CaliforniaSchoolsRussell Westbrook Why Not? High

Russell Westbrook Why Not? High

PublicRegularCharterGrades 912
Bell, California · Russell Westbrook Why Not? High District
SCHOOL SNAPSHOT
Students409
Student:Teacher17.0:1
Free/Reduced Lunch83%
Title INo

Key Indicators

At-a-glance snapshot, compared to state averages where available

State avg: 489
409
Total Enrollment
State avg: 65%
83%+18.2pp
Free/Reduced Lunch
17.0:1
Student : Teacher
Public
Sector
No
Title I
Charter
Charter
9–12
Grade Span
High
Level

Overview

Russell Westbrook Why Not? High is a public high serving grades 9–12 in Bell, California. The school enrolls 409 students. It is part of the Russell Westbrook Why Not? High District district. The school operates as a charter school.

Source: NCES CCD (2023)

Strengths & Things to Consider

Indicators pulled CCD and benchmarked against California state averages. This is not a ranking — different families value different things.

Strengths

Charter school with flexibility in curriculum
Publicly funded with greater autonomy over instruction and staffing

Things to Consider

Higher share of students from low-income families
83% free/reduced-lunch eligibility — schools in this range benefit from strong parent engagement programs

Key Facts

SectorPublic
School TypeRegular
LevelHigh
Grade Span9–12
DistrictRussell Westbrook Why Not? High District
County6037
CityBell
ZIP90201
CharterYes
MagnetNo
Title INo
NCES School ID060161214144

Student Demographics

Total Enrollment409
White0.0%
Hispanic / Latino72.1%
Black / African American0.0%
Asian27.5%
American Indian / Alaska Native0.0%
Native Hawaiian / Pacific Islander0.0%
Two or More Races0.5%

Race / Ethnicity Distribution

White
0.0%
Hispanic
72.1%
Black
0.0%
Asian
27.5%
Two+
0.5%
Source: NCES CCD (2023)

Equity & Title I

In the United States, Free/Reduced Lunch (FRL) eligibility is the primary federal proxy for student poverty. Schools with 40% or more FRL-eligible students typically qualify for Title I school-wide programs.

FRL %83%
State Avg65%
Title INo
Source: NCES CCD (2023)