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 | B2 1023+25 | 156.5986 | 25.7113 | 155.903697 | 25.966089 | 148.79406 | 14.812793 | 207.05661505 | 57.60744793 | 288.3095 | 56442.6428125 | 2013-05-30 15:25:39 | 56444.9133449074 | 2013-06-01 21:55:13 | 708044010 | 100.8874 | 100 | 100.8954 | 100.8874 | 0 | 100.8954 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 96.5787 | 96.5787 | 196.1298 | 2 | PROCESSED | 57611.461099537 | 2016-08-11 11:03:59 | 56821 | 2014-06-13 00:00:00 | 56455.8205324074 | 2013-06-12 19:41:34 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 082005 | We propose a deep (100 ksec) Suzaku observation of the recently discovered high redshift blazar candidate B2 1023+25 (z=5.3). A very hard (Gamma <2) spectrum would confirm its blazar nature, allowing to study the physical properties of the relativistic jet in this extremely powerful and very high redshift source. The proposed observation will yield an X-ray spectrum of sufficient quality to determine the X-ray shape. The confirmation of a second blazar at this redshift has profound cosmological implications, placing stronger constraints on the number density of high mass BH at high z | EXTRAGALACTIC COMPACT SOURCES | 7 | A | VALENTINA BRAITO | EUR | 8 | AO8 | THE HIGH-REDSHIFT BLAZAR CANDIDATE B2 1023+25 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708044010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '708044010'
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