Calculate satellite quenched fraction
Build a confirmed-satellite sample, apply the color--magnitude quenching criterion, and calculate binned quenched fractions with Jeffreys binomial intervals.
ELVES-Dwarf · Public data
Documentation for the public ELVES-Dwarf data products, with guidance on file contents, data access and usage, and definitions of all columns and fields.
Learn with the data
Short, reproducible examples that use the same public files documented below. Read the executed notebook on this site, download it, or open it in Google Colab.
Build a confirmed-satellite sample, apply the color--magnitude quenching criterion, and calculate binned quenched fractions with Jeffreys binomial intervals.
Catalog
Properties of the ELVES-Dwarf host galaxies. Please see Table 1 of Li et al. 2026 for the description and the full reference list.
from astropy.table import Table
cat = Table.read("ELVES-Dwarf_host_cat_v1.fits")
print(cat.colnames) | Column | Type | Unit | Description |
|---|---|---|---|
name | string (10 chars) | — | Host galaxy name. |
ra | float64 | deg | Right ascension (J2000). |
dec | float64 | deg | Declination (J2000). |
isolated | boolean | — | True if the host passes the ELVES-Dwarf isolation criterion. |
has_isolation | boolean | — | True if the host galaxy has tidal indices from Karachentsev (2013). |
dist_mpc | float64 | Mpc | Adopted host distance. |
dist_err_mpc | float64 | Mpc | Uncertainty on the adopted distance. |
dist_method | string (4 chars) | — | Distance indicator used. Values: TRGB, SBF, Ceph. |
v_h_km_s | float64 | km/s | Heliocentric radial velocity. |
theta1 | float64 | — | Tidal index, considering the influence of the most dominant perturber. Negative values indicate that the host is isolated. |
theta5 | float64 | — | Tidal index, considering the influence of the five most dominant perturbers. Negative values indicate that the host is isolated. |
log_l_ks_lsun | float64 | dex (L_sun) | Log of the K_s-band luminosity. |
M_V | float64 | mag | Absolute V-band magnitude. |
g_r_0 | float64 | mag | Extinction-corrected g - r color. |
log_mstar_msun | float64 | dex (M_sun) | Log stellar mass. |
log_mstar_err | float64 | dex | Uncertainty on the log stellar mass. |
rvir_kpc | float64 | kpc | Adopted virial radius. |
area_deg2 | float64 | deg2 | Sky area searched around the host. |
frac_unmasked | float64 | — | Fraction of the searched area left unmasked. |
data_source | string (32 chars) | — | Provenance of the imaging or of the literature satellite list. |
reference | string (36 chars) | — | Reference for the adopted host distance. |
No columns match that filter.
Catalog
Catalog of all satellite candidates in ELVES-Dwarf. Please see Table 3 of Li et al. 2026 for the description and the full reference list.
from astropy.table import Table
cat = Table.read("ELVES-Dwarf_master_cat_v1.fits")
print(cat.colnames) | Column | Type | Unit | Description |
|---|---|---|---|
name | string (13 chars) | — | Satellite candidate name. |
ra | float64 | deg | Right ascension (J2000). |
dec | float64 | deg | Declination (J2000). |
host | string (10 chars) | — | Host galaxy name; joins to "name" in the host catalog. |
host_dist | float64 | Mpc | Distance of the host galaxy. |
followup | string (9 chars) | — | Follow-up data used to decide membership. Values: TRGB, Velocity, HSC-LA, HSC-SMOKA, CFHT, GMOS, IMACS, None |
distance | float64 | Mpc | Measured distance of the candidate, where available. For SBF, this is the median of the posterior distribution. |
status | string (12 chars) | — | Membership classification. Values: Confirmed, Rejected, Unconfirmed, Not Observed |
reff_sersic | float64 | arcsec | Sersic effective radius. |
err_reff_sersic | float64 | arcsec | Uncertainty on the Sersic effective radius. |
m_g_sersic | float64 | mag | Sersic apparent g-band magnitude. |
err_m_g_sersic | float64 | mag | Uncertainty on the Sersic g-band magnitude. |
m_V_sersic | float64 | mag | Sersic apparent V-band magnitude. |
err_m_V_sersic | float64 | mag | Uncertainty on the Sersic V-band magnitude. |
mu_eff_g | float64 | mag/arcsec2 | Mean g-band surface brightness within the effective radius. |
mu_0_V | float64 | mag/arcsec2 | Central V-band surface brightness. |
gr_sersic | float64 | mag | Sersic g - r color. |
err_gr_sersic | float64 | mag | Uncertainty on the Sersic g - r color. |
gi_sersic | float64 | mag | Sersic g - i color. |
n_sersic | float64 | — | Sersic index. |
ell_sersic | float64 | — | Ellipticity, 1 - b/a. |
log_m_star | float64 | dex (M_sun) | Log stellar mass. |
err_log_m_star | float64 | dex | Uncertainty on the log stellar mass. |
velocity | float64 | km/s | Radial velocity, where available. |
dist_1sigma | float64 array (2) | Mpc | Lower and upper bounds of the 68% distance interval. |
dist_2sigma | float64 array (2) | Mpc | Lower and upper bounds of the 95% distance interval. |
dist_SNR | float64 | — | Signal-to-noise of the distance measurement. |
dist_comment | string (454 chars) | — | Free-text note on the distance measurement. |
dist_method | string (4 chars) | — | Distance indicator used. Values: TRGB, SBF, Vel, Ceph |
ang_proj_kpc | float64 | kpc | Projected separation from the host. |
ang_proj_Rvir | float64 | — | Projected separation in units of the host virial radius. |
Psat | float64 | — | Satellite probability (see paper for details). |
completeness | float64 | — | Estimated detection completeness. |
reference | string (35 chars) | — | Literature reference(s) for the candidate. |
No columns match that filter.
File set
Sky coverage of the imaging searched around each ELVES-Dwarf host, as a polygon per host. Provided both as GeoJSON (for programmatic use) and as a DS9 region file (for overlaying on images).
import json
with open("DDO046_survey_footprint.geojson") as f:
fp = json.load(f)
print(fp["metadata"])
ring = fp["features"][0]["geometry"]["coordinates"][0] # [[ra, dec], ...] | File | Format | Description |
|---|---|---|
<host>_survey_footprint.geojson | GeoJSON (ICRS / fk5, degrees) | FeatureCollection with a "metadata" block and one Polygon feature per contributing survey; ring coordinates are [RA, Dec] pairs in degrees. |
<host>_survey_footprint.reg | DS9 region file (fk5) | The same polygons as DS9 regions, with the metadata repeated in header comment lines. Loads directly in DS9, and readable with the "regions" package. |
| Field | Type | Unit | Description |
|---|---|---|---|
host | string | — | Host galaxy name; joins to "name" in the host catalog. |
ra | float | deg | Right ascension of the host (J2000). |
dec | float | deg | Declination of the host (J2000). |
bands | array of string | — | Imaging bands covering the footprint (e.g. ["g", "r"]). |
r_ang_deg | float | deg | Angular radius of the search region around the host. |
distance_Mpc | float | Mpc | Adopted host distance used to set the search radius. |
surveys | array of string | — | Imaging surveys contributing to the footprint. |
General