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\begin{document}
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\def\fonote#1{\footnote{#1}}
\def\tabcap#1#2{\smallskip\noindent{\bf Table\ts\ignorespaces #1\unskip.\ }
       \ignorespaces #2\vskip3mm}
%
\tabcap{1}{Observing log of Perseus galaxies}
\halign{#\hfill&\hfill#\hfill&\hfill#\hfill&\quad\hfill#&\quad\hfill#&\quad#\hfill\cr
\noalign{\medskip\hrule\medskip}
name  & run& filter& exp. time& seeing& notes\cr 
        & & & (min)& (arcsec)&\cr
\noalign{\medskip}
525-19   & dec94& V& 15& 1.7& \cr
525-29   & dec94& x& 15& 1.6& \cr
525-31   & feb95& V& 15& 1.5& \cr
525-6    & dec94& x& 15& 1.6& \cr
540-32   & feb95& V& 15& 1.3& \cr
540-33   & feb95& V& 15& 1.3& \cr
540-35   & dec94& V& 15& 1.6& \cr
540-36   & dec94& V& 15& 1.7& \cr
540-41   & feb95& V& 15& 1.6& \cr
540-42   & dec94& x& 15& 1.6& \cr
540-43   & dec94& x& 15& 1.6& \cr
540-45   & dec94& V& 15& 1.7& \cr
540-46   & sep89& r& 15& 1.3& archive, PIC, CCD=RCA1 F/10 pixel size=0.324 \cr
540-48   & feb95& V& 15& 1.2& \cr
540-51   & feb95& V& 15& 1.4& \cr
540-54   & dec94& x& 15& 1.5& \cr
540-56   & dec93& r& 20& 2.6& \cr
540-57   & feb95& V& 15& 1.3& \cr
540-59   & dec93& r& 20& 3.7& \cr
540-60   & dec94& x& 15& 1.6& \cr
540-62   & feb95& V& 15& 1.2& \cr
540-67   & dec93& r& 20& 2.6& \cr
540-68   & dec94& V& 15& 1.7& \cr
540-70   & dec94& x& 15& 1.6& \cr
540-73   & plate&  &   &    & OCA \#2977 \cr
540-74   & feb94& r& 20& 1.0& \cr
540-76   & feb94& r& 20& 1.2& \cr
540-80   & plate&  &   &    & OCA \#2977 \cr
540-81   & dec89& r& 10& 0.7& archive, CFH, CCD=RCA2 (see Paper I)\cr
540-82   & dec94& V& 15& 1.6& \cr
540-83   & plate&  &    &    & OCA \#2977 \cr
540-85   & feb95& V& 15& 1.3& \cr
540-85   & feb95& V& 15& 1.6& \cr
540-89   & feb95& V& 15& 1.4& \cr
540-97   & dec93& r& 20& 2.5& \cr
540-104  & plate&  &   &    & OCA \#2977 \cr
540-106  & feb95& V& 15& 1.5& \cr
540-114  & dec93& r& 20& 2.7& \cr
540-114  & plate&  &   &    & OCA \#2977 \cr
540-115  & dec94& V& 15& 1.5& \cr
541-3    & dec93& r&  2& 1.7& \cr
541-12   & dec93& r& 20& 1.8& \cr
541-14   & dec93& r& 20& 1.9& \cr
541-15S  & sep90& r& 30& 1.1& archive, PIC, CCD=Tho F/10 pixel size=0.2?\cr
541-16N  & feb95& V& 15& 1.4& \cr
541-16S  & feb95& V& 15& 1.4& \cr
541-112N & dec93& r& 20& 2.7& \cr
BGP41    & feb94& r& 15& 1.1& \cr
 T40     & feb95& V& 15& 1.4& \cr
 T40     & feb95& V& 15& 1.3& \cr
 T04     & dec93& r& 20& 1.8&  Not analyzed, bright star at 14"\cr
\noalign{\medskip\hrule\medskip}
}
\noindent
Notes : \hfill\break 
feb93: CCD Thompson 1024x1024, pixel size=0.24 \hfill\break
dec93: CCD Thompson 1024x1024, pixel size=0.48 (0.24 2x2 binned) \hfill\break
feb94: CCD Thompson 1024x1024, pixel size=0.24 (the observations
in the x filter were done with an unknown filter, because of
a mechanical fault). \hfill\break
dec94: CCD Tektronics 1024x1024, pixel size=0.30 \hfill\break
feb95: CCD Tektronics 1024x1024, pixel size=0.30 \hfill\break

