About Me

Hi, my name is Pablo. I am an astrophysicist from a wonderful city in the southern coastline of Spain called Málaga, currently living in Washington DC, where I work for the NASA Goddard Space Flight Center (GSFC).My scientific research is mainly focused on the study of galaxy formation and evolution in the very early Universe, for which I use the NASA/ESA/CSA's James Webb Space Telescope, whose unmatched capabilities allow me to analyze some of the most distant galaxies observed to date.Apart from a cosmos wonderer, I am also a persistent lifter, an avid reader, a board games enthusiast and a relentless optimistic.

Sobre mí

Hola, soy Pablo, un astrofísico procedente de una maravillosa ciudad en la costa sur de España llamada Málaga, actualmente viviendo en Washington DC, donde trabajo para el Centro de Vuelo Espacial Goddard (GSFC) de la NASA.Mi trabajo de investigación está fundamentalmente enfocado en el estudio de la formación y evolución de galaxias en el universo primitivo, para lo cual utilizo el telescopio espacial NASA/ESA/CSA James Webb, cuyas inigualables características me permiten analizar algunas de las galaxias más lejanas observadas hasta la fecha.Aparte de un curioso del cosmos, también soy un persistente levantador de pesas, un ávido lector, un entusiasta de los juegos de mesa y un optimista sin remedio.

Research

My scientific interests span a large variety of topics related with galaxy formation and evolution, protoclusters and structure formation, stellar population modeling, machine learning, data reduction, etc. But my recent work has been especially dedicated to the spectroscopic analysis of ultradistant galaxies in the very early Universe, many of them never seen before until the advent of the JWST.A large fraction of my recent scientific studies have been carried out in the frame of the Cosmic Evolution Early Release Science (CEERS) project, one of the very first surveys of the deep universe observed with the JWST, for which I have lead the spectroscopic efforts with the NIRSpec instrument. Along the way we have provided pre-launch simulations, scientific products and tools to help the community with the data processing.Apart from my close involvement in CEERS, I am also the principal investigator of two other programs executed during the first year of observations with the JWST: one aiming to confirm some of the most promising ultradistant candidates found in the first deep imaging data, and another to study environmental effects on the largest observed galaxy overdensity at the end of the Epoch of Reionization.Among the most interesting results from my research is the confirmation of the first bright ultradistant galaxies at z > 11, including Maisie's Galaxy, only 390 million years after the Big Bang, when the Universe was less than 3% of its current age. It is important to make clear that there were already three more distant galaxies confirmed back then, but those in our work were the most distant bright (MUV < -20 AB) galaxies confirmed at the time. Additionally, our sample represented an important milestone, as one of the most surprising results found in the first JWST deep images is the overabundance of these bright ultradistant candidates, in stark disagreement with the predictions from the pre-JWST galaxy evolution models for the very early Universe.Moreover, in that same work we also refuted CEERS-93316, a very bright and controversial z ~ 16 candidate that would have set a new redshift record by a large margin and would have represented a serious challenge for our models to explain. We instead found that the object was at z = 4.912, an epoch a thousand million years later than the originally predicted based on the imaging data only. We showed that, under peculiar circumstances (including a combination of strong reddening and emission lines at that specific redshift), that source mimics the emission pattern of an ultradistant galaxy in the imaging data. This finding was very educational as it made the high-z community aware of the existence of this rare but possible type of interlopers at very high redshifts.

