Difference: ObservingProposals (1 vs. 20)

Revision 202020-05-19 - SaraFrederick

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

CURRENT

Line: 33 to 33
 
  • Title: The First X-ray View of a New Class of Changing-Look AGN with XMM and NuSTAR
  • PI: Sara Frederick
  • Co-Is: Suvi Gezari, Matthew Graham, Richard Mushotzky
Changed:
<
<
  • Deadline: (Phase II) Jan 31, 2020 at 13:00 UT (opens Jan 8-17th )
>
>
  • Deadline: (Phase II Budget) July 12, 2020 at 5:30 PM EST
 
  • Date range: May 2020 - April 2021
  • Time allocated: 6 CL LINERs for 58 ks of XMM, and 4 of these with NuSTAR for 80 ks total
  • Observing Plan: joint XMM+NuSTAR single epoch observations

Revision 192019-12-10 - SaraFrederick

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

CURRENT

Line: 35 to 35
 
  • Co-Is: Suvi Gezari, Matthew Graham, Richard Mushotzky
  • Deadline: (Phase II) Jan 31, 2020 at 13:00 UT (opens Jan 8-17th )
  • Date range: May 2020 - April 2021
Changed:
<
<
  • Time allocated: 6 CL LINERs for 58 ks of XMM and 80 ks of NuSTAR
>
>
  • Time allocated: 6 CL LINERs for 58 ks of XMM, and 4 of these with NuSTAR for 80 ks total
 
  • Observing Plan: joint XMM+NuSTAR single epoch observations

EXPIRED

Revision 182019-12-04 - SaraFrederick

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

CURRENT

Line: 27 to 27
 
  • Co-Is: Suvi Gezari, Matthew Graham
  • Date range: 1 August 2019 - 31 January 2020 (2019B)
  • Time allocated: 7.55 hr on Gemini GMOS-N
Changed:
<
<
  • Observing plan: We propose for Gemini spectroscopic monitoring of 4 CL LINER candiates. The observations will have 3 epochs separated by 1 month, and a response time of <1 week for the initial epoch.
    .
>
>
  • Observing plan: We propose for Gemini spectroscopic monitoring of 4 CL LINER candiates. The observations will have 3 epochs separated by 1 month, and a response time of <1 week for the initial epoch.

XMM-Newton (PI: Frederick)

  • Status: Approved (AO-19)
  • Title: The First X-ray View of a New Class of Changing-Look AGN with XMM and NuSTAR
  • PI: Sara Frederick
  • Co-Is: Suvi Gezari, Matthew Graham, Richard Mushotzky
  • Deadline: (Phase II) Jan 31, 2020 at 13:00 UT (opens Jan 8-17th )
  • Date range: May 2020 - April 2021
  • Time allocated: 6 CL LINERs for 58 ks of XMM and 80 ks of NuSTAR
  • Observing Plan: joint XMM+NuSTAR single epoch observations
 

EXPIRED

HST (PI: Cenko)

  • Status: Accepted

Revision 172019-10-01 - SaraFrederick

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

CURRENT

Line: 20 to 20
 
  • Date range: Oct 2019 to August 2020
  • Time allocated: 11 orbits
  • Observing Plan: Both AT2018zr and AT2018hco were observed with HST STIS ~months after peak. We will revisit these two TDEs in Cycle 27 with HST STIS to obtain their late-time UV spectra and study line variability on a yearly timescale.
Changed:
<
<

>
>

Gemini (PI: Frederick)

  • Status: Accepted
  • Title: The Real-Time Appearance of the BLR in a New Class of Changing-Look LINERs Discovered by ZTF
  • PI: Sara Frederick
  • Co-Is: Suvi Gezari, Matthew Graham
  • Date range: 1 August 2019 - 31 January 2020 (2019B)
  • Time allocated: 7.55 hr on Gemini GMOS-N
  • Observing plan: We propose for Gemini spectroscopic monitoring of 4 CL LINER candiates. The observations will have 3 epochs separated by 1 month, and a response time of <1 week for the initial epoch.
    .
 

