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Arizona State University
4.2
based on 11 Reviews
Working at Arizona State University
Company Summary
Overall Rating
4.2/5
based on 11 reviews
14% above
industry average
Highly rated for
Company culture, Work-life balance, Work satisfaction
Critically rated for
Promotions
Work Policy
Monday to Friday
100% employees reported
Flexible timing
86% employees reported
No travel
83% employees reported
View detailed work policy
Top Employees Benefits
Office cab/shuttle
1 employee reported
View detailed benefits
About Arizona State University
Founded in--
India Employee Count--
Global Employee Count--
Headquarters--
Office Locations
--
Websiteasu.edu
Primary Industry
Other Industries
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Arizona State University Ratings
based on 11 reviews
Overall Rating
4.2/5
How AmbitionBox ratings work?
5
6
4
3
3
0
2
0
1
2
Category Ratings
4.1
Company culture
4.1
Work-life balance
3.8
Work satisfaction
3.7
Skill development
3.6
Job security
3.6
Salary
3.3
Promotions
Arizona State University is rated 4.2 out of 5 stars on AmbitionBox, based on 11 company reviews. This rating reflects a generally positive employee experience, indicating satisfaction with the company’s work culture, benefits, and career growth opportunities. AmbitionBox gathers authentic employee reviews and ratings, making it a trusted platform for job seekers and employees in India.
Read more
Arizona State University Reviews
Compare Arizona State University with Similar Companies
Change Company | Change Company | Change Company | ||
|---|---|---|---|---|
Overall Rating | 4.2/5 based on 11 reviews | 3.6/5 based on 38.9k reviews | 3.7/5 based on 89k reviews | 4.5/5 based on 32 reviews |
Highly Rated for | Work-life balance Company culture Work satisfaction | Job security | Job security Work-life balance | Skill development Company culture Work satisfaction |
Critically Rated for | Promotions | Salary Promotions Work satisfaction | Promotions Salary Work satisfaction | No critically rated category |
Primary Work Policy | - | Hybrid 86% employees reported | Work from office 80% employees reported | - |
Rating by Women Employees | 4.3 Good rated by 4 women | 3.7 Good rated by 11.6k women | 3.8 Good rated by 25.8k women | 4.9 Excellent rated by 11 women |
Rating by Men Employees | 3.8 Good rated by 5 men | 3.6 Good rated by 24.7k men | 3.6 Good rated by 58.1k men | 4.1 Good rated by 20 men |
Job security | 3.6 Good | 4.1 Good | 4.5 Good | 4.2 Good |
View more
Arizona State University Salaries
Arizona State University salaries have received with an average score of 3.6 out of 5 by 11 employees.
Data Scientist
(2 salaries)
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₹22.5 L/yr - ₹28.8 L/yr
Master Student
(2 salaries)
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₹14 L/yr - ₹17.8 L/yr
Data Analyst
(2 salaries)
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₹18.7 L/yr - ₹23.9 L/yr
Web Developer
(2 salaries)
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₹19.4 L/yr - ₹24.7 L/yr
Web Designer
(2 salaries)
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₹21.6 L/yr - ₹27.6 L/yr
Postdoctoral Research Associate
(2 salaries)
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₹32.2 L/yr - ₹41.2 L/yr
Java Developer
(1 salaries)
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₹27 L/yr - ₹34.5 L/yr
Graduate Teaching Assistant
(1 salaries)
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₹6.3 L/yr - ₹8 L/yr
Director Human Resources
(1 salaries)
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₹21.9 L/yr - ₹27.9 L/yr
Software Engineer
(1 salaries)
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₹12.6 L/yr - ₹16.1 L/yr
Arizona State University News
HonorHealth Research Institute Appoints Renowned Expert in Anti-Cancer Drug Development to Lead New Center for Translational Science
- HonorHealth Research Institute appoints Dr. Sunil Sharma as the Director of the new Center for Translational Science, heralding a significant advancement in anti-cancer drug development and research.
- Dr. Sharma, known for his extensive experience in anti-cancer drug development, assumes the role after a distinguished career spanning over three decades in the field.
