- GALEP programme
- MASGOMAS project
- GOYA survey
- Young second-generation clusters
- Brown dwarf in distant young clusters
- Search for massive star clusters
- AGN Galaxies
GALEP programme
ABSTRACT
To examine spectroscopically a representative selection of sources being discovered deep in the Galaxy along a number of different lines of sight. The majority of the objects lie very close to the Galactic Plane and high extinction means that these objects are impossible to observe at visible wavelengths and so the near IR has to be used.
TARGETS
Object types: RGBs, AGBs
Coordinates: l = 0, 4, 8, 12, 16, 20, 24, 28, 32 deg.
|b| ~ area: 15x15 arcmin
Setup: MOS (H,K).
MASGOMAS project
ABSTRACT
Search and characterization of massive star clusters on the Galactic plane.
TARGETS
Coordinates: l = [12 : 90] deg.
-1 < b < 2 deg.
Setup: MOS (H,K).
GOYA survey
ABSTRACT
GOYA will survey spectroscopically the galaxy population at intermediate redshifts (0.3 < z < 4) using both the long-slit and Multi-object spectroscopy of EMIR in the JHK bands. GOYA will also study the first high-redshift (z > 4) galaxies in these fields to connect the very early universe with the intermediate redshift epoch. Cosmological fields with the very much needed ancillary data from both ground-based telescopes and HST will be observed.
TARGETS
| Target Name | RA(2000) | Dec(2000) | Total reserved area (arcmin2) |
| Abell 370 | 02 39 52.0 | -01 34 39.0 | 7x7 |
| WUDS | 14 19 27.0 | +52 40 56.0 | 42.43x42.43 centred |
| EGS | 14 20 00.0 | +52 55 30.0 | 5x20 |
| UDS | 02 17 25.0 | -05 12 30.0 | 12.5x7.5 |
A detailed description of the covered fields around those pointings can be also found here.
Setup: MOS (J,H,K).
Young second-generation clusters
ABSTRACT
Characterize star formation mechanisms in young clusters located at the edges of HII regions.
TARGETS
* Cluster associated with Sh 104
* Cluster associated with Sh 241
* Cluster associated with Sh 217
* Cluster associated with Sh 219
* Clusters associated with Sh 271-272 and Sh 192-193-194
* Source at the periphery of Sh 212
Setup: Imaging - Y, J, H, Ks + MOS (H,K).
Brown dwarfs in distant young clusters
ABSTRACT
Study the low-mass end of the IMF to test the universality of the IMF by detecting very low mass stars and brown dwarfs in young clusters.
TARGETS
| Target Name | RA(2000) | Dec(2000) |
| NGC1502 | 04 07 50.0 | +62 19 54.0 |
| NGC2175 | 06 09 39.0 | +20 29 12.0 |
| NGC6318 | 17 14 18.0 | -39 24 00.0 |
| NGC6611 | 18 18 48.0 | -13 48 24.0 |
| NGC6623 | 19:43:00.0 | +23 18 00.0 |
| Berkeley82 | 19 43 12.0 | +12 59 00.0 |
Setup: Imaging - Y, J, H, Ks + MOS (J,H,K).
Search for massive star clusters
ABSTRACT
Multi-wavelenght, multi-object spectroscopic study of massive stars in clusters.
TARGETS
| Target Name | RA(2000) | Dec(2000) | Obs. Mode |
| Galactic Center (includes Central Cluster, Quintuplete and Arches) | 17 45 00.0 | -29 00 00.0 | MOS |
| Massive star-forming region W51A | 18 08 00.0 | -20 38 00.0 | MOS |
| Cluster Cl 1813-178 in W33 | 18 13 22.0 | -17 54 15.0 | MOS |
| Massive star-forming region W49 | 19 10 00.0 | +09 06 00.0 | MOS |
Setup: MOS (J,H,K).
AGN Galaxies
ABSTRACT
To study of the dynamics and stellar populations of the nuclear regions in AGN galaxies, with the aim of investigating the most probable mechanisms to trigger activity. We plan to estimate black hole masses, to determine central kinematic structures, such as disks, bars, etc. eventually responsible for the the fueling of the central black hole and host galaxy properties through the analysis of stellar populations.
TARGETS
| Target Name | RA(2000) | Dec(2000) |
| NGC2841 | 09 22 02.63 | +50 58 35.5 |
| NGC3031 | 09 55 33.17 | +69 03 55.1 |
| NGC4501 | 12 31 59.16 | +14 25 13.4 |
Setup: LSS (H,K).
Last modified: 28 June 2019
