THE NEW GALAXY SAMPLE FROM SDSS DR9 AT 0.003 ≤ Z ≤ 0.1

Автор(и)

  • D. V. Dobrycheva Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2013.26.82565

Ключові слова:

Galaxies, SDSS DR9.

Анотація

To test the relationships between morphological types of galaxies in pairs/groups and their physical properties (luminosity, mass, color index, the radial velocity, the inverse concentration index, the absolute magnitude, the radius of the de Vaucouleurs or scale radius, etc.) on a larger sample of the local Universe, we need the more representative data. With this aim we processed and prepared a sam­ple of galaxies with 0.003 ≤ z ≤ 0.1 based on the latest SDSS DR9. The initial sample was about 724,000 objects and, consequently, 407,000 galaxy images after the preliminary processing. Because of the large number of duplicate and faulty images, we checked its carefully and obtained finally about 260,000 galaxies in the studied sample at z < 0.1. We discuss this procedure and properties of the studied galaxy sample.

Посилання

Babyk I., Vavilova I.: 2013, Astrophys. Space Sci., DOI10.1007/s10509-013-1630-z

Babyk I., Vavilova I., Del Popolo A.: 2012, arXiv 1208. 2424

Blanton M.R., Brinkmann J. et al.: 2002, The Astronomical Journal 125, 2348.

Carollo C.M., Cibinel1 A., Lilly S.J. et al.: 2013, Astrophys. J. 776, 71.

Dobrycheva D., Melnyk O.: 2012, Advances in Astronomy and Space Physics 2, 42.

Elyiv A., Melnyk O., Vavilova I.: 2009, Mon. Not. R. Astron. Soc. 394, 1409.

Karachentseva V.E., Melnyk O.V., Vavilova I.B., Makarov D.I.: 2005, Kinematika i Fizika Nebesnykh Tel 21, 217.

Karachentseva V.E., Vavilova I.B.: 1994a, ESO Conference and Workshop Proceedings 49, 91

Karachentseva V.E., Vavilova I.B.: 1994b, Bulletin of the Special Astrophysics Observatory 37, 98.

Karachentseva V.E., Vavilova I.B.: 1995, Kinematics and Physics of Celestial Bodies 11, 38.

Luparello H.E., Lares M., Yaryura C.Y. et al.: 2013, arXiv:1304.0456

Melnik O.V., Elyiv A.A., Vavilova I.B.: 2009, Kinematics and Physics of Celestial Bodies 25, 43.

Melnyk O.V., Dobrycheva D.V., Vavilova I.B.: 2012, Astrophysics 5, 293.

Melnyk O.V., Vavilova I.B.: 2008, Advances in Space Research 42, 591.

Melnyk O.V., Elyiv A.A., Vavilova I.B.: 2006, Kinematika i Fizika Nebesnykh Tel 22, 283.

Poggianti B.M.: 1997, Astron Astrophys. 122, 399.

Pulatova N., Vavilova I., Berczik P.: 2013, IAU Symposium 290, 297.

Szabo T., Pierpaoli E.: 2013, AAS Meeting Abstracts, 221

Sheldon E.S., Cunha C.E., Mandelbaum R. et al.: 2012, Astrophys. J. Suppl., 201, 32.

Tempel E., Tago E., Liivamgi1 L.J.: 2012, Astron. Astrophys. 540, DOIdx.doi.org/10.1051/0004-6361/201118687

Tempel E., Saar E., Liivamgi L.J. et al.: 2011, arXiv:1012.1470

Vavilova I.B., Karachentseva V.E., Makarov D.I., Melnyk O.V.: 2005, Kinematika i Fizika Nebesnykh Tel, 21, 1.

Vavilova I.B., Melnyk O.V., Elyiv A.A.: 2009, Astron. Nachr., 330, 1004.

Vollmer B.: 2007, Planets, Stars and Stellar Systems, 207.

Yuan H.B., Liu X.W., Xiang M.S.: 2013, Mon. Not. R. Astron. Soc., 430, 2188.

##submission.downloads##

Опубліковано

2013-11-09

Номер

Розділ

Статті