source distance of about 0.8
Abell radii from the cluster centres exceeds the average value of all sources in the
present survey and does not show a pronounced maximum near the cluster centres.
There is a significant steepening of the spectra with decreasing 11.1 cm source flux
density, regardless of projected distance to the cluster centre.
------------------------------------------------------------------------------
VI. More observations of 34 Abell cluster areas at 11.1, 6.3 and 2.8 cm
and a preliminary statistical review of data in papers I-VI.
     Andernach H., Han Tie, Sievers A., Reuter H.-P., Junkes N., Wielebinski R.
    
    =1988A&AS...73..265A  (Paper 6)
                               Abstract
 Radio continuum maps of 26 Abell clusters of galaxies obtained with the
Effelsberg 100-m telescope at a wavelength of 11.1cm (HPBW=4.4 arcmin) are
presented.  Most of the maps cover the full Abell radius of 3 Mpc (H_0_=50
km/s Mpc) of the clusters and contain linear polarization information.
Selected cluster areas have also been mapped at a higher frequency and
angular resolution: six fields at wavelength 6.3cm (HPBW=2.5 arcmin) and
fourteen fields at wavelength 2.8cm (HPBW=1.2 arcmin). Radio data for 175
individual sources are listed and radio spectra for 141 of them have been
obtained using literature data. Only very few of these show spectral
steepening at high frequencies. This also holds for the local spectra
of those radio galaxy tails which could be resolved with the Effelsberg
antenna beam. Instead, the tail spectra steepen only with distance down
the tail. Except for some indication in A665 and A2152 no more examples
of radio halo sources were found at 2.7 GHz. Optical identifications for
35 of the detected sources are proposed on the basis of overlays with
Palomar or ESO sky surveys. The IRAS point source catalogue has been
searched for galaxy counterparts on the overlays and a total of 27 IRAS
galaxies were found, of which 8 are new identifications. A statistical
analysis of the entire survey data shows that for sources selected at
2.7 GHz the correlation between spectral index and projected cluster centre
distance is weaker than for low frequency source samples. A strong trend
for the spectra to steepen with decreasing flux density is evident.
A large fraction of the empty field sources are found to have steep
radio spectra and might constitute a "relic" population of cluster sources.
------------------------------------------------------------------------------
VII. 11.1 cm maps of 20 Abell clusters 6.3 cm maps of selected fields.
     Reuter H.-P., Andernach H.
    
    =1990A&AS...82..279R  (Paper 7)
                               Abstract
Radio continuum maps of 20 Abell clusters of galaxies obtained with the 
100-m Effelsberg telescope at 11.1 cm and maps of selected sources at 
6.3 cm are presented. All observations contain linear polarization 
information, and most of the 11-cm maps cover the full Abell radius of 3 
Mpc (H(0) = 50 km/s Mpc) of the clusters. Radio data for 86 sources are 
listed. Radio spectra were obtained for 56 sources using literature 
data. No evidence is found for the sources selected from a low frequency 
(151 MHz) survey to have systematically steeper radio spectra than the 
average of the entire Effelsberg cluster sample. Optical identifications 
are proposed for 40 sources. New identifications of two IRAS sources 
were found. Indirect evidence is presented for the presence of cluster 
radio halos in A948, A1329, A2176 and A2312. 

Author's  Abstract :
 Radio continuum maps of 20 Abell clusters of galaxies obtained with the
100-m Effelsberg telescope at at a wavelength of 11.1 cm (HPBW=4.4 arcmin),
and maps of selected sources at 6.3 cm are presented. All observations
contain linear polarization information, and most of the 11-cm maps cover the
full Abell radius of 3 Mpc (H(0) = 50 km/s Mpc) of the clusters. We list
radio data for 86 sources, 25 of them (=29\%) are new detections. Radio
spectra were obtained for 56 sources using literature data. No evidence is
found for the sources selected from a low frequency (151 MHz) survey to have
systematically steeper radio spectra than the average of the entire
Effelsberg cluster sample. Optical identifications using POSS or ESO prints
are proposed for 40 sources (=48\%), 27 of them are new identifications. Two
new identifications of IRAS sources were found. We find some indirect
evidence for the presence of cluster radio halos in A948, A1329, A2176 and
A2312.
================================================================================
ADC_Keywords: Clusters, galaxy ; Radio sources ; Spectroscopy ; Redshifts ;
              References ; Morphology
Keywords: clusters of galaxies - continuum maps - spectral index -
          radio spectra - linear polarization - radio sources -
          spectra of radio sources -
          optical and IR identification of radio sources

Description:
    Observations of Abell clusters at 11.1, 6.2, 6.3 and 2.8cm with the
    100m Effelsberg telescope. The data were compiled by H.J. Andernach.

