0
Assigned ID: 732
----- Attempting Submission 1 (Fri Apr 10 19:50:49 GMT 2015) -----
0
----- Attempting Submission 1 (Thu Jul 23 06:31:48 GMT 2015) -----
Characterizing the Circumgalactic Medium of Luminous Red Galaxies
We propose to survey the Circumgalactic Medium (CGM) of 15 Luminous Red Galaxies (LRGs) at z~0.5, drawn from the SDSS-III/Baryon Oscillation Spectroscopic Survey (BOSS). Through the analysis of SDSS quasar spectra lying fortuitously behind LRGs, we have established that these galaxies exhibit significant (even strong) MgII absorption on scales from several tens kpc to more than tens of Mpc (Zhu et al. 2014). The results at ~100 kpc, i.e. well within the virial radius of the LRG halos, reveal that these massive, non star-forming galaxies exhibit a cool and enriched CGM that even rivals that for modern, L* galaxies. With COS G140L spectroscopy, we will characterize the HI Lyman series and Lyman limit opacity of the LRG CGM at impact parameters r_p=30-400 kpc (2/3 of the LRG virial radius). These data will constrain the mass of the cool CGM of these massive galaxies and enable the estimate of the gas metallicity (especially for the systems that exhibit positive MgII absorption). Furthermore, these spectra will characterize the incidence of strong highly-ionized absorption lines, such as CIII, SiIII and OVI. Our results will inform on the processes that influence the origin and evolution of halo gas, e.g. the transition from a primarily cool CGM to a hot, X-ray halo as galaxies gain mass and evolve towards the group and cluster environment.
We will survey the Circumgalactic Medium (CGM) of 15 Luminous Red Galaxies (LRGs) at z~0.5 with higher-redshift background quasars, both drawn from the SDSS-III/Baryon Oscillation Spectroscopic Survey (BOSS). We will obtain FUV spectra of the background quasars with COS G140L at 1280 Angstrom. The total number of orbits is 33. All sources will be observed with the Primary Science Aperture at all four FP-POS positions.
QUASAR ABSORPTION LINES AND IGM
12
false
true
false
false
false
false
SUPPORTED
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
GALAXY
QSO
NO
This object was generated by the targetselector and retrieved from the GALEX database.
J2000
J2000
COS/FUV
Spectroscopic
No
No
G140L
1280
COS/FUV
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No
No
G140L
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COS/FUV
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COS/FUV
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G140L
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COS/FUV
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COS/FUV
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G140L
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COS/FUV
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COS/FUV
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Spectroscopic
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Spectroscopic
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G140L
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COS/FUV
Spectroscopic
No
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G140L
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COS/FUV
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G140L
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true
2
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 17.4009 in filter Galex/NUV
Redshift: z=0.997164
Emission Lines: None
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Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
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Emission Lines: None
The scheduling data was generated by CASM 23.2.
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true
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Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 18.4216 in filter Galex/NUV
Redshift: z=0.670011
Emission Lines: None
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Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 19.0276 in filter Galex/FUV
Redshift: z=0.670011
Emission Lines: None
The scheduling data was generated by CASM 23.2.
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true
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Target: [point source]
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Normalization: Renormalized to abmag = 17.425 in filter Galex/NUV
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Emission Lines: None
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Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 18.1241 in filter Galex/FUV
Redshift: z=0.77591
Emission Lines: None
The scheduling data was generated by CASM 23.2.
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true
4
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 18.8747 in filter Galex/NUV
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Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 19.7997 in filter Galex/FUV
Redshift: z=0.922655
The scheduling data was generated by CASM 23.2.
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true
4
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 18.9624 in filter Galex/NUV
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Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 20.0321 in filter Galex/FUV
Redshift: z=1.23041
The scheduling data was generated by CASM 23.2.
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true
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Target: [point source]
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Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 19.0599 in filter Galex/FUV
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Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
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Redshift: z=0.731663
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Normalization: Renormalized to abmag = 17.6568 in filter Galex/NUV
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Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
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true
4
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 18.6502 in filter Galex/NUV
Redshift: z=1.20985
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 20.4025 in filter Galex/FUV
Redshift: z=1.20985
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
1
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 17.4313 in filter Galex/NUV
Redshift: z=0.652754
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 18.2146 in filter Galex/FUV
Redshift: z=0.652754
Timing link suitability includes constraints ([16 After 11])
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
4
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 18.8854 in filter Galex/NUV
Redshift: z=1.46385
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 19.8932 in filter Galex/FUV
Redshift: z=1.46385
The scheduling data was generated by CASM 23.2.
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true
2
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 17.9309 in filter Galex/NUV
Redshift: z=0.946542
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 18.9855 in filter Galex/FUV
Redshift: z=0.946542
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
2
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 17.7664 in filter Galex/NUV
Redshift: z=0.798396
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 19.3295 in filter Galex/FUV
Redshift: z=0.798396
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
1
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 17.474 in filter Galex/NUV
Redshift: z=0.615606
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 17.913 in filter Galex/FUV
Redshift: z=0.615606
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
1
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 17.569 in filter Galex/NUV
Redshift: z=0.717006
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 18.5418 in filter Galex/FUV
Redshift: z=0.717006
Timing link suitability includes constraints ([16 After 11])
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
1
0
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.03 applied before normalization
Normalization: Renormalized to abmag = 18.8854 in filter Galex/NUV
Redshift: z=1.46385
Target: [point source]
Spectrum: Non-stellar Objects QSO (FOS based) [100, 3387 Ang z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.05 applied before normalization
Normalization: Renormalized to abmag = 19.8932 in filter Galex/FUV
Redshift: z=1.46385