\vfill\eject

\tabcap{2}{Galaxies classified as S from visual inspection of the plates 
OCA2842 and OCA2849 (all but two not presented in Paper I)}
% 
\halign{#&#&\quad#\hfill&\quad#\hfill&\quad#\hfill\cr
\noalign{\medskip\hrule\medskip}
GMP$_o$ & GMP$_a$ &       characteristics                 &other
observations     &notes\cr \noalign{\medskip}
0938 & 0315&   irr                     &run 10, S              &     \cr  
1353 & 0433&   asym                    &                       &dust, edge-on, uncertain type \cr
1367 & 0440&   irr, asym               &                       &                            \cr
1576 & 0507&   irr, asym               &run 9, S               &Irr\cr
1582 & 0510&   irr, asym, low SuBr     &                       &Irr\cr
2059 & 0686&   arms                    &run 7, S, GavIII, S    &\cr
2073 & 0689&   asym, irr               &                       &\cr
2347 & 0790&   irr, arms               &run 10, S              &\cr
2374 & 0804&   irr, arms               &GavI, S, GavIV, S      &beautiful S \cr
2431 & 0834&   irr?, spiP?             &                       &uncertain type, classified S by D80, BO \cr
2441 & 0837&   arms                    &GavI, S                &beautiful barred S                   \cr
2516 & 0867&   irr                     &run 9, SA0/a           &strange shape on plate \cr
2536 & 0875&   irr, asym               &                       &late type spiral or Irr                       \cr
2582 & 0892&   asym                    &                       &dust, no bulge \cr
2599 & 0897&   irr                     &                       &Irr          \cr
2640 & 0914&   asym, arms              &run 10, S              &\cr
2796 & 0978&   asym, irr               &                       &\cr
2834 & 1001&   irr                     &run 10, S              &outside the redshift limits\cr
3253 & 1193&   irr, asym               &                       &\cr
3271 & 1203&   asym                    &                       &\cr
3779 & 1420&   irr, asym               &GavIV, S               &\cr
4135 & 1555&   irr                     &GavIV, S               &Irr\cr
4159 & 1566&   irr, asym               &                       &Irr\cr
4192 & 1576&   arms                    &                       &\cr
4437 & 1675&   irr, asym               &GavIII, S              &\cr
4522 & 1711&   spiP                    &                       &beautiful barred S\cr
4597 & 1744&   spiP                    &                       &uncertain type, classified S by BO\cr
5643 & 2156&   irr                     &                       &Irr                            \cr
5678 & 2172&   irr, asym, spiP?        &                       &late type spiral\cr
5978 & 2275&   asym                    &                       &dust              \cr
\noalign{\medskip\hrule\medskip}
0983 & 0315&   asym \cr
2347 & 0790&   spiP  \cr
2834 & 1001&   irr, asym\cr
\noalign{\medskip\hrule\medskip}
1576 & 0507&   arms, irr&              march 94&               Irr, not in the published list\cr
1616 & 0518&   S in kp1608&    run 7, S&  not published in Paper I\cr
\noalign{\medskip\hrule\medskip}
}
\noindent
Notes:\hfill\break
BO= Butcher \& Oemler 1985\hfill\break
GavI= Gavazzi, Garilli \& Boselli 1990\hfill\break
GavIII= Gavazzi \& Randone 1994\hfill\break
GavIV= Gavazzi, Boselli \& Carrasco 1994\hfill\break
D80= Dressler 1980\hfill\break
kp1608= KPNO photographic plate (see Paper I)\hfill\break
run 7= CCD observations in March 1993 (see Paper I)\hfill\break

