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
1 HD432 2.3079 59.1397 1.651195 58.861536 35.116502 51.20601 117.53319828 -3.2889222 246.0535 54471.6956944444 2008-01-06 16:41:48 54472.297349537 2008-01-07 07:08:11 402034020 26.9844 27 26.9844 26.9844 0 26.9844 1 1 0 1 1 0 0 24.601 24.601 51.9759 0 PROCESSED 57541.2823958333 2016-06-02 06:46:39 54871 2009-02-09 00:00:00 54483.3863773148 2008-01-18 09:16:23 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021016 Suzaku XIS spectra of three "X-ray deficient" Hertzsprung gap giants will explore why they display anomalous coronal behavior compared with cooler giants only slightly further advanced in their evolution. The apparent sharp transition in coronal properties on the way to helium flash might be caused by disruption of a "fossil" magnetosphere by a newly born solar-like dynamo. A key discriminator is the coronal energy distribution, especially enhanced and sporadic hard emission associated with flaring. The proposed targets are the brightest not previously observed in X-rays at CCD resolution; all three have supporting high resolution UV spectra. Expanding the sample of high quality, high energy information on this key class of objects is essential for probing their odd behavior. GALACTIC POINT SOURCES 4 C THOMAS AYRES USA 2 AO2 ANOMALOUS CORONAE OF HERTZSPRUNG GAP GIANTS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402034020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402034020'

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