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 | HD432 | 2.3072 | 59.1394 | 1.650501 | 58.861236 | 35.115755 | 51.206006 | 117.5327944 | -3.28915956 | 247.7181 | 54469.7038310185 | 2008-01-04 16:53:31 | 54470.5154513889 | 2008-01-05 12:22:15 | 402034010 | 38.2406 | 40 | 38.2486 | 38.2406 | 0 | 38.2486 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 35.0503 | 35.0503 | 70.12 | 1 | PROCESSED | 57540.9911574074 | 2016-06-01 23:47:16 | 54908 | 2009-03-18 00:00:00 | 54483.4635532407 | 2008-01-18 11:07:31 | 3.0.22.43 | 5 | 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/ver3.0/402034010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402034010'
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