\tabcap{3} {Morphological description of spiral galaxies in Perseus}
\halign{#\hfill\ &#\hfill\ &#\hfill\ &#\hfill\ &#\hfill\ &#\hfill\ &#\hfill\ &#\hfill\ \cr
\noalign{\medskip\hrule\medskip}
 Name       & Palomar dig.        & OCA \#2977  & Notes OCA \#2977                  & CCD                         & Run n. \& Notes                  \cr
 %
\noalign{\medskip}
 Zw 525-6    &                     &          &                                & S                           & dec94                  \cr
 Zw 525-11   &                     & S        & very low SuBr                  &                             &                        \cr
 Zw 525-19   &                     &          &                                & (r)S barred                     & dec94                  \cr
 Zw 525-29   &                     &          &                                & S                           & dec94                  \cr
 Zw 525-31   &                     &          & too close to bright star & S                           & feb95                  \cr
 Zw 525-33   & Irr & & & & \cr
 Zw 525-39   & S & & & & \cr
 Zw 540-34   & S arms              &          &                                &                             &                        \cr
 Zw 540-35   &                     &          &                                & S                           & dec94                  \cr
 Zw 540-36   &                     &          &                                & S flocculent                & dec94                  \cr
 Zw 540-37   & S late              &          &                                &                             &                        \cr
 Zw 540-42   &                     &          &                                & S                           & dec94                  \cr
 Zw 540-43   &                     &          &                                & S asymm                     & dec94                  \cr
 Zw 540-45   &                     &          &                                & S                           & dec94                  \cr
 Zw 540-49   & S dust              & S        &                                &                             &                        \cr
 Zw 540-54   &                     &          &                                & S barred                        & dec94                  \cr
 Zw 540-58   & S irr               & Pec      & Interact                       &                             &                        \cr
 Zw 540-60   &                     &          &                                & 
S late                      & dec94                  \cr
 Zw 540-67   &                     &          &                                & Irr                         & dec93                  \cr
 Zw 540-68   &                     &          &                                & S                           & dec94                  \cr
 Zw 540-70   &                     & late type?&                                & S dusty                     & dec94                  \cr
 Zw 540-71   &                     & S        & low SuBr, asym                 &                             &                        \cr
 Zw 540-77   &                     & S        &                                &                             &                        \cr
 Zw 540-82   &                     &          &                                & S                           & dec94                  \cr
 Zw 540-84   &                     & Irr      &                                &                             &                        \cr
 Zw 540-90   & S late              & S        &                                &                             &                        \cr
 Zw 540-91   & S arms              & S        &                                &                             &                        \cr
 Zw 540-93   & S                   &          &                                &                             &                        \cr
 Zw 540-94   &                     & S        & low SuBr, elongated, -$>$dust   &                             &                        \cr
 Zw 540-97   &                     &          &                                & S two faint arms, bar, disk & dec93                  \cr
 Zw 540-106  & S                   & disk     & disk                           &                             & feb95                   \cr
 Zw 540-115  &                     &          & other galaxy at 6"             & S dusty                     & dec94                  \cr
 Zw 540-118  & S?                  & S        &                                &                             &                        \cr
 Zw 540-121  &                     & S        & disk, irr                      &                             &                        \cr
 Zw 541-3    & Irr    &          &                                &          Irr                   &  dec93, embedded ]\cr
& & & & & in the halo of ] \cr
& & & & & a bright star, \cr
 Zw 541-19   & S arms, HII reg.    &          &                                &                             & out of redshift ]\cr
& & & & & limits \cr
 Zw 541-112N &                     &          &                                & Pec (Interact?)              & dec93                  \cr\noalign{\medskip\hrule\medskip}
}

\vfill\eject


{\bf Description of Table 4 (Coma galaxies)}
\bigskip
  
\noindent (1) and (2) Number in the abridged and unabridged versions of the 
Godwin, Metcalf \& Peach (GMP) catalogue. 

\noindent (3) Number in Dressler's catalogue (Dressler 1980).

\noindent (4) Usual designation, such as NGC, IC (Dreyer 1888), and RB (Rood 
\& Baum 1967) numbers. 

\noindent (5) Asymptotic magnitude, in V (Johnson's system).
 
\noindent (6) Logarithm of the effective radius, in units of arcsec ($\log(r_e)$).
 
\noindent (7) Logarithm of the semi major axis of the effective isophote, in 
units of arcsec ($\log(l_e)$). 
 
\noindent (8) Mean SuBr inside the effective isophote, in V mag arcmin$^{-2}$. 
 
\noindent (9) Photometric evidence for a disk, coded as st (strong), cl (clear),
ft (faint), or no (none).
 
\noindent (10) Typical axis ratio, either its minimum value, if clearly defined,
or its value at the effective isophote otherwise.
 
\noindent (11) Location where the axis ratio was estimated, coded as ex (at its 
extremum), re (at the effective isophote), or co (if the value is the same at 
both locations).