EXPIRED

HST (PI: Cenko)

  • Status: Accepted

Revision 162019-09-17 - TiaraHung

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

CURRENT

Line: 11 to 11
 
  • Date range: May 2019 to April 2020
  • Time allocated: 6 TDEs x 2 x 18 ks = 216 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus one more epochs at t1+5 month.
Added:
>
>

HST (PI: Hung)

  • Status: Approved (Cycle 27)
  • Title: Late-time UV spectroscopy of Tidal Disruption Events with HST
  • PI: Tiara Hung
  • Co-Is: Brad Cenko, Sjoert van Velzen, Suvi Gezari, Nadia Blagorodnova, Nathan Roth, Ryan Foley
  • Deadline: N/A
  • Date range: Oct 2019 to August 2020
  • Time allocated: 11 orbits
  • Observing Plan: Both AT2018zr and AT2018hco were observed with HST STIS ~months after peak. We will revisit these two TDEs in Cycle 27 with HST STIS to obtain their late-time UV spectra and study line variability on a yearly timescale.

 

EXPIRED

HST (PI: Cenko)

  • Status: Accepted

Revision 152019-09-16 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Changed:
<
<

>
>

CURRENT

XMM-Newton (PI: Gezari)

  • Status: Approved (AO-18)
  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
  • PI: Suvi Gezari
  • Co-Is: Brad Cenko, Sjoert van Velzen, Sara Frederick, Shri Kulkarni, Nathan Roth, Tiara Hung,
  • Deadline: N/A
  • Date range: May 2019 to April 2020
  • Time allocated: 6 TDEs x 2 x 18 ks = 216 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus one more epochs at t1+5 month.

EXPIRED

 

HST (PI: Cenko)

  • Status: Accepted
  • Title: Multi-Wavelength Spectroscopy of Tidal Disruption Flares: A Legacy Sample for the LSST Era
Line: 21 to 31
 
  • Observing Plan: Two FAST follow-up observation in X-band, followed by 5 multi-frequency SED observations if detected.
  • Joint time: Chandra 60 Ksecs
Deleted:
<
<

XMM-Newton (PI: Gezari)

  • Status: Approved (AO-18)
  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
  • PI: Suvi Gezari
  • Co-Is: Brad Cenko, Sjoert van Velzen, Sara Frederick, Shri Kulkarni, Nathan Roth, Tiara Hung,
  • Deadline: N/A
  • Date range: May 2019 to April 2020
  • Time allocated: 6 TDEs x 2 x 18 ks = 216 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus one more epochs at t1+5 month.
 

Swift (PI: Gezari)

  • Status: Rejected
  • Title: Swift Observations of Infant Tidal Disruption Events in ZTF: Building a Legacy Sample

Revision 142019-09-15 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

Line: 22 to 22
 
  • Joint time: Chandra 60 Ksecs

XMM-Newton (PI: Gezari)

Changed:
<
<
  • Status: Approved
>
>
  • Status: Approved (AO-18)
 
  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
  • PI: Suvi Gezari
Changed:
<
<
  • Co-Is: Brad Cenko, Tiara Hung, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Erin Kara, Nathan Roth, Lin Yan
>
>
  • Co-Is: Brad Cenko, Sjoert van Velzen, Sara Frederick, Shri Kulkarni, Nathan Roth, Tiara Hung,
 
  • Deadline: N/A
Changed:
<
<
  • Date range: May 2018 to April 2019
  • Time allocated: 2 TDEs x 3 x 18 ks = 108 ks
  • Observing Plan: Observe 2 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.
>
>
  • Date range: May 2019 to April 2020
  • Time allocated: 6 TDEs x 2 x 18 ks = 216 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus one more epochs at t1+5 month.
 

Swift (PI: Gezari)

  • Status: Rejected
  • Title: Swift Observations of Infant Tidal Disruption Events in ZTF: Building a Legacy Sample

Revision 132019-04-16 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

Line: 31 to 31
 
  • Time allocated: 2 TDEs x 3 x 18 ks = 108 ks
  • Observing Plan: Observe 2 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.

Swift (PI: Gezari)

Changed:
<
<
  • Status: Submitted
>
>
  • Status: Rejected
 
  • Title: Swift Observations of Infant Tidal Disruption Events in ZTF: Building a Legacy Sample
  • PI: Suvi Gezari
  • Co-Is: Sjoert van Velzen, Tiara Hung,
Line: 39 to 39
 
  • Date range: April 2019 to April 2021
  • Time requested: 10 nuclear transients x 2 ksec in uvw2 each year; 20 x 2 ksec monitoring over 2 months for three X-ray bright TDE each year
  • Observing Plan: Observe 10 nuclear transients with one epoch of uvw2 to confirm UV-bright color of a TDE. Trigger monitoring with a cadence of 3 days over 2 months if confirmed TDE is detected by Swift XRT.
Deleted:
<
<
 

Gemini (PI: Hung)

