Gamma ray |
HESS (High Energy Stereoscopic System) |
TeV |
https://www.mpi-hd.mpg.de/hfm/HESS/pages/home/proposals/ |
October 1 for the next year proposal |
Gamma ray |
INTEGRAL |
3keV-10MeV |
https://www.cosmos.esa.int/web/integral/ao17 |
2019/4/5, 14:00 CEST |
Gamma ray |
Fermi |
GBM (10keV-25MeV); LAT(20MeV-300GeV) |
https://fermi.gsfc.nasa.gov/ssc/proposals/cycle12/ |
2019/3/20, 4:30 EST |
X-ray |
NuSTAR |
3-79 keV |
https://heasarc.gsfc.nasa.gov/docs/nustar/nupropthread.html |
2019/3/29, 4:30pm EDT |
X-ray |
NICER |
0.2-12 keV |
https://heasarc.gsfc.nasa.gov/docs/nicer/ |
can request TOO (within 4 hours) |
X-ray |
Chandra |
0.4-10 keV(HETG) |
http://cxc.harvard.edu/proposer/ |
2019/3/14, 6pm EDT |
X-ray |
XMM-Newton |
0.15-15 keV(EPIC) |
https://heasarc.gsfc.nasa.gov/docs/xmm/xmmhp_prop_tools.html |
2019/10/11, 12:00 UT |
X-ray |
ASTROSAT |
multi-wavelength: cover the visible (320–530 nm), near UV (180–300 nm), far UV (130–180 nm), soft X-ray (0.3–8 keV and 2–10 keV) and hard X-ray (3–80 keV and 10–150 keV) |
http://astrosat-ssc.iucaa.in/?q=proposal_preparation |
2019/4/23, 09:00 UT |
X-ray |
HXMT |
1-250 keV |
http://proposal.ihep.ac.cn/proposal/index.jspx |
??? |
X-ray |
Swift |
multi-wavelength: BAT (15-150 keV); XRT (0.2-10 keV); UVOT (1928A-5468A) |
https://swift.gsfc.nasa.gov/proposals/swiftgi.html |
2019/9/26, 7:30pm EDT |
UV |
Hubble Sapce Telescope |
ACS (350nm-1100nm), COS(90nm-320nm), FGS, STIS, and WFC3 |
http://www.stsci.edu/hst/proposing |
Phase I deadline: 2019/4/5, 8:00pm EDT |
Optical |
Keck (10m) |
https://www2.keck.hawaii.edu/inst/index.php |
https://www2.keck.hawaii.edu/observing/apply.html |
12 September 2019 NASA proposals; 18 September 2019 Yale proposals due; 27 September 2019 UC proposals due; TBD September 2019 (5pm AEST) Swinburne proposals due; 30 Septemberr 2019 (5:00pm PDT) CIT proposals due; 07 October 2019 (8:00pm CDT) Northwestern proposals due; TBD October 2019 UH proposals due |
Optical |
Subaru (8m) |
https://www.naoj.org/Observing/Instruments/index.html |
https://subarutelescope.org/Observing/Proposals/call.html |
Semester S22A: February 1, 2022 -- July 31, 2022 |
Optical |
Gemini (8m) |
https://www.gemini.edu/sciops/instruments/ |
http://www.gemini.edu/sciops/observing-gemini/semester-2020a-call-proposals |
2019/9/31 or 2019/10/1 depending on the participanting institutions, please refer to the link |
Optical |
SOAR (4.2m) |
optical and IR spectragraph or optical (with OA) imager |
http://www.ctio.noao.edu/soar/ |
2019/9/30, 11:59PM MST |
Optical |
WIYM (3.5 m) |
Optical and IR imager, spectragraph (IFU or fiber) |
http://www.wiyn.org/Observe/wiynusrhandbook.html#apply |
2019/9/30 |
Optical |
AAT (3.9 m) |
spectragraph |
http://ast.noao.edu/observing/call-for-proposals-2020a |
2019/9/30 |
Optical |
Las Cumbres Observatory (1m plus 2m network) |
optical imager |
https://lco.global/observatory/tools/ |
2019/9/30, 11:59PM MST (via NOAO) 2019/9/26, 17:00, CST (via China TAP 2020A) |
Optical |
CFHT (3.6m) |
http://www.cfht.hawaii.edu/en/science/Proposals/ |
tap.china-vo.org |
26 March 2019 17:00 China Standard Time (2019B); 2019/9/26, 17:00, CST (2020A) |
Optical |
MMT (6.5m) |
https://www.as.arizona.edu/mmt-65m-telescope |
tap.china-vo.org |
up to 6 nights via China TAP 2018A (26 September 2017 17:00 China Standard Time) |
Optical |
Palomar/P200 |
http://www.astro.caltech.edu/palomar/observer/200inchResources/P200filters.html |
tap.china-vo.org |
"26 March 2019 17:00 China Standard Time (2019B); 2019/9/26, 17:00, CST (TAP 2020A)" |
Optical |
Lijiang 2M4 telescope |
optical spectragraph |
http://www.gmg.org.cn/v2/ |
unknown |
Optical/IR/Radio |
ESO facilities |
Very Large Telescope (optical; e.g., X-SHOOTER spectrograph; VISTA (infared); VST (optical); NTT(3.6m; optical or IR spectroscopy; optical image); APEX (radio) |
https://www.eso.org/sci/observing.html |
run from 1 October through 31 March; run for 1 April through 30 September |
IR |
Spitzer |
IRAC:3.6/4.5/5.8/8 microns; IRS: 5.2 to 38 microns; MIPS:24, 70, and 160 microns |
http://ssc.spitzer.caltech.edu/warmmission/propkit/ |
