Grau, Sergi
En el primer capítulo del influyente libro The Content and the Form. Narrative Discourse and Historical Representation (Baltimore & London 1987), Hayden White plantea que ni siquiera el formato historiográfico mínimo de la crónica y del catálogo le permite escapar de la formulación literaria que todo relato conlleva. En este estudio pretendemos dem...
Zhang, Q. F. Qin, W. H. Ma, Y. L. Lainey, V. Cooper, N. J. Rambaux, N. Li, Y. Zhu, W. H.
Phoebe is the only major satellite of Saturn with a retrograde orbit. The Cassini Imaging Science Subsystem (ISS) took a lot of Phoebe images between 2004 and 2017, but only a selection of them has been reduced. In this paper, we reduced the remaining ISS images of Phoebe. In the reduction, the Gaia EDR3 catalogue was used to provide the reference ...
Parker, Quentin A.
Published in
Frontiers in Astronomy and Space Sciences
This review provides useful background and information on how we find, vet and compile Planetary Nebulae (PNe) candidates and verify them. It presents a summary of the known Galactic PNe population and their curation in the Hong Kong/AAO/Strasbourg/Hα PNe catalogue, “HASH”. It is a simple introduction for anyone interested in working with PNe, incl...
Dálya, G. Díaz, R. Bouchet, F. R. Frei, Z. Jasche, J. Lavaux, G. Macas, R. Mukherjee, S. Pálfi, M. de Souza, R. S.
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We present GLADE+, an extended version of the GLADE galaxy catalogue introduced in our previous paper for multimessenger searches with advanced gravitational-wave detectors. GLADE+ combines data from six separate but not independent astronomical catalogues: the GWGC, 2MPZ, 2MASS XSC, HyperLEDA, and WISExSCOSPZ galaxy catalogues, and the SDSS-DR16Q ...
Scicluna, P; Kemper, F; McDonald, I; Srinivasan, S; Trejo, A; Wallstrom, SHJ; 126568; Wouterloot, JGA; Cami, J; Greaves, J; He, Jinhua;
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status: published
Driver, Simon P. Bellstedt, Sabine Robotham, Aaron S.~G. Baldry, Ivan K. Davies, Luke J. Liske, Jochen Obreschkow, Danail Taylor, Edward N. Wright, Angus H. Alpaslan, Mehmet
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In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra, and, in combination with earlier surveys, results in 330 542 redshifts across five sky regions covering ∼250 deg2. The redshift density, is the highest available over such a sustained area, has excep...
Gatti, M. Sheldon, E. Amon, A. Becker, M. Troxel, M. Choi, A. Doux, C. MacCrann, N. Alsina, A. Navarro Harrison, I.
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We present and characterise the galaxy shape catalogue from the first 3 years of Dark Energy Survey (DES) observations, over an effective area of ~4143 deg$^2$ of the southern sky. We describe our data analysis process and our self-calibrating shear measurement pipeline METACALIBRATION, which builds and improves upon the pipeline used in the DES Ye...
Jarvis, M. Bernstein, G. M. Amon, A. Davis, C. Léget, P. F. Bechtol, K. Harrison, I. Gatti, M. Roodman, A. Chang, C.
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We introduce a new software package for modeling the point-spread function (PSF) of astronomical images, called Piff (PSFs In the Full FOV), which we apply to the first three years (known as Y3) of the Dark Energy Survey (DES) data. We describe the relevant details about the algorithms used by Piff to model the PSF, including how the PSF model vari...
Hartley, W. G. Choi, A. Amon, A. Gruendl, R. A. Sheldon, E. Harrison, I. Bernstein, G. M. Sevilla-Noarbe, I. Yanny, B. Eckert, K.
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We describe the Dark Energy Survey (DES) Deep Fields, a set of images and associated multi-wavelength catalogue ($ugrizJHKs$) built from Dark Energy Camera (DECam) and Visible and Infrared Survey Telescope for Astronomy (VISTA) data. The DES Deep Fields comprise 11 fields (10 DES supernova fields plus COSMOS), with a total area of $\sim30~$ square ...
Kourkchi, Ehsan Tully, R. Brent Courtois, Helene M. Dupuy, Alexandra Guinet, Daniel
The interstellar gas in spiral galaxies can constitute a significant fraction of the baryon mass and it has been demonstrated that the sum of stellar and gas components correlates well with the kinematic signature of the total mass content, the widths of HI line profiles. The correlation of baryonic mass with HI line widths is used here to obtain d...