PPCC 2022 - Postdoctoral position in spatially-resolved star formation at the nearby Universe
2022-05-03 9:45
Ref0101 / Deadline: June 3rd, 2022
Cerrado/ClosedOffer description
The "Centro de Estudios de Física del Cosmos de Aragón" (CEFCA) invites applications for a postdoctoral position starting as soon as possible. The position, with a duration of at least 2 years, is conceived within the framework of the Complementary Plans (Planes Complementarios) Programme 2022-2025 Astrophysics and High Energy Physics: “Tecnologías avanzadas para la exploración del universo y sus componentes”; an action of the Recovery, Transformation and Resilience Plan (PRTR-C17.I1).
The applicant will conduct research related with the estimation and analysis of the spatially-resolved star-formation main sequence at the nearby Universe using the J-PLUS DR3, covering more than 3000 deg² with 12 optical filters. The J-PLUS data are sensitive to H-α emission at d < 75 Mpc, providing unbiased estimates of the star formation rate and the local main sequence [1, 2]. The one arcsecond spatial resolution of J-PLUS allows the study of the resolved star-formation main sequence (rSFMS) and the estimation of star-formation radial profiles, complementing integral field unit surveys such as CALIFA, MaNGA, SAMI or WEAVE. The successful candidate will use the J-PLUS DR3 data to derive the rSFMS and star-formation gradients for around 1000 galaxies at d < 75 Mpc, and analyze their dependence on stellar mass and morphology. The study of the low surface brightness structures at the outskirts of the nearests galaxies will be also explored, looking for low levels of star formation and complementing the multilter information with the deeper JEDIS-g and Euclid images. Finally, the spatially-resolved star formation properties of the nearby galaxies in the available J-PAS data will be studied.
CEFCA in a nutshell
CEFCA is a research institution located in Teruel, Spain, in charge of the operation, data management and scientific exploitation of the Observatorio Astrofísico de Javalambre (OAJ), an astronomical facility specifically suited for carrying out large astronomical surveys with very large field-of-view (FoV) telescopes: the 2.5m Javalambre Survey Telescope (JST250; 3deg diameter FoV) and the 83cm Javalambre Auxiliary Survey Telescope (JAST80; 2deg diameter FoV).
JST250 is equipped with JPCam, a ~1.2Mpix panoramic camera consisting of a mosaic of 14 CCDs of ~9.2k x 9.2kpix. The JPCam@JST250 system provides a 4.7 deg2 FoV and hosts a completely new set of 54 filters of ~140A width, covering the whole optical spectral range plus two broader filters at the blue and the red ends. The technical first light of JPCam@JST250 was achieved in June 2020. During the next years, JPCam@JST250 will be mostly devoted to carrying out the Javalambre Physics of the accelerating Universe Astrophysical Survey (J-PAS), which will produce photo-spectra of hundreds of millions of astronomical objects with a wide range of applications in Astrophysics and Cosmology.
JAST80 is equipped with the panoramic camera T80Cam, hosting one CCD identical to those in JPCam. The T80Cam@JAST80 system provides an effective FoV of 2 deg2. Since 2016, it is primarily devoted to conducting the Javalambre Photometric Local Universe Survey (J-PLUS), whose third data release, amounting ~3000 deg2 is expected in September 2022.
The OAJ is a Spanish ICTS (Unique Scientific and Technical Infrastructure). As such, CEFCA offers 20% of OAJ Open Time to competitive PI projects. In addition, CEFCA is a leading node of the Ground Segment OU-EXT of the ESA Euclid mission, JPCam@JST250 will conduct the Javalambre-Euclid Deep Imaging Survey in g-band (JEDIS-g) in the next years.
The OAJ data are reduced, calibrated and released by the Unit for Processing and Archiving Data (UPAD) at CEFCA. In addition, the data from the main CEFCA surveys like J-PAS and J-PLUS are validated and exploited at a scientific level by the members of the Research Area at CEFCA.
Valuable Knowledge and Experience
- Excellent research record in the topic of star-forming galaxies at any cosmic time.
- Experience in the analysis of medium- and narrow-band photometry will be an asset.
- Expertise in spatially-resolved studies of galaxies, either with photometry or spectroscopy.
Evaluation process
The committee, formed by several CEFCA members, will first evaluate the suitability of the candidates on the basis of their CVs, research statements and reference letters. The best candidates will be shortlisted for a final interview.
