Participants:

Monica Rodriguez	INAOE
Miriam Peña	IA-CU
Laurence Sabin	IA-Ensenada-UNAM
Roberto Vazquez	IA-Ensenada-UNAM
Michael Richer	IA-Ensenada-UNAM
Christophe Morisset	IA-Ensenada-UNAM
Gerardo Ramos Larios	UdG
Arturo Gomez Ruiz	INAOE
Diego Bryan Hernandez Juarez	IA-CU-UNAM
Francisco Riuz Escobedo	IA-Ensenada-UNAM
Valeria Beltran	IA-CU-UNAM
Liliana Hernández	UNAM

PROJECT:

• Estudiando el Factor de Discrepancia de Abundancias (ADF) en nebulosas planetarias.

TALKs:

1. Redes de modelos y regresores en espacios multidimensionales.
   Christophe Morisset

Participants:

Bolivia Cuevas	BUAP
David Fernández Arenas	CFHT, Hawaii, USA
Héctor Ibarra Medel	IA-CU-UNAM
Jorge Barrera	IA-CU-UNAM
Mariana Cano	IA-CU-UNAM
Joel Sánchez	IA-CU-UNAM
Aida Wofford	IA-Ensenada-UNAM
Christophe Morisset	IA-Ensenada-UNAM
Ary Rodríguez	ICN-UNAM
Jorge Osorio Caballero	ICN-UNAM
Divakara Mayya	INAOE
Fabián Rosales Ortega	INAOE
Elena Terlevich	INAOE
Ivanio Puerari	INAOE
Lino Rodríguez	INAOE
Sergio Martínez	INAOE
Olga Vega	INAOE
Avinash Chandrakumar	INAOE
Guillermo Romero	INAOE
Luz Itzel Álvarez	INAOE
Mauricio Portilla	INAOE
Miguel Ángel López Santamaría	INAOE
Ignacio Vega	IPN
Sandra Zamora	UniPi, Italy

PROJECTs:

• Star formation and the effect of the feedback in the ISM.

SUMMARY

Study of extragalactic star formation (SF) has reached a massive boost with the advent of James Webb Space Telescope (JWST) and other coordinated multiwavelength observation programs. PHANGS (Physics at High Angular Resolution in Nearby GalaxieS) is one such program. This new set of observational data traces stellar as well as multi-phase interstellar medium (ISM) at spatial scales better than the physical scales at which processes related to SF occur. This allows us to understand in detail the process of star formation as well as the effect of its feedback on the ISM. More importantly, most of these data are available to the general public for its scientific exploitation. Researchers at Mexican institutes have proven expertise in the exploration of the extragalactic star formation, both from the observational and theoretical fronts, that would allow further our understanding of star formation and feedback processes. The Guillermo Haro workshop-2024 is bringing together researchers and students at different institutes and universities in Mexico that are working on fields related to extragalactic star formation to discuss research topics that would help to make best use of observational resources Mexico has in the form of direct access to present and future large observational facilities such as GTC, LMT, LSST, ngVLA etc.

WORKSHOPs:

• JWST data reduction - Avinash Chandrakumar
  • Requirements:

Proposed TALKs:

1. Bolivia Cuevas - Dynamical Evolution of star clusters using CMC simulations
2. Miguel Lopez Santamaria - Age and metallicity of globular and fuzzy clusters using GTC/OSIRIS spectra
3. Luz Itzel Alvarez Cruz - Determination of velocity dispersion of star clusters using MEGARA high resolution spectroscopy
4. Avinash Chandrakumar - Study of stellar metallicity gradients of disk galaxies using the TRGB magnitudes in JWST filters
5. Divakara Mayya - Ages of stellar populations inside the bubbles detected in the JWST/MIRI images
6. Mauricio Portilla - Photometric and dynamical properties of Tidal Dwarf Galaxies
7. Pedro Ovando - Spectroscopic and photometric analysis of old cluster populations of NGC3077
8. Mariana Cano - Studying the Spatially Resolved Star Formation Main Sequence in nearby galaxies.
9. Sandra Zamora - TBD
10. Guillermo Romero - Stellar feedback analysis in the central region of NGC 1087 using data from the GTC-MEGARA instrument of the BEARD program.
11. Ignacio Vega - Star Formation in the Tidal Tails of Interacting Galaxies.
12. Ary Rodríguez - TBD

