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 - We thank the anonymous referee for helpful suggestions, which substantially improved this paper. This work was funded in part by NSF AAG grants 1616199 and 2307440 to the University of Illinois, 1615960 and 2307441 to the University of Maryland, and 1616924 to the University of California-Berkeley. R.C.L. acknowledges partial support from a NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-2102625. M.R. wishes to acknowledge partial support from ANID Basal FB210003. V.V. acknowledges support from the scholarship ANID-FULBRIGHT BIO 2016-56160020 and funding from NRAO Student Observing Support SOSPADA-015. J.B.-B. acknowledges support from the grant IA-101522 (DGAPA-PAPIIT, UNAM) and funding from the CONACYT grant CF19-39578. Support for CARMA construction was derived from the Gordon and Betty Moore Foundation, the Kenneth T. and Eileen L. Norris Foundation, the James S. McDonnell Foundation, the Associates of the California Institute of Technology, the University of Chicago, the states of California, Illinois, and Maryland, and the NSF. CARMA development and operations were supported by the NSF under a cooperative agreement and by the CARMA partner universities. This research is based on observations collected at the Centro Astron\u00F3mico Hispano-Alem\u00E1n (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut f\u00FCr Astronomie (MPA) and the Instituto de Astrofisica de Andalucia (CSIC). This research has made use of NASA\u2019s Astrophysics Data System. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.
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 -