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91探花
An image of the GOODS-South field as observed by JWST. More than 45,000 galaxies are visible here.

An image of the GOODS-South field as observed by JWST. More than 45,000 galaxies are visible here. In this image, blue, green, and red were assigned to Webb鈥檚 NIRCam (Near-Infrared Camera) data at 0.9, 1.15, and 1.5 microns; 2.0, 2.77, and 3.55 microns; and 3.56, 4.1, and 4.44 microns (F090W, F115W, and F150W; F200W, F277W, and F335M; and F356W, F410M, and F444W), respectively.

Credit: NASA, ESA, CSA, B. Robertson (UC Santa Cruz), B. Johnson (Center for Astrophysics, Harvard & Smithsonian), S. Tacchella (Univers

Dr Jacopo Chevallard

Postdoctoral Research Assistant

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
jacopo.chevallard@physics.ox.ac.uk
Telephone: 01865 273467
Denys Wilkinson Building, room 463
  • About
  • Publications

The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas* 鈭 Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.

The Astrophysical Journal Supplement Series American Astronomical Society 261:2 (2022) 31

Authors:

Danielle A Berg, Bethan L James, Teagan King, Meaghan McDonald, Zuyi Chen, John Chisholm, Timothy Heckman, Crystal L Martin, Dan P Stark, Alessandra Aloisi, Ricardo O Amor铆n, Karla Z Arellano-C贸rdova, Matthew Bayliss, Rongmon Bordoloi, Jarle Brinchmann, St茅phane Charlot, Jacopo Chevallard, Ilyse Clark, Dawn K Erb, Anna Feltre, Max Gronke, Matthew Hayes, Alaina Henry, Svea Hernandez, Anne Jaskot, Tucker Jones, Lisa J Kewley, Nimisha Kumari, Claus Leitherer, Mario Llerena, Michael Maseda, Matilde Mingozzi, Themiya Nanayakkara, Masami Ouchi, Adele Plat, Richard W Pogge, Swara Ravindranath, Jane R Rigby, Ryan Sanders, Claudia Scarlata, Peter Senchyna, Evan D Skillman, Charles C Steidel, Allison L Strom, Yuma Sugahara, Stephen M Wilkins, Aida Wofford, Xinfeng Xu

Direct Constraints on the Extremely Metal-poor Massive Stars Underlying Nebular C iv Emission from Ultra-deep HST/COS Ultraviolet Spectroscopy

The Astrophysical Journal American Astronomical Society 930:2 (2022) 105

Authors:

Peter Senchyna, Daniel P Stark, St茅phane Charlot, Adele Plat, Jacopo Chevallard, Zuyi Chen, Tucker Jones, Ryan L Sanders, Gwen C Rudie, Thomas J Cooper, Gustavo Bruzual

Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 Using the Galaxy Zoo

The Astrophysical Journal American Astronomical Society 912:1 (2021) 49-49

Authors:

Vihang Mehta, Claudia Scarlata, Lucy Fortson, Hugh Dickinson, Dominic Adams, Jacopo Chevallard, St茅phane Charlot, Melanie Beck, Sandor Kruk, Brooke Simmons

Abstract:

