From star-forming galaxies to AGN: The global HI content from a stacking experiment
K. Geréb,Raffaella Morganti,Tom Oosterloo,Laura Hoppmann,Lister Staveley-Smith,Lister Staveley-Smith +5 more
Reads0
Chats0
TLDR
In this article, the atomic neutral hydrogen (H I) content of ∼1600 galaxies up to z ∼ 0.1 was studied using stacking techniques. But the results were limited to the SDSS South Galactic Cap.Abstract:
We study the atomic neutral hydrogen (H I) content of ∼1600 galaxies up to z ∼ 0.1 using stacking techniques. The observations were carried out with the Westerbork Synthesis Radio Telescope (WSRT) in the area of the SDSS South Galactic Cap (SSGC), where we selected a galaxy sample from the SDSS spectroscopic catalog. Multi-wavelength information is provided by SDSS, NVSS, GALEX, and WISE. We use the collected information to study H I trends with color, star-forming, and active galactic nuclei (AGN) properties. Using near-UV (NUV) − r colors, galaxies are divided into blue cloud, green valley and red sequence galaxies. As expected based on previous observations, we detect H I in green valley objects with lower amounts of H I than blue galaxies, while stacking onlyread more
Citations
More filters
Journal ArticleDOI
Cold gas stripping in satellite galaxies: from pairs to clusters
Toby Brown,Toby Brown,Barbara Catinella,Luca Cortese,Claudia del P. Lagos,Romeel Davé,Virginia A. Kilborn,Martha P. Haynes,Riccardo Giovanelli,Mika Rafieferantsoa +9 more
TL;DR: In this paper, the authors investigate environment driven gas depletion in satellite galaxies, taking full advantage of the atomic hydrogen (HI) spectral stacking technique to quantify the gas content for the entire gas-poor to -rich regime.
Journal ArticleDOI
The Many Routes to AGN Feedback
TL;DR: In this article, a review summarizes some of the recent observational results obtained in different wavebands, tracing different phases of the gas, and summarizes the new insights they have brought, and the constraints they provide to numerical simulations of galaxy formation and evolution.
Journal ArticleDOI
AGN feedback and star formation of quasar host galaxies: insights from the molecular gas
TL;DR: In this paper, the authors used CO(2-1) observations from a new ALMA survey, in conjunction with literature measurements, to investigate the molecular gas properties of a representative sample of 40 z < 0.3 Palomar-Green quasars.
Journal ArticleDOI
Extragalactic HI surveys
TL;DR: In this paper, the authors review the results of HI line surveys of extragalactic sources in the local universe and provide an overview of currently ongoing and planned surveys which will explore the cosmic evolution of properties of the HI population.
Journal ArticleDOI
The Effect of AGNs on the Global H i Content of Isolated Low-mass Galaxies
TL;DR: In this article, the authors investigate the global neutral hydrogen (HI) content of isolated galaxies selected from the SDSS spectroscopic survey with optical evidence of Active Galactic Nuclei (AGN).
References
More filters
Journal ArticleDOI
The Sloan Digital Sky Survey: Technical Summary
TL;DR: The Sloan Digital Sky Survey (SDSS) as mentioned in this paper provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the Universe: a photometrically and astrometrically calibrated digital imaging survey of pi steradians above about Galactic latitude 30 degrees in five broad optical bands.