\noindent (12) Typical $e_4$ parameter, either its extremum value, if clearly 
defined, or its value at the effective isophote otherwise. The estimates are 
in \%.  
 
\noindent (13) Location where the $e_4$ parameter was estimated, coded as ex 
(at its extremum), re (at the effective isophote), or co (if the value is the 
same at both locations). 

\noindent (14) Axis ratio in the envelope, i.e. at the isophote $\mu_V$ = 
24.85 mag arcsec$^{-2}$. 
 
\noindent (15) Amplitude of isophotal twist in the range of reliable 
measurements, in degrees. 

\noindent (16) Detection of a bar, coded as follows : bar (bar seen), bar? (bar 
suspected), -no (no bar seen). 
 
\noindent (17) Detection and classification of a disk, coded as follows: emDi 
(embedded disk), miDi (mixed disk), exDi (extended disk), -?Di (detected but 
unclassified disk), -no- (no disk seen). 
 
\noindent (18) Detection of a spiral pattern, coded as follows: spiP  (spiral 
pattern seen), spiP? (spiral pattern suspected), -no-  (no spiral pattern 
seen). 
 
\noindent (19) Classification of an envelope, coded as follows: spH 
(spheroidal halo), thD (thick disk), exD (extended disk), pec (peculiar 
envelope), -?- (unclassified envelope). 
 
\noindent (20) Our morphological classification, coded as follows: boE (boxy 
E), unE (undetermined E), diE (disky E), SA0, SAB0, SB0, Sa, etc., S... 
(spiral of unknown stage). 
 
\noindent (21) An asterisk refers to a note in Sect. 5 about specific features 
such as important dust pattern, ring or lens, low SuBr, $f_4$-asymmetry, etc., 
and about uncertainties of various sources. 
\smallskip 

Note that, when a parameter has not been measured, or when a specific 
morphological component has not been studied, the relevant code is replaced by 
a dash. 