Participants:

Alice Pasetto	IRyA
Anna Lia Longinotti	IA-CU-UNAM
Irene Cruz-Gonzalez	IA-CU-UNAM
Hector Ibarra	IA-CU-UNAM
Alenka Negrete	IA-CU-UNAM
Jorge Barrera	IA-CU-UNAM
Mariana Cano	IA-CU-UNAM
Martin Herrera	IA-CU-UNAM
Takamitsu Miyaji	IA-Ensenada-UNAM
Vahram Chavushyan	INAOE
Victor Patiño	INAOE
Diego Gonzalez Buitrago	IA-Ensenada-UNAM
Edgar Cortés Suarez	INAOE
Raquel Baza Medina	IA-CU-UNAM

TOPICS:

• AGN con IFU en banda óptica and e-ROSITA AGN
• SDSS Black Hole Mapper
• AGN SED fitting

TALKs:

1. AGNs con MaNGA
   Mariana Cano , Jorge Barrera
2. AGN clustering with e-ROSITA
   Takamitsu Miyaji
3. SDSS-IV BOSS spectroscopy
   Hector Ibarra (IA)
4. Charlas: AGN reverberation mapping 
   Alenka Negrete , Diego Gonzalez
5. Overview proyectos para estudiar cuásares con el BHM
   Hector Ibarra
6. SED fitting en AGN
   Martin Herrera , Victor Patiño
7. La emisión de los AGN en rayos Gamma y altas energías
   Vahram Chavushyan , Victor Patiño
8. Charla: AGN radio-loud
   Vahram Chavushyan Victor Patiño

WORKSHOPs:

• Taller datos del SDSS-IV Héctor Javier Ibarra
  • Requirements:
• SED en AGNs con  CIGALE Martin Herrera
  • Requirements:
• Taller sobre datos de Fermi Victor Patiño
  • Requirements:

Participants:

Roberto Terlevich	INAOE
Elena Terlevich	INAOE
Ricardo Chaez Murillo	IRyA
Ana Luisa Gonzalez Moran	UAS-Culiacan
David Fernandez Arenas	CFHT, Hawaii,USA
Sandra Zamora	UniPi, Italy
José Fernando Valencia Hernández	INAOE

TALKs:

1. Reconstructing Cosmic History: JWST-Extended Mapping of the Hubble Flow from z∼0 to z∼7.5 with HII Galaxies
   Ricardo Chávez
2. Challenging the standard cosmological model using HII galaxies
   Ana Luisa González Morán
3. Dissecting star formation, AGN activity and ionized gas properties on parsec scales in NGC 4258, a Low-luminosity Seyfert Galaxy in SIGNALS survey
   David Fernández Arenas

Project Summary:

Over twenty years ago, type Ia Supernovae observations revealed an accelerating Universe expansion, suggesting a significant dark energy presence, often modelled as a cosmological constant, Λ. Despite its pivotal role in cosmology, the standard ΛCDM model remains largely under-explored in the redshift range between the most distant SNIa and the Cosmic Microwave Background. Our group aims to use the James Webb Space Telescope’s advanced capabilities to extend the Hubble flow mapping across an unprecedented redshift range from z ≈ 0 to z ≈ 13.

Utilising a dataset of 231 HII galaxies and extragalactic HII regions, we employ the L − σ relation, correlating the luminosity of Balmer emission lines with their velocity dispersion, to define a competitive technique for measuring cosmic distances that can potentially map the Universe’s expansion over more than 13 billion years, covering almost 98% of its age.