How does a public policy reform become seemingly inevitable? How and why does bureaucratic 鈥渃ommon sense鈥 override empirical evidence? What are the overlaps between accountability and corruption? These open-ended questions drive my study of a neglected object of analysis: the well-intentioned people and institutions working within Australia鈥檚 Indigenous affairs local government policy arena. In July 2008 the Northern Territory鈥檚 local government sector underwent the most sweeping reform of its history, when 53 councils (governing predominantly rural and majority-Indigenous communities) were forcibly amalgamated into eight regional shires. According to the official narrative, the sector had reached a point of crisis: many councils were administratively too small to manage their growing responsibilities. Despite trenchant popular opposition, amalgamations were justified as technically effective, financially efficient -- even morally imperative. Based on a decade of ethnographic research in the Northern Territory including extensive interviews and professional involvement over many years, my thesis moves beyond an empirical evaluation of these events to explore how government actors establish, maintain and self-assess a policy reform. Despite bureaucracy鈥檚 claims on rationality and evidence, I argue that factors such morality, routines and aesthetics play more important roles in policy formation than acknowledged. Influenced by the Deleuzian concepts of assemblage and the minor event, I analyse this reform through mundane bureaucratic habits, obscured settler colonial social relations, and near-forgotten events: the rendering of Indigenous totemic art into a corporate logo; a sport and recreation funding agreement as a site of bureaucratic violence; the mobilisation of a created statistic. This perspective invites an alternative to orthodox policy evaluation, whereby the policy cycle is understood ecologically, as a complex assemblage of force, violence and effect. In July 2008 the Northern Territory鈥檚 local government sector underwent the most sweeping reform of its history, when 53 councils (governing predominantly rural and majority-Indigenous communities) were forcibly amalgamated into eight regional shires. According to the official narrative, the sector had reached a point of crisis: many councils were administratively too small to manage their growing responsibilities. Despite trenchant popular opposition, amalgamations were justified as technically effective, financially efficient -- even morally imperative. Based on a decade of ethnographic research in the Northern Territory including extensive interviews and professional involvement over many years, my thesis moves beyond an empirical evaluation of these events to explore how government actors establish, maintain and self-assess a policy reform. Despite bureaucracy鈥檚 claims on rationality and evidence, I argue that factors such morality, routines and aesthetics play more important roles in policy formation than acknowledged. Influenced by the Deleuzian concepts of assemblage and the minor event, I analyse this reform through mundane bureaucratic habits, obscured settler colonial social relations, and near-forgotten events: the rendering of Indigenous totemic art into a corporate logo; a sport and recreation funding agreement as a site of bureaucratic violence; the mobilisation of a created statistic. This perspective invites an alternative to orthodox policy evaluation, whereby the policy cycle is understood ecologically, as a complex assemblage of force, violence and effect

Lyman-alpha spectroscopy of extreme [O iii] emitting galaxies at z 鈮 2-3: implications for Ly伪 visibility and LyC leakage at z > 6

Monthly Notices of the Royal Astronomical Society 91探花 University Press (OUP) 503:3 (2021) 4105-4117

Authors:

Mengtao Tang, Daniel P Stark, Jacopo Chevallard, St茅phane Charlot, Ryan Endsley, Enrico Congiu

Metal-THINGS: On the Metallicity and Ionization of ULX Sources in NGC 925

The Astrophysical Journal American Astronomical Society 906:1 (2021) 42-42

Authors:

Maritza A Lara-L贸pez, Igor A Zinchenko, Leonid S Pilyugin, Madusha LP Gunawardhana, Omar L贸pez-Cruz, Shane P O鈥橲ullivan, Anna Feltre, Margarita Rosado, M贸nica S谩nchez-Cruces, Jacopo Chevallard, Maria Emilia De Rossi, Sami Dib, Jacopo Fritz, Isaura Fuentes-Carrera, Luis E Gardu帽o, Eduardo Ibar

Abstract:

We present an analysis of the optical properties of three Ultra Luminous X-ray (ULX) sources identified in NGC 925. We use Integral field unit data from the George Mitchel spectrograph in the context of the Metal-THINGS survey. The optical properties for ULX-1 and ULX-3 are presented, while the spaxel associated with ULX-2 had a low S/N, which prevented its analysis. We also report the kinematics and dimensions of the optical nebula associated with each ULX using ancillary data from the PUMA Fabry-Perot spectrograph. A BPT analysis demonstrates that most spaxels in NGC 925 are dominated by star-forming regions, including those associated with ULX-1 and ULX-3. Using the resolved gas-phase metallicities, a negative metallicity gradient is found, consistent with previous results for spiral galaxies, while the ionization parameter tends to increase radially throughout the galaxy. Interestingly, ULX-1 shows a very low gas metallicity for its galactocentric distance, identified by two independent methods, while exhibiting a typical ionization. We find that such low gas metallicity is best explained in the context of the high-mass X-ray binary population, where the low-metallicity environment favours active Roche lobe overflows that can drive much higher accretion rates. An alternative scenario invoking accretion of a low-mass galaxy is not 91探花ed by the data in this region. Finally, ULX-3 shows both a high metallicity and ionization parameter, which is consistent with the progenitor being a highly-accreting neutron star within an evolved stellar population region.Comment: Accepted by Ap

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