Related papers: The effects of environment on morphological evolut…

Evolution of Galaxies and their Environments at z = 0.1 to 3 in COSMOS

Large-scale structures (LSS) out to z $< 3.0$ are measured in the Cosmic Evolution Survey (COSMOS) using extremely accurate photometric redshifts (photoz). The Ks-band selected sample (from Ultra-Vista) is comprised of 155,954 galaxies. Two…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 N. Scoville , S. Arnouts , H. Aussel , A. Benson , A. Bongiorno , K. Bundy , M. A. A. Calvo , P. Capak , M. Carollo , F. Civano , J. Dunlop , M. Elvis , A. Faisst , A. Finoguenov , Hai Fu , M. Giavalisco , Q. Guo , O. Ilbert , A. Iovino , M. Kajisawa , J. Kartaltepe , A. Leauthaud , O. Le Fe`vre , E. LeFloch , S. J. Lilly , C. T-C. Liu , S. Manohar , R. Massey , D. Masters , H. J. McCracken , B. Mobasher , Y-J. Peng , A. Renzini , J. Rhodes , M. Salvato , D. B. Sanders , B. D. Sarvestani , C. Scarlata , E. Schinnerer , K. Sheth , P. L. Shopbell , V. Smol'cic , Y. Taniguchi , J. E. Taylor , S. D. M. White , L. Yan

The evolution of early and late type galaxies in the COSMOS up to z~1.2

The Cosmic Evolution Survey (COSMOS) allows for the first time a highly significant census of environments and structures up to redshift one, as well as a full morphological description of the galaxy population. In this paper we present a…

Cosmology and Nongalactic Astrophysics · Physics 2009-08-05 Maurilio Pannella , Armin Gabasch , Yuliana Goranova , Niv Drory , Ulrich Hopp , Stefan Noll , Roberto P. Saglia , Veronica Strazzullo , Ralf Bender

Environment and self-regulation in galaxy formation

The environment is known to affect the formation and evolution of galaxies considerably best visible through the well-known morphology-density relationship. In this paper we study the effect of environment on the evolution of early-type…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Daniel Thomas , Claudia Maraston , Kevin Schawinski , Marc Sarzi , Joseph Silk

The zCOSMOS Redshift Survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z~1

For more than two decades we have known that galaxy morphological segregation is present in the Local Universe. It is important to see how this relation evolves with cosmic time. To investigate how galaxy assembly took place with cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 L. A. M. Tasca , J. P. Kneib , A. Iovino , O. Le Fevre , K. Kovac , M. Bolzonella , S. J. Lilly , R. G. Abraham , P. Cassata , O. Cucciati , L. Guzzo , L. Tresse , G. Zamorani , P. Capak , B. Garilli , M. Scodeggio , K. Sheth , D. Vergani , E. Zucca , C. M. Carollo , T. Contini , V. Mainieri , A. Renzini , S. Bardelli , A. Bongiorno , K. Caputi , G. Coppa , S. de la Torre , L. de Ravel , P. Franzetti , P. Kampczyk , C. Knobel , A. Koekemoer , F. Lamareille , J. F. Le Borgne , V. Le Brun , C. Maier , M. Mignoli , R. Pello , Y. Peng , E. Perez Montero , E. Ricciardelli , J. D. Silverman , M. Tanaka , U. Abbas , D. Bottini , A. Cappi , A. Cimatti , O. Ilbert , A. Leauthaud , D. Maccagni , C. Marinoni , H. J. McCracken , P. Memeo , B. Meneux , P. Oesch , C. Porciani , L. Pozzetti , R. Scaramella , C. Scarlata

The Cosmic Evolution Survey (COSMOS): The morphological content and enviromental dependence of the galaxy color-magnitude relation at z~0.7

We study the enviromental dependence and the morphological composition of the galaxy color-magnitude diagram at z~0.7, using a pilot sub-sample of ~2000 galaxies from the COSMOS surve, with I_AB<24, photometric redshift within 0.61<z<0.85…

Astrophysics · Physics 2009-12-15 P. Cassata , L. Guzzo , A. Franceschini , N. Scoville , P. Capak , R. S. Ellis , A. Koekemoer , H. J. McCracken , B. Mobasher , A. Renzini , E. Ricciardelli , M. Scodeggio , Y. Taniguchi , D. Thompson