File Summary:
-----------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
-----------------------------------------------------------------------------
ReadMe             80        .   This file
clopt             133       25   Optical data for the clusters studied
                                  (Paper 3)
clopx             161       48   Optical and X-ray data for the clusters studied
                                  (Papers 3 and 4)
clparam           140       77   Relevant Parameters for observed Cluster
                                  (Papers 6 and Paper 7)
clir               84        8   Optical and radio identifications of IRAS point
                                   sources (Paper 7)
r2700a            111      124   11.1cm (2.7GHz) radio data (Papers 1 and 2)
r2700b            258      484   11.1cm (2.7GHz) radio data, and optical
                                  identifications (Papers 4, 5, 6, and 7)
r4850             196       90   6.2cm (4.85GHz) radio data (Paper 3)
r4750              94       59   6.3cm (4.75GHz) radio data (Papers 5, 6 and 7)
r10700            123       46   2.8cm (10.7GHz) radio data (Paper 5 and 6)
ref1               46       54   r2700a file references
ref2d              46       62   r2700b file references (D series)
ref2e              61      133   r2700b file references (E series)
ref2g              59       31   r2700b file references (G series)
ref2t              84      173   r2700b file references (T series)
ref3               62      105   r4850  file references
ref4               63       52   clopx   file references
ref5               87       55   clparam file references
------------------------------------------------------------------------------

Byte-by-byte Description of file: clopt
------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
------------------------------------------------------------------------------
   1-  5  A5    ---      Abell    Abell cluster number
   8-  9  I2    h        RAh      Right ascension (1950)
  11- 14  F4.1  min      RAm      Right ascension (1950)
      16  A1    ---      DE-      Declination sign
  17- 18  I2    deg      DEd      Declination (1950)
  20- 21  I2    arcmin   DEm      Declination (1950)
  23- 28  A6    ---      BM       Bautz-Morgan class
      29  A1    ---    n_BM       Note on BM (1)
  31- 32  A2    ---      RS       Rood-Sastry classification
      33  A1    ---    n_RS       Note on RS (2)
      35  I1    ---      Rich     Richness class (Abell, 1958 Cat. )
      37  I1    Mpc      Dist     Distance (Abell, 1958 Cat. )
  39- 44  F6.4  ---      zEst     ? Estimated Redshift
  45- 46  A2    ---    n_zEst     Note on zEst (3)
  48- 53  F6.4  ---      zMeas    ? Measured redshift
      54  A1    ---    n_zMeas    [NSB] Note on zMeas (3)
  56- 59  F4.1  arcmin   RAbell   Abell radius
  61- 64  F4.1  arcmin   RCluster ? Cluster radius (4)
  66- 69  F4.1  mag      magBr    ? Brightest galaxy magnitude
  71- 74  F4.1  mag      mag10th  ? 10th brightest galaxy magnitude
  76- 79  F4.2  arcmin   aMaj     ? Major axis of the brightest galaxy
  81- 84  F4.2  arcmin   aMin     ? Minor axis of the brightest galaxy
  86- 89  F4.1  arcmin   DistC    ? Distance from center
  91-122  A32   ---      Xname    ? Possible identification with an X-ray
                                   source (5)
 124-125  A2    ---    l_RadX     [<=] Limit flag on RadX
 126-127  I2    arcmin   RadX     ? X-ray core radius
     129  I1    arcmin e_RadX     ? rms uncertainty on RadX
 131-133  F3.1  arcmin   RadO     ? Optical core radius
--------------------------------------------------------------------------------
Note (1): * : Corwin's estimate (1974AJ.....79.1356C)
Note (2): + = estimate by Bahcall, Harris and Strom (1976ApJ...209L..17B)
          * = Owen's (1975AJ.....80..263O) estimate
          : = uncertainty flag
Note (3): Ow: Owen (1974AJ.....79..427O)
           *: Owen (1975AJ.....80..263O)
           R: Riley (1975MNRAS.170...53R)
          MH: Mills & Hoskins (1977AuJPh..30..509M)
           N: Noonan (1973AJ.....78...26N)
           S: Sargent (1973PASP...85..281S)
           B: Bridle and Folamont (1976A&A....52..107B)
           C: Corwin (1974AJ.....79.1356C)
Note (4): Estimates from Leir & Van den Bergth (1977ApJS...34..381L)
Note (5): Giaconni et al. (1974ApJS...27...37G)
          Cooke et al., (1978MNRAS.182..489C)
          Forman et al., (1978ApJS...38..357F)
          For A 2079, 3U 1526+29 not fulfilling the 3U catalogue criteria
--------------------------------------------------------------------------------