Investigación

Mis intereses científicos abarcan una gran variedad de materias relacionadas con la formación y evolución de galaxias, protocúmulos y formación de estructuras, ajuste de poblaciones estelares, machine learning, reducción de datos, etc. Pero mi trabajo reciente ha estado especialmente dedicado al análisis espectroscópico de galaxias ultralejanas en el universo muy temprano, muchas de ellas nunca vistas antes hasta la llegada del JWST.Gran parte de mis estudios recientes han sido llevados a cabo en el marco del proyecto CEERS (Cosmic Evolution Early Release Science), uno de los primerísimos cartografiados del universo profundo observados con el JWST, para el cual he liderado los esfuerzos dedicados a la espectroscopía con el instrumento NIRSpec. Durante este proceso hemos proporcionado simulaciones, productos científicos y herramientas para ayudar a la comunidad con el procesamiento de datos.Aparte de mi fuerte implicación en CEERS, también soy el investigador principal de otros dos programas ejecutados durante el primer año de observaciones con el JWST: uno enfocado a intentar confirmar algunos de los candidatos más prometedores a galaxias ultralejanas en los primeros datos de imagen profunda, y otro para estudiar los efectos del ambiente en el mayor protocúmulo de galaxias observado al final de la Era de la Reionización.Entre los resultados más interesantes de mi investigación cabe destacar la confirmación de las primeras galaxias ultralejanas brillantes a z > 11, incluyendo Maisie's Galaxy, tan solo 390 millones de años después del Big Bang, cuando el universo tenía menos de un 3% de su edad actual. Es importante aclarar que ya había tres galaxias más lejanas confirmadas en ese momento, pero las presentadas en nuestro trabajo eran las galaxias más lejanas brillantes (MUV < -20 AB) y representaron un hito importante debido a que uno de los resultados más sorprendentes encontrados en las primeras imágenes profundas de JWST es la sobreabundancia de candidatos a galaxias brillantes ultralejanas, en desacuerdo con las predicciones para el universo primitivo de los modelos de evolución de galaxias pre-JWST.Además, en ese mismo trabajo también refutamos el objeto CEERS-93316, un controvertido candidato a z ~ 16 muy brillante que habría batido el récord de desplazamiento al rojo por mucho y habría supuesto un desafío serio para poder explicar su existencia dentro de nuestros modelos. En su lugar, nosotros encontramos que el objeto está realmente a z = 4.912, una época mil millones de años posterior a la originalmente predicha basándose solo en los datos de imagen. En nuestro trabajo mostramos que, bajo circustancias muy particulares (incluyendo la combinación de un fuerte enrojecimiento por polvo y fuertes líneas de emisión a ese desplazamiento al rojo en concreto), esta fuente imita el patrón de emisión de una galaxia ultralejana en los datos de imagen. Este hallazgo fue muy educativo, puesto que puso a la comunidad de alto z sobre aviso acerca de la existencia de este raro pero posible tipo de objetos intrusos en las muestras a muy alto desplazamiento al rojo.

Press & Media

The number of press articles reporting interesting results from different JWST studies I am part of is (thanks to my awesome collaborators) huge. The compilation below is limited to part of the media coverage of my direct work or where I explicitly appear:

Prensa y Medios

El número de artículos de prensa informando sobre resultados interesantes de diferentes estudios con el JWST de los que formo parte es (gracias a mis increíbles colaboradores) enorme. La selección aquí mostrada se limita a parte de la cobertura mediática de mi trabajo directo o en la que aparezco explícitamente:

Outreach

I unfortunately cannot dedicate as much time as I would like to outreach events at this point within my usually demanding research activity, but every now and then I like to make short posts in Facebook and Instagram (usually in Spanish) talking about interesting astronomical findings or milestones that might go unnoticed in the mainstream media.Occasionally, nonetheless, I can take part in a few more dedicated outreach events:

Divulgación

Desafortunadamente, en la actualidad no puedo dedicar tanto tiempo como me gustaría a eventos de divulgación dentro de mi normalmente demandante actividad científica, pero de vez en cuando me gusta escribir pequeñas publicaciones en Facebook e Instagram (normalmente en español) hablando sobre hitos y hallazgos astronómicos interesantes que pueden pasar desapercibidos en los medios de comunicación habituales.Ocasionalmente, no obstante, sí que puedo participar en algún que otro evento divulgativo más dedicado:

List of Publications

Refereed: 38; Submitted: 18; First author: 4 (updated as of November 2023)

First author:

  • P. Arrabal Haro, M. Dickinson, S. L. Finkelstein, J. S. Kartaltepe, and 33 coauthors. Confirmation and refutation of very luminous galaxies in the early Universe. Nature, 622, 707, 2023

  • P. Arrabal Haro, M. Dickinson, S. L. Finkelstein, S. Fujimoto, and 44 coauthors. Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ≃ 8-10. ApJL, 951, L22, 2023

  • P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón, D. Sobral, and 5 coauthors. Differences and similarities of stellar populations in LAEs and LBGs at z ~ 3.4-6.8. MNRAS, 495, 1807, 2020

  • P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón, P. G. Pérez-González, and 14 coauthors. A simultaneous search for high-z LAEs and LBGs in the SHARDS survey. MNRAS, 478, 3740, 2018

