J/A+AS/139/141      Galaxies in the Perseus Cluster   (Brunzendorf+, 1999)

The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types Brunzendorf J., Meusinger H. <Astron. Astrophys. Suppl. Ser. 139, 141 (1999)> =1999A&AS..139..141B 1999A&AS..139..141B
ADC_Keywords: Clusters, galaxy ; Magnitudes ; Radial velocities ; Morphology Keywords: galaxies: clusters: individual: A 426 - galaxies: fundamental parameters - galaxies: luminosity function Description: A new catalogue of 660 galaxies within a field of about 10 square degrees in the Perseus cluster region is presented. The catalogue contains accurate positions, isophotal magnitudes, angular radii, position angles, radial velocities, morphological types, and detailed informations on morphological peculiarities. If available, cross identifications and radial velocities are also given. The catalogue is estimated to be complete to a 25mag isophotal B magnitude of about 18. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 122 660 galaxies in A426 -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Sequence Running number in this catalogue 6- 20 A15 --- Names Common names 23- 23 I1 h RAh Right ascension (J2000) 25- 26 I2 min RAm Right ascension (J2000) 28- 32 F5.2 s RAs Right ascension (J2000) 34 A1 --- DE- Declination (sign) 35- 36 I2 deg DEd Declination (J2000) 38- 39 I2 arcmin DEm Declination (J2000) 41- 44 F4.1 arcsec DEs Declination (J2000) 47- 50 F4.1 mag Mag25 *Apparent B magnitude within B25 mag/arcsec2 isophote 51 A1 --- u_Mag25 *Uncertainty flag for Mag25 54- 57 F4.1 mag SuBr *Central B surface brightness 58 A1 --- u_SuBr *Uncertainty flag for SuBr 61- 62 I2 arcsec a25 Major axis of the B25 mag/arcsec2 isophote 65- 66 I2 arcsec b25 Minor axis of the B25 mag/arcsec2 isophote 69- 71 I3 deg PA Position angle, North to East 74 I1 --- REM *[1/2]? Remark number about size or photometry 77- 81 I5 km/s HRV ? Heliocentric radial velocity 84- 95 A12 --- Mtype Morphological Type 98-122 A25 --- n_Mtype *Note on morphology and/or environment -------------------------------------------------------------------------------- Note on Mag25, SuBr: Without corrections for Galactic foreground extinction and inclination. Note on u_Mag25, u_SuBr: Typical uncertainties of Mag25 are 0.1 to 0.2 mag. Larger uncertainties due to difficulties in the removal of foreground stars are marked by a colon Note on REM: 1: a25, b25, PA are difficult to estimate for the individual components of this merger system 2: Mag25, a25, b25, PA are related to the central knot; the outer ring has a radius of 27 arcsec Note on n_Mtype: The following symbols are used: IN: systems with signs of strong interaction in the form of bridges (br) and/or tails (ta) DIS: systems with signs of distortions, which can show one or several of the following features coded by a number: (1) peculiar spiral arms (2) three-armed spirals (3) M51 type (4) unusual dust absorption (5) elliptical galaxy with isophote twist (6) non-concentric core (7) loops/shells (8) jet-like structures (9) fuzzy structure in the outer regions (10) radial spikes CH(n): n systems (n>1) within a common halo PL: polar ring galaxies or related objects f*: estimation of morphology hampered by a nearby foreground star The strength of the morphological peculiarity is indicated (+ for strong, - for weak). -------------------------------------------------------------------------------- Acknowledgements: Helmut Meusinger
(End) Helmut Meusinger [TLS Tautenburg] 19-Jul-1999
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line