Byte-by-byte Description of file: clopx
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  5  A5    ---     Abell     Abell cluster number
   7-  8  I2    h       RAh       Right ascension (1950)
  10- 13  F4.1  min     RAm       Right ascension (1950)
  14- 15  A2    ---     NotePos   Note on position
      17  A1    ---     DE-       Declination sign
  18- 19  I2    deg     DEd       Declination (1950)
  21- 24  F4.1  arcmin  DEm       Declination (1950)
  26- 32  A7    ---     BM        Bautz-Morgan class
  34- 35  I2    ---   r_BM        ? BM references (see ref4 file) (1)
  37- 39  A3    ---     RS        Rood-Sastry classification
  41- 42  I2    ---   r_RS        ? Reference on RS (see ref4 file)
      44  I1    ---     Rich      ? Richness class (Abell, 1958 Cat. )
      46  I1    Mpc     Dist      ? Distance (Abell, 1958 Cat. )
  48- 54  F7.5  ---     z         ? Redshift
      55  A1    ---   n_z         [abcdefgh] Note on Redshift (1)
  57- 58  I2    ---   r_z         ? Redshift reference (see ref4 file)
      59  A1    ---   n_r_z       Note on redshift reference (1)
  61- 62  I2    ----    Ngal      ? Number of galaxies used for determining the
                                     redshift (5)
  64- 66  I3    arcmin  RAbell    ? Abell radius
  68- 70  I3    arcmin  RCluster  ? Cluster radius (2)
  72- 75  F4.1  mag     magBr     ? Brightest galaxy magnitude (2)
  77- 80  F4.1  mag     mag10th   ? 10th brightest galaxy magnitude (3)
  82- 85  F4.2  mm      aMaj      ? Major axis of the brightest galaxy (2)
  87- 90  F4.2  mm      aMin      ? Minor axis of the brightest galaxy (2)
  92- 93  A2    ---     Map       [I X] I,II : states whether 11.1cm data were
                                         already published in Paper I or II
                                        X : Refers to 6.2cm Effelsberg
                                          observations presented in Paper III
  95-128  A34   ---     Xnames    X-ray sources associated with the cluster (4)
 130-143  A14   ---     RefX      References for X-ray flux (see ref4 file)
 145-149  A5    ---     RefXsp    References for X-ray spectra (see ref4 file)
     150  A1    ---   l_RadX      Limit flag on X-ray core radius
 151-154  F4.1  arcmin  RadX      ? X-ray core radius
 156-157  I2    ---   r_RadX      ? X-ray core radius reference (see ref4 file)
 159-161  F3.1  arcmin  RadO      ? Optical core radius
--------------------------------------------------------------------------------
Note (1): a: mean of estimates by Corwin (1974AJ.....79.1356C),
              Owen (1975ApJ...195..593O),
              Leir and van den Bergh (1977ApJS...34..381L),
              and Mills and Hoskins (1977AuJPh..30..867M).
          b: mean of estimates by Corwin (1974AJ.....79.1356C),
              Owen (1975ApJ...195..593O),
              and Mills and Hoskins (1977uJPh..30..867M).
          c: mean of estimates by Corwin (1974AJ.....79.1356C),
              Owen (1975ApJ...195..593O),
              and Leir and van den Bergh (1977ApJS...34..381L)
          d: mean of estimates by Owen (1975ApJ...195..593O),
              Leir and van den Bergh, (977ApJS...34..381L)
              and Mills and Hoskins (1977AuJPh..30..867M).
          e: Both A2255 and A2319 may consist of two clusters nearly
              superimposed along the line of sight, but only for A2319 we use
              the weighted mean of the redshifts of the subclusters.
          f: Bahcall (1975ApJ...198..249B) found the cluster centre to be
              coincident with the dominant cD galaxy. We measured the position
              of this galaxy on our overlay and took that as the cluster centre
              position.
          g: Measured redshift for foreground (?) galaxy z=0.036C
          h: The radiosource in A1836 is identified with a foreground galaxy
              with z=0.025C
Note (2): Data from Leir and van den Bergh (1977ApJS...34..381L)
Note (3): When only the 10th magnitude is given, the entry is from Sastry and
           Rood (1971ApJS...83..371S)
Note (4): Detection of an X-ray source in the 3U/4U or 2A catalogues
           (Giaconni et al., 1974ApJS...27...37G;
           Forman et al. 1978ApJS...38..357F; Cooke et al. 1978MNRAS.182..489C)
           or with the HEAO-A (HA) or HEAO-B (HB) satellites
           (Schwartz et al., 1979ApJ...231L.105S; Ku, 1979, Priv. communication;
           upper limits (in brackets): Ulmer et al., 1980ApJ...235..351U)
          For A2079, 3U 1526+29 not fulfilling the 3U criteria
Note (5): A blank implies that the number was not given by the author or the
              redshift is an estimate only.
--------------------------------------------------------------------------------