Key contribution as coauthor:

  • A. L. González-Morán, P. Arrabal Haro, C. Muñoz-Tuñón, J. M. Rogríguez-Espinosa, and 14 coauthors. The PAU survey: classifying low-z SEDs using Machine Learning clustering. MNRAS, 524, 3569, 2023

  • D. D. Kocevski, M. Onoue, K. Inayoshi, J. R. Trump, P. Arrabal Haro, and 36 coauthors. Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS. ApJL, 954, L4, 2023

  • R. L. Larson, S. L. Finkelstein, D. D. Kocevski, T. A. Hutchison, J. R. Trump, P. Arrabal Haro, and 47 coauthors. A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars. ApJL, 953, L29, 2023

  • S. Fujimoto, P. Arrabal Haro, M. Dickinson, S. L. Finkelstein, and 40 coauthors. CEERS Spectroscopic Confirmation of NIRCam-selected z ≳ 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of Their Properties. ApJL, 949, L25, 2023

  • J. R. Trump, P. Arrabal Haro, R. C. Simons, B. E. Backhaus, and 62 coauthors. The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations. ApJ, 945, 35, 2023

  • I. Jung, S. L. Finkelstein, P. Arrabal Haro, M. Dickinson, and 28 coauthors. CEERS: Diversity of Lyman-Alpha Emitters during the Epoch of Reionization. arXiv:2304.05385, 2023

  • S. L. Finkelstein, M. B. Bagley, P. Arrabal Haro, M. Dickinson, and 118 coauthors. A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging. ApJL, 940, L55, 2022

  • K. Z. Arellano-Córdova, D. A. Berg, J. Chisholm, P. Arrabal Haro, and 8 coauthors. A First Look at the Abundance Pattern-O/H, C/O, and Ne/O-in z > 7 Galaxies with JWST/NIRSpec. ApJL, 940, L23, 2022

  • R. Calvi, H. Dannerbauer, P. Arrabal Haro, J. M. Rodríguez Espinosa, and 3 coauthors. Probing the existence of a rich galaxy overdensity at z = 5.2. MNRAS, 502, 4558, 2021

Coauthor:

  • K. Chworowsky, S. L. Finkelstein, M. Boylan-Kolchin, E. J. McGrath, and 35 coauthors. Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4 to 8 from CEERS. arXiv:2311.14804, 2023

  • S. L. Finkelstein, G. C. K. Leung, M. B. Bagley, M. Dickinson, and 51 coauthors. The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5. arXiv:2311.04279, 2023

  • E. M. Ward, A. de la Vega, B. Mobasher, E. J. McGrath, and 18 coauthors. Evolution of the Size-Mass Relation of Star-forming Galaxies Since z = 5.5 Revealed by CEERS. arXiv:2311.02162, 2023

  • L. Costantin, P. G. Pérez-González, Y. Guo, C. Buttitta, and 29 coauthors. A Milky Way-like barred spiral galaxy at a redshift of 3. Nature, 623, 499, 2023

  • A. Callabrò, L. Pentericci, A. Feltre, P. Arrabal Haro, and 34 coauthors. Near-infrared emission line diagnostics for AGN from the local Universe to z ~ 3. A&A, 679, A80, 2023

  • V. Pandya, H. Zhang, M. Huertas-Company, K. G. Iyer, and 52 coauthors. Galaxies Going Bananas: Inferring the 3D Geometry of High-Redshift Galaxies with JWST-CEERS. arXiv:2310.15232, 2023

  • K. Ronayne, C. Papovich, G. Yang, L. Shen, and 32 coauthors. CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI. arXiv:2310.07766, 2023

  • G. Yang, C. Papovich, M. Bagley, H. Ferguson, and 34 coauthors. CEERS MIRI Imaging: Data Reduction and Quality Assessment. ApJL, 956, L12 2023

  • H. Akins, C. M. Casey, N. Allen, M. B. Bagley, and 57 coauthors. Two massive, compact, and dust-obscured candidate z ~ 8 galaxies discovered by JWST. ApJ, 956, 61, 2023

  • S. Fujimoto, S. L. Finkelstein, D. Burgarella, C. Carilli, and 49 coauthors. ALMA FIR View of Ultra-high-redshift Galaxy Candidates at z ~ 11-17: Blue Monsters or Low-z Red Interlopers?. ApJ, 955, 130, 2023