Journal ArticleDOI
The Sloan Digital Sky Survey: Technical summary
Donald G. York,Jennifer Adelman,John E. Anderson,Scott F. Anderson,James Annis,Neta A. Bahcall,J. A. Bakken,Robert H. Barkhouser,Steven Bastian,E. Berman,William N. Boroski,Steve Bracker,Charlie Briegel,John W. Briggs,Jon Brinkmann,Robert J. Brunner,Scott Burles,Larry N. Carey,Michael A. Carr,Francisco J. Castander,Francisco J. Castander,Bing Chen,Patrick L. Colestock,Andrew J. Connolly,James H. Crocker,István Csabai,István Csabai,Paul C. Czarapata,John Eric Davis,Mamoru Doi,Tom Dombeck,Daniel J. Eisenstein,Nancy Ellman,Brian R. Elms,Brian R. Elms,Michael L. Evans,Xiaohui Fan,Glenn R. Federwitz,Larry Fiscelli,Scott D. Friedman,Joshua A. Frieman,Joshua A. Frieman,Masataka Fukugita,Bruce Gillespie,James E. Gunn,Vijay K. Gurbani,Ernst De Haas,M. Haldeman,Frederick H. Harris,Jeffrey J. E. Hayes,Timothy M. Heckman,Gregory S. Hennessy,Robert B. Hindsley,S. Holm,Donald J. Holmgren,Chi Hao Huang,Charles L. Hull,Don Husby,Shin-Ichi Ichikawa,Takashi Ichikawa,Zěljko Ivezić,Stephen M. Kent,Rita S. J. Kim,E. Kinney,Mark A. Klaene,A. N. Kleinman,Scot Kleinman,Gillian R. Knapp,John Korienek,Richard G. Kron,Richard G. Kron,Peter Z. Kunszt,D. Q. Lamb,Brian C. Lee,R. French Leger,Siriluk Limmongkol,Carl Lindenmeyer,Dan Long,Craig Loomis,Jon Loveday,Rich Lucinio,Robert H. Lupton,Bryan Mackinnon,Bryan Mackinnon,Edward J. Mannery,Paul M. Mantsch,Bruce Margon,Peregrine M. McGehee,Timothy A. McKay,Avery Meiksin,Aronne Merelli,David G. Monet,Jeffrey A. Munn,Vijay K. Narayanan,Thomas Nash,Eric H. Neilsen,Rich Neswold,Heidi Jo Newberg,Heidi Jo Newberg,Robert C. Nichol,T. Nicinski,T. Nicinski,Mario Nonino,Norio Okada,Sadanori Okamura,Jeremiah P. Ostriker,Russell Owen,A. George Pauls,John Peoples,R. Peterson,Don Petravick,Jeffrey R. Pier,Adrian Pope,Ruth Pordes,Angela Prosapio,R. Rechenmacher,Thomas R. Quinn,Gordon T. Richards,Michael Richmond,Claudio H. Rivetta,Constance M. Rockosi,Kurt Ruthmansdorfer,Dale Sandford,David J. Schlegel,Donald P. Schneider,Maki Sekiguchi,G. Sergey,Kazuhiro Shimasaku,Walter A. Siegmund,Stephen A. Smee,J. Allyn Smith,S. A. Snedden,Robert Stone,Chris Stoughton,Michael A. Strauss,Christopher W. Stubbs,Mark SubbaRao,Alexander S. Szalay,István Szapudi,Gyula P. Szokoly,Anirudda R. Thakar,Christy Tremonti,Douglas L. Tucker,Alan Uomoto,Daniel E. Vanden Berk,Michael S. Vogeley,Patrick Waddell,Shu I. Wang,Masaru Watanabe,David H. Weinberg,Brian Yanny,Naoki Yasuda +151 more
TL;DR: The Sloan Digital Sky Survey (SDSS) as discussed by the authors provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the universe: a photometrically and astrometrically calibrated digital imaging survey of π sr above about Galactic latitude 30° in five broad optical bands to a depth of g' ~ 23 mag.
Journal ArticleDOI
The wide-field infrared survey explorer (wise): mission description and initial on-orbit performance
Edward L. Wright,Peter Eisenhardt,Amy Mainzer,Michael E. Ressler,Roc M. Cutri,Thomas H. Jarrett,J. Davy Kirkpatrick,Deborah L. Padgett,Robert S. McMillan,Michael F. Skrutskie,Spencer A. Stanford,Spencer A. Stanford,Martin Cohen,Russell G. Walker,John C. Mather,David Leisawitz,Thomas N. Gautier,Ian S. McLean,Dominic J. Benford,Carol J. Lonsdale,Andrew Blain,B. Mendez,William R. Irace,Valerie G. Duval,Fengchuan Liu,Don Royer,I. Heinrichsen,Joan Howard,Mark A. Shannon,Martha Kendall,Amy L. Walsh,Mark F. Larsen,Joel Cardon,Scott Schick,Mark Schwalm,Mohamed Abid,Beth Fabinsky,Larry Naes,Chao-Wei Tsai +38 more
TL;DR: The Wide-field Infrared Survey Explorer (WISE) is mapping the whole sky following its launch on 14 December 2009 and completed its first full coverage of the sky on July 17 as discussed by the authors.