Byte-by-byte Description of file: clparam
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  5  A5    ---     Abell     Abell cluster number
       6  A1    ---   m_Abell     Multiplicity index on Abell number
   9- 10  I2    h       RAh       Optical right ascension (1950)
  12- 13  I2    min     RAm       Optical right ascension (1950)
  15- 18  F4.1  s       RAs       Optical right ascension (1950)
      20  A1    ---     DE-       Declination sign
  21- 22  I2    deg     DEd       Optical declination (1950)
  24- 25  I2    arcmin  DEm       Optical declination (1950)
  27- 30  F4.1  arcsec  DEs       Optical declination (1950)
  32- 33  I2    ---     RefPos    Position reference (1)
  35- 37  A3    ---     RS        Rood-Sastry classification
  39- 40  I2    ---   r_RS        ? References for RS classification (1)
      43  I1    ---     BM        ? Bautz-Morgan classification
      44  A1    ---   u_BM        Uncertainty flag on BM classification
  45- 49  A5    ---   r_BM        ? References for BM classification (1)
      51  I1    Mpc     Dist      ? Distance (Abell 1958, Cat. )
      53  I1    ---     Rich      Richness (Abell 1958, Cat. )
  55- 59  F5.4  ---     z         Redshift
      60  A1    ---   n_z         [abe] e = estimated (2)
  62- 66  A5    ---   r_z         Redshift reference (1)
  67- 71  F5.1  arcmin  RAbell    Apparent Abell radius
      72  A1    ---   n_RAbell    [ab] Note on Abell radius (2)
  74- 77  F4.1  arcmin  ROpt      ? Optical radius
      78  A1    ---   u_ROpt      [)] Uncertainty flag on ROpt
      79  A1    ---   l_log(LX)   Limit flag on log(LX)
  80- 84  F5.2  10-7W   log(LX)   X-ray cluster luminosity
  86- 87  I2    ---   r_log(LX)   X-ray cluster luminosity reference (1)
  89-109  A21   ---     Obs11.1cm Observation Epoch minus 1900.0 at 11.1cm
 111-127  A17   ---     Obs6.3cm  Observation Epoch minus 1900.0 at 6.3cm
 129-140  A12   ---     Obs2.8cm  Observation Epoch minus 1900.0 at 2.8cm
--------------------------------------------------------------------------------
Note (1): References are in ref5 file
Note (2): a: recently z=0.0318 (RAbell=56.7') had been measured
              (Kalinkov 1985, priv. comm.)
          b: a more recent estimate is z=0.0856, RAbell=22.8'
              (Kalinkov 1985, priv. comm.)
--------------------------------------------------------------------------------

Byte-by-byte Description of file: clir
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  5  A5    ---     Abell     Abell cluster name
   6-  8  A3    ---   m_Abell     Multiplicity (several clusters)
  11- 12  I2    h       RAh       Infrared right ascension (B1950)
  13- 14  I2    min     RAm       Infrared right ascension (B1950)
  15- 18  F4.1  s       RAs       Infrared right ascension (B1950)
      19  A1    ---     DE-       Declination sign
  20- 21  I2    deg     DEd       Infrared declination (B1950)
  22- 23  I2    arcmin  DEm       Infrared declination (B1950)
  24- 25  I2    arcsec  DEs       Infrared declination (B1950)
      27  A1    ---   l_S100/S60  Limit flag on S100/S60
  28- 31  F4.2  ---     S100/S60  Ratio of IR flux densities (S100um/S60um)
      33  A1    ---   l_SpI       Limit flag on SpI
  34- 37  F4.2  ---     SpI       Radio-IR spectral index
                                   (between 2.7GHz and 100um)
  39- 51  A13   ---     IdOpt     Optical identification
  53- 84  A32   ---     Rem       Remarks
--------------------------------------------------------------------------------