\vfill\eject\


\tabcap{4}{Morphological description of early-type galaxies in Coma}
\halign{#\hfill\ &#\hfill\ \ &\hfill\ \ #&\hfill\ #&\quad\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&
\hfill\ #\ \hfill& \hfill\ #&\hfill\ #\ \hfill&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #\ &#\hfill\ &#\hfill\ \cr
\noalign{\medskip\hrule\medskip}
(1)& (2)& (3)& (4)& (5)& (6)& (7)& (8)& (9)& (10)& (11)& (12)& (13)& (14)& (15)& (16)& (17)& (18)& (19)& (20)& (21)\cr
0552 & 1715&  141& NGC 4927& 13.56& 0.93& 1.02& 11.31& no& 0.70& co& 1.2& co& 0.73&  3& -no & miDi& -no-&  thD& diE  &* \cr    
0607 & 1853&  190&      & --.--& -.--& -.--& --.--& st& 0.26& ex& 8.0& ex& 0.29&  2& -no & miDi& -no-&  thD& SA0  &* \cr 
0718 & 2157&   79& NGC 4919& 13.73& 0.71& 0.80& 10.39& st& 0.72& re& 2.2& ex& 0.49&  4& -no & -?Di& -no-&  pec& SA0  &* \cr
0750R& 2237&   80&      & 14.63& 0.55& 0.65& 10.47& st& 0.59& ex& 3.0& co& 0.99&  2& -no & emDi& -no-&  spH& SA0  &* \cr
0750 & 2237&   80&      & 15.06& 0.55& 0.65& 10.91& st& 0.59& ex&  3.0& co& 0.92& 30& -no & emDi& -no-&  spH& SA0  &* \cr
0754 & 2259&  229&      & 15.01& 0.59& 0.64& 11.03& no& 0.80& re& 1.8& co& 0.71& 10& -no & miDi& -no-&  exD& diE  &* \cr
0828 & 2417&  167& NGC 4908& 13.77& 0.70& 0.78& 10.39& ft& 0.67& ex& -0.8& ex& 0.65&  8& -no & -no-& -no-&  -?-& unE  &* \cr
0857 & 2495&  231&      & 14.55& 0.42& 0.54&  9.73& cl& 0.50& ex& 4.0& ex& 0.60&  0& -no & miDi& -no-&  spH& SA0  &  \cr
0908 & 2629&  232& NGC 4896& 13.77& 0.87& 1.00& 11.20& ft& 0.52& ex& 0.0& re& 0.55&  3& -no & -no-& -no-&  -?-& unE  &* \cr
0924 & 2670&   27&      & 15.26& 0.51& 0.57& 10.90& ft& 0.80&  ex& 1.6& ex& 0.82&  3& -no & -?Di& -no-&  -?-& diE  &  \cr
0967 & 2776&   39&      & 14.91& 0.54& 0.58& 10.73& no& 0.78&  ex& 0.0& co& 0.78&  2& -no & -no-& -no-&  -?-& unE  &* \cr
1109 & 3073&  175& NGC 4883& 14.24& 0.61& 0.64& 10.44& cl& 0.71& ex& -1.0& re& 0.82& 45& bar & -?Di& -no-&  -?-& SB0  &* \cr
1154 & 3165&   57&      & 13.85& 0.65& 0.81& 10.22& st& 0.25&  ex& 8.0& ex& 0.34&  4& -no & emDi& -no-&  spH& SA0  &* \cr
1232 & 3328&  242&      & 15.01& 0.36& 0.44&  9.91& cl& 0.50&  ex& 2.5& ex& 0.52&  2& -no & miDi& -no-&  thD& SA0  &  \cr
1432 & 3818&  218&      & 14.18& 0.60& 0.70& 10.26& no& 0.45&  ex& 2.5& co& 0.45& 11& -no & -?Di& spiP&  exD& S..  &* \cr
1560 & 4147&     &      & 14.27& 0.64& 0.74& 10.59& st& 0.50&  ex& 3.2& co& 0.61&  1& -no & emDi& -no-&  spH& SA0  &  \cr
1564 & 4156&   43& NGC 4853& 13.49& 0.54& 0.58&  9.29& st& 0.78&  ex& 0.0& re& 0.82& 10& -no & -no-& -no-&  -?-& SAB0p&* \cr
1594 & 4230&  161& RB 241& 13.98& 0.76& 0.80& 10.89& no& 0.87& co& -0.8& co& 0.91& 20& -no & -no-& -no-&  -?-& boE  &* \cr
1625 & 4315&  137& NGC 4850& 14.23& 0.58& 0.65& 10.24& cl& 0.74& co& 3.1& co& 0.93& 30& bar & -?Di& -no-&  -?-& SB0  &* \cr
1844 & 4849&  211&      & 14.31& 0.78& 1.01& 11.30& st& 0.31&  ex& 7.1& co& 0.44&  5& -no & emDi& -no-&  spH& SA0  &* \cr
1852 & 4866&  212&      & 14.88& 0.67& 0.77& 11.32& cl& 0.50&  ex& 1.4& co& 0.56& 12& bar?& -?Di& -no-&  thD& SAB0 &* \cr
1925 & 5038&   16&      & 15.11& 0.67& 0.73& 11.54& cl& 0.72&  co& 4.1& co& 0.89& 60& -no & emDi& -no-&  pec& SA0  &* \cr
2047 & 5341&  221&      & 14.98& 0.47& 0.55& 10.44& cl& 0.64&  ex& 4.9& co& 0.95& 74& bar & -?Di& -no-&  -?-& SB0  &  \cr
2085 & 5428&     &      & 14.46& 0.64& 0.66& 10.74& no& 0.91&  co& -0.8& co& 0.90&  9& -no & -no-& -no-&  -?-& boE  &* \cr
2109 & 5495&     &      & 14.51& 0.47& 0.51&  9.94& no& 0.79&  ex& 1.0& ex& 0.88& 15& -no & -?Di& -no-&  -?-& unE  &* \cr
2134 & 5568&     & NGC 4816& 12.66& 1.40& 1.44& 12.74& no& 0.79& re& -1.0& ex& 0.74& 20& -no & -no-& -no-&  -?-& boEp &* \cr 
2220 & 5799&     &      & 15.14& 0.38& 0.44& 10.13& cl& 0.69&  ex& 2.9& co& 0.81& 30& bar & -?Di& -no-&  -?-& SB0  &  \cr
2283 & 5999&     &      & 14.03& 1.00& 1.09& 12.13& no& 0.78&  ex& 0.0& co& 0.80&  0& -no & -no-& -no-&  -?-& unE  &* \cr
\noalign{\medskip\hrule\medskip}
}

\vfill\eject\

{\bf Notes to Table 4 (Coma galaxies)}
\bigskip


\noindent {\bf 0552}: dust along the major axis. Type given in Paper I 
confirmed. 
  