Participants:

Itziar Aretxaga	INAOE
Alfredo Montaña	INAOE
Araceli Nava	INAOE
Vladimir Avila	IA-CU-UNAM
Aldo Rodriguez Puebla	IA-CU-UNAM
Hector Ibarra	IA-CU-UNAM
Daniel Salazar Santiago	IA-CU-UNAM

TALKs:

1. The most extended stellar structures in the Universe: observations and simulations
   Vladimir Avila
2. The star formation and assembly history of the galaxies since z~10; mocking the observed universe
   Aldo Rodríguez Puebla
3. Catálogo simulado de galaxias polvorientas formadoras de estrellas para estudios milimétricos profundos
   Araceli Nava
4. The differences between mass- and light-derived structural parameters over time for MaNGA elliptical galaxies.
   Héctor Ibarra.
5. ¿Hay segregación por medio ambiente en la conexión galaxia-halo?
   Daniel Salazar Santiago

Participants:

TALKs:

Participants:

 

Emmaly Aguilar	INAOE
Ma. Teresa Orozco	INAOE
Iván Rodríguez	INAOE
Alejandro García Pérez	INAOE
Araceli Nava	INAOE
Alenka Negrete	IA-CU-UNAM
Héctor Ibarra Medel	IA-CU-UNAM
Olga Vega	INAOE

TALKs:

Participants:

Héctor Hernández Toledo	IA-CU-UNAM
José Antonio Vázquez	IA-CU-UNAM
Luis León Anaya	IA-CU-UNAM
Octavio Valenzuela	IA-CU-UNAM
José Antonio de Diego	IA-CU-UNAM
Cesar Miguel Aguirre	IA-CU-UNAM
Diego García Aguilar	IA-CU-UNAM
Andrea Muñoz Gutiérrez	IA-CU-UNAM
Gibran Fuentes Pineda	IIMAS-UNAM
Gabriela Aguilar Argüello	IIMAS-UNAM
Erik Molino Minero Re	IIMAS-UNAM
Álvaro Callejas	IIMAS-UNAM
Enrique Succar Succar	INAOE
Enrique Herbert Pucheta	IPN
Isabel Abigail Valadez Polanco	UADY
Abel Santillán Rodríguez	UAQ
Juan Carlos Cuevas Tello	UASLP
Rene Parlange	UASLP
Rebeca Abigail Mendoza Farias	UASLP
Fernando Juriel Ojeda Gutiérrez	UASLP
Isaí Vicente Moreno Lara	UASLP
Fernando Antonio Ramírez Martínez	UASLP
Alexis Páez	UNAM
Efraín Condés Luna	UNAM
Lenin Pavón Álvarez	UNAM

Workshops and TALKs:

First Week:

July, 15, 16 and 17.

Workshop I: Aprendizaje de Máquina aplicado a Imágenes Astronómicas: Introducción
Gibran Fuentes Pineda, et al.

Workshop II: Entrenamiento de algoritmos, datos y el método de clasificación SOM.
Erik Molino Minero Re, et al.

July, 18 and 19.

Workshop I: Series de tiempo y Ciencia de Datos, aplicaciones a clasificación automática de curvas de luz, time delay en lentes gravitacionales.
Juan Carlos Cuevas Tello, et al.

Second week:

July 22,23, and 24.

Workshop : Simulaciones Aceleradas por ML. Presentación aplicaciones a diferentes problemas, asesorías a interesados.
Octavio Valenzuela et al.

Third week:

July, 29,30 and 31.

Talks:

1. Herramientas de ML y sus aplicaciones a galaxias.
   José Antonio de Diego.
2. Búsqueda y análisis de exoplanetas con Machine Learning.
   Enrique Succar Succar

Workshop: El uso del ML en el análisis químico de espectros
Enrique Herbert Pucheta.

Participants:

William Lee	IA-CU-UNAM
Beatriz Sánchez	IA-CU-UNAM
Salvador Cuevas	IA-CU-UNAM
Esperanza Carrasco	INAOE
Alberto Carramiñana	INAOE
José Ramón Valdés	INAOE
Filiberto Hueyotl	UNACH
Cesar Alvarez	UNACH

 

TALKs:

1. José Ramón Valdés
   "GTC: estatus de la instrumentación"
2. Beatriz Sánchez
   "FRIDA I: desarrollo del proyecto"
3. Salvador Cuevas
   "FRIDA II: aspectos instrumentales"
4. Esperanza Carrasco
   "MEGARA - estatus del MOS"
5. Alberto Carramiñana
   "HAWC: una década de operación"
6. Alberto Carramiñana
   "HAWC y SWGO: el futuro a mediano y largo plazo"