Byte-by-byte Description of file: r2700a
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  8  A8    ---     Source    Source name (1)
  10- 11  I2    h       RAh       Right ascension (1950)
  13- 14  I2    min     RAm       Right ascension (1950)
  16- 19  F4.1  s       RAs       ? Right ascension (1950)
      21  A1    ---     DE-       Declination sign
  22- 23  I2    deg     DEd       Declination (1950)
  25- 26  I2    arcmin  DEm       Declination (1950)
  28- 29  I2    arcsec  DEs       ? Declination (1950)
      30  A1    ---   u_Pos       Uncertainty flag on position
      31  A1    ---   l_S2.7GHz   Limit flag on S2.7GHz
  32- 35  I4    mJy     S2.7GHz   ? Flux density at 2695 MHz (11.1cm)
      36  A1    ---   u_S2.7GHz   Uncertainty flag on S2.7GHz
  38- 82  A45   ---     Catal     Source catalogue name
  83-111  A29   ---     Ref       References (see ref1 file)
--------------------------------------------------------------------------------
Note (1): We have labelled each prominent source with a subnumber (A85.1 etc.),
           regardless of cluster membership, in increasing order of right
           ascension for each cluster area mapped. We have only labelled the
           most prominent sources.
--------------------------------------------------------------------------------

Byte-by-byte Description of file: r2700b
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---     Source    Source name
      11  A1    ---   n_Source    [ABCDEFabdg] Note on Source (1)
  12- 13  I2    h       RAh       Right ascension (1950)
  15- 16  I2    min     RAm       Right ascension (1950)
  18- 21  F4.1  s       RAs       ? Right ascension (1950)
      23  A1    ---     DE-       Declination sign
  24- 25  I2    deg     DEd       Declination (1950)
  27- 28  I2    arcmin  DEm       Declination (1950)
  30- 31  I2    arcsec  DEs       ? Declination (1950)
  32- 33  A2    ---     NotePos   [: abdefijlmnopqsAB] Note on position (2)
      34  A1    ---   l_S2.7GHz   Limit flag on S2.7GHz
  35- 38  I4    mJy     S2.7GHz   ? Integrated flux density at 2.7GHz
      39  A1    ---   u_S2.7GHz   [):] Uncertainty flag on S2.7GHz
  41- 43  I3    mJy   e_S2.7GHz   ? rms uncertainty on S2.7GHz
      44  A1    ---   n_S2.7GHz   [45EHabcdeghikt] Note (3)
  46- 49  F4.1  mJy     rmsI      ? rms noise level at 2.7GHz in total intensity
                                     (in mJy/beam area)
  51- 54  F4.1  mJy     rmsP      ? rms noise level at 2.7GHz in polarized
                                     intensity (in mJy/beam area)
      55  A1    ---   n_rmsI      [uvf] Note on rmsI and rmsP (2)
  56- 60  F5.1  deg     PA        ? Position angle of the major axis
      61  A1    ---   n_PA        [)Cr:?] Uncertainty flag on PA
                                    :)?=uncertainty flag, C=complex, r: resolved
  62- 63  I2    deg   e_PA        ? rms uncertainty on PA
      65  A1    ---   l_MajAxis   Limit flag on MajAxis
  66- 69  F4.1  arcmin  MajAxis   ? Deconvolved half width along major axis
      70  A1    ---   n_MajAxis   [C:] C=complex, : uncertainty flag
      72  A1    ---   l_MinAxis   Limit flag on MinAxis
  73- 75  F3.1  arcmin  MinAxis   ? Deconvolved half width along minor axis
      76  A1    ---   n_MinAxis   [C:] C=complex, : uncertainty flag
      77  A1    ---   l_m         Limit flag on m
  78- 81  F4.1  %       m         ? Integrated degree of linear polarization
      82  A1    ---   u_m         Uncertainty flag on m
  83- 86  F4.1  %     e_m         ? rms uncertainty on m
      87  A1    ---   n_m         [:fc] Note on m (4)
  89- 93  F5.1  deg     Xi        ? Integrated polarization position angle of
                                     electric field vector
  95- 96  I2    deg   e_Xi        ? rms uncertainty on Xi
      97  A1    ---   u_Xi        Uncertainty flag on Xi
      98  A1    ---   l_Pdist     Limit flag on Pdist
  99-102  F4.2  ---     Pdist     ? Projected distance of source to the cluster
                                     center in units of one Abell radius
     103  A1    ---   u_Pdist     [):] Uncertainty flag on Pdist
     104  A1    ---   l_P2.7      Limit flag on P2.7
 105-110  F6.2  ---     P2.7      ? Spectral power at 2.7GHz assuming cluster
                                     membership
     111  A1    ---   n_P2.7      [:a] : = uncertainty flag, a = redshift taken
                                   from A2319A, see table2e
 112-124  A13   ---     IdOpt     Optical identification
     125  I1    ---     OptCl     ? Optical class
     126  A1    ---   n_IdOpt     [EGT] Note on ref file (5)
 127-139  A13   ---   r_IdOpt     [0-9, ] Reference for optical data
     141  I1    ---     MemCl     ? Membership class
     143  A1    ---   l_SpI       Limit flag on SpI
 144-148  F5.2  ---     SpI       ? Average spectral index
     149  A1    ---   u_SpI       Uncertainty flag on SpI
 150-153  F4.2  ---   e_SpI       ? rms uncertainty on SpI
 156-159  A4    ---     SpCl      Spectral class (6)
     160  A1    ---   n_Ref       [DEGT] note for ref file (5)
 161-260  A100  ---     Ref       [0-9, ] Radio references (5)
--------------------------------------------------------------------------------
Note (1): A: Source reported by Swarup (1984JApA....5..139S)
          B: central part only
          C: position from Harris et al. (1980A&AS...39..215H)
          D: For A1060 and A2199 (data of 1988A&AS...73..265A), a renumbering
              was necessary for some sources.
          E: Renumbered with respect to data in 1980A&AS...41..339A
          F: A1060.0 same as A1060.1 in 1980A&AS...41..339A (r4750 file)
          a: source claimed by Slee & Quinn 1980PASAu...3..332S
          b: position from Andernach et al. 1980A&AS...41..339A (paper III)
          d: source claimed by Owen 1974AJ.....79..427O
          g: source named A2220.1 in Andernach et al. 1980A&AS...41..339A
                         (paper III)
Note (2): A: source detected by Mayer (1980, Ph.D. Thesis, Cambridge University
          B: 11 cm position
          a: from McHardy (1978MNRAS.184..783M)
          b: position from Andernach et al. 1980A&AS...41..339A (paper III)
         %c: from Dickey and Salpeter (1984ApJ...284..461D)
          d: from Dickey and Salpeter (1984ApJ...284..461D) and uncertain value
          e: from Perola and Valentijn (1979A&A....73...54P)
          f: east part of map is less sensitive
          i: correction of typo in original paper
          j: position from McHardy (1978MNRAS.185..927M
          l: same as A1060.1 of Paper III (1980A&AS...41..339A)
          m: central part of map is more sensitive
          n: position from Lauberts (1982, Cat. )
          o: detected by Fanti et al. (1983A&AS...51..179F, 1983A&AS...52..411F)
          p: detected by Douglas et al. (1973AJ.....78....1D)
          q: B2 position (Colla et al., 1972A&AS....7....1C)
          s: NE component of 4CP66.16.1
          u: data for outer part
          v: data for central part
         ':' : uncertainty flag
Note (3): 4: see table4e for Flux density to Xi data
          5: see table5e for Flux density to Xi data
          E: including two components 8' SE and NW of main source
          H: distorted due to map artefact
          a: includes N extension
          b: including overall extent
          c: including extension due SW
          d: not including extensions due NE and SE
          e: assuming a point source at the given position
          g: excluding extension due E
          h: Three satellite sources provide for another 50 mJy
          i: not including extension due W
          k: including overall extent
          t: not including the SE extension
Note (4): ':' : uncertainty flag
          f: main contribution from NW component
          c: main contribution from SW part of source
Note (5): E: the following references are in ref2e file
          D: the following references are in ref2d file
          G: the following references are in ref2g file
          T: the following references are in ref2t file
Note (6): S: straight power law
          C+: concave
          C-: convex
          Cmax: low frequency turnover
          C: complex
--------------------------------------------------------------------------------