- His appointment marks a strategic move by the institute to enhance patient outcomes through innovative medical research and bridge the gap between laboratory discoveries and clinical application.
- Dr. Sharma's expertise in research design, drug development, and clinical trial methodology positions him as a key figure in advancing cancer therapies at the institute.
- Under his leadership, a multidisciplinary team will collaborate to develop cutting-edge therapies that aim to improve the quality of life for cancer patients.
- The appointment aligns with HonorHealth Research Institute's partnership with Arizona State University, promoting a seamless transfer of knowledge and technology for enhanced patient care.
- Dr. Sharma's notable accomplishments include advancing cancer treatment through therapies like ceritinib, pembrolizumab, and nivolumab, contributing to personalized medicine and tailored treatment strategies.
- His focus on translational medicine underscores a commitment to developing innovative therapies that consider both the biological aspects of the disease and patient-centered approaches for holistic well-being.
- Dr. Sharma's appointment to the Virginia G. Piper Distinguished Chair in Innovative Cancer Research exemplifies the institute's support for his pioneering initiatives in cancer research and clinical trials.
- His leadership at the Center for Translational Science signifies a promising future for cancer care, emphasizing research excellence, patient-centric treatment modalities, and transformative outcomes.
Bioengineer | 18 Feb, 2025
Ancient meteorite discovery may explain Earth’s missing elements
- Moderately volatile elements (MVEs) are essential for planetary chemistry, but the Earth and Mars lack vital MVEs such as copper, zinc, and potassium.
- Two potential hypotheses propose that MVEs never fully condensed in the early solar nebula, or were lost while forming planetesimals.
- Arizona State University analyzed iron meteorites, which are remnants of the metallic cores of early planetesimals. The team found evidence that inner solar system planetesimals retained significant amounts of MVEs on their first formation.
- Intense collisions during later planetary growth led to their depletion in these elements.
- MVEs were not distributed equally throughout planetesimals in the early solar system, and the loss of MVEs in terrestrial planets was more likely caused by intense collisions.
- Magmatic iron meteorites represent the metallic cores of ancient planetesimals, and are a new tool for understanding planetary formation.
- This study suggests that rather than starting out with MVEs-poor building blocks, Earth and Mars contained significant amounts of these elements, with their loss a later consequence of the shaping of terrestrial planets.
- Future research will likely identify specific types of collisions and impacts that contributed to the volatile depletion of terrestrial planets and help unravel the intricate history of the solar system.
- The study highlights the crucial role that cosmic radiation and collisions play in the formation of planets.
- Scientists' new understanding of how MVEs were initially distributed in the early solar system can refine existing models of planetary formation and help to elucidate how Earth evolved into a habitable planet.
Brighter Side of News | 9 Feb, 2025
This hot Jupiter probably formed close to its star
- Astronomers have noted that many of the gas giants observed orbited close to their stars, known as “Hot Jupiters”
- A team from Arizona State University’s School Of Earth and Space Exploration (ASU-SESE) examined the atmospheric chemistry of several Hot and Ultra-Hot Jupiters
- After examining WASP-121b, the team came to the unexpected conclusion that it likely formed close to its star.
- The research was conducted by Graduate Associate Peter C. B. Smith and other members of the ASU-SESE.
- The instrument is part of the Gemini South telescope in Chile, one of two telescopes that make up the International Gemini Observatory.
- This program aims to learn more about the protoplanetary disks from which hot gas giants formed.
- The team obtained measurements WASP-121b to determine the ratio of rocky and gaseous elements thanks to it being an ultra-hot Jupiter.
- Spectra showed that WASP-121b has a high rock-to-ice ratio, indicating that it accreted an excess of rocky material while forming.
- These results may resolve the mystery of Hot Jupiters by demonstrating that gas giants need not be composed predominantly of gaseous volatile elements, but heavier elements that are heated to the point that they become vapor.
- The team hopes that future surveys using IGRINS successor instrument – IGRINS-2 – which was commissioned for the Gemini North telescope in Hawai‘i and is currently being calibrated for science operations.
