Access to Astronomical Catalogues

J/A+AS/145/263      Kinematical data on early-type galaxies. V. (Simien+, 2000)
Kinematical data on early-type galaxies. V.
    Simien F., Prugniel P.
      <Astron. Astrophys. Suppl. Ser. 145, 263 (2000)>
      =2000A&AS..145..263S      (SIMBAD/NED BibCode)
ADC_Keywords: Radial velocities ; Galaxies, rotation ; Velocity dispersion

Keywords: galaxies: elliptical & lenticular, cD -
          galaxies: kinematics and dynamics - galaxies: fundamental parameters -
          galaxies: general

Abstract:
    We present kinematical data for a sample of 26 galaxies. Rotation
    curves and velocity-dispersion profiles are determined for all
    objects. This is our fifth paper in a series devoted to the
    presentation of data on elliptical and S0 galaxies, derived from
    long-slit absorption spectroscopy; the series now gathers 119 galaxies
    with homogeneous data.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table1.dat        94       26   Catalog elements and kinematical results
table2.dat        35       29   Log of the observations
table3.dat        37      548   Profiles of velocity dispersion and rotation


See also:
 J/A+AS/122/521 : Kinematical data on early-type galaxies. I. (Simien+ 1997)
 J/A+AS/126/15  : Kinematical data on early-type galaxies. II. (Simien+ 1997)
 J/A+AS/126/519 : Kinematical data on early-type galaxies. III. (Simien+ 1997)
 J/A+AS/131/287 : Kinematical data on early-type galaxies. IV. (Simien+ 1998)
 J/A+A/360/439  : Stellar and ionized gas kinematics in NGC 4672 (Sarzi+, 2000)
 J/A+A/374/394  : Gas and stars kinematics in disc galaxies (Vega Beltran+ 2001)
 J/A+AS/105/433 : Kinematical data of 14 early-type galaxies (Longo+ 1994)
 J/A+AS/133/317 : Stellar kinematics in spiral galaxies (Heraudeau+ 1998)
 J/A+AS/136/509 : Stellar kinematics in spiral galaxies. II. (Heraudeau+ 1999)
 J/A+AS/131/105 : NGC 6221 ionized gas kinematics (Vega Beltran+ 1998)
 J/A+AS/127/117 : Kinematics of galaxies (Prugniel+ 1998)
 J/A+A/382/488  : Stellar and ionized gas kinematics in NGC 2855 (Corsini+ 2002)


Byte-by-byte Description of file: table1.dat

   Bytes Format  Units   Label    Explanations

   1-  9  A9     ---     Name     ! Object identification
  11- 12  I2     ---     Mtype    ! Morphological type
  14- 15  I2     h       RAh      ! Right Ascension 1950 (hours)
  17- 18  I2     min     RAm      ! Right Ascension 1950 (minutes)
  20- 23  F4.1   s       RAs      ! Right Ascension 1950 (seconds)
      25  A1     -       DE-      ! Declination 1950 (sign)
  26- 27  I2     deg     DEd      ! Declination 1950 (degrees)
  29- 30  I2     arcmin  DEm      ! Declination 1950 (minutes)
  32- 33  I2     arcsec  DEs      ! Declination 1950 (seconds)
  35- 39  F5.2   mag     Bt       ! Integrated blue magnitude
  40- 45  F6.2   mag     BMag    *! -M_B_, B-band absolute magnitude
  47- 51  F5.1   arcsec  Radeff   ?=999.9 Effective radius
  53- 56  F4.2   ---     Eps      ! Ellipticity
  58- 60  I3     deg     PA      *?=999 Position angle of slit
      62  I1     ---     r_PA    *! Reference for PA
  64- 68  I5     km/s    HRV      ?=99999 Heliocentric radial velocity
      69  A1     ---     u_HRV    Uncertainty flag on Vhel
  70- 72  I3     km/s    e_HRV    ?=999 Mean error on Vhel
  74- 76  I3     km/s    sig0     ?=999 Central velocity dispersion
      77  A1     ---     u_sig0  *Uncertainty flag on sig0
  78- 80  I3     km/s    e_sig0   ?=999 Mean error on sig0
      82  A1     ---     l_Vmax   Upper- or lower-limit flag on Vmax
  83- 85  I3     km/s    Vmax     ?=999 Maximum rotational velocity
      86  A1     ---     u_Vmax   Uncertainty flag on Vmax
  88- 90  I3     km/s    e_Vmax   ?=999 Mean error on Vmax
  92- 94  I3     arcsec  rmax     ?=999 radius: Vmax is measured in [-rmax,rmax]

Note on PA:
    PA (North --> East) as given in the range [0, 180[ by the LEDA database
    (status: 17 January 2000).
Note on BMag:
    for H0=75 km/s/Mpc
Note on r_PA:
   1 = Djorgovski (1985, PhD thesis. Univ. of California, Berkeley)
   2 = LEDA, http://www-obs.univ-lyon1.fr/base/
   3 = this work, from DSS images (acknowledgements in printed version of paper)
Note on u_sig0:
    Uncertainty due to bad seeing conditions.


Byte-by-byte Description of file: table2.dat

   Bytes Format  Units     Label      Explanations

   1-  9  A9     ---       Name       ! Object identification
  11- 18  A8    "DD/MM/YY" Date       ! Date of observation
      20  I1     ---       Setup     *! Spectrograph setup
  22- 24  I3     deg       PA        *! Position angle of slit
      26  I1     ---       Nexp       ! Number of exposures
  28- 30  I3     min       Texp       ! Exposure time
  32- 34  F3.1   arcsec    Seeing     ?=9.9 Seeing FWHM
      35  A1     ---       u_Seeing   Uncertainty flag on Seeing

Note on Setup:
    Setup=1 corresponds to a dispersion of 66 Angtroems per mm
    Setup=2 corresponds to a dispersion of 33 Angtroems per mm
Note on PA:
    PA (North --> East) is in the range [0, 360[, and with the following
    convention on the subsequent radius r in the profiles (Table 3):
    - for 0<PA<180, r<0 corresponds to the eastern side of the galaxy,
    - for 180<PA<360, r<0 corresponds to the western side,
    - and for PA=0, r<0 is to the North.


Byte-by-byte Description of file: table3.dat

   Bytes Format  Units   Label     Explanations

   1-  9  A9     ---     Name      ! Object identification
  11- 13  I3     deg     PA       *! Position angle of slit
  15- 20  F6.1   arcsec  r        *! Radius (<0 and >0 on opposite semi-axes)
  22- 25  I4     km/s    Vrot     *?=999 Proj. mean stellar rotation velocity
  27- 29  I3     km/s    e_Vrot    ?=999 Mean error on V
  31- 33  I3     km/s    sigma    *?=999 Projected velocity dispersion
  35- 37  I3     km/s    e_sigma   ?=999 Mean error on sigma

Note on Vrot and sigma:
    Rotation and dispersion velocities are projected along the line of sight;
    rotation values are with respect to the point r=0.
Note on PA and r:
    PA (North --> East) is in the range [0, 360[, and with the following
    convention:
    - for 0<PA<180, r<0 corresponds to the eastern side of the galaxy,
    - for 180<PA<360, r<0 corresponds to the western side,
    - and for PA=0, r<0 is to the North.


Acknowledgements: Francois SIMIEN 

(End)                                         Patricia Bauer [CDS]   22-Jun-2000