Byte-by-byte Description of file: r4750
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  8  A8    ---     Source    Source name (1)
  10- 11  I2    h       RAh       Right ascension (B1950)
  13- 14  I2    min     RAm       Right ascension (B1950)
  16- 19  F4.1  s       RAs       ? Right ascension (B1950)
      20  A1    ---     NotePos   [abc] Note on position (2)
      22  A1    ---     DE-       Declination sign
  23- 24  I2    deg     DEd       Declination (B1950)
  26- 27  I2    arcmin  DEm       Declination (B1950)
  29- 32  F4.1  arcsec  DEs       ? Declination (B1950)
      33  A1    ---   u_Pos       Uncertainty flag on B1950 position
      34  A1    ---   l_S4.75GHz  Limit flag on S4.75GHz
  35- 37  I3    mJy     S4.75GHz  ? Flux density at 4.75GHz (6.3cm)
  39- 41  I3    mJy   e_S4.75GHz  ? rms uncertainty on S4.75GHz
      42  A1    ---   n_S4.75GHz  [a] Note on S4.75GHz (3)
  43- 46  F4.1  mJy     rmsI      ? rms noise level at 2.7GHz in total intensity
                                     (in mJy/beam area)
  48- 51  F4.1  mJy     rmsP      ? rms noise level at 2.7GHz in polarized
                                     intensity (in mJy/beam area)
  53- 55  I3    deg     PA        ? Position angle of major axis of
                                     extended sources
      56  A1    ---   n_PA        [:C] C = complex, : uncertainty flag
      58  A1    ---   l_MajAxis   Limit flag on MajAxis
  59- 61  F3.1  arcmin  MajAxis   ? Deconvolved half width along major axis
      62  A1    ---   n_MajAxis   [:Cr] C = complex, r = resolved,
                                        : uncertainty flag
      63  A1    ---   l_MinAxis   Limit flag on MinAxis
  64- 66  F3.1  arcmin  MinAxis   ? Deconvolved half width along minor axis
      67  A1    ---   n_MinAxis   [:Cr] C = complex, r = resolved,
                                        : uncertainty flag
      68  A1    ---   l_m         Limit flag on m
  69- 72  F4.1  %       m         ? Integrated degree of linear polarization
  74- 76  F3.1  %     e_m         ? rms uncertainty on m
  78- 80  I3    deg     Xi        ? Integrated polarization position angle of
                                       electric field vector
  82- 83  I2    deg   e_Xi        ? rms uncertainty on Xi
  85- 87  F3.2  ---     Pdist     ? Projected distance
      89  A1    ---   l_P4.75     Limit flag on P4.75
  90- 94  F5.2  ---     P4.75     ? Spectral power at 4.75GHz assuming cluster
                                     membership
--------------------------------------------------------------------------------
Note (1): For the reobserved fields, the nomenclature is consistent with
           previous papers, except for A1060 and A2199, for which a renumbering
           was necessary.
Note (2): a) 11 cm position
          b) position from 2.8 cm map
          c) position from Harris et al. (1980A&AS...39..215H)
Note (3): a) excluding EW extension
--------------------------------------------------------------------------------