Evolution Since z=1 of the Morphology-density Relation of Galaxies

We measure the morphology-density relation of galaxies at z=1 across the full three orders of magnitude in projected galaxy density available in low-redshift studies. Our study adopts techniques that are comparable with those applied at…

Astrophysics · Physics 2010-04-06 Graham P. Smith , Tommaso Treu , Richard S. Ellis , Sean M. Moran , Alan Dressler

The Cosmic Evolution Survey (COSMOS): a large-scale structure at z=0.73 and the relation of galaxy morphologies to local environment

We have identified a large-scale structure at z~0.73 in the COSMOS field, coherently described by the distribution of galaxy photometric redshifts, an ACS weak-lensing convergence map and the distribution of extended X-ray sources in a…

Astrophysics · Physics 2009-11-13 L. Guzzo , P. Cassata , A. Finoguenov , R. Massey , N. Z. Scoville , P. Capak , R. S. Ellis , B. Mobasher , Y. Taniguchi , D. Thompson , M. Ajiki , H. Aussel , H. Boehringer , M. Brusa , D. Calzetti , A. Comastri , A. Franceschini , G. Hasinger , M. M. Kasliwal , M. G. Kitzbichler , J. -P. Kneib , A. Koekemoer , A. Leauthaud , H. J. McCracken , T. Murayama , T. Nagao , J. Rhodes , D. B. Sanders , S. Sasaki , Y. Shioya , L. Tasca , J. E. Taylor

And the winner is: galaxy mass

The environment is known to affect the formation and evolution of galaxies considerably best visible through the well-known morphology-density relationship. We study the effect of environment on the evolution of early-type galaxies for a…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Daniel Thomas

The role of environment in the morphological transformation of galaxies in 9 intermediate redshift clusters

[abridged] We analyze a sample of 9 massive clusters at 0.4<z<0.6 observed with MegaCam in 4 photometric bands (g,r,i,z) from the core to a radius of 5 Mpc (~4000 galaxies). Galaxy cluster candidates are selected using photometric redshifts…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 M. Huertas-Company , G. Foex , G. Soucail , R. Pello

Evidence for Morphology and Luminosity Transformation of Galaxies at High Redshifts

We study the galaxy morphology-luminosity-environmental relation and its redshift evolution using a spectroscopic sample of galaxies in the Great Observatories Origins Deep Survey (GOODS). In the redshift range of $0.4\leq z\leq1.0$ we…

Cosmology and Nongalactic Astrophysics · Physics 2009-07-22 Ho Seong Hwang , Changbom Park

The relation between morphology, star formation history, and environment in local universe galaxies

The observed properties of galaxies are strongly dependent on both their total stellar mass and their morphology. Furthermore, the environment is known to play a strong role in shaping them. The galaxy population in the local universe that…

Astrophysics of Galaxies · Physics 2023-03-01 D. Pérez-Millán , Jacopo Fritz , Rosa A. González-Lópezlira , Alessia Moretti , Bernardo Cervantes Sodi , Benedetta Vulcani , Marco Gullieuszik , Gustavo Bruzual , Stéphane Charlot , Daniela Bettoni

Morphological Evolution of Galaxies

We simulate the growth of large-scale structure in the universe using a N-body code. By combining these simulations with a Monte-Carlo method, we generate galaxy distributions at present that reproduces the observed morphology-density…

Astrophysics · Physics 2009-10-30 Hugo Martel , Premana Premadi , Richard Matzner

The star formation history of early-type galaxies as a function of mass and environment

Using the third data release of the Sloan Digital Sky Survey (SDSS) we have rigorously defined a volume limited sample of early-type galaxies in the redshift range z < 0.1. We have defined the density of the local environment for each…

Astrophysics · Physics 2009-11-11 M. S. Clemens , A. Bressan , B. Nikolic , P. Alexander , F. Annibali , R. Rampazzo

The 10k zCOSMOS: morphological transformation of galaxies in the group environment since z~1