DDT proposals,the final date for executing Spitzer observations will be January 29, 2020;Cycle 14:Friday, 23 March 2018, 2 PM PDT |
Radio |
National Radio Astronomy Observatory (NRAO) |
Karl G. Jansky Very Large Array (VLA): From 1.0 GHz to 50 GHz; the Green Bank Telescope (GBT); the Very Long Baseline Array (VLBA):0.3 GHz – 96 GHz (90 cm – 3 mm); High Sensitivity Array (HSA) |
https://science.nrao.edu/observing/call-for-proposals |
2020A:2019/08/01, 21:00 (UTC); 2020B:2020/02/21 |
Radio |
ALMA |
From 31 GHz to 950 GHz |
https://almascience.nrao.edu/proposing/7m-array-supplemental-call/7m-array-supplemental-call-main |
2019/10/1, 15:00(UT) |
Radio |
ATCA |
Australia Telescope Compact Array Parkes Telescope; Australian Long Baseline Array (LBA); Tidbinbilla 70-m and 34-m antennas |
https://www.parkes.atnf.csiro.au/observing/schedules/ |
around 07/15 obs:10/01--05/31; around 12/15 obs: 04/01-09/30 |
Radio |
Murchison Wildfield Array |
70MHz-300MHz |
http://www.mwatelescope.org/data/observing |
2019B: Friday 7th June 2019, 5pm Australian Western Standard Time (AWST) or 2019A: Tuesday 15th October 2018, 5pm Australian Western Standard Time (AWST) |
Radio |
The Submillimeter Array |
180 GHz to 418 GHz |
http://sma1.sma.hawaii.edu/proposing.html |
"The deadline for the 2019B semester |
(observing period: 16 Nov 2019 - 15 May 2020) is September 05, 2019" |
|
|
|
|
Radio |
Taeduk Radio Astronomy Observatory (TRAO) |
VLBI observations at 22 and 43 GHz |
https://radio.kasi.re.kr/kava/proposal_info.php |
3rd June, 2019, 08:00 UT (KST 17:00) |
Radio |
Taeduk Radio Astronomy Observatory (TRAO) |
14m radio telescope |
https://radio.kasi.re.kr/trao/proposal.php |
the end of August 2019 |
Radio |
GMRT |
50, 153, 233, 325, 610 and 1420 MHz. |
http://www.ncra.tifr.res.in/ncra/gmrt/gtac |
A: 15 January, obs:April-Sep.; B: 15 July, obs:Oct-March |
IR/Sub-mm |
SOFIA |
0.3-1600 um (image or spectroscopy) |
https://www.sofia.usra.edu/science/proposing-and-observing/proposal-calls |
2019/09/07 4:00(UTC; obs:2020/04/25--2021/04/25 |
IR |
IRTF |
1:SpeX, a 0.7-5.3 micron medium-resolution spectrograph and imager; 2:MORIS, an optical imager and as an optical guider for SpeX; 3: iSHELL, a 1.06 – 5.3 micron cross-dispersed echelle spectrograph (up to R=80,000) and imager; 4: MIRSI/MOC, a 5 – 20 micron camera and grism spectrograph and optical imager |
http://irtfweb.ifa.hawaii.edu/observing/callForProposals.php |
A: 12:00AM on September 01, 2019; B: 5:00PM on October 01, 2019 HST |
Radio |
Arecibo 305-m telescope |
305 meters |
http://www.naic.edu/ao/scientist-user-portal/proposal-submission-system/call-for-proposals |
the first Thursdays of March and September; September 5, 2019 (17:00 AST, 21:00 UTC) |
Radio |
South Africa Radio Observatory |
MeerKAT 900–1670 MHz |
http://www.ska.ac.za/science-engineering/meerkat/observers/observing-programme/ |
Dec-18 |
Radio |
Radio Telescope Effelsberg |
100 meters |
https://www.mpifr-bonn.mpg.de/247288/Call-for-proposals |
around February 05, June 05, October 05; Deadline 02 October 2019 (15:00 UT) |
Radio |
IRAM Telescopes |
30 meters(3, 2, 1, and 0.9mm), NOEMA(1.3 mm) |
https://www.iram-institute.org/EN/content-page-169-7-57-169-0-0.html |
mid-March (obs:01 June - 30 November); mid-September (obs01 December - 31 May); 12 September 2019, 17:00 CEST (UT + 2 hours) |
Radio |
Tianma 65m |
|
http://english.shao.cas.cn/rh/scientific/201901/t20190115_204050.html |
Deadline: 28 February 2019 (BJT 17:00) |
Radio |
JCMT |
|
https://www.eaobservatory.org/jcmt/proposals/ |
mid September for obs: February 1st to July 31st; mid March for obs:August 1st to January 31st |
Radio |
SMA |
|
https://www.eaobservatory.org/east-asia-observatory/sma/ |
Friday, 6 September 2019, 04:00 CST (Taipei); obs:(2019 Nov 16 – 2020 May 15) |
Radio |
LOFAR |
High Band Antennas (HBA, 110-240 MHz) and Low Band Antennas (LBA, 10-90 MHz); 8,000 antennas spread across the continent |
https://www.radionet-org.eu/radionet/lofar-call-for-proposal/ |
DDT proposals at any time 11 September 2019, 12 UT for obs: December 2019 - 31 May 2020 around mid March and mid Sep for 2 semesters |
|
|
|
|
|