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 | A 2218 OFFSETB | 249.9091 | 65.2119 | 249.835523 | 65.307656 | 180.044789 | 81.713752 | 96.37864193 | 38.09205953 | 233.3309 | 53670.1916319444 | 2005-10-27 04:35:57 | 53670.4620833333 | 2005-10-27 11:05:24 | 800020010 | 14.9215 | 15 | 14.9375 | 14.9335 | 14.9215 | 14.9415 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 14.1931 | 14.1931 | 23.3561 | 0 | PROCESSED | 57527.6596180556 | 2016-05-19 15:49:51 | 54247 | 2007-05-27 00:00:00 | 54036.8343981482 | 2006-10-28 20:01:32 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001096 | To confirm the presence of redshifted oxygen lines from the WHIM surrounding A2218, we propose observations of 2 positions. One is a 35 ksec pointing on A2218 to raise the photon statistics of the oxygen feature, and the other is a 15 ksec pointing at about 1 degree west of the cluster to know the amplitude of the intensity variation of the Galactic oxygen lines. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | TAKAYA OHASHI | JAP | 0 | SWG | SEARCH FOR OXYGEN LINES FROM WARM IGM | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800020010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '800020010'
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