Changed:
<
<
  • Status: Pending
>
>
  • Status: Accepted
 
  • Title: Early spectroscopic evolution of tidal disruption events
  • PI: Tiara Hung
  • Co-Is: Nathan Roth, Ryan Foley, Suvi Gezari, Sjoert van Velzen, Nadia Blagorodnova, Brad Cenko, Jonathan Brown, Cesar Rojas-Bravo, Charles Kilpatrick, Lixin Dai

Revision 122018-10-07 - TiaraHung

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Changed:
<
<
>
>

 

HST (PI: Cenko)

  • Status: Accepted
  • Title: Multi-Wavelength Spectroscopy of Tidal Disruption Flares: A Legacy Sample for the LSST Era
Line: 40 to 40
 
  • Time requested: 10 nuclear transients x 2 ksec in uvw2 each year; 20 x 2 ksec monitoring over 2 months for three X-ray bright TDE each year
  • Observing Plan: Observe 10 nuclear transients with one epoch of uvw2 to confirm UV-bright color of a TDE. Trigger monitoring with a cadence of 3 days over 2 months if confirmed TDE is detected by Swift XRT.
  • Link on overleaf (view only): https://v2.overleaf.com/read/qhwfzdwqczfb
Added:
>
>

Gemini (PI: Hung)

  • Status: Pending
  • Title: Early spectroscopic evolution of tidal disruption events
  • PI: Tiara Hung
  • Co-Is: Nathan Roth, Ryan Foley, Suvi Gezari, Sjoert van Velzen, Nadia Blagorodnova, Brad Cenko, Jonathan Brown, Cesar Rojas-Bravo, Charles Kilpatrick, Lixin Dai
  • Date range: February 1, 2019 to July 31, 2019
  • Time allocated: 10.25 hr on Gemini GMOS-N
  • Observing plan: We propose for Gemini spectroscopic monitoring of 2 rising, bright TDEs that are no older than 2 weeks. The observations will have 7 epochs, with the first 4 separated by 10 days and then 3 later epochs separated by 20 days.

Revision 112018-10-01 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 31 to 31
 
  • Time allocated: 2 TDEs x 3 x 18 ks = 108 ks
  • Observing Plan: Observe 2 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.

Swift (PI: Gezari)

Changed:
<
<
  • Status: In Prep
  • Title: Infant Tidal Disruption Events in ZTF: Swift-Enabled Early Discovery and Multi-band Characterization
>
>
  • Status: Submitted
  • Title: Swift Observations of Infant Tidal Disruption Events in ZTF: Building a Legacy Sample
 
  • PI: Suvi Gezari
  • Co-Is: Sjoert van Velzen, Tiara Hung,
  • Deadline: Sep 27th at 4:30pm Eastern
  • Date range: April 2019 to April 2021
Changed:
<
<
  • Time requested: 30 nuclear transients x 2 ksec in uvw2 each year; 20 x 2 ksec monitoring over 2 months for one X-ray bright TDE each year
  • Observing Plan: Observe 30 nuclear transients with one epoch of uvw2 to confirm UV-bright color of a TDE. Trigger monitoring with a cadence of 3 days over 2 months if confirmed TDE is detected by Swift XRT.
>
>
  • Time requested: 10 nuclear transients x 2 ksec in uvw2 each year; 20 x 2 ksec monitoring over 2 months for three X-ray bright TDE each year
  • Observing Plan: Observe 10 nuclear transients with one epoch of uvw2 to confirm UV-bright color of a TDE. Trigger monitoring with a cadence of 3 days over 2 months if confirmed TDE is detected by Swift XRT.
  \ No newline at end of file

Revision 102018-09-25 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 30 to 30
 
  • Date range: May 2018 to April 2019
  • Time allocated: 2 TDEs x 3 x 18 ks = 108 ks
  • Observing Plan: Observe 2 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.
Added:
>
>

Swift (PI: Gezari)

  • Status: In Prep
  • Title: Infant Tidal Disruption Events in ZTF: Swift-Enabled Early Discovery and Multi-band Characterization
  • PI: Suvi Gezari
  • Co-Is: Sjoert van Velzen, Tiara Hung,
  • Deadline: Sep 27th at 4:30pm Eastern
  • Date range: April 2019 to April 2021
  • Time requested: 30 nuclear transients x 2 ksec in uvw2 each year; 20 x 2 ksec monitoring over 2 months for one X-ray bright TDE each year
  • Observing Plan: Observe 30 nuclear transients with one epoch of uvw2 to confirm UV-bright color of a TDE. Trigger monitoring with a cadence of 3 days over 2 months if confirmed TDE is detected by Swift XRT.
  • Link on overleaf (view only): https://v2.overleaf.com/read/qhwfzdwqczfb
 \ No newline at end of file