  • B. Magnelli, C. Gómez-Guijarro, D. Elbaz, E. Daddi, and 22 coauthors. CEERS: MIRI deciphers the spatial distribution of dust-obscured star formation in galaxies at 0.1 < z < 2.5. A&A, 678, A83, 2023

  • B. W. Holwerda, C. Hsu, N. Hathi, L. Bisigello, and 19 coauthors. Cosmic Evolution Early Release Science Survey (CEERS): Multi-classing Galactic Dwarf Stars in the deep JWST/NIRCam. arXiv:2309.05835, 2023

  • T. Herard-Demanche, R. J. Bouwens, P. A. Oesch, R. P. Naidu, and 20 coauthors. Mapping dusty galaxy growth at z > 5 with FRESCO: Detection of Hα in submm galaxy HDF850.1 and the surrounding overdense structures. arXiv:2309.04525, 2023

  • S. Mascia, L. Pentericci, A. Calabrò, P. Santini, and 27 coauthors. New insight on the nature of cosmic reionizers from the CEERS survey. arXiv:2309.02219, 2023

  • C. Gómez-Guijarro, B. Magnelli, D. Elbaz, S. Wuyts, and 37 coauthors. JWST CEERS probes the role of stellar mass and morphology in obscuring galaxiesg. A&A, 677, A34, 2023

  • R. T. Coogan, E. Daddi, A. Le Bail, D. Elbaz, and 24 coauthors. A z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making. A&A, 677, A3, 2023

  • A. Kirkpatrick, G. Yang, A. Le Bail, G. Troiani, and 32 coauthors. CEERS Key Paper VII: JWST/MIRI Reveals a Faint Population of Galaxies at Cosmic Noon Unseen by Spitzer. arXiv:2308.09750, 2023

  • X. Wang, H. I. Teplitz, B. T. Smith, R. Windhorst, and 73 coauthors. The Lyman Continuum Escape Fraction of Star-forming Galaxies at 2.4 ≲ z ≲ 3.7 from UVCANDELS. arXiv:2308.09064, 2023

  • V. Mehta, H. I. Teplitz, C. Scarlata, X. Wang, and 29 coauthors. A Spatially Resolved Analysis of Star Formation Burstiness by Comparing UV and Hα in Galaxies at z ~ 1 with UVCANDELS. ApJ, 952, 133, 2023

  • L. Bisigello, G. Gandolfi, A. Grazian, G. Rodighiero, and 20 coauthors. Delving deep: A population of extremely dusty dwarfs observed by JWST. A&A, 676, A76, 2023

  • B. E. Backhaus, J. R. Trump, N. Pirzkal, G. Barro, and 36 coauthors. CEERS Key Paper VIII: Emission Line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z>2. arXiv:2307.09503, 2023

  • A. Le Bail, E. Daddi, D. Elbaz, M. Dickinson, and 25 coauthors. JWST/CEERS Sheds Light on Dusty Star-Forming Galaxies: Forming Bulges, Lopsidedness and Outside-In Quenching at Cosmic Noon. arXiv:2307.07599, 2023

  • K. E. Heintz, D. Watson, G. Brammer, S. Vejlgaard, and 17 coauthors. Extreme damped Lyman-α absorption in young star-forming galaxies at z = 9-11. arXiv:2306.00647, 2023

  • G. Yang, K. I. Caputi, C. Papovich, P. Arrabal Haro, and 34 coauthors. CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts. ApJL, 950, L5, 2023

  • L. Shen, C. Papovich, G. Yang, J. Matharu, and 37 coauthors. CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes. ApJ, 950, 7, 2023

  • C. Papovich, J. W. Cole, G. Yang, S. L. Finkelstein, and 45 coauthors. CEERS Key Paper. V. Galaxies at 4 < z < 9 Are Bluer than They Appear-Characterizing Galaxy Stellar Populations from Rest-frame 1 μm Imaging. ApJL, 949, L18, 2023

  • G. Barro, P. G. Pérez-González, D. D. Kocevski, E. McGrath, and 26 coauthors. Extremely red galaxies at z = 5-9 with MIRI and NIRSpec: dusty galaxies or obscured AGNs?. arXiv:2305.14418, 2023