We study the evolution of galaxies inside and outside of the group environment since z=1 using a large well defined set of groups and galaxies from the zCOSMOS-bright redshift survey in the COSMOS field. The fraction of galaxies with…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 K. Kovac , S. J. Lilly , C. Knobel , M. Bolzonella , A. Iovino , C. M. Carollo , C. Scarlata , M. Sargent , O. Cucciati , G. Zamorani , L. Pozzetti , L. A. M. Tasca , M. Scodeggio , P. Kampczyk , Y. Peng , P. Oesch , E. Zucca , A. Finoguenov , T. Contini , J. -P. Kneib , O. Le Fevre , V. Mainieri , A. Renzini , S. Bardelli , A. Bongiorno , K. Caputi , G. Coppa , S. de la Torre , L. de Ravel , P. Franzetti , B. Garilli , F. Lamareille , J. -F. Le Borgne , V. Le Brun , C. Maier , M. Mignoli , R. Pello , E. Perez Montero , E. Ricciardelli , J. D. Silverman , M. Tanaka , L. Tresse , D. Vergani , U. Abbas , D. Bottini , A. Cappi , P. Cassata , A. Cimatti , M. Fumana , L. Guzzo , A. M. Koekemoer , A. Leauthaud , D. Maccagni , C. Marinoni , H. J. McCracken , P. Memeo , B. Meneux , C. Porciani , R. Scaramella , N. Z. Scoville

Evolution and environment of early-type galaxies

We study the photometric and spectral properties of 39320 early-type galaxies within the SDSS, as a function of both local environment and redshift. The distance to the nearest cluster of galaxies and the distance to the 10th nearest…

Astrophysics · Physics 2008-11-26 M. Bernardi , R. C. Nichol , R. K. Sheth , C. J. Miller , J. Brinkmann

Tracking the impact of environment on the Galaxy Stellar Mass Function up to z~1 in the 10k zCOSMOS sample

We study the impact of the environment on the evolution of galaxies in the zCOSMOS 10k sample in the redshift range 0.1<z<1.0 over an area of ~1.5 deg2. The considered sample of secure spectroscopic redshifts contains about 8500 galaxies,…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-30 M. Bolzonella , K. Kovac , L. Pozzetti , E. Zucca , O. Cucciati , S. J. Lilly , Y. Peng , A. Iovino , G. Zamorani , D. Vergani , L. A. M. Tasca , F. Lamareille , P. Oesch , K. Caputi , P. Kampczyk , S. Bardelli , C. Maier , U. Abbas , C. Knobel , M. Scodeggio , C. M. Carollo , T. Contini , J. -P. Kneib , O. Le Fevre , V. Mainieri , A. Renzini , A. Bongiorno , G. Coppa , S. de la Torre , L. de Ravel , P. Franzetti , B. Garilli , J. -F. Le Borgne , V. Le Brun , M. Mignoli , R. Pello , E. Perez-Montero , E. Ricciardelli , J. D. Silverman , M. Tanaka , L. Tresse , D. Bottini , A. Cappi , P. Cassata , A. Cimatti , L. Guzzo , A. M. Koekemoer , A. Leauthaud , D. Maccagni , C. Marinoni , H. J. McCracken , P. Memeo , B. Meneux , C. Porciani , R. Scaramella , H. Aussel , P. Capak , C. Halliday , O. Ilbert , J. Kartaltepe , M. Salvato , D. Sanders , C. Scarlata , N. Scoville , Y. Taniguchi , D. Thompson

Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$

The extent to which the environment affects galaxy evolution has been under scrutiny by researchers for decades. With the first data from Euclid, we can begin to systematically study a wide range of environments and their effects as a…