Journal ArticleDOI
The NRAO VLA Sky Survey
James J. Condon,W. D. Cotton,Eric W. Greisen,Q. F. Yin,Richard A. Perley,G. B. Taylor,J. J. Broderick +6 more
TL;DR: The NRAO VLA Sky Survey (NVSS) covers the sky north of J2000 at 1.4 GHz as discussed by the authors, including a set of 2326 4?? 4? continuum cubes with three planes containing Stokes I, Q, and U images plus a catalog of almost 2? 106 discrete sources stronger than S 2.5 mJy.
Journal ArticleDOI
The Global Schmidt law in star forming galaxies
TL;DR: In this paper, the Schmidt law was used to model the global star formation law over the full range of gas densities and star formation rates observed in galaxies, and the results showed that the SFR scales with the ratio of the gas density to the average orbital timescale.
Related Papers (5)
Energy input from quasars regulates the growth and activity of black holes and their host galaxies
The Arecibo Legacy Fast ALFA survey. I. Science goals, survey design, and strategy
Riccardo Giovanelli,Martha P. Haynes,Brian R. Kent,Philip Perillat,Amelie Saintonge,Noah Brosch,Barbara Catinella,G. Lyle Hoffman,Sabrina Stierwalt,Kristine Spekkens,M. S. Lerner,Karen L. Masters,Emmanuel Momjian,Jessica L. Rosenberg,C. M. Springob,Alessandro Boselli,Vassilis Charmandaris,Jeremy Darling,Jonathan Ivor Davies,Diego G. Lambas,Giuseppe Gavazzi,Carlo Giovanardi,Eduardo Hardy,Leslie K. Hunt,A. Iovino,Igor D. Karachentsev,Valentina E. Karachentseva,Rebecca A. Koopmann,Christian Marinoni,Robert F. Minchin,Erik Muller,Mary E. Putman,C. Pantoja,John J. Salzer,Marco Scodeggio,Evan D. Skillman,José M. Solanes,José M. Solanes,Carlos Valotto,Wim van Driel,Liese van Zee +40 more
The Arecibo Legacy Fast ALFA Survey: the α.40 H I source catalog, its characteristics and their impact on the derivation of the H I mass function
Martha P. Haynes,Riccardo Giovanelli,Ann M. Martin,Kelley M. Hess,Amélie Saintonge,Elizabeth A. K. Adams,Gregory Hallenbeck,G. Lyle Hoffman,Shan Huang,Brian R. Kent,Rebecca A. Koopmann,Emmanouil Papastergis,Sabrina Stierwalt,Thomas J. Balonek,David W. Craig,Sarah J.U. Higdon,D. A. Kornreich,Jeffrey R. Miller,Aileen A. O'Donoghue,Ronald P. Olowin,Jessica L. Rosenberg,Kristine Spekkens,Parker Troischt,Eric M. Wilcots +23 more
The Arecibo Legacy Fast ALFA Survey: The alpha.40 HI Source Catalog, its Characteristics and their Impact on the Derivation of the HI Mass Function
Martha P. Haynes,Riccardo Giovanelli,Ann M. Martin,Kelley M. Hess,Amelie Saintonge,Elizabeth A. K. Adams,Gregory Hallenbeck,G. Lyle Hoffman,Shan Huang,Brian R. Kent,Rebecca A. Koopmann,Emmanouil Papastergis,Sabrina Stierwalt,Thomas J. Balonek,David W. Craig,Sarah J.U. Higdon,David A. Kornreich,Jeffrey R. Miller,Aileen A. O'Donoghue,Ronald P. Olowin,Jessica L. Rosenberg,Kristine Spekkens,Parker Troischt,Eric M. Wilcots +23 more