TY - JOUR
T1 - The EDGE-CALIFA Survey
T2 - An Extragalactic Database for Galaxy Evolution Studies
AU - Wong, Tony
AU - Cao, Yixian
AU - Luo, Yufeng
AU - Bolatto, Alberto D.
AU - Sánchez, Sebastián F.
AU - Barrera-Ballesteros, Jorge K.
AU - Blitz, Leo
AU - Colombo, Dario
AU - Dannerbauer, Helmut
AU - Green, Alex
AU - Kalinova, Veselina
AU - Khan, Ferzem
AU - Kim, Andrew
AU - Lacerda, Eduardo A.D.
AU - Leroy, Adam K.
AU - Levy, Rebecca C.
AU - Lin, Xincheng
AU - Luo, Yuanze
AU - Rosolowsky, Erik W.
AU - Rubio, Mónica
AU - Teuben, Peter
AU - Utomo, Dyas
AU - Villanueva, Vicente
AU - Vogel, Stuart N.
AU - Wang, Xinyu
N1 - Publisher Copyright:
© 2024. The Author(s). Published by the American Astronomical Society.
PY - 2024/3/1
Y1 - 2024/3/1
N2 - The EDGE-CALIFA survey provides spatially resolved optical integral-field unit and CO spectroscopy for 125 galaxies selected from the Calar Alto Legacy Integral Field Area Survey (CALIFA) Data Release 3 sample. The Extragalactic Database for Galaxy Evolution (EDGE) presents the spatially resolved products of the survey as pixel tables that reduce the oversampling in the original images and facilitate comparison of pixels from different images. By joining these pixel tables to lower-dimensional tables that provide radial profiles, integrated spectra, or global properties, it is possible to investigate the dependence of local conditions on large-scale properties. The database is freely accessible and has been utilized in several publications. We illustrate the use of this database and highlight the effects of CO upper limits on the inferred slopes of the local scaling relations between the stellar mass, star formation rate (SFR), and H2 surface densities. We find that the correlation between H2 and SFR surface density is the tightest among the three relations.
AB - The EDGE-CALIFA survey provides spatially resolved optical integral-field unit and CO spectroscopy for 125 galaxies selected from the Calar Alto Legacy Integral Field Area Survey (CALIFA) Data Release 3 sample. The Extragalactic Database for Galaxy Evolution (EDGE) presents the spatially resolved products of the survey as pixel tables that reduce the oversampling in the original images and facilitate comparison of pixels from different images. By joining these pixel tables to lower-dimensional tables that provide radial profiles, integrated spectra, or global properties, it is possible to investigate the dependence of local conditions on large-scale properties. The database is freely accessible and has been utilized in several publications. We illustrate the use of this database and highlight the effects of CO upper limits on the inferred slopes of the local scaling relations between the stellar mass, star formation rate (SFR), and H2 surface densities. We find that the correlation between H2 and SFR surface density is the tightest among the three relations.
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U2 - 10.3847/1538-4365/ad20c9
DO - 10.3847/1538-4365/ad20c9
M3 - Article
AN - SCOPUS:85187369011
SN - 0067-0049
VL - 271
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
IS - 1
M1 - 35
ER -