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|The Arizona-New Mexico Spectroscopic Survey of Galaxies. III. On Galaxy Populations|
We examine the population statistics for two samples of galaxies in thedirection of the Perseus supercluster. One sample, with N=258 galaxieshaving MB<=-19.52+5log(h) and vh<=8000 kms-1, is complete for those galaxies within the boundaries ofour survey region that have apparent magnitudes mp<=15.0in the Zwicky catalog. A more restrictive sample with N=177 galaxieshaving MB<=-20.00+5log(h) (with the same redshift range)is complete in both luminosity and volume. We derive the statistics forthe relative incidence of galaxies in the following spectroscopicclasses: (1) absorption line only, (2) collisionally-excited emissionlines only, (3) nuclear H II region, (4) starburst, (5) LINER, and (6)Seyfert 1.8-2.
|The Arizona-New Mexico Spectroscopic Survey of Galaxies. I. Data for the Western End of the Perseus Supercluster|
We present new optical spectroscopic data for 347 galaxies in the regionof the Perseus supercluster. The new data were obtained using theSteward Observatory 2.3 m telescope and cover the whole optical window.Included are redshifts (for 345 objects), absorption-line equivalentwidths, a continuum index measuring the 4000 Å break, andemission-line flux ratios. After 11 objects are rejected for being toofaint and redshifts for 26 objects are added from the literature, wearrive at a complete sample of 361 galaxies. The distribution ofredshifts for the whole sample is examined, and we show the relationshipof the continuum index to morphology.
|Arcsecond Positions of UGC Galaxies|
We present accurate B1950 and J2000 positions for all confirmed galaxiesin the Uppsala General Catalog (UGC). The positions were measuredvisually from Digitized Sky Survey images with rms uncertaintiesσ<=[(1.2")2+(θ/100)2]1/2,where θ is the major-axis diameter. We compared each galaxymeasured with the original UGC description to ensure high reliability.The full position list is available in the electronic version only.
|Galaxy coordinates. II. Accurate equatorial coordinates for 17298 galaxies|
Using images of the Digitized Sky Survey we measured coodinates for17298 galaxies having poorly defined coordinates. As a control, wemeasured with the same method 1522 galaxies having accurate coordinates.The comparison with our own measurements shows that the accuracy of themethod is about 6 arcsec on each axis (RA and DEC).
|A Deep Survey of H I-selected Galaxies: The Sample and the Data|
In a 21 cm neutral hydrogen survey of approximately 55 deg^2 out to aredshift of cz = 8340 km s^-1, we have identified 75 extragalactic H Isources. These objects comprise a well-defined sample of extragalacticsources chosen by means that are independent of optical surfacebrightness selection effects. In this paper we describe the Arecibosurvey procedures and H I data, follow-up VLA H I observations made ofseveral unusual sources, and Kitt Peak B-, R-, and I-band photometry fornearly all of the galaxies. We have also gathered information for someof the optically detected galaxies within the same search volume. Weexamine how samples generated by different types of search techniquesoverlap with selection by H I flux. Only the least massive H I object,which is among the lowest mass H I sources previously found, does nothave a clear optical counterpart, but a nearby bright star may hide lowsurface brightness emission. However, the newly detected systems do haveunusual optical properties. Most of the 40 galaxies that were notpreviously identified in magnitude-limited catalogs appear to begas-dominated systems, and several of these systems have H Imass-to-light ratios among the largest values ever previously found.These gas-dominated objects also tend to have very blue colors, lowsurface brightnesses, and no central bulges, which correlate stronglywith their relative star-to-gas content.
|A 21 CM survey of the Pisces-Perseus supercluster. II - The declination zone +21.5 to +27.5 degrees|
Neutral-hydrogen 21-cm line spectra and derived parameters are presentedfor a sample of spiral galaxies in the region bounded by an R.A. greaterthan 22 h and less then 0.04 h, and a declination greater than +21 deg30 min and less than +27 deg 30 min, covering the Zwicky fields 470 to488, as the second installment of a survey of the region of thePisces-Perseus supercluster. New H I line observations made with theArecibo 305 m telescope detected 275 galaxies of 318 studied. Atabulation of derived galaxian properties is given. The redshiftdistribution shows gross departures from that expected for a sample withsimilar magnitude characteristics but homogeneously located in space.These new data will be incorporated into the overall survey of thethree-dimensional structure in the Pisces-Perseus region.
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