Astrophysics of Galaxies · Physics 2026-04-20 Euclid Collaboration , C. Cleland , S. Mei , G. De Lucia , F. Fontanot , H. Fu , C. C. Lovell , M. Magliocchetti , N. Mai , D. Roberts , F. Shankar , J. G. Sorce , M. Baes , P. Corcho-Caballero , S. Eales , C. Tortora , N. Aghanim , B. Altieri , A. Amara , S. Andreon , N. Auricchio , H. Aussel , C. Baccigalupi , M. Baldi , A. Balestra , S. Bardelli , P. Battaglia , A. Biviano , A. Bonchi , D. Bonino , E. Branchini , M. Brescia , J. Brinchmann , S. Camera , G. Cañas-Herrera , V. Capobianco , C. Carbone , J. Carretero , S. Casas , F. J. Castander , M. Castellano , G. Castignani , S. Cavuoti , K. C. Chambers , A. Cimatti , C. Colodro-Conde , G. Congedo , C. J. Conselice , L. Conversi , Y. Copin , F. Courbin , H. M. Courtois , M. Cropper , A. Da Silva , H. Degaudenzi , A. M. Di Giorgio , C. Dolding , H. Dole , F. Dubath , X. Dupac , A. Ealet , S. Escoffier , M. Farina , R. Farinelli , F. Faustini , S. Ferriol , F. Finelli , S. Fotopoulou , M. Frailis , E. Franceschi , M. Fumana , S. Galeotta , K. George , B. Gillis , C. Giocoli , J. Gracia-Carpio , B. R. Granett , A. Grazian , F. Grupp , S. Gwyn , S. V. H. Haugan , J. Hoar , W. Holmes , F. Hormuth , A. Hornstrup , P. Hudelot , K. Jahnke , M. Jhabvala , B. Joachimi , E. Keihänen , S. Kermiche , A. Kiessling , B. Kubik , M. Kümmel , M. Kunz , H. Kurki-Suonio , O. Lahav , Q. Le Boulc'h , A. M. C. Le Brun , D. Le Mignant , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , G. Mainetti , D. Maino , E. Maiorano , O. Mansutti , S. Marcin , O. Marggraf , M. Martinelli , N. Martinet , F. Marulli , R. Massey , S. Maurogordato , E. Medinaceli , Y. Mellier , M. Meneghetti , E. Merlin , G. Meylan , A. Mora , M. Moresco , L. Moscardini , R. Nakajima , C. Neissner , S. -M. Niemi , J. W. Nightingale , C. Padilla , S. Paltani , F. Pasian , K. Pedersen , W. J. Percival , V. Pettorino , S. Pires , G. Polenta , M. Poncet , L. A. Popa , L. Pozzetti , F. Raison , R. Rebolo , A. Renzi , J. Rhodes , G. Riccio , E. Romelli , M. Roncarelli , R. Saglia , Z. Sakr , D. Sapone , B. Sartoris , J. A. Schewtschenko , P. Schneider , M. Scodeggio , A. Secroun , G. Seidel , S. Serrano , P. Simon , C. Sirignano , G. Sirri , L. Stanco , J. Steinwagner , P. Tallada-Crespí , A. N. Taylor , H. I. Teplitz , I. Tereno , N. Tessore , S. Toft , R. Toledo-Moreo , F. Torradeflot , I. Tutusaus , L. Valenziano , J. Valiviita , T. Vassallo , G. Verdoes Kleijn , A. Veropalumbo , Y. Wang , J. Weller , A. Zacchei , G. Zamorani , F. M. Zerbi , I. A. Zinchenko , E. Zucca , V. Allevato , M. Ballardini , M. Bolzonella , E. Bozzo , C. Burigana , R. Cabanac , A. Cappi , D. Di Ferdinando , J. A. Escartin Vigo , L. Gabarra , J. Martín-Fleitas , S. Matthew , M. Maturi , N. Mauri , R. B. Metcalf , A. Pezzotta , M. Pöntinen , C. Porciani , I. Risso , V. Scottez , M. Sereno , M. Tenti , M. Viel , M. Wiesmann , Y. Akrami , S. Alvi , I. T. Andika , S. Anselmi , M. Archidiacono , F. Atrio-Barandela , C. Benoist , K. Benson , D. Bertacca , M. Bethermin , A. Blanchard , L. Blot , H. Böhringer , S. Borgani , M. L. Brown , S. Bruton , A. Calabro , F. Caro , C. S. Carvalho , T. Castro , F. Cogato , A. R. Cooray , O. Cucciati , S. Davini , F. De Paolis , G. Desprez , A. Díaz-Sánchez , J. J. Diaz , S. Di Domizio , J. M. Diego , P. -A. Duc , A. Enia , Y. Fang , A. G. Ferrari , P. G. Ferreira , A. Finoguenov , A. Fontana , A. Franco , K. Ganga , J. García-Bellido , T. Gasparetto , V. Gautard , E. Gaztanaga , F. Giacomini , F. Gianotti , A. H. Gonzalez , G. Gozaliasl , M. Guidi , C. M. Gutierrez , A. Hall , W. G. Hartley , C. Hernández-Monteagudo , H. Hildebrandt , J. Hjorth , J. J. E. Kajava , Y. Kang , V. Kansal , D. Karagiannis , K. Kiiveri , C. C. Kirkpatrick , S. Kruk , L. Legrand , M. Lembo , F. Lepori , G. Leroy , G. F. Lesci , J. Lesgourgues , L. Leuzzi , T. I. Liaudat , A. Loureiro , J. Macias-Perez , G. Maggio , E. A. Magnier , F. Mannucci , R. Maoli , C. J. A. P. Martins , L. Maurin , M. Miluzio , P. Monaco , C. Moretti , G. Morgante , K. Naidoo , A. Navarro-Alsina , S. Nesseris , F. Passalacqua , K. Paterson , L. Patrizii , A. Pisani , D. Potter , S. Quai , M. Radovich , P. -F. Rocci , G. Rodighiero , S. Sacquegna , M. Sahlén , D. B. Sanders , E. Sarpa , C. Scarlata , J. Schaye , A. Schneider , M. Schultheis , D. Sciotti , E. Sellentin , L. C. Smith , S. A. Stanford , K. Tanidis , G. Testera , R. Teyssier , S. Tosi , A. Troja , M. Tucci , C. Valieri , A. Venhola , D. Vergani , G. Verza , P. Vielzeuf , N. A. Walton , D. Scott

