Difference: NEOZTF_FollowUp (1 vs. 8)

Revision 82018-12-19 - ChowChoongNgeow

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META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

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APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
LOT* ~11' x ~11' ~20.5   Chow-Choong Ngeow cngeow@astro.ncu.edu.tw
Spacewatch       Melissa Brucker, mbrucker@lpl.arizona.edu
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GROWTH-INDIA 0.7deg x 0.7 deg ~21   Varun Bhalerao varunb@iitb.ac.in;
IAO 12.3' x 12.3' g=18.7, r=19.0, i=17.8   Takashi Horiuchi (takashi.horiuchi@nao.ac.jp), Hidekazu Hanayama (hanayama.hidekazu@nao.ac.jp)
 

Apache Point Observatory (APO)

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<		We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken in a single half-night block. Typically need a few nights to arrange scheduling before follow up can occur. APO is a 3.5m, with an imager with 7.5 sq arcminute FOV (6 filters available), as well as other instruments. This follow up time is probably most useful to investigate new objects of particular interest (such as mini-moons, interstellar objects, or objects where we pick up new activity), but could also help clean up astrometry for batches of NEOs (especially if this occurs at the same time as another trigger). https://www.apo.nmsu.edu/
>
>		We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken in a single half-night block. Typically need a few nights to arrange scheduling before follow up can occur. APO is a 3.5m, with an imager with 7.5 sq arcminute FOV (6 filters available), as well as other instruments. This follow up time is probably most useful to investigate new objects of particular interest (such as mini-moons, interstellar objects, or objects where we pick up new activity), but could also help clean up astrometry for batches of NEOs (especially if this occurs at the same time as another trigger). https://www.apo.nmsu.edu/
 

Lulin One-meter Telescope (LOT)

ToO can be requested for Solar-system follow-up. Most of the time LOT is equipped with Princeton Instrument's SOPHIA CCD (2k x 2k) with standard broadband filters, occasionally there will have instruments change. PS: Quan-Zhi can also trigger LOT ToO follow-up.

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GROWTH-India

The GROWTH-India telescope is a 0.7m telescope with a 0.7 degree field of view. We can go to about 21st mag in g band in 5-10 min exposures (depending on observing conditions). Currently, Varun can be the contact person for NEA followups.

Ishigakijima Astronomical Observatory (IAO), NAOJ

105 cm Murikabushi Telescope/MITSuME

 -- Emily Kramer - 2018-10-29 \ No newline at end of file

Revision 72018-10-29 - EmilyKramer

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Follow Up Observatory Resources

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 From the International Asteroid Warning Network (IAWN): http://iawn.net/features/astrometric.shtml

Facility Field of View Limiting Magnitude Pointing limits Contact info
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<
<
Facility 1 Field of view 1 Limiting mag 1 Pointing limit 1 Contact info 1
 
APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
LOT* ~11' x ~11' ~20.5   Chow-Choong Ngeow cngeow@astro.ncu.edu.tw
Spacewatch       Melissa Brucker, mbrucker@lpl.arizona.edu

Revision 62018-10-29 - EmilyKramer

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META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

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Facility 1 Field of view 1 Limiting mag 1 Pointing limit 1 Contact info 1
APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
LOT* ~11' x ~11' ~20.5   Chow-Choong Ngeow cngeow@astro.ncu.edu.tw
Added:
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>
Spacewatch       Melissa Brucker, mbrucker@lpl.arizona.edu
 

Apache Point Observatory (APO)

Added:
>
>
 We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken in a single half-night block. Typically need a few nights to arrange scheduling before follow up can occur. APO is a 3.5m, with an imager with 7.5 sq arcminute FOV (6 filters available), as well as other instruments. This follow up time is probably
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 https://www.apo.nmsu.edu/

Lulin One-meter Telescope (LOT)

Deleted:
<
<		ToO can be requested for Solar-system follow-up. Most of the time LOT is equipped with Princeton Instrument's SOPHIA CCD (2k x 2k) with standard broadband filters, occasionally there will have instruments change. PS: Quan-Zhi can also trigger LOT ToO follow-up.
 
