Powered by OpenAIRE graph
Found an issue? Give us feedback
ZENODOarrow_drop_down
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
versions View all 2 versions
addClaim

Data for figures in paper "Luminosity and stellar mass functions of faint photometric satellites around spectroscopic central galaxies from DESI Year-1 Bright Galaxy Survey"

Authors: Wang, Wenting;

Data for figures in paper "Luminosity and stellar mass functions of faint photometric satellites around spectroscopic central galaxies from DESI Year-1 Bright Galaxy Survey"

Abstract

This repository provides all data that can be used to reproduce figures in following paper: Luminosity and stellar mass functions of faint photometric satellites around spectroscopic central galaxies from DESI Year-1 Bright Galaxy Survey ----------------------------------------------------------------------------------Description of contents: #tab1.txt.tar.gz: Data for Figure 1 of the paper. After decompressing the tar file, there are two separate files named 'tab1.txt' and 'tab1_mean_median_scatter.txt'. tab1.txt contains data for black scatter points in Figure 1, and tab1_mean_median_scatter.txt contains data for the mean, median and scatter. #tab2.txt.tar.gz: Data for Figure 2 of the paper. After decompressing the tar file, there are three separate files named 'tab2_black.txt', 'tab2_green.txt' and 'tab2_red.txt', corresponding to the black plain, green plain and red hatched histograms in Figure 2. #tab3.txt: Data for Figure 3 of the paper. #tab4.txt.tar.gz: Data for Figure 4 of the paper. After decompressing the tar file, there are four separate files named 'tab4_desi.txt', 'tab4_sdss.txt', 'tab4_matched_desimass.txt' and 'tab4_matched_sdssmass.txt', corresponding to the measurements in Figure 4 based on DESI stellar mass, on SDSS stellar mass, on the matched part between DESI and SDSS but using DESI stellar mass, and on the matched part using SDSS stellar mass, respectively. All 10 panels with stellar mass above logM_\ast/msun>7.1 are merged in a single file for the most massive panel to less massive panels, with different panels separated by an empty line. #tab5.txt.tar.gz: Data for Figure 5 of the paper. After decompressing the tar file, there are two separate files named 'tab5_cigale.txt' and 'tab5_fastspecfit.txt', corresponding to the measurements based on Cigale and DESI stellar masses, respectively. All 10 panels with stellar mass above logM_\ast/msun>7.1 are merged in a single file for the most massive panel to less massive panels, with different panels separated by an empty line. #tab6.txt.tar.gz: Data for Figure 6 of the paper. After decompressing the tar file, there are two separate files named 'tab6.txt' and 'tab6_median_scatter.txt'. tab6.txt contains data for scatter points in Figure 6, with the third column indicating FLAGINFRARED, which is adopted to color code the points in gray scale. tab6_median_scatter.txt contains data for the associated median and scatter. #tab7.txt: Data for Figure 7 of the paper. All 10 panels with stellar mass above logM_\ast/msun>7.1 are merged in a single file for the most massive panel to less massive panels, with different panels separated by an empty line. #tab8.txt: Data for Figure 9 of the paper. All 10 panels with stellar mass above logM_\ast/msun>7.1 are merged in a single file for the most massive panel to less massive panels, with different panels separated by an empty line. -----------------------------------------------------------------------------------System requirements: All data files are in ASCII formates, without particular system requirements to read. -----------------------------------------------------------------------------------Additional comments: Data associated with Figures 8 and 10 are provided in tables of the main text, and are thus not separatedly provided. If you use data associated with this paper, please incorporate a reference.

Related Organizations
  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average