  • A. S. Long, J. Antwi-Danso, E. L. Lambrides, C. C. Lovell, and 29 coauthors. Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS. arXiv:2305.04662, 2023

  • M. Huertas-Company, K. G. Iyer, E. Angeloudi, M. B. Bagley, and 25 coauthors. Galaxy Morphology from z ~ 6 through the eyes of JWST. arXiv:2305.02478, 2023

  • M. Kuschel, C. Scarlata, V. Mehta, H. I. Teplitz, and 35 coauthors. Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups. ApJ, 947, 17, 2023

  • P. G. Pérez-González, G. Barro, M. Annunziatella, L. Costantin, and 51 coauthors. CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies. ApJL, 946, L16, 2023

  • J. S. Kartaltepe, C. Rose, B. N. Vanderhoof, E. McGrath, and 58 coauthors. CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3-9 with JWST. ApJL, 946, L15, 2023

  • D. D. Kocevski, G. Barro, E. McGrath, S. L. Finkelstein, and 56 coauthors. CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST. ApJL, 946, L14, 2023

  • S. L. Finkelstein, M. B. Bagley, H. C. Ferguson, S. M. Wilkins, and 63 coauthors. CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST. ApJL, 946, L13, 2023

  • M. B. Bagley, S. L. Finkelstein, A. M. Koekemoer, H. C. Ferguson, P. Arrabal Haro, and 35 coauthors. CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results. ApJL, 946, L12, 2023

  • Y. Guo, S. Jogee, S. L. Finkelstein, Z. Chen, and 44 coauthors. First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging. ApJL, 945, L10, 2023

  • J. Vega-Ferrero, M. Huertas-Company, L. Costantin, P. G. Pérez-González, and 25 coauthors. On the nature of disks at high redshift seen by JWST/CEERS with contrastive learning and cosmological simulations. arXiv:2302.07277, 2023

  • A. García-Argumánez, P. G. Pérez-González, A. Gil de Paz, G. F Snyder, P. Arrabal Haro, and 18 coauthors. Probing the Earliest Phases in the Formation of Massive Galaxies with Simulated HST+JWST Imaging Data from Illustris. ApJ, 944, 3, 2023

  • J. A. Zavala, V. Buat, C. M. Casey, S. L. Finkelstein, and 121 coauthors. Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations. ApJL, 943, L9, 2023

  • C. Rose, J. S. Kartaltepe, G. F. Snyder, V. Rodriguez-Gomez, and 22 coauthors. Identifying Galaxy Mergers in Simulated CEERS NIRCam Images Using Random Forests. ApJ, 942, 54, 2023

  • S. Santos, D. Sobral, J. Butterworth, A. Paulino-Afonso, and 6 coauthors. The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ~ 2 to z ~ 6. MNRAS, 505, 1117, 2021

  • S. Santos, D. Sobral, J. Matthee, J. Calhau, and 5 coauthors. The evolution of rest-frame UV properties, Ly α EWs, and the SFR-stellar mass relation at z ~ 2-6 for SC4K LAEs. MNRAS, 493, 141, 2020

  • A. Lumbreras-Calle, C. Muñoz-Tuñón, J. Méndez-Abreu, J. M. Mas-Hesse, and 10 coauthors. Star-forming galaxies at low-redshift in the SHARDS survey. A&A, 621, A52, 2019

Listado de Publicaciones

Aceptadas: 38; Enviadas: 18; Primer autor: 4 (actualizado a noviembre de 2023)

Primer autor:

  • P. Arrabal Haro, M. Dickinson, S. L. Finkelstein, J. S. Kartaltepe, and 33 coauthors. Confirmation and refutation of very luminous galaxies in the early Universe. Nature, 622, 707, 2023

  • P. Arrabal Haro, M. Dickinson, S. L. Finkelstein, S. Fujimoto, and 44 coauthors. Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ≃ 8-10. ApJL, 951, L22, 2023

  • P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón, D. Sobral, and 5 coauthors. Differences and similarities of stellar populations in LAEs and LBGs at z ~ 3.4-6.8. MNRAS, 495, 1807, 2020

  • P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón, P. G. Pérez-González, and 14 coauthors. A simultaneous search for high-z LAEs and LBGs in the SHARDS survey. MNRAS, 478, 3740, 2018

Contribución clave como coautor:

  • A. L. González-Morán, P. Arrabal Haro, C. Muñoz-Tuñón, J. M. Rogríguez-Espinosa, and 14 coauthors. The PAU survey: classifying low-z SEDs using Machine Learning clustering. MNRAS, 524, 3569, 2023

  • D. D. Kocevski, M. Onoue, K. Inayoshi, J. R. Trump, P. Arrabal Haro, and 36 coauthors. Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS. ApJL, 954, L4, 2023

  • R. L. Larson, S. L. Finkelstein, D. D. Kocevski, T. A. Hutchison, J. R. Trump, P. Arrabal Haro, and 47 coauthors. A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars. ApJL, 953, L29, 2023

  • S. Fujimoto, P. Arrabal Haro, M. Dickinson, S. L. Finkelstein, and 40 coauthors. CEERS Spectroscopic Confirmation of NIRCam-selected z ≳ 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of Their Properties. ApJL, 949, L25, 2023

  • J. R. Trump, P. Arrabal Haro, R. C. Simons, B. E. Backhaus, and 62 coauthors. The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations. ApJ, 945, 35, 2023

  • I. Jung, S. L. Finkelstein, P. Arrabal Haro, M. Dickinson, and 28 coauthors. CEERS: Diversity of Lyman-Alpha Emitters during the Epoch of Reionization. arXiv:2304.05385, 2023

  • S. L. Finkelstein, M. B. Bagley, P. Arrabal Haro, M. Dickinson, and 118 coauthors. A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging. ApJL, 940, L55, 2022

  • K. Z. Arellano-Córdova, D. A. Berg, J. Chisholm, P. Arrabal Haro, and 8 coauthors. A First Look at the Abundance Pattern-O/H, C/O, and Ne/O-in z > 7 Galaxies with JWST/NIRSpec. ApJL, 940, L23, 2022

  • R. Calvi, H. Dannerbauer, P. Arrabal Haro, J. M. Rodríguez Espinosa, and 3 coauthors. Probing the existence of a rich galaxy overdensity at z = 5.2. MNRAS, 502, 4558, 2021

Coautor:

  • K. Chworowsky, S. L. Finkelstein, M. Boylan-Kolchin, E. J. McGrath, and 35 coauthors. Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4 to 8 from CEERS. arXiv:2311.14804, 2023

  • S. L. Finkelstein, G. C. K. Leung, M. B. Bagley, M. Dickinson, and 51 coauthors. The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5. arXiv:2311.04279, 2023

  • E. M. Ward, A. de la Vega, B. Mobasher, E. J. McGrath, and 18 coauthors. Evolution of the Size-Mass Relation of Star-forming Galaxies Since z = 5.5 Revealed by CEERS. arXiv:2311.02162, 2023

  • L. Costantin, P. G. Pérez-González, Y. Guo, C. Buttitta, and 29 coauthors. A Milky Way-like barred spiral galaxy at a redshift of 3. Nature, 623, 499, 2023

  • A. Callabrò, L. Pentericci, A. Feltre, P. Arrabal Haro, and 34 coauthors. Near-infrared emission line diagnostics for AGN from the local Universe to z ~ 3. A&A, 679, A80, 2023

  • V. Pandya, H. Zhang, M. Huertas-Company, K. G. Iyer, and 52 coauthors. Galaxies Going Bananas: Inferring the 3D Geometry of High-Redshift Galaxies with JWST-CEERS. arXiv:2310.15232, 2023

  • K. Ronayne, C. Papovich, G. Yang, L. Shen, and 32 coauthors. CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI. arXiv:2310.07766, 2023

  • G. Yang, C. Papovich, M. Bagley, H. Ferguson, and 34 coauthors. CEERS MIRI Imaging: Data Reduction and Quality Assessment. ApJL, 956, L12 2023

  • H. Akins, C. M. Casey, N. Allen, M. B. Bagley, and 57 coauthors. Two massive, compact, and dust-obscured candidate z ~ 8 galaxies discovered by JWST. ApJ, 956, 61, 2023

  • S. Fujimoto, S. L. Finkelstein, D. Burgarella, C. Carilli, and 49 coauthors. ALMA FIR View of Ultra-high-redshift Galaxy Candidates at z ~ 11-17: Blue Monsters or Low-z Red Interlopers?. ApJ, 955, 130, 2023

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