DATE MOON INST OBSERVER PI AND PROGRAM FILT Jan 1 Wed 0.41 KEPcam Bieryla R Bieryla TESS TOI KEP NEW YEAR's DAY Jan 2 Thu 0.50 " " " " Jan 3 Fri 0.60 " " " " Jan 4 Sat 0.69 " " " " Jan 5 Sun 0.78 " " " " Jan 6 Mon 0.86 " " " " Jan 7 Tue 0.92 " " " " Jan 8 Wed 0.97 " " " " Jan 9 Thu 1.00 " " " " Jan 10 Fri 1.00 " " " " Jan 11 Sat 0.97 " " " " Jan 12 Sun 0.91 " " " " Jan 13 Mon 0.84 " " " " Jan 14 Tue 0.74 " " " " Jan 15 Wed 0.63 " " " " Jan 16 Thu 0.52 " " " " Jan 17 Fri 0.41 " " " " Jan 18 Sat 0.30 " " " " Jan 19 Sun 0.21 " " " " Jan 20 Mon 0.13 " " " " MLK DAY Jan 21 Tue 0.07 " " " " Jan 22 Wed 0.03 " Falco Falco Eng " Jan 23 Thu 0.00 " Gomez R Gomez FLEET " Jan 24 Fri 0.00 " Bieryla R Bieryla TESS TOI " Jan 25 Sat 0.02 " " " " Jan 26 Sun 0.05 " " " " Jan 27 Mon 0.10 " " " " Jan 28 Tue 0.17 " " " " Jan 29 Wed 0.24 " " " " Jan 30 Thu 0.33 " " " " Jan 31 Fri 0.42 " " " " ** MOON IS FRACTIONAL MOON ILLUMINATION AT MIDDLE OF NIGHT **** DATE IS STANDARD TIME AT START OF NIGHT
Observers are required to spend no more than 10% of their time doing the following service observing: Hosseinzadeh (GW events), Gomez (FLEET), Green (CLQ monitoring), Benbow (Blazars).
NOTE: Projects are listed in order of decreasing priority per their TAC
grades. Rare TOO targets (GRBs, XRNs) have highest priority.
48" Schedule for the Month of February 2020
(as of 11 December 2019)
December 2019
January February
March April
January 2021
Mt. Hopkins
Programs
PDF
Schedules
DATE MOON INST OBSERVER PI AND PROGRAM FILT Feb 1 Sat 0.51 KEPcam Bieryla R Bieryla TESS TOI KEP Feb 2 Sun 0.61 " " " " Feb 3 Mon 0.71 " " " " Feb 4 Tue 0.80 " " " " Feb 5 Wed 0.88 " " " " Feb 6 Thu 0.94 " " " " Feb 7 Fri 0.98 " " " " Feb 8 Sat 1.00 " " " " Feb 9 Sun 0.98 " " " " Feb 10 Mon 0.94 " " " " Feb 11 Tue 0.87 " " " " Feb 12 Wed 0.78 " " " " Feb 13 Thu 0.67 " " " " Feb 14 Fri 0.56 " " " " Feb 15 Sat 0.45 " " " " Feb 16 Sun 0.35 " " " " Feb 17 Mon 0.25 " " " " PRESIDENT'S DAY Feb 18 Tue 0.17 " " " " Feb 19 Wed 0.10 " " " " Feb 20 Thu 0.05 " Falco Falco Eng " Feb 21 Fri 0.02 " Gomez R Gomez FLEET " Feb 22 Sat 0.00 " Bieryla R Bieryla TESS TOI " Feb 23 Sun 0.01 " " " " Feb 24 Mon 0.03 " " " " Feb 25 Tue 0.06 " " " " Feb 26 Wed 0.11 " " " " Feb 27 Thu 0.18 " " " " Feb 28 Fri 0.26 " " " " Feb 29 Sat 0.34 " " " " ** MOON IS FRACTIONAL MOON ILLUMINATION AT MIDDLE OF NIGHT **** DATE IS STANDARD TIME AT START OF NIGHT
Observers are required to spend no more than 10% of their time doing the following service observing: Hosseinzadeh (GW events), Gomez (FLEET), Green (CLQ monitoring), Benbow (Blazars).
NOTE: Projects are listed in order of decreasing priority per their TAC
grades. Rare TOO targets (GRBs, XRNs) have highest priority.