Revision 92018-06-21 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 30 to 30
 
  • Date range: May 2018 to April 2019
  • Time allocated: 2 TDEs x 3 x 18 ks = 108 ks
  • Observing Plan: Observe 2 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.
Deleted:
<
<

Swift (PI: Hung)

  • Status: Submitted
  • Title: Photometric reverberation mapping of Tidal Disruption Events from ZTF
  • PI: Tiara Hung
  • Co-Is: Suvi Gezari, Brad Cenko, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Nathan Roth, Lin Yan
  • Date range: April 2018 to April 2019
  • Time allocated: Requested 2 x 30 x 2 ks = 120 ks
  • Observing Plan: Observe 2 rising TDEs with magnitudes accessible by SEDM. The goal is to use Swift to sample TDE light curves on a daily cadence with XRT and 6 filters of UVOT (UV + optical) to map reverberation in TDEs.
 \ No newline at end of file

Revision 82018-02-03 - SaraFrederick

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 39 to 39
 
  • Date range: April 2018 to April 2019
  • Time allocated: Requested 2 x 30 x 2 ks = 120 ks
  • Observing Plan: Observe 2 rising TDEs with magnitudes accessible by SEDM. The goal is to use Swift to sample TDE light curves on a daily cadence with XRT and 6 filters of UVOT (UV + optical) to map reverberation in TDEs.
Deleted:
<
<

Swift (PI: Frederick)

  • Status: Submitted
  • Title: Caught in the Act: Investigating the X-ray/UV Variability Connection in Changing-Look AGN Mined with ZTF
  • PI: Sara Frederick
  • Co-Is: Suvi Gezari, Tiara Hung, Erin Kara, Richard Mushotzky, Drew Hogg
  • Date range: April 2018 to April 2019
  • Time allocated: 2 x 15 x 5 ks = 150 ks
  • Observing Plan: Observe 2 new CLAGNs with 15 observations with a 3 day cadence.

Revision 72017-11-29 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 22 to 22
 
  • Joint time: Chandra 60 Ksecs

XMM-Newton (PI: Gezari)

Changed:
<
<
  • Status: Submitted
>
>
  • Status: Approved
 
  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
  • PI: Suvi Gezari
  • Co-Is: Brad Cenko, Tiara Hung, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Erin Kara, Nathan Roth, Lin Yan
  • Deadline: N/A
  • Date range: May 2018 to April 2019
Changed:
<
<
  • Time allocated: Requested 6 x 3 x 15 ks = 270 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.
>
>
  • Time allocated: 2 TDEs x 3 x 18 ks = 108 ks
  • Observing Plan: Observe 2 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.
 

Swift (PI: Hung)

  • Status: Submitted

Revision 62017-11-13 - SjoertVanVelzen

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 11 to 11
 
  • Time allocated: 70 orbits with STIS, plus 2 nights of Gemini
  • Observing plan: Here we propose to obtain a sequence of UV (HST) and optical (Gemini/GMOS) spectra for a sample of 5 TDFs discovered by the Zwicky Transient Facility, doubling the number of TDFs with UV spectra.
Added:
>
>

VLA (PI: van Velzen)

  • Status: Accepted (Priority B)
  • Title: Systematic radio follow-up of stellar tidal disruption flares
  • PI: Sjoert van Velzen
  • Co-Is: Suvi Gezari, Brad Cenko, James Miller-Jones, Tiara Hung, Shri Kulkarni, Nadejda Blagorodnova, Yan Lin
  • Date range: 2018A and 2018B
  • Time allocated/requested: 32 hours (15 FAST triggers; 2 SED triggers)
  • Observing Plan: Two FAST follow-up observation in X-band, followed by 5 multi-frequency SED observations if detected.
  • Joint time: Chandra 60 Ksecs
 

XMM-Newton (PI: Gezari)

  • Status: Submitted
  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
Line: 38 to 48
 
  • Date range: April 2018 to April 2019
  • Time allocated: 2 x 15 x 5 ks = 150 ks
  • Observing Plan: Observe 2 new CLAGNs with 15 observations with a 3 day cadence.
Deleted:
<
<

VLA (PI: van Velzen)

