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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
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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
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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