Zobrazeno 1 - 10
of 23
pro vyhledávání: '"T. M. Heckman"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 379:894-908
The prevalence of radio-loud AGN activity in present-day massive halos is determined using a sample of 625 nearby groups and clusters selected from the Sloan Digital Sky Survey. Brightest group and cluster galaxies (BCGs) are more likely to host a ra
Autor:
M. S. Oey, G. R. Meurer, S. Yelda, E. J. Furst, S. M. Caballero‐Nieves, D. J. Hanish, E. M. Levesque, D. A. Thilker, G. L. Walth, J. Bland‐Hawthorn, M. A. Dopita, H. C. Ferguson, T. M. Heckman, M. T. Doyle, M. J. Drinkwater, K. C. Freeman, R. C. Kennicutt, Jr., V. A. Kilborn, P. M. Knezek, B. Koribalski, M. Meyer, M. E. Putman, E. V. Ryan‐Weber, R. C. Smith, L. Staveley‐Smith, R. L. Webster, J. Werk, M. A. Zwaan
Publikováno v:
The Astrophysical Journal. 661:801-814
We use the first data release from the SINGG H-alpha survey of HI-selected galaxies to study the quantitative behavior of the diffuse, warm ionized medium (WIM) across the range of properties represented by these 109 galaxies. The mean fraction f_WIM
Autor:
V. Smolčić, Ž. Ivezić, M. Gaćeša, K. Rakos, K. Pavlovski, S. Ilijić, M. Obrić, R. H. Lupton, D. Schlegel, G. Kauffmann, C. Tremonti, J. Brinchmann, S. Charlot, T. M. Heckman, G. R. Knapp, J. E. Gunn, J. Brinkmann, I. Csabai, M. Fukugita, J. Loveday
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 371:121-137
We discuss the colors of 99,088 galaxies selected from the Sloan Digital Sky Survey Data Release 1 "main" spectroscopic sample (a flux limited sample, rPet < 17.77, for 1360 deg 2 ) in the rest-frame Stromgren system (uz, vz, bz, yz). This narrow-ban
Autor:
Gerhardt R. Meurer, D. J. Hanish, H. C. Ferguson, P. M. Knezek, V. A. Kilborn, M. E. Putman, R. C. Smith, B. Koribalski, M. Meyer, M. S. Oey, E. V. Ryan‐Weber, M. A. Zwaan, T. M. Heckman, R. C. Kennicutt, Jr., J. C. Lee, R. L. Webster, J. Bland‐Hawthorn, M. A. Dopita, K. C. Freeman, M. T. Doyle, M. J. Drinkwater, L. Staveley‐Smith, J. Werk
Publikováno v:
The Astrophysical Journal Supplement Series. 165:307-337
We introduce the Survey for Ionization in Neutral Gas Galaxies (SINGG), a census of star formation in HI-selected galaxies. The survey consists of H-alpha and R-band imaging of a sample of 468 galaxies selected from the HI Parkes All Sky Survey (HIPA
Autor:
S. G. Neff, D. A. Thilker, M. Seibert, A. Gil de Paz, L. Bianchi, D. Schiminovich, D. C. Martin, B. F. Madore, R. M. Rich, T. A. Barlow, Y.-I. Byun, J. Donas, K. Forster, P. G. Friedman, T. M. Heckman, P. N. Jelinsky, Y.-W. Lee, R. F. Malina, B. Milliard, P. Morrissey, O. H. W. Siegmund, T. Small, A. S. Szalay, B. Y. Welsh, T. K. Wyder
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2005, 619L, pp.91. ⟨10.1086/426137⟩
The Astrophysical Journal, 2005, 619L, pp.91. ⟨10.1086/426137⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astrophysical Journal, American Astronomical Society, 2005, 619L, pp.91. ⟨10.1086/426137⟩
The Astrophysical Journal, 2005, 619L, pp.91. ⟨10.1086/426137⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
New GALEX observations have detected significant FUV (1530 Angstroms) and NUV (2310 Angstroms) emission from stellar substructures within the tidal tails of four ongoing galaxy mergers. The UV-bright regions are optically faint and are coincident wit
Autor:
Huub Röttgering, T. M. Heckman, C. J. Lonsdale, J. J. Condon, Q. F. Yin, Seb Oliver, Helen Smith, C. D. Martin, D. Schiminovich, W. D. Cotton
Publikováno v:
Symposium - International Astronomical Union. 216:363-370
Far-infrared (FIR), ultraviolet (UV), and soft X-ray observations are easily degraded by dust and gas between the source and the telescope. They must be made from space, where they are still affected by the interstellar medium (ISM) of our Galaxy. Fo
Autor:
G. A. Bower, R. F. Green, A. Danks, T. Gull, S. Heap, J. Hutchings, C. Joseph, M. E. Kaiser, R. Kimble, S. Kraemer, D. Weistrop, B. Woodgate, D. Lindler, R. S. Hill, E. M. Malumuth, S. Baum, V. Sarajedini, T. M. Heckman, A. S. Wilson, D. O. Richstone
Publikováno v:
The Astrophysical Journal. 492:L111-L114
We present optical long-slit spectroscopy of the nucleus of the nearby radio galaxy M84 (NGC 4374 = 3C 272.1) obtained with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope (HST). Our spectra reveal that the nuclear g