Byte-by-byte Description of file: r4850
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  8  A8    ---     Source    Source name (1)
  12- 13  I2    h       RAh       ? Right ascension (1950)
  14- 15  I2    min     RAm       ? Right ascension (1950)
  16- 19  F4.1  s       RAs       ? Right ascension (1950)
      20  A1    ---     DE-       Declination sign
  21- 22  I2    deg     DEd       ? Declination (1950)
  23- 24  I2    arcmin  DEm       ? Declination (1950)
  25- 26  I2    arcsec  DEs       ? Declination (1950)
      27  A1    ---   u_Pos       Uncertainty flag on position
      29  A1    ---   l_S4850MHz  Limit flag on S4850MHz
  30- 33  I4    mJy     S4850MHz  ? Flux density at 4850 MHz
      34  A1    ---   u_S4850MHz  Uncertainty flag on S4850MHz
  35- 37  I3    mJy   e_S4850MHz  ? rms uncertainty on S4850MHz
  40- 42  F3.1  ---     rms       ? rms noise level of the cluster map,
                                     calculated for areas where there are no
                                     sources (in mJy/beam area)
  44- 46  I3    deg     PA        ? Position angle of the major axis of
                                     extended sources
      47  A1    ---   u_PA        [:?] Uncertainty flag on PA
      49  A1    ---   l_MajAxis   Limit flag on MajAxis
  50- 53  F4.1  arcmin  MajAxis   ? Half-power width along major axis
      54  A1    ---   u_MajAxis   Uncertainty flag on MajAxis
      56  A1    ---   l_MinAxis   Limit flag on MinAxis
  57- 59  F3.1  arcmin  MinAxis   ? Half-power width along minor axis
      60  A1    ---   u_MinAxis   Uncertainty flag on MinAxis
  62- 65  F4.2  ---     d/R       ? Projected distance (ratio of distance from
                                     the cluster center to the Abell radius) in
                                     units of Abell radius
      67  A1    ---   l_SpI       Limit flag on SpI
  68- 71  F4.2  ---     SpI       ? Mean spectral index between 600 and 4800MHz
      72  A1    ---   u_SpI       [:?] Uncertainty flag on SpI
  74- 77  A4    ---     SpCl      Classification of the radio spectrum (2)
  80-101  A22   ---     CatName   Catalogue names for the different cluster
                                   sources or the cluster as a whole as taken
                                   from the available literature
 103-202  A100  ---     Ref       References (see ref3 file)
--------------------------------------------------------------------------------
Note (1): We have labelled each prominent source with a subnumber (A85.1 etc.),
           regardless of cluster membership, in increasing order of right
           ascension for each cluster area mapped. We have only labelled the
           most prominent sources.
          For sources appearing complex at 11.1cm (Paper I (1978A&AS...31...99H
           or II1979A&AS...36..237W), and being resolved by the present
           observation, we preserved the subnumbering already given to the
           source and distinguished the subcomponents by small letters
           following the subnumber (A407.4a etc.).
Note (2):   S: straight spectra
           C-: convex spectra
         Cmax: spectra showing a low-frequency cut-off
          C+l: concave spectra with low-frequency excess
          C+s: concave spectra with high-frequency excess
          CPX: complex spectra
--------------------------------------------------------------------------------

