DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | A2061_2 | 230.6122 | 30.8661 | 230.100044 | 31.043682 | 216.595507 | 47.269453 | 48.57175305 | 56.92431824 | 121.1842 | 56307.485625 | 2013-01-15 11:39:18 | 56308.5460185185 | 2013-01-16 13:06:16 | 807030010 | 41.788 | 40 | 41.788 | 41.788 | 0 | 41.788 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 37.7529 | 37.7529 | 91.6018 | 1 | PROCESSED | 57608.5263888889 | 2016-08-08 12:38:00 | 56707 | 2014-02-19 00:00:00 | 56338.5482291667 | 2013-02-15 13:09:27 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070070 | We propose to conduct multi-pointing observations to cover the entire region of A2061 hosting radio relic. We discovered that the radio relic is located in the cluster outskirts of the opposite side of the filamentary large-scale structure. We found the same trend for 3 relic clusters compiling NVSS radio and SDSS optical data-sets, though the sample number is small. It suggests that an universal process to form radio relic potentially exists. We therefore aim to map out the temperature, density, pressure, and entropy of the intra-cluster medium (ICM) to understand the interplays among the large-scale structure, the ICM and radio relic. Our study provides us a comprehensive picture of the ICM in the radio relic cluster. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | NOBUHIRO OKABE | JAP | 7 | AO7 | SUZAKU OBSERVATION OF THE OUTSKIRTS IN RADIO RELIC CLUSTER A2061 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807030010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807030010'
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