  • Status: Submitted
  • Title: Systematic radio follow-up of stellar tidal disruption flares
  • PI: Sjoert van Velzen
  • Co-Is: Suvi Gezari, Brad Cenko, James Miller-Jones, Tiara Hung, Shri Kulkarni, Nadejda Blagorodnova, Yan Lin
  • Date range: 2018A and 2018B
  • Time allocated/requested: 32 hours (15 FAST triggers; 2 SED triggers)
  • Observing Plan: Two FAST follow-up observation in X-band, followed by 5 multi-frequency SED observations if detected.
  • Joint time: Chandra 60 Ksecs

Revision 52017-11-09 - SjoertVanVelzen

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

HST (PI: Cenko)

Added:
>
>
  • Status: Accepted
 
  • Title: Multi-Wavelength Spectroscopy of Tidal Disruption Flares: A Legacy Sample for the LSST Era
  • PI: Brad Cenko
  • Co-Is: Suvi Gezari, Tiara Hung, Nadia Blagorodnova, Shri Kulkarni, Lin Yan, Nathan Roth, Sylvain Veilleux, Erin Kara, Sjoert van Velzen
Deleted:
<
<
  • Deadline: N/A
  • Status: Accepted
 
  • Date range: October 1, 2017 to September 30, 2018
  • Time allocated: 70 orbits with STIS, plus 2 nights of Gemini
  • Observing plan: Here we propose to obtain a sequence of UV (HST) and optical (Gemini/GMOS) spectra for a sample of 5 TDFs discovered by the Zwicky Transient Facility, doubling the number of TDFs with UV spectra.

XMM-Newton (PI: Gezari)

Added:
>
>
  • Status: Submitted
 
  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
  • PI: Suvi Gezari
  • Co-Is: Brad Cenko, Tiara Hung, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Erin Kara, Nathan Roth, Lin Yan
  • Deadline: N/A
Deleted:
<
<
  • Status: Submitted
 
  • Date range: May 2018 to April 2019
  • Time allocated: Requested 6 x 3 x 15 ks = 270 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.

Swift (PI: Hung)

Added:
>
>
  • Status: Submitted
 
  • Title: Photometric reverberation mapping of Tidal Disruption Events from ZTF
  • PI: Tiara Hung
  • Co-Is: Suvi Gezari, Brad Cenko, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Nathan Roth, Lin Yan
Deleted:
<
<
  • Deadline: N/A
  • Status: Submitted
 
  • Date range: April 2018 to April 2019
  • Time allocated: Requested 2 x 30 x 2 ks = 120 ks
  • Observing Plan: Observe 2 rising TDEs with magnitudes accessible by SEDM. The goal is to use Swift to sample TDE light curves on a daily cadence with XRT and 6 filters of UVOT (UV + optical) to map reverberation in TDEs.

Swift (PI: Frederick)

Added:
>
>
  • Status: Submitted
 
  • Title: Caught in the Act: Investigating the X-ray/UV Variability Connection in Changing-Look AGN Mined with ZTF
  • PI: Sara Frederick
  • Co-Is: Suvi Gezari, Tiara Hung, Erin Kara, Richard Mushotzky, Drew Hogg
Deleted:
<
<
  • Deadline: N/A
  • Status: Submitted
 
  • Date range: April 2018 to April 2019
  • Time allocated: 2 x 15 x 5 ks = 150 ks
  • Observing Plan: Observe 2 new CLAGNs with 15 observations with a 3 day cadence.
Changed:
<
<

-- SuviGezari - 20 Oct 2017

>
>

VLA (PI: van Velzen)

  • Status: Submitted
  • Title: Systematic radio follow-up of stellar tidal disruption flares
  • PI: Sjoert van Velzen
  • Co-Is: Suvi Gezari, Brad Cenko, James Miller-Jones, Tiara Hung, Shri Kulkarni, Nadejda Blagorodnova, Yan Lin
  • Date range: 2018A and 2018B
  • Time allocated/requested: 32 hours (15 FAST triggers; 2 SED triggers)
  • Observing Plan: Two FAST follow-up observation in X-band, followed by 5 multi-frequency SED observations if detected.
  • Joint time: Chandra 60 Ksecs

Revision 42017-10-31 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 32 to 32
 
  • Time allocated: Requested 2 x 30 x 2 ks = 120 ks
  • Observing Plan: Observe 2 rising TDEs with magnitudes accessible by SEDM. The goal is to use Swift to sample TDE light curves on a daily cadence with XRT and 6 filters of UVOT (UV + optical) to map reverberation in TDEs.
Changed:
<
<

