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 V2491 CYG 295.7679 32.3068 295.285617 32.186831 307.093304 52.481406 67.2208484 4.33923679 253.6206 55503.4390162037 2010-11-03 10:32:11 55505.2709837963 2010-11-05 06:30:13 405036010 74.4004 70 74.4004 74.4004 0 74.4004 2 2 0 2 1 0 0 57.2065 57.2065 158.2519 2 PROCESSED 57553.9866087963 2016-06-14 23:40:43 55885 2011-11-20 00:00:00 55518.4178356482 2010-11-18 10:01:41 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051213 We propose to observe again one of the most luminous and intriguing classical novae of the last two years, after it has returned to quiescence. The goala are to understand how accretion is re-estabilished, investigate the claim that the white dwarf an intermediate polar (IP), estimate mass accretion are and white dwarf mass. IP are a class of X-ray sources that Suzaku is ideally suited to study, and we want to study the influence of the magnetic field on the nova evolution. GALACTIC POINT SOURCES 4 C MARINA ORIO USA 5 AO5 REVISITING AN X-RAY LUMINOUS NOVA NOVA AFTER THE ERUPTION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405036010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '405036010'

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