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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