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 | U SCO | 245.6288 | -17.8156 | 244.907071 | -17.699112 | 246.808077 | 3.684973 | 357.72079613 | 21.90901194 | 93.2747 | 55233.0102430556 | 2010-02-06 00:14:45 | 55234.2918865741 | 2010-02-07 07:00:19 | 404018010 | 46.0764 | 20 | 46.0764 | 46.0764 | 0 | 46.0764 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 37.6117 | 37.6117 | 110.7199 | 1 | PROCESSED | 57550.518599537 | 2016-06-11 12:26:47 | 55617 | 2011-02-25 00:00:00 | 55250.1559375 | 2010-02-23 03:44:33 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040057 | We propose a 100ks TOO observation of a recurrent novae burst in our Galaxy. Using Suzaku's wide-energy coverage and excellent spectral performance at the iron K complex, we aim to derive the amount of mass loss at a classical nova burst. We plan to visit a nova withinin a few days and take spectra at five epochs spanning 10 days with 20ks each. | GALACTIC POINT SOURCES | 4 | A | DAI TAKEI | JAP | 4 | AO4-TOO | TOO OBSERVATION OF A RECURRENT NOVA EXPLOSION | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404018010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404018010'
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