The KPNO International Spectroscopic Survey. III. [O [CSC]iii[/CSC]]-selected Survey List

Salzer, John J.; Grönwall, C.; Sarajedini, Vicki L.; Lipovetsky, V. A.; Kniazev, A. Y.; Moody, J. W.; Boroson, Todd A.; Thuan, T. X.; Izotov, Y. I.; Herrero, José Luís Caro; Frattare, L. M.

doi:10.1086/339024

Cited by 34 publications

(24 citation statements)

References 29 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…These objects are from the Huchra et al (1990) NGP +30 zone complete sample of 1093 galaxies with m pg F15:5 and additional 92 fainter galaxies. These galaxies have been identified as UVor emission-line galaxies from the Kiso (e.g., Takase & MiyauchiIsobe 1985), Mrk (Markarian et al 1989), KISS (e.g., Salzer et al 2002), Wasilewski (1983), and other surveys of active and star-forming objects or are known peculiar galaxies according to their morphological structure (e.g., NGC 2608 in the sample is Arp 12), or integral properties (e.g., NGC 2415 in the sample is the high surface brightness galaxy Haro 1 = Ark 136). The inclusion in the sample of galaxies with peculiar morphologies and/or integral properties, which very often are the outcomes of merging or close interaction, follows the wide belief that, in general, star formation or nuclear activity in these galaxies is enhanced (e.g., Tomita & Maehara 2002;Malkan & Hunt 2004).…”

Section: The Samplesmentioning

confidence: 99%

Active and Star-forming Galaxies and Their Supernovae

Петросян¹,

Navasardyan²,

McLean³

et al. 2005

Astron J

View full text Add to dashboard Cite

To investigate the extent to which nuclear starbursts or other nuclear activity may be connected with enhanced star formation activity in the host galaxy, we perform a statistical investigation of supernovae (SNe) discovered in host galaxies from four samples: the Markarian galaxies sample, the Second Byurakan Survey (SBS) sample, the north Galactic pole ( NGP) sample of active or star-forming galaxies, and the NGP sample of normal galaxies. Forty-seven SNe in 41 Mrk galaxies, 10 SNe in six SBS galaxies, 29 SNe in 26 NGP active or star-forming galaxies, and 29 SNe in 26 NGP normal galaxies have been studied. We find that the rate of SNe, particularly core-collapse ( Types Ib/c and II) SNe, is higher in active or star-forming galaxies in comparison with normal galaxies. Active or star-forming host galaxies of SNe are generally of later morphological type and have lower luminosity and smaller linear size than normal host galaxies of SNe. The radial distribution of SNe in active and star-forming galaxies shows a higher concentration toward the center of the active host galaxy than is the case for normal host galaxies, and this effect is more pronounced for core-collapse SNe. Ib/c-type SNe have been discovered only in active and star-forming galaxies of our samples. About 78% of these SNe are associated with H ii regions or are located very close to the nuclear regions of these active galaxies, which are in turn hosting AGNs or starburst nuclei. Besides these new results, our study also supports the conclusions of several other earlier papers. We find that Type Ia SNe occur in all galaxy types, whereas core-collapse SNe of Types Ib/c and II are found only in spiral and irregular galaxies. The radial distribution of Type Ib SNe in their host galaxies is more centrally concentrated than that of Type II and Ia SNe. The radial distances of Types Ib/c and II SNe, from the nuclei of their host galaxies, is larger for barred spiral hosts. Core-collapse SNe are concentrated in spiral arms and are often close to or in the H ii regions, whereas Type Ia SNe show only a loose association with spiral arms and no clear association with H ii regions.

show abstract

Section: The Samplesmentioning

confidence: 99%

Active and Star-forming Galaxies and Their Supernovae

Петросян¹,

Navasardyan²,

McLean³

et al. 2005

Astron J

View full text Add to dashboard Cite

show abstract

“…The sample of optically compact galaxies studied in this paper was produced using specific selection criteria designed to identify star-forming galaxies with compact stellar components; ADBS 113845+2008 and IC 2271 were already known to have such characteristics from previous imaging. Starting with the full KPNO International Spectroscopic Survey (KISS, an objective-prism survey for extragalactic emission-line objects; Salzer et al 2000Salzer et al , 2001Salzer et al , 2002 database, we searched for emission-line objects that were spectroscopically-confirmed. To maximize physical resolution an upper velocity constraint was set at V sys < 5,000 km s −1 .…”

