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 | V1280 SCO | 254.4172 | -32.3368 | 253.607248 | -32.260102 | 256.681689 | -9.612724 | 351.33470039 | 6.5596985 | 97.7451 | 55605.3662615741 | 2011-02-13 08:47:25 | 55608.0501851852 | 2011-02-16 01:12:16 | 405029010 | 99.683 | 100 | 99.699 | 99.683 | 0 | 99.699 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 86.9306 | 86.9306 | 231.8739 | 2 | PROCESSED | 57600.9978472222 | 2016-07-31 23:56:54 | 55983 | 2012-02-26 00:00:00 | 55617.4142361111 | 2011-02-25 09:56:30 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050110 | We propose a 100 ks observation of the C-rich classical nova V1280 Sco. Using Suzaku's excellent spectral performance in the soft X-ray energy band, we aim to detect and to resolve emission lines from C, N, and O. | GALACTIC POINT SOURCES | 4 | A | DAI TAKEI | JAP | 5 | AO5 | X-RAY SPECTROSCOPY OF THE C-RICH CLASSICAL NOVA V1280 SCO | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405029010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '405029010'
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