Telescope (PI: xx)

  • Title:
  • PI:
  • Co-Is:
  • Deadline:
  • Status:
  • Date range:
  • Time allocated:
  • Observing Plan:
>
>

Swift (PI: Frederick)

  • Title: Caught in the Act: Investigating the X-ray/UV Variability Connection in Changing-Look AGN Mined with ZTF
  • PI: Sara Frederick
  • Co-Is: Suvi Gezari, Tiara Hung, Erin Kara, Richard Mushotzky, Drew Hogg
  • Deadline: N/A
  • Status: Submitted
  • Date range: April 2018 to April 2019
  • Time allocated: 2 x 15 x 5 ks = 150 ks
  • Observing Plan: Observe 2 new CLAGNs with 15 observations with a 3 day cadence.
 

Revision 32017-10-25 - TiaraHung

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Line: 22 to 22
 
  • Time allocated: Requested 6 x 3 x 15 ks = 270 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.
Added:
>
>

Swift (PI: Hung)

  • Title: Photometric reverberation mapping of Tidal Disruption Events from ZTF
  • PI: Tiara Hung
  • Co-Is: Suvi Gezari, Brad Cenko, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Nathan Roth, Lin Yan
  • Deadline: N/A
  • Status: Submitted
  • Date range: April 2018 to April 2019
  • Time allocated: Requested 2 x 30 x 2 ks = 120 ks
  • Observing Plan: Observe 2 rising TDEs with magnitudes accessible by SEDM. The goal is to use Swift to sample TDE light curves on a daily cadence with XRT and 6 filters of UVOT (UV + optical) to map reverberation in TDEs.
 

Telescope (PI: xx)

  • Title:
  • PI:

Revision 22017-10-23 - SuviGezari

Line: 1 to 1
 
META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS
Changed:
<
<

HST

>
>

HST (PI: Cenko)

 
  • Title: Multi-Wavelength Spectroscopy of Tidal Disruption Flares: A Legacy Sample for the LSST Era
  • PI: Brad Cenko
  • Co-Is: Suvi Gezari, Tiara Hung, Nadia Blagorodnova, Shri Kulkarni, Lin Yan, Nathan Roth, Sylvain Veilleux, Erin Kara, Sjoert van Velzen
Line: 12 to 12
 
  • Time allocated: 70 orbits with STIS, plus 2 nights of Gemini
  • Observing plan: Here we propose to obtain a sequence of UV (HST) and optical (Gemini/GMOS) spectra for a sample of 5 TDFs discovered by the Zwicky Transient Facility, doubling the number of TDFs with UV spectra.
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XMM-Newton (PI: Gezari)

  • Title: Probing the Accretion Timescales in TDEs with ZTF and XMM
  • PI: Suvi Gezari
  • Co-Is: Brad Cenko, Tiara Hung, Sjoert van Velzen, Shri Kulkarni, Nadia Blagorodnova, Erin Kara, Nathan Roth, Lin Yan
  • Deadline: N/A
  • Status: Submitted
  • Date range: May 2018 to April 2019
  • Time allocated: Requested 6 x 3 x 15 ks = 270 ks
  • Observing Plan: Observe 6 TDEs that are discovered pre-peak. Take an initial observation within a week of discovery (t1) , plus two more epochs at t1+1 month and t1+3 months.

Telescope (PI: xx)

 
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Revision 12017-10-20 - SuviGezari

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META TOPICPARENT name="AGNTDEWorkingGroup"
OBSERVING PROPOSALS

HST

  • Title: Multi-Wavelength Spectroscopy of Tidal Disruption Flares: A Legacy Sample for the LSST Era
  • PI: Brad Cenko
  • Co-Is: Suvi Gezari, Tiara Hung, Nadia Blagorodnova, Shri Kulkarni, Lin Yan, Nathan Roth, Sylvain Veilleux, Erin Kara, Sjoert van Velzen
  • Deadline: N/A
  • Status: Accepted
  • Date range: October 1, 2017 to September 30, 2018
  • Time allocated: 70 orbits with STIS, plus 2 nights of Gemini
  • Observing plan: Here we propose to obtain a sequence of UV (HST) and optical (Gemini/GMOS) spectra for a sample of 5 TDFs discovered by the Zwicky Transient Facility, doubling the number of TDFs with UV spectra.

Telescope

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  • PI:
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  • Deadline:
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  • Abstract:

-- SuviGezari - 20 Oct 2017

View topic | History: r20 < r19 < r18 < r17 | More topic actions...
 
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