Section: Survey Selection Criteriamentioning

confidence: 99%

“…Moment maps showing integrated H i emission and velocity structures were created using the techniques discussed in detail in Cannon et al (2009). Table 3, the total H i flux integrals derived for the sample galaxies are each lower than the Arecibo Observatory single dish observations (Rosenberg & Schneider 2000, 2002Lee et al 2002). The cause of these differences is at least partly due to the missing short uv spacings of the VLA compared to a single dish measurement.…”

Section: Vla H I Spectral Line Observationsmentioning

confidence: 99%

“…While the properties of isolated BCDs have been studied in some detail (e.g., the studies of NGC 2915 by Meurer et al 1994Meurer et al , 1996, a particularly intriguing system was discovered in the Arecibo Dual Beam Survey (ADBS) by Rosenberg & Schneider (2000, 2002: ADBS 113845+2008. This galaxy was subsequently cataloged as a UV-excess source in the 2nd KISO survey (Miyauchi-Isobe & Maehara, 2000).…”

Section: Introductionmentioning

confidence: 99%

See 1 more Smart Citation

Exploring the Interstellar Media of Optically Compact Dwarf Galaxies

Cannon¹,

Salzer²,

Rosenberg³

et al. 2013

Self Cite

View full text Add to dashboard Cite

We present new Very Large Array H i spectral line, archival Sloan Digital Sky Survey, and archival Spitzer Space Telescope imaging of eight star-forming -2blue compact dwarf galaxies that were selected to be optically compact (optical radii <1 kpc). These systems have faint blue absolute magnitudes (M B > ∼ −17), ongoing star formation (based on emission-line selection by the Hα or [O III] lines), and are nearby (mean velocity = 3315 km s −1 ≃ 45 Mpc). One galaxy in the sample, ADBS 113845+2008, is found to have an H i halo that extends 58 r-band scale lengths from its stellar body. In contrast, the rest of the sample galaxies have H i radii to optical-scale-length ratios ranging from 9.3 to 26. The size of the H i disk in the "giant disk" dwarf galaxy ADBS 113845+2008 appears to be unusual as compared to similarly compact stellar populations.

show abstract

“…Cross-checking includes well-known optical surveys of A /SF galaxies, e.g., Markarian ( Petrosian et al 2007), Kiso (e.g., Takase & Miyauchi-Isobe 1985), KISS (e.g., Salzer et al 2002), Wasilewski (1983) and others, as well as all X-ray and radio surveys, which cover the NGP 6 strip area. Cross-checking also includes the lists of known peculiar morphological structure galaxies (e.g., NGC 2608 in the sample is Arp 12), or lists of galaxies with peculiar integral properties (e.g., NGC 2415 in the sample is the high surface brightness galaxy Haro 1 = Ark 136).…”

Section: Introductionmentioning

confidence: 99%

The North Galactic Pole +30° Zone Galaxies. I. A Comparative Study of Galaxies with Different Nuclear Activity

Петросян¹,

McLean²,

Allen³

et al. 2008

ASTROPHYS J SUPPL S

View full text Add to dashboard Cite

A database containing 618 active and star-forming (A/SF) galaxies and 564 normal galaxies in a 120 ; 6 wide strip crossing the north Galactic pole was constructed in order to compare the global properties of ''active'' galaxies against a control sample of ''normal'' galaxies. This database combines a literature and catalog search with new optical measurements from the F pg (red) and J pg (blue) band images of the STScI Digitized Sky Survey (DSS). We provide alternative names, accurate coordinates, morphological type, activity classes, red and blue apparent magnitudes, 2MASS near-infrared JÀH and HÀK colors, apparent diameters, axial ratios, position angles, and number counts of neighboring objects in a circle of radius 50 kpc. We also present an atlas of 103 interacting and merging systems among these galaxies. The integrated properties of A/SF and normal galaxies in this sample are compared using a multivariate factor analysis, which reveals that A/SF galaxies are objects with relatively late morphological types, and are more inclined and have bluer optical colors than normal galaxies. In this sample, all merging and interacting galaxies are A/SF objects. Star-forming galaxies are objects with relatively late morphological types, lower absolute luminosities and linear sizes, bluer colors, and higher inclination than sample X-ray or radio sources, as well as Seyfert galaxies. The near-infrared colors of the sample galaxies are independent parameters and do not correlate with activity level or any other parameter of the galaxies.

show abstract

The KPNO International Spectroscopic Survey. III. [O [CSC]iii[/CSC]]-selected Survey List

Cited by 34 publications

References 29 publications

Active and Star-forming Galaxies and Their Supernovae

Active and Star-forming Galaxies and Their Supernovae

Exploring the Interstellar Media of Optically Compact Dwarf Galaxies

The North Galactic Pole +30° Zone Galaxies. I. A Comparative Study of Galaxies with Different Nuclear Activity

Contact Info

Product

Resources

About