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 | NGC 2300 GROUP | 112.834 | 85.6974 | 108.693645 | 85.79613 | 93.629136 | 62.546385 | 127.72312729 | 27.79205873 | 339.9186 | 55237.1794907407 | 2010-02-10 04:18:28 | 55238.2502777778 | 2010-02-11 06:00:24 | 804030020 | 52.5611 | 100 | 52.5611 | 52.5611 | 0 | 52.5611 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 47.712 | 47.712 | 92.498 | 0 | PROCESSED | 57550.5807986111 | 2016-06-11 13:56:21 | 55633 | 2011-03-13 00:00:00 | 55266.3365625 | 2010-03-11 08:04:39 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040055 | We propose to observe the NGC 2300 group for 100 ks and a offset pointing for 200 ks to evaluate the background emission from the Galaxy. The purpose of the observations are to measure O, Mg, Si and Fe abundances of intragaractic medium to study metal synthesis in this small group of galaxies. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KYOKO MATSUSHITA | JAP | 4 | AO4 | O, MG, S AND FE ABUNDANCES OF INTRAGROUP MEDIUM IN THE NGC 2300 GROUP | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804030020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '804030020'
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