\noindent {\bf 0718}: two bumps on the major axis profile. Inner ring and lens.
Type given in Paper I confirmed.
 
\noindent {\bf 0750R}: image of run 9 (see Paper I).
 
\noindent {\bf 0750}: 30 degree twist at r $\sim 10$ arcsec on the V image. 
same twist in R, but image not deep enough for full confirmation. Type given in 
Paper I confirmed. 
 
\noindent {\bf 0754}: type given in Paper I fully confirmed.
 
\noindent {\bf 0828}: E boxy outside $r_e$ and possibly disky inside. In Paper 
I it is classified diE because the boxiness of the outer region is not 
detected with certainty, partly because of the presence of a companion galaxy 
at 15 arcsec in the minor axis direction. 
 
\noindent {\bf 0857}: the bar suspected in Paper I is not detected in our 
better images. 
 
\noindent {\bf 0908}: slightly boxy isophotes out to $r_e$, then slightly 
disky isophotes. Uncertain detailed classification. 
 
\noindent {\bf 0967}: focus problems made the PSF slightly elongated in the NS 
direction and galaxy data inside 3 arcsec not usable. 
 
\noindent {\bf 1109}: the bar suspected in Paper I is detected.
 
\noindent {\bf 1154}: asymmetric with respect to its major axis.
 
\noindent {\bf 1432}: classified SA0/a by morphologists, probably because of 
the low contrast spiP. 
 
\noindent {\bf 1564}: ellipticity and $e_4$ profile unusual for a lenticular 
galaxy. It seems to be asymmetric. 
 
\noindent {\bf 1594}: the better data with respect to Paper I allow us to 
classify it elliptical. 
 
\noindent {\bf 1625}: the bar suspected in Paper I is detected.
 
\noindent {\bf 1844}: isophote twist toward GMP 1852. Type given in Paper I 
confirmed. 
 
\noindent {\bf 1852}: isophote twist opposite to GMP 1844, bar suspected but 
nearby star slightly elongated in the same direction. Type given in Paper I 
confirmed. 
 
\noindent {\bf 1925}: large isophote twist at low SuBr.
 
\noindent {\bf 2085}: rich in globular clusters\fonote{The expression 
``globular cluster" here and hereafter does not imply a group of dynamically 
bound stars, but a clump of light.}. The better data with respect to Paper I  
allow us to classify it elliptical. 
 
\noindent {\bf 2109}: focus problems made the PSF slightly elongated in a 
direction orthogonal to the galaxy major axis. Data inside 4 arcsec are not 
usable. Also classified unE with CFH data of Paper I. 
 
\noindent {\bf 2134}: rich in globular clusters. Its intensity profile obeys 
the $r^{-1.44}$ law from 1 arcsec out to 60 arcsec, putting this galaxy in the 
D class following Schombert (1987) and Tonry (1987). Classified as unE in 
Paper I from a slightly shallower image. 

\noindent {\bf 2283}: the analysis is made difficult by the crowded field and a 
nearby saturated star.


\vfill\eject

{\bf Description of Table 5 (Perseus galaxies)}
\bigskip


\noindent (1) Zwicky name.
 
\noindent (2) Usual designation, such as NGC, UGC (Nilson 1976), T (Tiff 1976), 
BGP (Bucknell, Godwin \& Peach 1979)
and CR (Chincarini and Rood 1977) numbers. 
 
\noindent (3) Flag for filter or observational material. 
 
\noindent (4) Asymptotic magnitude.
 
\noindent (5) Logarithm of the effective radius, in units of arcsec.
 
\noindent (6) Logarithm of the semi major axis of the effective isophote, in 
units of arcsec. 

\noindent (7)  Mean SuBr inside the effective isophote, in mag arcmin$^{-2}$.

\noindent (8) to (12) Same as columns (9) to (13) of Table 4.

\noindent (13) Axis ratio in the envelope, i.e. at the isophote V=24.85 or R=24 
mag arcsec$^{-2}$.
 
\noindent (14) to (20) Same as columns (15) to (21) of Table 4.
\smallskip 

Note that a ``(1)" in the table means that the parameter has not been computed 
because the night was not photometric, or because of the pan-chromaticity of 
the plate. 