Being aware of the impact of family leaves on scientific careers (maternity, paternity, adoption, or leaves to take care of family members with serious health conditions), properly justified family leaves will be taken into consideration during the evaluation process.
Terms and conditions
Education: | Applicants should hold a PhD in Physics/Astronomy or equivalent. |
Languages: | Fluent in English |
Work Place: | CEFCA Headquarters, Teruel, Spain |
Contract Duration: | The appointment is for at least 2 years, with possible extensions subject to funding availability and the timescale of the project. |
Deadline: | June 3rd, 2022, 14:00h CEST |
Applications: | In order to be considered, the applications should include: 1) a CV, 2) a brief research statement regarding J-PLUS on the spatially-resolved star formation topic, and 3) a minimum of two reference letters, to be submitted via email (Subject: "Ref.0101. Postdoc PPCC-IFU”) to jobs@cefca.es by the aforementioned deadline. The letters should be directly submitted to the email address by the referees.
CEFCA is an equal opportunity employer committed to increasing diversity in its workplace. Applications of candidates from underrepresented social groups in our staff are welcome. CEFCA is committed to promoting gender parity among its staff. Hence, applications from women are strongly welcome. |
For further information, please contact:
C. López San Juan, clsj@cefca.es
Contrato financiado con el PRTR
El Plan de Recuperación, Transformación y Resiliencia del Gobierno traza la hoja de ruta para la modernización de la economía española, la recuperación del crecimiento económico y la creación de empleo, para la reconstrucción económica sólida, inclusiva y resiliente tras la crisis de la COVID, y para responder a los retos de la próxima década. Este Plan recibirá la financiación de los fondos Next Generation EU, entre ellos el Mecanismo de Recuperación y Resiliencia.
El componente 17 del Plan, denominado "Reforma institucional y fortalecimiento de las capacidades del sistema nacional de ciencia, tecnología e innovación", pretende reformar el Sistema Español de Ciencia, Tecnología y de Innovación (SECTI) para adecuarlo a los estándares internacionales y permitir el desarrollo de sus capacidades y recursos. Se propone utilizar los recursos públicos para realizar cambios rápidos que adapten y mejoren la eficacia, la coordinación y colaboración y transferencia entre los agentes del SECTI y la atracción del sector privado, con gran impacto en el corto plazo sobre la recuperación económica y social del país. El compromiso claro del país de incrementar y acelerar la inversión en I+D+I de forma sostenible a largo plazo, hasta alcanzar la media europea en 2027, requerirá cambios estructurales, estratégicos y de digitalización en el sistema para ser eficiente. En este componente se marca una orientación estratégica y coordinada que permitirá la inversión en áreas prioritarias de I+D+I y el incremento del volumen de ayudas públicas a la innovación empresarial, en particular a las PYMEs.
Concretamente, esta convocatoria está incluida dentro del área de interés científico-técnica “Astrofísica y Física de Altas Energías” de los Planes Complementarios de I+D+I con las comunidades autónomas. Estos planes permitirán establecer colaboraciones y alinear los esfuerzos de la administración central, las comunidades autónomas y los fondos europeos ante retos clave de nuestro país, respondiendo a los criterios de la UE para la aplicación de medidas transformadoras para nuestra economía en el Plan de Recuperación.
Conforme a la Ley Orgánica 15/1999, de Protección de Datos de Carácter Personal, le informamos que los datos facilitados por usted mediante su currículum vitae serán incorporados y/o actualizados en los ficheros de Fundación Centro de Estudios de Física del Cosmos de Aragón y debidamente inscritos en el Registro de la Agencia de Protección de Datos, de los que es responsable Fundación Centro de Estudios de Física del Cosmos de Aragón, con CIF G44227148.
La finalidad de esta recogida de datos será la de gestionar el proceso de selección de personal actual o futuro. Usted da, como titular de los datos, su consentimiento y autorización para la inclusión de los mismos en el fichero anteriormente detallado.
En el caso que se produzca en un futuro alguna modificación de sus datos, le rogamos nos lo comunique debidamente por escrito.
En cualquier caso, podrá ejercitar gratuitamente los derechos de acceso, rectificación, cancelación y oposición mediante escrito acompañado de copia de su DNI a la dirección CEFCA, Plaza San Juan 1, 2ª Planta, 44001 Teruel o enviándonos un correo electrónico firmado electrónicamente a la dirección jobs@cefca.es.