Autor:
J. Iglesias‐Paramo, V. Buat, T. T. Takeuchi, K. Xu, S. Boissier, A. Boselli, D. Burgarella, B. F. Madore, A. Gil de Paz, L. Bianchi, T. A. Barlow, Y.‐I. Byun, J. Donas, K. Forster, P. G. Friedman, T. M. Heckman, P. N. Jelinski, Y.‐W. Lee, R. F. Malina, D. C. Martin, B. Milliard, P. F. Morrissey, S. G. Neff, R. M. Rich, D. Schiminovich, M. Seibert, O. H. W. Siegmund, T. Small, A. S. Szalay, B. Y. Welsh, T. K. Wyder
Publikováno v:
Astrophysical Journal Supplement
Astrophysical Journal Supplement, American Astronomical Society, 2006, 164, pp.38
The Astrophysical Journal Supplement
The Astrophysical Journal Supplement, 2006, 164, pp.38
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Astrophysical Journal Supplement, American Astronomical Society, 2006, 164, pp.38
The Astrophysical Journal Supplement
The Astrophysical Journal Supplement, 2006, 164, pp.38
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
This work presents the main ultraviolet (UV) and far-infrared (FIR) properties of two samples of nearby galaxies selected from the GALEX ($\lambda = 2315$\AA, hereafter NUV) and IRAS ($\lambda = 60\mu$m) surveys respectively. They are built in order
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f682772de41a3cbf2bc7d4157285e9de
https://hal.archives-ouvertes.fr/hal-00082572
https://hal.archives-ouvertes.fr/hal-00082572
Autor:
S. Arnouts, D. Schiminovich, O. Ilbert, L. Tresse, B. Milliard, M. Treyer, S. Bardelli, T. Budavari, T. K. Wyder, E. Zucca, O. Le Fèvre, D. C. Martin, G. Vettolani, C. Adami, M. Arnaboldi, T. Barlow, L. Bianchi, M. Bolzonella, D. Bottini, Y.-I. Byun, A. Cappi, S. Charlot, T. Contini, J. Donas, K. Forster, S. Foucaud, P. Franzetti, P. G. Friedman, B. Garilli, I. Gavignaud, L. Guzzo, T. M. Heckman, C. Hoopes, A. Iovino, P. Jelinsky, V. Le Brun, Y.-W. Lee, D. Maccagni, B. F. Madore, R. Malina, B. Marano, C. Marinoni, H. J. McCracken, A. Mazure, B. Meneux, R. Merighi, P. Morrissey, S. Neff, S. Paltani, R. Pellò, J. P. Picat, A. Pollo, L. Pozzetti, M. Radovich, R. M. Rich, R. Scaramella, M. Scodeggio, M. Seibert, O. Siegmund, T. Small, A. S. Szalay, B. Welsh, C. K. Xu, G. Zamorani, A. Zanichelli
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, 2005, 619, pp.43A. ⟨10.1086/426733⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2005, 619, pp.43A. ⟨10.1086/426733⟩
The Astrophysical journal letters, 2005, 619, pp.43A. ⟨10.1086/426733⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2005, 619, pp.43A. ⟨10.1086/426733⟩
We present the first measurement of the galaxy luminosity function (LF) at 1500 Å in the range 0.2=alpha>=-1.65, with a marginally significant hint of increase at higher z. (3) We split the sample in three rest-frame (B-I) intervals, providing an ap
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::213af39e7d4fd49575823d619c360771
https://hal.science/hal-00012578
https://hal.science/hal-00012578
Autor:
D. Schiminovich, O. Ilbert, S. Arnouts, B. Milliard, L. Tresse, O. Le Fèvre, M. Treyer, T. K. Wyder, T. Budavári, E. Zucca, G. Zamorani, D. C. Martin, C. Adami, M. Arnaboldi, S. Bardelli, T. Barlow, L. Bianchi, M. Bolzonella, D. Bottini, Y.-I. Byun, A. Cappi, T. Contini, S. Charlot, J. Donas, K. Forster, S. Foucaud, P. Franzetti, P. G. Friedman, B. Garilli, I. Gavignaud, L. Guzzo, T. M. Heckman, C. Hoopes, A. Iovino, P. Jelinsky, V. Le Brun, Y.-W. Lee, D. Maccagni, B. F. Madore, R. Malina, B. Marano, C. Marinoni, H. J. McCracken, A. Mazure, B. Meneux, P. Morrissey, S. Neff, S. Paltani, R. Pellò, J. P. Picat, A. Pollo, L. Pozzetti, M. Radovich, R. M. Rich, R. Scaramella, M. Scodeggio, M. Seibert, O. Siegmund, T. Small, A. S. Szalay, G. Vettolani, B. Welsh, C. K. Xu, A. Zanichelli
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2005, 619L, pp.47. ⟨10.1086/427077⟩
The Astrophysical Journal, 2005, 619L, pp.47. ⟨10.1086/427077⟩
The Astrophysical Journal, American Astronomical Society, 2005, 619L, pp.47. ⟨10.1086/427077⟩
The Astrophysical Journal, 2005, 619L, pp.47. ⟨10.1086/427077⟩
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and at higher z using existing data sets. In this paper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6fa168a615571ba5fe85b2e9dec86131
https://hal.archives-ouvertes.fr/hal-00015220
https://hal.archives-ouvertes.fr/hal-00015220