\tabcap{5}{Morphological description of early-type galaxies in Perseus}
\halign{#\hfill\ &#\hfill\ \ &\hfill\ \ #&\quad\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&
\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #&\hfill\ #\ &#\hfill\ &#\hfill\ \cr
\noalign{\medskip\hrule\medskip}
(1)& (2)& (3)& (4)& (5)& (6)& (7)& (8)& (9)& (10)& (11)& (12)& (13)& (14)& (15)& (16)& (17)& (18)& (19)& (20)\cr
\noalign{\medskip}
540-32& NGC 1175&  V        &  13.81& 0.90& 0.92& 11.41& no& 0.92& ex& -0.8& ex& 0.92:& 15:& -no& -no-& -no-& -no& boE& *\cr
540-33& NGC 1177&  V        &  12.52& 1.04& 1.19& 10.79& st& 0.27& ex& -7.2& co& 0.30:&   0& -no& emDi& -no-& thD& SA0& *\cr
540-41&      & V         &  14.28& 0.86& 0.94& 11.66& st& 0.62& co&  5.3& co&   1.0&  20& bar& emDi& -no-& spH& SB0& *\cr
540-46& UGC 2559& R        &    (1)& 0.95& 1.03&   (1)& st& 0.39& ex&  5.0& ex&   (1)&  10& bar& -?Di& -no-&  -?-& SB0& *\cr
540-48&      & V         &  14.41& 0.56& 0.66& 10.31& st& 0.52& ex&  3.0& ex&  0.63&   9& -no& miDi& -no-& thD& SA0& \cr
540-51&      & V        &  14.10& 0.77& 0.83& 11.06& st& 0.58& ex&  0.0& re&  0.65&  25& bar& -?Di& -no-& thD& SB0& \cr
540-56&      & R        &    (1)&   --&   --&   (1)& st& 0.39& ex&  7.0& ex&   (1)&   3& -no& miDi& -no-& thD& SA0& \cr
540-57&      & V         &  13.55& 0.78& 0.84& 10.54& no& 0.62& ex& -2.0& ex&  0.70&  10& -no& -no-& -no-&  -?-& boE& *\cr
540-59&      & R        &    (1)& 0.72& 0.78&   (1)& st& 0.46& ex&  5.6& ex&   (1)&  12& bar& -?Di& -no-& thD& SB0& \cr
540-62&      & V         &  13.40& 0.74& 0.82& 10.22& no& 0.67& ex& -1.0& co& 0.76:&   0& -no& -no-& -no-&  spH& boE& \cr
540-73&  CR 6 & plate    &    (1)&  -- & --  &   (1)&   &     &  &      & &    &&   &     &     &    & SA0& *\cr
540-74& BGP 37& R        &    (1)& 0.75& 0.80&   (1)& st& 0.75& co&    0& co&   (1)&   3& -no&   --& -no-& thD& SA0& *\cr
540-74& BGP 37& plate    &    (1)& 0.76& 0.83&   (1)& ft& 0.85& co&    0& co&   (1)&  10& -no&   --& -no-& -?-& SA0& *\cr
540-76&      & R        &       &     &     &      &   &     &    &    &   &      &    &    &     &     &    & SA0& *\cr
540-80&      & plate    &  14.38& 0.81& 0.89& 11.55& st& 0.75& ex&    0& co&  0.75&  25& bar& -?Di& -no-&  -?-& SB0& \cr
540-81&      & R        &       &     &     &       &   &    &  &       & &    && &       &   &      & SA0& *\cr
540-83& BGP 34& plate    &    (1)&  -- & --  &   (1)& cl& 0.23& ex&  9.0& ex&   (1)&   0& -no& emDi& -no-& thD& SA0& \cr
540-85& CR 15 & 2 V images &  13.91& 0.68& 0.73& 10.40& no& 0.72& co&  0.3& co&  0.76&   3& -no& -no-& -no-&  -?-& diE& \cr
540-89& CR 22 & V        &  14.06& 0.88& 1.03& 11.54& cl& 0.42& ex&  3.0& ex&    --&  15& -no&   --& -no-&  -?-& SA0& *\cr
540-106&     & V         &  14.24& 0.58& 0.73& 10.25& st& 0.32& ex&  6.1& ex&    --&  10& -no& emDi& spiP&  -?-& S  & *\cr
540-114&     & R        &    (1)&   --&   --&   (1)& st& 0.31& ex&  8.3& ex&   (1)&   0& -no& miDi& -no-& thD& SA0& *\cr
540-114&     &plate     &    (1)& 0.72& 0.88&   (1)& st& 0.35& ex&  6.9& ex&   (1)&   0& -no& miDi& -no-& exD& SA0& *\cr
541-12&      & R        &    (1)& 0.71& 0.86&   (1)& st& 0.31& ex&  8.1& ex&   (1)&   2& -no& emDi& -no-& spH& SA0& \cr
541-14&      & R        &    (1)& 0.93& 1.04&   (1)& st& 0.56& ex&  5.2& ex&   (1)&  25& bar& -?Di& -no-& spH& SB0& \cr
541-15S& UGC 2755&  V       &    (1)& 0.97& 0.99&   (1)& ft& 0.75& ex&  2.0& ex&   (1)&  60& bar& -?Di& -no-&  -?-& SB0& *\cr
541-16N &     & V        &  14.19& 0.90& 1.08& 11.79& cl& 0.42& ex&  0.5& ex&    --&   3& -no& miDi& -no-& thD& SA0& *\cr
541-16S&      & V        &  14.10& 0.60& 0.62& 10.19& no& 0.75& ex& -1.8& co&   --&   40& bar& -?Di& -no-&  -?-& SB0& *\cr
       & BGP 41& R       &    (1)& 0.74& 0.81&   (1)& cl& 0.70& ex&  2.0& ex&   (1)&  12& bar& -?Di& -no-& spH& SB0& \cr
       & T 40  & 2 V images&  14.31& 0.75& 0.80& 11.17& st& 0.78& ex&  1.7& co&  0.86&   5& -no& emDi& -no-& spH& SA0& \cr
\noalign{\medskip\hrule\medskip}
}