Byte-by-byte Description of file: r10700
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---     Source   Source name (1)
  11- 12  I2    h       RAh      ? Right ascension (B1950)
  14- 15  I2    min     RAm      ? Right ascension (B1950)
  17- 20  F4.1  s       RAs      ? Right ascension (B1950)
      23  A1    ---     DE-      Declination sign
  24- 25  I2    deg     DEd      ? Declination (B1950)
  27- 28  I2    arcmin  DEm      ? Declination (B1950)
  30- 31  I2    arcsec  DEs      ? Declination (B1950)
      32  A1    ---     NotePos  [a:] a: peak positions only, : uncertainty flag
      34  A1    ---   l_S10.7GHz  Limit flag on S10.7GHz
  35- 40  F6.1  mJy     S10.7GHz Flux density ar 10.7GHz (2.8cm)
  42- 45  F4.1  mJy   e_S10.7GHz ? rms uncertainty on S10.7GHz
      47  A1    ---   n_S10.7GHz  [bc] Note on S10.7GHz (2)
  49- 52  F4.2  mJy     rmsI     ? rms noise level at the maps area which
                                    - bona fide - do not contain radio sources
                                    (in mJy/beam area)
  54- 57  F4.1  mJy     rmsP     ? rms noise level in linearly polarized
                                    intensity (in mJy/beam area)
  61- 63  I3    deg     PA       ? Position angle of the major axis of
                                    extended sources
      64  A1    ---   u_PA       [:C?)] Uncertainty flag on PA (C=complex)
      66  A1    ---   l_MajAxis  Limit flag on MajAxis
  67- 70  F4.2  arcmin  MajAxis  ? Major axis half power width
      71  A1    ---   u_MajAxis  [:C] Uncertainty flag on MajAxis  (C=complex)
      73  A1    ---   l_MinAxis  Limit flag on MinAxis
  74- 77  F4.2  arcmin  MinAxis  ? Minor axis half power width
      78  A1    ---   u_MinAxis  [C] Uncertainty flag on MinAxis  (C=complex)
      79  A1    ---   l_m        Limit flag on m
  80- 83  F4.1  %       m        ? Integrated degree of linear polarization
      84  A1    ---   u_m        [:)] Uncertainty flag on m
  85- 86  I2    %     e_m        ? rms uncertainty on m
  88- 90  I3    deg     Xi       ? Weighted mean of the electric field vector
                                    position angle
  92- 93  I2    deg   e_Xi       ? rms uncertainty on Xi
      94  A1    ---   u_Xi       [)] Uncertainty flag on Xi
  95-124  A30   ---     Note     Note
--------------------------------------------------------------------------------
Note (1): We have labelled each prominent source with a subnumber (A85.1 etc.),
           regardless of cluster membership, in increasing order of right
           ascension for each cluster area mapped. We have only labelled the
           most prominent sources.
Note (2): b) includes contribution from surrounding emission feature
          c) possibly variable, flux at epoch 1979.7 was 180 mJy
--------------------------------------------------------------------------------

Byte-by-byte Description of file: ref*
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---     RefNo     Reference number
   5- 23  A19   ---     BibCode   Bibcode
  25- 87  A63   ---     Authors   List of the authors
--------------------------------------------------------------------------------

History: The data were supplied by Heinz Andernach (catalog A043 in his list).
    A few annex tables (clopt, clopx, ref4 and 5) were prepared
    via OCR at CDS.

Acknowledgements: It is a pleasure to thank Heinz Andernach
    who kindly supplied his data to CDS.

References:
  Caswell, 1966, Ph. D. Thesis, University of Cambridge
  Crowther, 1966, Ph. D. Thesis, University of Cambridge
  Foster, 1961, Ph. D. Thesis, University of Cambridge
  Mayer, 1980, Ph. D. Thesis, University of Cambridge
  Schallwich, 1982, Ph. D. Thesis, Bochum University
  Waldthausen, 1980, Ph. D. Thesis, Bonn University
================================================================================
(End)                     Patricia Bauer, Francois Ochsenbein [CDS]  28-Nov-1997