LUCIFER SDT (December 5-16, 2009)
Due by December 2nd for each project:
- README file with a basic description of the project, including
- Contact information should clarification be necessary
- LUCIFER Observing script(s)
- Finding Chart(s) clearly identifying at least the source and guide star
- Any special calibration needs
Please send this information to Dave Thompson.
LUCIFER SDT Approved Projects:
Priority A Projects |
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---|---|---|
PI (Partner) |
Time (hr) |
Title |
Thompson (OSU/RC) |
0.36 |
Massive Star CSI: Late Time Near-IR Imaging of SN 2008S |
Skillman (OSU/RC) |
1.0 |
Characterizing Galaxy Evolution and Enrichment: Asymptotic Giant Branch Star in Local Group Dwarf Galaxies |
Garnavich (OSU/RC) |
1.4 |
Are Old Type Ia Supernovae Red? |
Wong (OSU/RC) |
0.8 |
Narrow-band, Near-InfraredMolecular Gas Imaging of the Luminous Infrared Galaxy IC 5298 |
Martini (OSU/RC) |
2.6 |
Gas-Phase Metallicity of a Strongly Lensed Galaxy at z = 2.03 |
Assef (OSU/RC) |
1.5 |
Measuring Black Hole Masses of High Redshift Lensed QSOs with LUCIFER |
Cresci (INAF) |
3.2 |
Spatially resolved chemical properties at z~2 |
Beltran (INAF) |
1.0 |
Searching for disks and jets associated with high-mass protostars |
Longhetti (INAF) |
2.0 |
Were early-type galaxies denser in the past? |
Kurk (LBTB) |
3.0A 3.0B |
Direct constraints on feedback and first black hole weighing in an individual star-forming galaxy at z=2.2 |
Inskip (LBTB) |
0.5 |
Hbeta -based black hole mass of the gravitationally lensed quasar HE0047–1756 at z=1.67 |
Lamer (LBTB) |
0.5A 0.5B |
NIR Imaging of a Distant XMM/LBT Cluster Candidate |
Germeroth (LBTB) |
0.5 |
The cluster environment of the QSO SDSS J0222-0003 |
Bik (LBTB) |
1.4 |
The stellar content of high-mass star-forming region S255 |
Fan (AZ) |
3.0 |
LUCIFER Spectroscopy of the Most Distant Quasars at z > 6:2: Probing the Earliest Supermassive Black Holes |
McLinden (AZ) |
4.0 |
Metallicities and Kinematics of Lyman-alpha Galaxies at z=3.1 |
Priority B Projects |
||
Johnson (OSU/RC) |
1.75 | Reconstructing the Sagittarius dSph and its Impact on the MilkyWay Halo |
Woodward (OSU/RC) |
0.85 | LUCIFER Spectroscopy of Classical Novae in Outburst |
Dietrich (OSU/RC) |
1.7 | A LUCIFER SDT proposal to measure black hole masses and luminosities of high redshift quasars |
Kochanek (OSU/RC) |
0.5 | The Source Redshift of an Infra-Red Einstein Ring |
Dietrich (OSU/RC) |
0.43 | AGN Outflows and HeI 10830 Absorption |
Reines (OSU/RC) |
0.67 | AGN Activity in Henize 2-10 |
Andreon (INAF) |
5.5 | The mass build up history of cluster galaxies in the last 10.2 Gyr |
Scandariato (INAF) |
0.3 | Understanding PAR 2208, the reddest source in the Orion Nebula |
Piranomonte (INAF) |
4.0 | We can be EROs ... just for one night |
Quirrenbach (LBTB) |
1.0 | SBS 0335−052 E: A Vigorously Star-Forming Metal-Poor Galaxy |
Brandner (LBTB) |
0.8 | Massive Stellar Content of Giant HII regions in M31 |
Krause (LBTB) |
1.0 | Imaging of the Cas A Supernova Remnant |
Zibetti (LBTB) |
2.55 | Testing stellar population synthesis models in the NIR: the impact of the TP-AGB phase in post-starburst galaxies |
Bechtold (AZ) |
3.8 | Under the Microscope: LUCIFER Observations of High-Redshift Lensed Galaxies |
Bian (AZ) |
1.5 | Rest-frame Optical Spectra of Two Lensed Lyman Break Galaxies (LBGs) at z ~2 |
McGreer (AZ) |
3.75 | Investigating black hole growth at z~2.2 through IR spectroscopy of quasars |
LUCIFER SDT Publication Policy:
- Data obtained during SDT will be immediately available to all of the other SDT participants (across all partners) via the LBT data archive;
- All papers based on SDT data should be circulated to the SDT email list two weeks prior to submission;
- All SDT participants may be co-authors on any other papers based on SDT data if they request co-authorship. LUCIFER instrument team members, LBTO and SDT observers are encouraged to request co-authorship;
- Co-authors from outside the LBT partnership are allowed to request co-authorship if they contribute significantly to a specific paper, although LBT partners are to lead all papers. Such request should also be sent to the SDT mailing list by the project PI with a short justification, and be approved by the paper first author. Any dispute in authorship will be resolved by the LBTO director;
- All LBT papers should include the standard LBT credit line as described on the LBT Instrumentation webpage.
LUCIFER SDT (December 5-16, 2009)
- The SDT Call for Proposals (PDF)
- A latex template and style file
- Offered for seeing-limited imaging and long-slit spectroscopy
- Proposals due at each partner as specified in the Call for Proposals
- The LUCIFER Exposure Time Calculator (ETC)