48" Schedule for the Month of March 2020
(as of 11 December 2019)
December 2019
January February
March April
January 2021
Mt. Hopkins
Programs
PDF
Schedules
DATE MOON INST OBSERVER PI AND PROGRAM FILT Mar 1 Sun 0.44 KEPcam Bieryla R Bieryla TESS TOI KEP Mar 2 Mon 0.54 " " " " Mar 3 Tue 0.64 " " " " Mar 4 Wed 0.74 " " " " Mar 5 Thu 0.83 " " " " Mar 6 Fri 0.91 " " " " Mar 7 Sat 0.97 " " " " Mar 8 Sun 1.00 " " " " Mar 9 Mon 0.99 " " " " Mar 10 Tue 0.96 " " " " Mar 11 Wed 0.90 " " " " Mar 12 Thu 0.81 " " " " Mar 13 Fri 0.72 " " " " Mar 14 Sat 0.61 " " " " Mar 15 Sun 0.50 " " " " Mar 16 Mon 0.40 " " " " Mar 17 Tue 0.30 " Berger Astro100 " Mar 18 Wed 0.22 " " " " Mar 19 Thu 0.14 " " " " Mar 20 Fri 0.09 " Bieryla R Bieryla TESS TOI " Mar 21 Sat 0.04 " " " " Mar 22 Sun 0.01 " " " " Mar 23 Mon 0.00 " Gomez R Gomez FLEET " Mar 24 Tue 0.01 " Falco Falco Eng " Mar 25 Wed 0.03 " Bieryla R Bieryla TESS TOI " Mar 26 Thu 0.07 " " " " Mar 27 Fri 0.13 " " " " Mar 28 Sat 0.20 " " " " Mar 29 Sun 0.28 " " " " Mar 30 Mon 0.38 " " " " Mar 31 Tue 0.48 " " " " ** MOON IS FRACTIONAL MOON ILLUMINATION AT MIDDLE OF NIGHT **** DATE IS STANDARD TIME AT START OF NIGHT
Observers are required to spend no more than 10% of their time doing the following service observing: Hosseinzadeh (GW events), Gomez (FLEET), Green (CLQ monitoring), Benbow (Blazars).
NOTE: Projects are listed in order of decreasing priority per their TAC
grades. Rare TOO targets (GRBs, XRNs) have highest priority.
48" Schedule for the Month of April 2020
(as of 11 December 2019)
December 2019
January February
March April
January 2021
Mt. Hopkins
Programs
PDF
Schedules
DATE MOON INST OBSERVER PI AND PROGRAM FILT Apr 1 Wed 0.58 KEPcam Bieryla R Bieryla TESS TOI KEP Apr 2 Thu 0.69 " " " " Apr 3 Fri 0.79 " " " " Apr 4 Sat 0.88 " " " " Apr 5 Sun 0.95 " " " " Apr 6 Mon 0.99 " " " " Apr 7 Tue 1.00 " " " " Apr 8 Wed 0.98 " " " " Apr 9 Thu 0.93 " " " " Apr 10 Fri 0.85 " " " " Apr 11 Sat 0.76 " " " " Apr 12 Sun 0.66 " " " " Apr 13 Mon 0.56 " " " " Apr 14 Tue 0.46 " " " " Apr 15 Wed 0.36 " " " " Apr 16 Thu 0.27 " " " " Apr 17 Fri 0.19 " " " " Apr 18 Sat 0.13 " " " " Apr 19 Sun 0.07 " " " " Apr 20 Mon 0.03 " " " " Apr 21 Tue 0.01 " Falco Falco Eng " Apr 22 Wed 0.00 " Gomez R Gomez FLEET " Apr 23 Thu 0.01 " Bieryla R Bieryla TESS TOI " Apr 24 Fri 0.04 " " " " Apr 25 Sat 0.09 " " " " Apr 26 Sun 0.15 " " " " Apr 27 Mon 0.23 " " " " Apr 28 Tue 0.33 " " " " Apr 29 Wed 0.43 " " " " Apr 30 Thu 0.54 " " " " ** MOON IS FRACTIONAL MOON ILLUMINATION AT MIDDLE OF NIGHT **** DATE IS STANDARD TIME AT START OF NIGHT
Observers are required to spend no more than 10% of their time doing the following service observing: Hosseinzadeh (GW events), Gomez (FLEET), Green (CLQ monitoring), Benbow (Blazars).
NOTE: Projects are listed in order of decreasing priority per their TAC grades. Rare TOO targets (GRBs, XRNs) have highest priority.
PI | Title | Dark | Gray | Bright |
---|---|---|---|---|
Griffin Hosseinzadeh | Keplercam Follow-up of Gravitational Wave Events | 1 | 0 | 0 |
Allyson Bieryla | Follow-up Observations of TESS Objects of Interests (TOIs) | 35 | 22 | 48 |
Edo Berger | Astro100: Using the FLWO 1.2m Telescope for Undergraduate Education | 0 | 3 | 0 |
Sebastian Gomez | FLEET: Finding Luminous and Exotic Extragalactic Transients | 6 | 0 | 0 |
Paul J Green | Monitoring of Changing-Look Quasars and Candidates | 2 | 0 | 0 |
Wystan Benbow | Understanding Blazars using Broadband Spectra and Light Curves | 4 | 0 | 0 |