Added:
>
>		ToO can be requested for Solar-system follow-up. Most of the time LOT is equipped with Princeton Instrument's SOPHIA CCD (2k x 2k) with standard broadband filters, occasionally there will have instruments change. PS: Quan-Zhi can also trigger LOT ToO follow-up.
 
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<		-- EmilyKramer - 24 Aug 2018
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>		-- Emily Kramer - 2018-10-29
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Revision 52018-09-10 - ChowChoongNgeow

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META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

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Facility Field of View Limiting Magnitude Pointing limits Contact info
Facility 1 Field of view 1 Limiting mag 1 Pointing limit 1 Contact info 1
APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
Changed:
<
<
>
>
LOT* ~11' x ~11' ~20.5   Chow-Choong Ngeow cngeow@astro.ncu.edu.tw
 

Apache Point Observatory (APO)

We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken
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 new activity), but could also help clean up astrometry for batches of NEOs (especially if this occurs at the same time as another trigger). https://www.apo.nmsu.edu/
Added:
>
>

Lulin One-meter Telescope (LOT)

ToO can be requested for Solar-system follow-up. Most of the time LOT is equipped with Princeton Instrument's SOPHIA CCD (2k x 2k) with standard broadband filters, occasionally there will have instruments change. PS: Quan-Zhi can also trigger LOT ToO follow-up.
 -- EmilyKramer - 24 Aug 2018 \ No newline at end of file

Revision 42018-08-24 - EmilyKramer

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META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

This page will have a table of follow-up observatories and their capabilities so that the daily Shepherd has these resources handy.

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>
>		From the International Asteroid Warning Network (IAWN): http://iawn.net/features/astrometric.shtml
 
Facility Field of View Limiting Magnitude Pointing limits Contact info
Facility 1 Field of view 1 Limiting mag 1 Pointing limit 1 Contact info 1
APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
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 new activity), but could also help clean up astrometry for batches of NEOs (especially if this occurs at the same time as another trigger). https://www.apo.nmsu.edu/
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<		-- EmilyKramer - 20 Aug 2018
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>		-- EmilyKramer - 24 Aug 2018
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Revision 32018-08-20 - EmilyKramer

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META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

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APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
Changed:
<
<		* APO: We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken
>
>

Apache Point Observatory (APO)

We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken
 in a single half-night block. Typically need a few nights to arrange scheduling before follow up can occur. APO is a 3.5m, with an imager with 7.5 sq arcminute FOV (6 filters available), as well as other instruments. This follow up time is probably most useful to investigate new objects of particular interest (such as mini-moons, interstellar objects, or objects where we pick up new activity), but could also help clean up astrometry for batches of NEOs (especially if this occurs at the same time as another trigger).
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>		https://www.apo.nmsu.edu/
 
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<		-- EmilyKramer - 10 Aug 2018
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>		-- EmilyKramer - 20 Aug 2018

Revision 22018-08-20 - LynneJones

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META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

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Facility Field of View Limiting Magnitude Pointing limits Contact info
Facility 1 Field of view 1 Limiting mag 1 Pointing limit 1 Contact info 1
Added:
>
>
APO* 7.5 sq arcminutes 23.5   Bryce Bolin bryce@b612foundation.org
 
Added:
>
>		* APO: We are currently requesting 1 half night per quarter for general solar system ToO follow up, which needs to be taken in a single half-night block. Typically need a few nights to arrange scheduling before follow up can occur. APO is a 3.5m, with an imager with 7.5 sq arcminute FOV (6 filters available), as well as other instruments. This follow up time is probably most useful to investigate new objects of particular interest (such as mini-moons, interstellar objects, or objects where we pick up new activity), but could also help clean up astrometry for batches of NEOs (especially if this occurs at the same time as another trigger).
  -- EmilyKramer - 10 Aug 2018

Revision 12018-08-10 - EmilyKramer

Line: 1 to 1
Added:
>
>
META TOPICPARENT name="NEOZTFScanning"

Follow Up Observatory Resources

This page will have a table of follow-up observatories and their capabilities so that the daily Shepherd has these resources handy.

Facility Field of View Limiting Magnitude Pointing limits Contact info
Facility 1 Field of view 1 Limiting mag 1 Pointing limit 1 Contact info 1

-- EmilyKramer - 10 Aug 2018

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