VII/180   Galaxies in Fornax Cluster and five nearby groups  (Ferguson+ 1990)

Population studies in groups and clusters of galaxies. II. A catalog of galaxies in the central 3.5 degs of the Fornax Cluster Ferguson H.C. <Astron. J., 98, 367 (1989)> =1989AJ.....98..367F 1989AJ.....98..367F Population Studies in Groups and Clusters of Galaxies. III. A Catalog of Galaxies in Five Nearby Groups Ferguson H.C., Sandage A. <Astron. J., 100, 1 (1990)> =1990AJ....100....1F 1990AJ....100....1F
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs Description: This catalog represents the combination of results published in two papers: Ferguson, H.C. 1989 A.J. 98, 367 (Paper II) and Ferguson, H.C. and Sandage, A. 1990 A.J. 100, 1 (Paper III). See the Historical Notes section below. Please note that the data from Paper II were previously archived as catalog VII/160. This catalog supersedes that earlier dataset. The following paragraphs describe the data included from the two papers. (Paper II) This paper presents a catalog of 2678 galaxies within an area of nearly 40 deg2 centered on the Fornax Cluster at α=3h35m and δ=-35.7deg. The data have been obtained from visual inspection of 26 deep large-scale (10.9arcsec/mm) plates taken with the du Pont 2.5m reflector at the Las Campanas Observatory, and from digital photometry of an ESO/SRC blue survey plate covering roughly the same area of the sky. The catalog is essentially diameter limited, with a limiting diameter of 17arcsec at an isophoto of BT =26.5. Within this survey region, the catalog includes 340 likely cluster members and 2338 likely background galaxies. For cluster members, this listing should be complete to BT=18 (corresponding to MBT=13.0, assuming a distance modulus of m-M=31.9) and contains likely members down to BT=20. Cluster membership is for the most part based on galaxy morphology. By virtue of their low surface brightness, dwarf galaxies in the cluster can be distinguished with a high degree of certainty from background galaxies. Radial velocities are included for 89 galaxies in the survey, providing a reliable indicator of membership in these cases. As additional support for our rejection of background galaxies, we model the spatial distribution of various types of galaxies as the sum of a King model cluster component superimposed on a uniform background. Using maximum-likelyhood fits to these spatial distributions, we find a core radius of 0.7deg. for a King model fit to the cluster, and show that there are few, if any, cluster members contained in the sample of background galaxiesBD (Paper III) Five nearby groups of galaxies have been surveyed using large-scale plates from the 2.5 m duPont Telescope at Las Campanas Observatory. Catalogs of galaxies brighter than BT ∼ 20 are presented for the Leo, Dorado, NGC 1400, NGC 5044, and Antlia groups. A total of 1044 galaxies are included, from visual inspection of 14 plates, covering 31deg square. Galaxies have been classified in the extended Hubble system, and group memberships have been assigned based on velocity (where available) and morphology. About half the galaxies listed are likely members of one of the nearby groups. The catalogs are complete to BT ∼ 18, although the completeness limits vary slightly from group to group. Based on King model fits to the surface density profiles, the core radii of the groups range from 0.3 to 1 Mpc, and central densities range from 120 to 1900 galaxies Mpc-3 brighter than MBT = -12.5. Dynamical analysis indicates that all of the groups of likely to be gravitationally bound. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file p2tbl2.dat 132 340 Likely Fornax Cluster members p2tbl3.dat 79 2338 Possible members and likely background galaxies notes.dat 35 122 Notes to Table 3 (="p2tbl3") p3tbl2.dat 148 52 Galaxy catalogue in Leo group p3tbl3.dat 148 79 Galaxy catalogue in Dorado group p3tbl4.dat 148 120 Galaxy catalogue in NGC1400 group p3tbl5.dat 148 162 Galaxy catalogue in NGC5044 group p3tbl6.dat 148 375 Galaxy catalogue in Antlia group -------------------------------------------------------------------------------- Byte-by-byte Description of file: p2tbl2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- FCC [1,340]+ Fornax Cluster Catalog number 6- 7 I2 h RAh [3] right ascension (hours) (B1950) 9- 10 I2 min RAm [09,51]+= right ascension (minutes) 12- 15 F4.1 s RAs [0,60] right ascension (seconds) 17 A1 --- DE- [-] declination sign 18- 19 I2 deg DEd declination (degrees) (B1950) 21- 22 I2 arcmin DEm declination (minutes) 24- 25 I2 arcsec DEs [0,60] declination (seconds) 27 I1 --- Mem [1/6] membership status of the galaxy (G1) 29- 53 A25 --- MType ! morphological type 55- 58 F4.1 mag BTmag total blue apparent magnitude 60- 64 F5.1 arcsec Reff [0,]? effective radius (arcsec) 66- 69 F4.2 [0.1arcmin] logD decimal logarithm of the diameter in units of 0.1arcmin at an isophoto 71- 72 I2 --- r_Reff Source of coordinates, magnitudes, and effective radii. (G2) 74- 78 I5 km/s Vhel ? heliocentric velocity (km/s) 80- 83 I4 km/s e_Vhel ? uncertainty of the velocity (km/s) 86 I1 --- r_Vhel *[1/3]? source of the velocity 89 I1 --- Note [1/5]? additional notes on individual galaxies listed in the paper 91-122 A32 --- Names names of the galaxy (up to 4) 124-132 A9 --- IAU [ 0-9±] IAU coordinate designation -------------------------------------------------------------------------------- Note on r_Vhel: 1 = Richter and Sadler (1985A&AS...59..433R 1985A&AS...59..433R), 2 = Jones and Jones (1980MNRAS.191..685J 1980MNRAS.191..685J), 3 = Lauberts (1982, Cat. VII/34) -------------------------------------------------------------------------------- Byte-by-byte Description of file: p2tbl3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- bgGal [B] prefix of Fornax Cluster Catalog number indicating the background galaxy 2- 5 I4 --- FCC [1,2338] Fornax Cluster Catalog number 6 A1 --- f_FCC [*] Flag indicates that velocity or alt. name listed in file "notes.dat" 8- 9 I2 h RAh [3] right ascension (hours) (B1950) 11- 12 I2 min RAm [09,52]+= right ascension (minutes) 14- 17 F4.1 s RAs [0,60] right ascension (seconds) 19 A1 --- DE- [-] declination sign 20- 21 I2 deg DEd declination (degrees) (B1950) 23- 24 I2 arcmin DEm declination (minutes) 26- 27 I2 arcsec DEs [0,60] declination (seconds) 29 I1 --- Mem [1/6] membership status of the galaxy (G1) 31- 60 A30 --- MType Morphological type 62- 65 F4.1 mag BTmag total blue apparent magnitude 67- 71 F5.1 arcsec Reff [0,]? effective radius (arcsec) 73- 76 F4.2 [0.1arcmin] logD decimal logarithm of the diameter in units of 0.1arcmin at an isophoto 78- 79 I2 --- r_Reff Source of coordinates, magnitudes, and effective radii (G2) -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- bgGal [B] prefix of Fornax Cluster Catalog number indicating the background galaxy 2- 5 I4 --- FCC [1,2338] Fornax Cluster Catalog number 9- 40 A32 --- Note notes for galaxy designated '*'in Table 3, column 6. Velocity or alternate name. -------------------------------------------------------------------------------- Byte-by-byte Description of file: p3tbl*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- N [1,400]+ galaxy number 5- 9 A5 --- Plate designation as Las Campanas plate ID+number 11- 12 I2 h RAh right ascension (hours) (B1950) 14- 15 I2 min RAm right ascension (minutes) 17- 18 I2 s RAs right ascension (seconds) 20 A1 --- DE- declination sign 21- 22 I2 deg DEd declination (degrees) (B1950) 24- 27 F4.1 arcmin DEm declination (minutes) 29 I1 --- Mem [1,3] membership class (G1) 30 A1 --- --- [,] comma (if another membership class follows) 31 I1 --- Mem2 [0,4]? another membership class when class or reality is uncertain 33- 36 F4.1 mag BTmag total B magnitude 38- 40 I3 arcsec MajAxis [0,] major axis in arcsec (eye estimate) 42- 44 I3 arcsec MinAxis [0,] minor axis in arcsec (eye estimate) 46- 78 A33 --- MType morphological type 80-103 A24 --- Name alternate name(s) 105-109 I5 km/s Vhel ? heliocentric (usually) velocity (km/s) 111-113 I3 km/s e_Vhel ? uncertainty of Vhel 115-116 I2 --- r_Vhel [1,10]? reference of Vhel (1) 118-119 I2 --- r_BTmag [1,11]? reference of BT (1) 121-122 I2 --- Note [1,11]? notes (2) 124-134 A11 --- Morph [0-9a-m]! morphological type code (3) 136 I1 --- Conj [0-3] morphological type conjunction (4) 138-148 A11 --- Morph2 [0-9a-m]! alternate morphological type(3) -------------------------------------------------------------------------------- Note (1): References of velocities: 1 = RC2 (Cat. VII/122) 2 = Burstein, D. et al. 1987ApJS...64..601B 1987ApJS...64..601B 3 = Lauberts ESO atlas, Cat. VII/34 4 = Hoffman, G. L. et al. 1987ApJS...63..247H 1987ApJS...63..247H 5 = Sandage,A. & Tammann,G.A. 1987. Revised Shapley-Ames Gatalog of Bright Galaxies. (Washington: Carnegie) (See Cat. VII/51) 6 = daCosta, L. N. et al. 1984AJ.....89.1310D 1984AJ.....89.1310D 7 = Maia, M.A.G., daCosta, L.N., and Latham, D. W. 1989ApJS...69..809M 1989ApJS...69..809M (1988 CfA preprint #2741). 