Environmental Dependence of Properties of Galaxies in the Sloan Digital Sky Survey

We investigate the dependence of physical properties of galaxies brighter than M_r=-18.0 in the SDSS on environment, as measured by local density using an adaptive smoothing kernel. We find that variations of galaxy properties with…

Astrophysics · Physics 2019-08-16 Changbom Park , Yun-Young Choi , Michael S. Vogeley , J. Richard Gott , Michael R. Blanton

The DEEP3 Galaxy Redshift Survey: The Impact of Environment on the Size Evolution of Massive Early-type Galaxies at Intermediate Redshift

Using data drawn from the DEEP2 and DEEP3 Galaxy Redshift Surveys, we investigate the relationship between the environment and the structure of galaxies residing on the red sequence at intermediate redshift. Within the massive (10 <…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Michael C. Cooper , Roger L. Griffith , Jeffrey A. Newman , Alison L. Coil , Marc Davis , Aaron A. Dutton , S. M. Faber , Puragra Guhathakurta , David C. Koo , Jennifer M. Lotz , Benjamin J. Weiner , Christopher N. A. Willmer , Renbin Yan

The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1

We measure the spatial clustering of galaxies as a function of their morphological type at z~0.8, for the first time in a deep redshift survey with full morphological information. This is obtained by combining high-resolution HST imaging…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 S. de la Torre , O. Le Fèvre , C. Porciani , L. Guzzo , B. Meneux , U. Abbas , L. Tasca , C. M. Carollo , T. Contini , J. -P. Kneib , S. J. Lilly , V. Mainieri , A. Renzini , M. Scodeggio , G. Zamorani , S. Bardelli , M. Bolzonella , A. Bongiorno , K. Caputi , G. Coppa , O. Cucciati , L. de Ravel , P. Franzetti , B. Garilli , C. Halliday , A. Iovino , P. Kampczyk , C. Knobel , A. M. Koekemoer , K. Kovac , F. Lamareille , J. -F. Le Borgne , V. Le Brun , C. Maier , M. Mignoli , R. Pelló , Y. Peng , E. Perez-Montero , E. Ricciardelli , J. Silverman , M. Tanaka , L. Tresse , D. Vergani , E. Zucca , D. Bottini , A. Cappi , P. Cassata , A. Cimatti , A. Leauthaud , D. Maccagni , C. Marinoni , H. J. McCracken , P. Memeo , P. Oesch , L. Pozzetti , R. Scaramella