\vfill\eject\
{\bf Notes to Table 5 (Perseus galaxies)}
\bigskip


\noindent {\bf T40}: the identification of Tiff 40 is doubtful. The observed 
galaxy is the nearest one to the Tiff 40 coordinates. A brighter (spiral) 
galaxy is 4 arcmin SE, which is more likely Tiff 40, if we believe Kent \& 
Sargent's (1983) classification (S). 

\noindent {\bf 540-32}: companion of NGC 1177, roundish.
 
\noindent {\bf 540-33}: peanut shaped SA0.
 
\noindent {\bf 540-41}: face on.
 
\noindent {\bf 540-46}: the small field of view did not allow us to image the 
whole envelope. 
 
\noindent {\bf 540-57}: there is a bump on the major axis SuBr profile at V=23 
mag arcsec$^2$. 
 
\noindent {\bf 540-73}: this galaxy is 19 arcsec from a very bright star, 
preventing the detailed structural analysis. However, bulge and disk are 
clearly visually detected as a change of axis ratio and as a bump on the major 
axis profile, leading to our estimated type.  The galaxy is edge-on. 
 
\noindent {\bf 540-74}: our morphological type fully confirms that of Poulain, 
Nieto \& Davoust (1992). 

\noindent {\bf 540-76}: strong, but smooth, dust lane on major axis. A second 
faint dust lane is present with an inclination of about 10 degrees with 
respect to the galaxy major axis 10 arcsec Southward. 
 
\noindent {\bf 540-81}: dust just in the inner part of this galaxy observed 
near the CCD's edge. 
 
\noindent {\bf 540-89}: a very brigh star 20 arcsec from the galaxy center 
perturbs the isophotal analysis at that radius. $e_4$ never dominates the 
Fourier terms, $f_4$ asymmetry. 
 
\noindent {\bf 540-106}: almost edge-on, a bit S-shaped, asymmetric.
 
\noindent {\bf 540-114}: the c/a profile starts to rise at fainter SuBr than 
sampled by plate, thus explaining the difference in the envelope 
classification. 
 
\noindent {\bf 541-15S}: face on.

\noindent {\bf 541-16N}: the galaxy Zw 540-16S and nearby stars prevented us 
from measuring the shape of this galaxy's envelope. 

\noindent {\bf 541-16S}: the galaxy 540-16N makes it impossible to measure the 
SuBr profile at $r>12$ arcsec. 


\vfill\eject\

%\bye

\end{document}