8 = CfA redshift survey (see Cat. VII/193) 9 = Hopp, U. and Materne, J. 1985A&AS...61...93H 1985A&AS...61...93H 10 = Tully 1988. Nearby Galaxies Catalog. (Cambridge: Cambridge University Press), Cat. VII/145 Note (2): Individual notes: 1 = Velocity not heliocentric. 2 = Galaxy is at the edge of the plate. 3 = Magnitude and size apply to the dE only. 4 = Ring of HII regions around nucleus. 5 = In halo of bright galaxy. 6 = Well developed arms with no dust or SF (smooth armed Sa) 7 = Bright HII regions in nucleus, well developed arms with no dust of SF. 8 = Shells? 9 = Large, LSB dwarf 10 = Figure 8 morphology 11 = Multiple Nuclei? Note (3): See the "Morphological type codes" section below. Note (4): the conjunction is coded as follows: 1 / 2 + 3 or -------------------------------------------------------------------------------- Global Notes: * Tables are not the same with those in the paper. * The format of item 13 in "expl.txt" file is not correct. It is corrected in the Byte-by-byte Description of file, above. * For the series of this paper, [paper I] Astron. J. 96, 1520 (1988AJ.....96.1520F 1988AJ.....96.1520F) [paper IV] Astron. J. 101, 765 (1991AJ....101..765F 1991AJ....101..765F) (There is no catalogue in these papers.) * A similar catalogue of Virgo cluster is in Astron. J. 90, 1681 (1985AJ.....90.1681B 1985AJ.....90.1681B). Note (G1): Membership codes: 1 = definite member, 2 = likely member, 3 = possible member, 4 = likely background, 5 = definite background, 6 = likely plate flaw Note (G2): Source of coordinates, magnitudes, and effective radii: 1 = SRC plate only. Image not saturated. 2 = SRC plate only. Image saturated 3 = SRC and Las Campanas plates. SRC image not saturated. 4 = SRC and Las Campanas plates. SRC image saturated. 5 = Las Campanas plate only. 10 = Welch, Chincarini, and Rood, 1975AJ.....80...77W 1975AJ.....80...77W 20 = Jones and Jones, 1980MNRAS.191..685J 1980MNRAS.191..685J 30 = Burstein et al., 1987ApJS...64..601B 1987ApJS...64..601B Morphological type codes: Dwarf / outer ring 0 - 1 d 2 d: 3 R Basic 0 - 1 E 2 S 3 I 4 BCD 5 Amorphous 6 merger 7 pre-merger 8 pec late 9 filament 10a flaw 11b pair 12c group Bar 0 - 1 B Lateness 0 - 1 0 2 a 3 ab 4 b 5 bc 6 c 7 cd 8 d 9 dm 10a m 11b 0/a S0 subtype 0 - 1 1 2 1/2 3 2 4 2/3 5 3 Spiral Morphology 0 - 1 (r) 2 (s) 3 (rs) 4 (sr) 5 (r:) 6 (s:) E class 0 - 1 1 2 2 3 3 4 4 5 5 6 6 7 7 8 8 9 9 10a 0 Luminosity class 0 - 1 I 2 I-II 3 II 4 II-II 5 III 6 III-IV 7 IV 8 IV-V 9 V Description 1 0 - 1 (dust) 2 (dust arms) 3 (smooth) 4 (on edge) 5 (tidal plumes) 6 (tides) 7 (...) (tides) 8 (cD) 9 (M32?) 10a (in cluster) 11b (interacting) 12c (boxy) 13d (star contamination) 14e (nonuniform background) 15f (cross) 16g (LSB) 17h (Seyfert?) 18i (High SB) 19j (pair) 20k (multiple N) 21l (+ globulars?) 22m (displaced N) Description 2 0 - 1 ring 2 pec 3 pec: 4 pec? 5 P 6 ? Nucleus 0 - 1 N 2 N: 3 N? 4 N pec 5 N pec? Historical notes: The catalogue was provided by courtesy of H.C. Ferguson to H. Andernach; it was numbered A102 and A112 in H. Andernach's "List of Astronomical Catalogues and Documents kindly provided on request by various authors" * 23-Jan-1993: Paper II was archived as VII/160/. * 08-Nov-1993: Paper III was archived as J/AJ/100/1/. * 14-Mar-1994: Both papers were joined into VII/180/. (The date of the latest archive, see the date of each file.) * 29-Jul-1997: ReadMe Document standardized. * 30-Dec-2000: ReadMe Document revised
(End) Koichi Nakajima [CDS], James Gass [SSDOO/ADC] 29-Jul-1997
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