Knowridge | 6 Feb, 2025
This Hot Jupiter Probably Formed Close to Its Star
- A team of scientists have discovered that a planet, WASP-121b, which has been traditionally classified as a gas giant, may have formed close to its star. The research was conducted by Graduate Associate Peter C. B. Smith and other members of the Arizona State University’s School of Earth and Space Exploration. The team examined several Hot and Ultra-Hot Jupiters and came to the unexpected conclusion that WASP-121b likely formed close to its star.
- The team measured the ratio of rocky and gaseous elements in WASP-121b in order to determine how far from its parent star the planet may have formed. Previous measurements that obtained this ratio required multiple observations in both visible and infrared light, whereas WASP-121b was observed with the Immersion GRating INfrared Spectrograph, allowing the team to obtain high-resolution spectral data from just one observation.
- The planet's ultra-hot temperatures caused rocky material and metals to vaporize into the atmosphere, which was then blown to the night side of the planet and condensed. This resulted in the planet experiencing different types of metal rain. These findings suggest that gas giants need not be composed predominantly of gaseous volatile elements, but heavier elements that are heated to the point that they become vapor.
- As part of the Roasting Marshmallows Program, the current study could lead to astronomers updating protoplanetary disk models and planet formation theories. The program aims to study the atmospheres of hot and ultra-hot Jupiters using the Immersion GRating INfrared Spectrograph (IGRINS).
- The issue of hot Jupiters and the possibility of planets migrating is still being debated. The result of the current study adds new evidence into discussion, which could further shape the estimates about the possible number and orbits of gas giants in the future.
- The team hopes that the future surveys using IGRINS successor instrument – IGRINS-2 – will provide an even better opportunity to understand how protoplanetary disks from which hot gas giants form. IGRINS-2, which was commissioned for the Gemini North telescope in Hawai‘i and is currently being calibrated for science operations.
- The paper which presents the study welcomes discussions and further research on the existence of Hot Jupiters and the possible migration of planets. As more data comes in, there may be more conclusions and answers regarding the formation of planets.
- The Gemini South telescope in Chile, one of two telescopes that make up the International Gemini Observatory funded in part by the National Science Foundation, played an important role in the study.
- Astronomers hope that the insights from the current study help us find more about the solar system and beyond.
- The current research was presented in a paper in The Astronomical Journal. The paper is titled “Probing the Breezes of WASP-121b: Comprehensive Retrieval Analysis of HST/WFC3 Data”.
Universe Today | 6 Feb, 2025
Chip Industry Technical Paper Roundup: Nov. 5
- New technical papers recently added to Semiconductor Engineering’s library:
- - Communication Characterization of AI Workloads for Large-scale Multi-chiplet Accelerators by Universitat Politecnica de Catalunya
- - Recent Advances in Metal-Oxide-Based Photoresists for EUV Lithography by University of South–Eastern Norway
- - Impact of external magnetic fields on STT-MRAM by Univ. Grenoble Alpes, Everspin, GF, imec, et al.
- - Hacking the Fabric: Targeting Partial Reconfiguration Fault Injection in FPGA Fabrics by Arizona State University and Karlsruhe Institute of Technology (KIT)
Semiengineering | 5 Nov, 2024
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Arizona State University FAQs
Does Arizona State University have good work-life balance?
Arizona State University has a work-life balance rating of 4.1 out of 5 based on 10+ employee reviews on AmbitionBox. 82% employees rated Arizona State University 4 or above on work-life balance. This rating reflects the company's efforts to help employees maintain a healthy balance between their personal and professional lives. We encourage you to read Arizona State University reviews for more details
Is Arizona State University good for career growth?
Career growth at Arizona State University is rated as moderate, with a promotions and appraisal rating of 3.3. 18% employees rated Arizona State University 3 or below, while 82% employees rated it 4 or above on promotions/appraisal. This rating suggests that while some employees view growth opportunities favorably, there is scope for improvement based on employee feedback. We recommend reading Arizona State University reviews for more detailed insights.
What are the pros and cons of working in Arizona State University?
Working at Arizona State University comes with several advantages and disadvantages. It is highly rated for company culture, work life balance and work satisfaction. However, it is poorly rated for promotions / appraisal, based on 10+ employee reviews on AmbitionBox.
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